Outputs (196)

The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation (2024)
Journal Article
Manzoni, G., Baugh, C. M., Norberg, P., Cabayol, L., van den Busch, J. L., Wittje, A., …Tortorelli, L. (2024). The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation. Monthly Notices of the Royal Astronomical Society, 530(2), 1394-1413. https://doi.org/10.1093/mnras/stae659

We use the GALFORM semi-analytical galaxy formation model implemented in the Planck Millennium N-body simulation to build a mock galaxy catalogue on an observer’s past lightcone. The mass resolution of this N-body simulation is almost an order of mag... Read More about The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation.

A new test of gravity – II. Application of marked correlation functions to luminous red galaxy samples (2024)
Journal Article
Armijo, J., Baugh, C. M., Norberg, P., & Padilla, N. D. (2024). A new test of gravity – II. Application of marked correlation functions to luminous red galaxy samples. Monthly Notices of the Royal Astronomical Society, 528(4), 6631-6636. https://doi.org/10.1093/mnras/stae449

We apply the marked correlation function test proposed by Armijo et al. (Paper I) to samples of luminous red galaxies (LRGs) from the final data release of the Sloan Digital Sky Survey (SDSS) III. The test assigns a density-dependent mark to galaxies... Read More about A new test of gravity – II. Application of marked correlation functions to luminous red galaxy samples.

The two-point correlation function covariance with fewer mocks (2023)
Journal Article
Trusov, S., Zarrouk, P., Cole, S., Norberg, P., Zhao, C., Aguilar, J. N., …Zhou, Z. (2024). The two-point correlation function covariance with fewer mocks. Monthly Notices of the Royal Astronomical Society, 527(3), 9048-9060. https://doi.org/10.1093/mnras/stad3710

We present FITCOV an approach for accurate estimation of the covariance of two-point correlation functions that requires fewer mocks than the standard mock-based covariance. This can be achieved by dividing a set of mocks into jackknife regions and f... Read More about The two-point correlation function covariance with fewer mocks.

The DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation (2023)
Journal Article
Hahn, C., Wilson, M. J., Ruiz-Macias, O., Cole, S., Weinberg, D. H., Moustakas, J., …Zou, H. (2023). The DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation. Astronomical Journal, 165(6), Article 253. https://doi.org/10.3847/1538-3881/accff8

Over the next 5 yr, the Dark Energy Spectroscopic Instrument (DESI) will use 10 spectrographs with 5000 fibers on the 4 m Mayall Telescope at Kitt Peak National Observatory to conduct the first Stage IV dark energy galaxy survey. At z < 0.6, the DESI... Read More about The DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation.

A sparse regression approach for populating dark matter haloes and subhaloes with galaxies (2022)
Journal Article
Icaza-Lizaola, M., Bower, R. G., Norberg, P., Cole, S., & Schaller, M. (2022). A sparse regression approach for populating dark matter haloes and subhaloes with galaxies. Monthly Notices of the Royal Astronomical Society, 518(2), 2903-2920. https://doi.org/10.1093/mnras/stac3265

We use sparse regression methods (SRMs) to build accurate and explainable models that predict the stellar mass of central and satellite galaxies as a function of properties of their host dark matter haloes. SRMs are machine learning algorithms that p... Read More about A sparse regression approach for populating dark matter haloes and subhaloes with galaxies.

A light-cone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS (2022)
Journal Article
Smith, A., Cole, S., Grove, C., Norberg, P., & Zarrouk, P. (2022). A light-cone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS. Monthly Notices of the Royal Astronomical Society, 516(3), 4529 - 4542. https://doi.org/10.1093/mnras/stac2519

The use of realistic mock galaxy catalogues is essential in the preparation of large galaxy surveys, in order to test and validate theoretical models and to assess systematics. We present an updated version of the mock catalogue constructed from the... Read More about A light-cone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS.

Solving small-scale clustering problems in approximate light-cone mocks (2022)
Journal Article
Smith, A., Cole, S., Grove, C., Norberg, P., & Zarrouk, P. (2022). Solving small-scale clustering problems in approximate light-cone mocks. Monthly Notices of the Royal Astronomical Society, 516(1), 1062 - 1071. https://doi.org/10.1093/mnras/stac2219

Realistic light-cone mocks are important in the clustering analyses of large galaxy surveys. For simulations where only the snapshots are available, it is common to create approximate light-cones by joining together the snapshots in spherical shells.... Read More about Solving small-scale clustering problems in approximate light-cone mocks.

The DESI N-body simulation project – I. Testing the robustness of simulations for the DESI dark time survey (2022)
Journal Article
Grove, C., Chuang, C., Devi, N. C., Garrison, L., L’Huillier, B., Feng, Y., …Valenzuela, O. (2022). The DESI N-body simulation project – I. Testing the robustness of simulations for the DESI dark time survey. Monthly Notices of the Royal Astronomical Society, 515(2), https://doi.org/10.1093/mnras/stac1947

Analysis of large galaxy surveys requires confidence in the robustness of numerical simulation methods. The simulations are used to construct mock galaxy catalogues to validate data analysis pipelines and identify potential systematics. We compare th... Read More about The DESI N-body simulation project – I. Testing the robustness of simulations for the DESI dark time survey.

Making use of sub-resolution haloes in N-body simulations (2021)
Journal Article
Armijo, J., Baugh, C. M., Padilla, N. D., Norberg, P., & Arnold, C. (2022). Making use of sub-resolution haloes in N-body simulations. Monthly Notices of the Royal Astronomical Society, 510(1), 29-33. https://doi.org/10.1093/mnrasl/slab122

Conservative mass limits are often imposed on the dark matter halo catalogues extracted from N-body simulations. By comparing simulations with different mass resolutions, at z = 0 we find that even for haloes resolved by 100 particles, the lower reso... Read More about Making use of sub-resolution haloes in N-body simulations.

Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys (2021)
Journal Article
Zarrouk, P., Ruiz-Macias, O., Cole, S., Norberg, P., Baugh, C., Brooks, D., …Tarlé, G. (2022). Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys. Monthly Notices of the Royal Astronomical Society, 509(1), 1478-1493. https://doi.org/10.1093/mnras/stab2814

We characterize the selection cuts and clustering properties of a magnitude-limited sample of bright galaxies that is part of the Bright Galaxy Survey (BGS) of the Dark Energy Spectroscopic Instrument (DESI) using the ninth data release of the Legacy... Read More about Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys.

A sparse regression approach to modelling the relation between galaxy stellar masses and their host haloes (2021)
Journal Article
Icaza-Lizaola, M., Bower, R. G., Norberg, P., Cole, S., Schaller, M., & Egan, S. (2021). A sparse regression approach to modelling the relation between galaxy stellar masses and their host haloes. Monthly Notices of the Royal Astronomical Society, 507(3), 4584-4602. https://doi.org/10.1093/mnras/stab2368

Sparse regression algorithms have been proposed as the appropriate framework to model the governing equations of a system from data, without needing prior knowledge of the underlying physics. In this work, we use sparse regression to build an accurat... Read More about A sparse regression approach to modelling the relation between galaxy stellar masses and their host haloes.

Rosella: a mock catalogue from the P-Millennium simulation (2021)
Journal Article
Safonova, S., Norberg, P., & Cole, S. (2021). Rosella: a mock catalogue from the P-Millennium simulation. Monthly Notices of the Royal Astronomical Society, 505(1), 325-338. https://doi.org/10.1093/mnras/stab1286

The scientific exploitation of the Dark Energy Spectroscopic Instrument Bright Galaxy Survey (DESI BGS) data requires the construction of mocks with galaxy population properties closely mimicking those of the actual DESI BGS targets. We create a high... Read More about Rosella: a mock catalogue from the P-Millennium simulation.

Baryon acoustic oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys (2021)
Journal Article
Zarrouk, P., Rezaie, M., Raichoor, A., Ross, A. J., Alam, S., Blum, R., …Zhao, C. (2021). Baryon acoustic oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys. Monthly Notices of the Royal Astronomical Society, 503(2), 2562-2582. https://doi.org/10.1093/mnras/stab298

We search for the baryon acoustic oscillations in the projected cross-correlation function binned into transverse comoving radius between the SDSS-IV DR16 eBOSS quasars and a dense photometric sample of galaxies selected from the DESI Legacy Imaging... Read More about Baryon acoustic oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys.

Characterizing the target selection pipeline for the Dark Energy Spectroscopic Instrument Bright Galaxy Survey (2021)
Journal Article
Ruiz-Macias, O., Zarrouk, P., Cole, S., Baugh, C. M., Norberg, P., Lucey, J., …Wilson, M. (2021). Characterizing the target selection pipeline for the Dark Energy Spectroscopic Instrument Bright Galaxy Survey. Monthly Notices of the Royal Astronomical Society, 502(3), 4328-4349. https://doi.org/10.1093/mnras/stab292

We present the steps taken to produce a reliable and complete input galaxy catalogue for the Dark Energy Spectroscopic Instrument (DESI) Bright Galaxy Survey (BGS) using the photometric Legacy Survey DR8 DECam. We analyse some of the main issues face... Read More about Characterizing the target selection pipeline for the Dark Energy Spectroscopic Instrument Bright Galaxy Survey.

The PAU Survey: an improved photo-z sample in the COSMOS field (2021)
Journal Article
Alarcon, A., Gaztanaga, E., Eriksen, M., Baugh, C. M., Cabayol, L., Casas, R., …Tallada-Crespí, P. (2021). The PAU Survey: an improved photo-z sample in the COSMOS field. Monthly Notices of the Royal Astronomical Society, 501(4), 6103-6122. https://doi.org/10.1093/mnras/staa3659

We present – and make publicly available – accurate and precise photometric redshifts in the ACS footprint from the COSMOS field for objects with iAB ≤ 23. The redshifts are computed using a combination of narrow-band photometry from PAUS, a survey w... Read More about The PAU Survey: an improved photo-z sample in the COSMOS field.

The Pan-STARRS1 Database and Data Products (2020)
Journal Article
Flewelling, H., Magnier, E., Chambers, K., Heasley, J., Holmberg, C., Huber, M., …Shiao, B. (2020). The Pan-STARRS1 Database and Data Products. Astrophysical Journal Supplement, 251(1), Article 7. https://doi.org/10.3847/1538-4365/abb82d

This paper describes the organization of the database and the catalog data products from the Pan-STARRS1 3π Steradian Survey. The catalog data products are available in the form of an SQL-based relational database from MAST, the Mikulski Archive for... Read More about The Pan-STARRS1 Database and Data Products.

Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS (2020)
Journal Article
Manzoni, G., Scodeggio, M., Baugh, C., Norberg, P., De Lucia, G., Fritz, A., …Vergani, D. (2021). Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS. New Astronomy, 84, Article 101515. https://doi.org/10.1016/j.newast.2020.101515

We study the evolution of the colour-magnitude relation for galaxies in the VIMOS Public Extragalactic Redshift Survey (VIPERS) by introducing the concept of the bright edge, and use this to derive constraints on the quenching of star formation activ... Read More about Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS.

Do model emission line galaxies live in filaments at z∼1? (2020)
Journal Article
Gonzalez-Perez, V., Cui, W., Contreras, S., Baugh, C., Comparat, J., Griffin, A., …Norberg, P. (2020). Do model emission line galaxies live in filaments at z∼1?. Monthly Notices of the Royal Astronomical Society, 498(2), 1852-1870. https://doi.org/10.1093/mnras/staa2504

Current and future cosmological surveys are targeting star-forming galaxies at z∼ 1 with nebular emission lines. We use a state-of-the-art semi-analytical model of galaxy formation and evolution to explore the large scale environment of star-forming... Read More about Do model emission line galaxies live in filaments at z∼1?.

Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra (2020)
Journal Article
Gunawardhana, M., Brinchmann, J., Weilbacher, P., Norberg, P., Monreal-Ibero, A., Nanayakkara, T., …Kollatschny, W. (2020). Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra. Monthly Notices of the Royal Astronomical Society, 497(3), 3860-3895. https://doi.org/10.1093/mnras/staa2158

We have modelled the stellar and nebular continua and emission-line intensity ratios of massive stellar populations in the Antennae galaxy using high resolution and self-consistent libraries of model H II regions around central clusters of ageing sta... Read More about Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra.

An optimized tiling pattern for multiobject spectroscopic surveys: application to the 4MOST survey (2020)
Journal Article
Tempel, E., Tuvikene, T., Muru, M., Stoica, R., Bensby, T., Chiappini, C., …de Jong, R. (2020). An optimized tiling pattern for multiobject spectroscopic surveys: application to the 4MOST survey. Monthly Notices of the Royal Astronomical Society, 497(4), 4626-4643. https://doi.org/10.1093/mnras/staa2285

Large multiobject spectroscopic surveys require automated algorithms to optimize their observing strategy. One of the most ambitious upcoming spectroscopic surveys is the 4MOST survey. The 4MOST survey facility is a fibre-fed spectroscopic instrument... Read More about An optimized tiling pattern for multiobject spectroscopic surveys: application to the 4MOST survey.

Probabilistic fibre-to-target assignment algorithm for multi-object spectroscopic surveys (2020)
Journal Article
Tempel, E., Norberg, P., Tuvikene, T., Bensby, T., Chiappini, C., Christlieb, N., …de Jong, R. (2020). Probabilistic fibre-to-target assignment algorithm for multi-object spectroscopic surveys. Astronomy & Astrophysics, 635, Article A101. https://doi.org/10.1051/0004-6361/201937228

Context. Several new multi-object spectrographs are currently planned or under construction that are capable of observing thousands of Galactic and extragalactic objects simultaneously. Aims. In this paper we present a probabilistic fibre-to-target a... Read More about Probabilistic fibre-to-target assignment algorithm for multi-object spectroscopic surveys.

Estimating the galaxy two-point correlation function using a split random catalog (2019)
Journal Article
Keihänen, E., Kurki-Suonio, H., Lindholm, V., Viitanen, A., Suur-Uski, A., Allevato, V., …Sánchez, A. (2019). Estimating the galaxy two-point correlation function using a split random catalog. Astronomy & Astrophysics, 631, Article A73. https://doi.org/10.1051/0004-6361/201935828

The two-point correlation function of the galaxy distribution is a key cosmological observable that allows us to constrain the dynamical and geometrical state of our Universe. To measure the correlation function we need to know both the galaxy positi... Read More about Estimating the galaxy two-point correlation function using a split random catalog.

A new approach to finding galaxy groups using Markov Clustering (2019)
Journal Article
Stothert, L., Norberg, P., & Baugh, C. (2019). A new approach to finding galaxy groups using Markov Clustering. Monthly Notices of the Royal Astronomical Society: Letters, 485(1), L126-L130. https://doi.org/10.1093/mnrasl/slz045

We present a proof of concept of a new galaxy group finder method, Markov graph CLustering (MCL) that naturally handles probabilistic linking criteria. We introduce a new figure of merit, the variation of information (VI) statistic, used to optimize... Read More about A new approach to finding galaxy groups using Markov Clustering.

The Effect of Assembly Bias on Redshift Space Distortions (2019)
Journal Article
Padilla, N., Contreras, S., Zehavi, I., Baugh, C., & Norberg, P. (2019). The Effect of Assembly Bias on Redshift Space Distortions. Monthly Notices of the Royal Astronomical Society, 486(1), 582-595. https://doi.org/10.1093/mnras/stz824

We study potential systematic effects of assembly bias on cosmological parameter constraints from redshift space distortion measurements. We use a semi-analytic galaxy formation model applied to the Millennium N-body WMAP-7 simulation to study the ef... Read More about The Effect of Assembly Bias on Redshift Space Distortions.

The PAU Survey: early demonstration of photometric redshift performance in the COSMOS field (2019)
Journal Article
Eriksen, M., Alarcon, A., Gaztanaga, E., Amara, A., Cabayol, L., Carretero, J., …Tortorelli, L. (2019). The PAU Survey: early demonstration of photometric redshift performance in the COSMOS field. Monthly Notices of the Royal Astronomical Society, 484(3), 4200-4215. https://doi.org/10.1093/mnras/stz204

The Physics of the Accelerating Universe Survey (PAUS) is an innovative photometric survey with 40 narrow-bands at the William Herschel Telescope (WHT). The narrow-bands are spaced at 100 Å intervals covering the range 4500–8500 Å and, in combination... Read More about The PAU Survey: early demonstration of photometric redshift performance in the COSMOS field.

Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey (2019)
Journal Article
Smith, A., He, J., Cole, S., Stothert, L., Norberg, P., Baugh, C., …Wechsler, R. H. (2019). Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey. Monthly Notices of the Royal Astronomical Society, 484(1), 1285-1300. https://doi.org/10.1093/mnras/stz059

The Dark Energy Spectroscopic Instrument (DESI) Bright Galaxy Survey (BGS) will be a survey of bright, low-redshift galaxies, which is planned to cover an area of ∼14000 square degrees in three passes. Each pass will cover the survey area with ∼2000... Read More about Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey.

Galaxy and Mass Assembly (GAMA): The environmental dependence of the galaxy main sequence (2018)
Journal Article
Wang, L., Norberg, P., Brough, S., Brown, M., da Cunha, E., Davies, L., …Wright, A. (2018). Galaxy and Mass Assembly (GAMA): The environmental dependence of the galaxy main sequence. Astronomy & Astrophysics, 618, Article A1. https://doi.org/10.1051/0004-6361/201832697

Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) plays any role in shaping the galaxy star formation main sequence (MS). Methods: The Galaxy and Mass Assembly project (GAMA) combines a spectroscopic sur... Read More about Galaxy and Mass Assembly (GAMA): The environmental dependence of the galaxy main sequence.

The PAU Survey: spectral features and galaxy clustering using simulated narrow-band photometry (2018)
Journal Article
Stothert, L., Norberg, P., Baugh, C., Alarcon, A., Amara, A., Carretero, J., …Tortorelli, L. (2018). The PAU Survey: spectral features and galaxy clustering using simulated narrow-band photometry. Monthly Notices of the Royal Astronomical Society, 481(3), 4221-4235. https://doi.org/10.1093/mnras/sty2491

We present a mock catalogue for the Physics of the Accelerating Universe Survey (PAUS) and use it to quantify the competitiveness of narrow-band imaging for measuring spectral features and galaxy clustering. The mock agrees with observed number count... Read More about The PAU Survey: spectral features and galaxy clustering using simulated narrow-band photometry.

The impact of assembly bias on the halo occupation in hydrodynamical simulations (2018)
Journal Article
Artale, M., Zehavi, I., Contreras, S., & Norberg, P. (2018). The impact of assembly bias on the halo occupation in hydrodynamical simulations. Monthly Notices of the Royal Astronomical Society, 480(3), 3978-3992. https://doi.org/10.1093/mnras/sty2110

We investigate the variations in galaxy occupancy of the dark matter haloes with the large-scale environment and halo formation time, using two state-of-the-art hydrodynamical cosmological simulations, EAGLE and Illustris. For both simulations, we us... Read More about The impact of assembly bias on the halo occupation in hydrodynamical simulations.

Multiwavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations (2018)
Journal Article
Jakobs, A., Viola, M., McCarthy, I., van Waerbeke, L., Hoekstra, H., Robotham, A., …Wang, L. (2018). Multiwavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations. Monthly Notices of the Royal Astronomical Society, 480(3), 3338-3355. https://doi.org/10.1093/mnras/sty2017

We study the scaling relations between the baryonic content and total mass of groups of galaxies, as these systems provide a unique way to examine the role of non-gravitational processes in structure formation. Using Planck and ROSAT data, we conduct... Read More about Multiwavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations.

Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering (2018)
Journal Article
Gunawardhana, M., Norberg, P., Zehavi, I., Farrow, D., Loveday, J., Hopkins, A., …Wright, A. (2018). Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering. Monthly Notices of the Royal Astronomical Society, 479(2), 1433-1464. https://doi.org/10.1093/mnras/sty1638

Statistical studies of galaxy–galaxy interactions often utilize net change in physical properties of progenitors as a function of the separation between their nuclei to trace both the strength and the observable time-scale of their interaction. In th... Read More about Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering.

Galaxy Tagging: photometric redshift refinement and group richness enhancement (2018)
Journal Article
Kafle, P., Robotham, A., Driver, S., Deeley, S., Norberg, P., Drinkwater, M., & Davies, L. (2018). Galaxy Tagging: photometric redshift refinement and group richness enhancement. Monthly Notices of the Royal Astronomical Society, 479(3), 3746-3758. https://doi.org/10.1093/mnras/sty1536

We present a new scheme, galtag, for refining the photometric redshift measurements of faint galaxies by probabilistically tagging them to observed galaxy groups constructed from a brighter, magnitude-limited spectroscopy survey. First, this method i... Read More about Galaxy Tagging: photometric redshift refinement and group richness enhancement.

The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos (2018)
Journal Article
Zehavi, I., Contreras, S., Padilla, N., Smith, N. J., Baugh, C. M., & Norberg, P. (2018). The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos. Astrophysical Journal, 853(1), Article 84. https://doi.org/10.3847/1538-4357/aaa54a

We study the dependence of the galaxy content of dark matter halos on large-scale environment and halo formation time using semi-analytic galaxy models applied to the Millennium simulation. We analyze subsamples of halos at the extremes of these dist... Read More about The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos.

Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3 (2017)
Journal Article
Baldry, I., Liske, J., Brown, M., Robotham, A., Driver, S., Dunne, L., …Wilkins, S. (2018). Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3. Monthly Notices of the Royal Astronomical Society, 474(3), 3875-3888. https://doi.org/10.1093/mnras/stx3042

We describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The GAMA survey is a spectroscopic redshift and multiwavelength photometric survey in three equatorial regions each of 60.0 deg2 (G09, G12, and G15), and two southern reg... Read More about Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3.

Galaxy and Mass Assembly (GAMA): small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies (2017)
Journal Article
Loveday, J., Christodoulou, L., Norberg, P., Peacock, J., Baldry, I., Bland-Hawthorn, J., …Taylor, E. (2018). Galaxy and Mass Assembly (GAMA): small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies. Monthly Notices of the Royal Astronomical Society, 474(3), 3435-3450. https://doi.org/10.1093/mnras/stx2971

The galaxy pairwise velocity dispersion (PVD) can provide important tests of non-standard gravity and galaxy formation models. We describe measurements of the PVD of galaxies in the Galaxy and Mass Assembly (GAMA) survey as a function of projected se... Read More about Galaxy and Mass Assembly (GAMA): small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies.

The abundance of ultra-diffuse galaxies from groups to clusters (2017)
Journal Article
van der Burg, R. F., Hoekstra, H., Muzzin, A., Sifón, C., Viola, M., Bremer, M. N., …Valentijn, E. (2017). The abundance of ultra-diffuse galaxies from groups to clusters. Astronomy & Astrophysics, 607, Article A79. https://doi.org/10.1051/0004-6361/201731335

In recent years, many studies have reported substantial populations of large galaxies with low surface brightness in local galaxy clusters. Various theories that aim to explain the presence of such ultra-diffuse galaxies (UDGs) have since been propos... Read More about The abundance of ultra-diffuse galaxies from groups to clusters.

The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5 (2017)
Journal Article
Gonzalez-Perez, V., Comparat, J., Norberg, P., Baugh, C., Contreras, S., Lacey, C., …Humphries, J. (2018). The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5. Monthly Notices of the Royal Astronomical Society, 474(3), 4024-4038. https://doi.org/10.1093/mnras/stx2807

Emission line galaxies (ELGs) are used in several ongoing and upcoming surveys (SDSSIV/eBOSS, DESI) as tracers of the dark matter distribution. Using a new galaxy formation model, we explore the characteristics of [O II] emitters, which dominate opti... Read More about The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5.

Galaxy-galaxy lensing in EAGLE: comparison with data from 180 deg² of the KiDS and GAMA surveys (2017)
Journal Article
Velliscig, M., Cacciato, M., Hoekstra, H., Schaye, J., Heymans, C., Hildebrandt, H., …Kuijken, K. (2017). Galaxy-galaxy lensing in EAGLE: comparison with data from 180 deg² of the KiDS and GAMA surveys. Monthly Notices of the Royal Astronomical Society, 471(3), 2856-2870. https://doi.org/10.1093/mnras/stx1789

We present predictions for the galaxy–galaxy lensing (GGL) profile from the EAGLE hydrodynamical cosmological simulation at redshift z = 0.18, in the spatial range 0.02 < R/(h− 1 Mpc) < 2, and for five logarithmically equispaced stellar mass bins in... Read More about Galaxy-galaxy lensing in EAGLE: comparison with data from 180 deg² of the KiDS and GAMA surveys.

Galaxy and Mass Assembly (GAMA): halo formation times and halo assembly bias on the cosmic web (2017)
Journal Article
Tojeiro, R., Eardley, E., Peacock, J. A., Norberg, P., Alpaslan, M., Driver, S. P., …Wild, V. (2017). Galaxy and Mass Assembly (GAMA): halo formation times and halo assembly bias on the cosmic web. Monthly Notices of the Royal Astronomical Society, 470(3), 3720-3741. https://doi.org/10.1093/mnras/stx1466

We present evidence for halo assembly bias as a function of geometric environment (GE). By classifying Galaxy and Mass Assembly (GAMA) galaxy groups as residing in voids, sheets, filaments or knots using a tidal tensor method, we find that low-mass h... Read More about Galaxy and Mass Assembly (GAMA): halo formation times and halo assembly bias on the cosmic web.

A lightcone catalogue from the Millennium-XXL simulation (2017)
Journal Article
Smith, A., Cole, S., Baugh, C., Zheng, Z., Angulo, R., Norberg, P., & Zehavi, I. (2017). A lightcone catalogue from the Millennium-XXL simulation. Monthly Notices of the Royal Astronomical Society, 470(4), 4646-4661. https://doi.org/10.1093/mnras/stx1432

Future galaxy surveys require realistic mock catalogues to understand and quantify systematics in order to make precise cosmological measurements. We present a halo lightcone catalogue and halo occupation distribution (HOD) galaxy catalogue built usi... Read More about A lightcone catalogue from the Millennium-XXL simulation.

Small-scale galaxy clustering in the eagle simulation (2017)
Journal Article
Artale, M. C., Pedrosa, S. E., Trayford, J. W., Theuns, T., Farrow, D. J., Norberg, P., …Schaller, M. (2017). Small-scale galaxy clustering in the eagle simulation. Monthly Notices of the Royal Astronomical Society, 470(2), 1771-1787. https://doi.org/10.1093/mnras/stx1263

We study present-day galaxy clustering in the EAGLE cosmological hydrodynamical simulation. EAGLE’s galaxy formation parameters were calibrated to reproduce the redshift z = 0.1 galaxy stellar mass function, and the simulation also reproduces galaxy... Read More about Small-scale galaxy clustering in the eagle simulation.

Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function to z = 0.1 from the r-band selected equatorial regions (2017)
Journal Article
Wright, A., Robotham, A., Driver, S., Alpaslan, M., Andrews, S., Baldry, I., …Wilkins, S. (2017). Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function to z = 0.1 from the r-band selected equatorial regions. Monthly Notices of the Royal Astronomical Society, 470(1), 283-302. https://doi.org/10.1093/mnras/stx1149

We derive the low-redshift galaxy stellar mass function (GSMF), inclusive of dust corrections, for the equatorial Galaxy And Mass Assembly (GAMA) data set covering 180 deg2. We construct the mass function using a density-corrected maximum volume meth... Read More about Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function to z = 0.1 from the r-band selected equatorial regions.

Galaxy And Mass Assembly (GAMA): the environments of high- and low-excitation radio galaxies (2017)
Journal Article
Ching, J., Croom, S., Sadler, E., Robotham, A., Brough, S., Baldry, I., …Wang, L. (2017). Galaxy And Mass Assembly (GAMA): the environments of high- and low-excitation radio galaxies. Monthly Notices of the Royal Astronomical Society, 469(4), 4584-4599. https://doi.org/10.1093/mnras/stx1173

We study the environments of low- and high-excitation radio galaxies (LERGs and HERGs, respectively) in the redshift range 0.01 < z < 0.4, using a sample of 399 radio galaxies and environmental measurements from the Galaxy And Mass Assembly (GAMA) su... Read More about Galaxy And Mass Assembly (GAMA): the environments of high- and low-excitation radio galaxies.

Galaxy And Mass Assembly: search for a population of high-entropy galaxy groups (2017)
Journal Article
Pearson, R., Ponman, T., Norberg, P., Robotham, A., Babul, A., Bower, R., …Pimbblet, K. (2017). Galaxy And Mass Assembly: search for a population of high-entropy galaxy groups. Monthly Notices of the Royal Astronomical Society, 469(3), 3489-3504. https://doi.org/10.1093/mnras/stx1081

Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a sample of 10 galaxy groups selected from the Galaxy And Mass Assembly survey's optical Friends-of-Friends group catalogue. Our groups have been screene... Read More about Galaxy And Mass Assembly: search for a population of high-entropy galaxy groups.

Evidence against a supervoid causing the CMB Cold Spot (2017)
Journal Article
Mackenzie, R., Shanks, T., Bremer, M. N., Cai, Y., Gunawardhana, M. L., Kovács, A., …Szapudi, I. (2017). Evidence against a supervoid causing the CMB Cold Spot. Monthly Notices of the Royal Astronomical Society, 470(2), 2328-2338. https://doi.org/10.1093/mnras/stx931

We report the results of the 2dF-VST ATLAS Cold Spot galaxy redshift survey (2CSz) based on imaging from VST ATLAS and spectroscopy from 2dF AAOmega over the core of the CMB Cold Spot. We sparsely surveyed the inner 5° radius of the Cold Spot to a li... Read More about Evidence against a supervoid causing the CMB Cold Spot.

A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups (2017)
Journal Article
Dvornik, A., Cacciato, M., Kuijken, K., Viola, M., Hoekstra, H., Nakajima, R., …Wang, L. (2017). A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups. Monthly Notices of the Royal Astronomical Society, 468(3), 3251-3265. https://doi.org/10.1093/mnras/stx705

We investigate possible signatures of halo assembly bias for spectroscopically selected galaxy groups from the Galaxy And Mass Assembly (GAMA) survey using weak lensing measurements from the spatially overlapping regions of the deeper, high-imaging-q... Read More about A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups.

Galaxy and Mass Assembly (GAMA): probing the merger histories of massive galaxies via stellar populations (2017)
Journal Article
Ferreras, I., Hopkins, A., Gunawardhana, M., Sansom, A., Owers, M., Driver, S., …Bremer, M. (2017). Galaxy and Mass Assembly (GAMA): probing the merger histories of massive galaxies via stellar populations. Monthly Notices of the Royal Astronomical Society, 468(1), 607-619. https://doi.org/10.1093/mnras/stx503

The merging history of galaxies can be traced with studies of dynamically close pairs. These consist of a massive primary galaxy and a less massive secondary (or satellite) galaxy. The study of the stellar populations of secondary (lower mass) galaxi... Read More about Galaxy and Mass Assembly (GAMA): probing the merger histories of massive galaxies via stellar populations.

Galaxy and Mass Assembly (GAMA): Exploring the WISE Web in G12 (2017)
Journal Article
Jarrett, T., Cluver, M., Magoulas, C., Bilicki, M., Alpaslan, M., Bland-Hawthorn, J., …Wang, L. (2017). Galaxy and Mass Assembly (GAMA): Exploring the WISE Web in G12. Astrophysical Journal, 836(2), Article 182. https://doi.org/10.3847/1538-4357/836/2/182

We present an analysis of the mid-infrared Wide-field Infrared Survey Explorer (WISE) sources seen within the equatorial GAMA G12 field, located in the North Galactic Cap. Our motivation is to study and characterize the behavior of WISE source popula... Read More about Galaxy and Mass Assembly (GAMA): Exploring the WISE Web in G12.

Galaxy And Mass Assembly (GAMA): Gas Fueling of Spiral Galaxies in the Local Universe. I. The Effect of the Group Environment on Star Formation in Spiral Galaxies (2017)
Journal Article
Grootes, M., Tuffs, R., Popescu, C., Norberg, P., Robotham, A., Liske, J., …Rushton, M. (2017). Galaxy And Mass Assembly (GAMA): Gas Fueling of Spiral Galaxies in the Local Universe. I. The Effect of the Group Environment on Star Formation in Spiral Galaxies. Astronomical Journal, 153(3), Article 111. https://doi.org/10.3847/1538-3881/153/3/111

We quantify the effect of the galaxy group environment (for group masses of 1012.5–1014.0 M ⊙) on the current star formation rate (SFR) of a pure, morphologically selected sample of disk-dominated (i.e., late-type spiral) galaxies with redshift ≤0.13... Read More about Galaxy And Mass Assembly (GAMA): Gas Fueling of Spiral Galaxies in the Local Universe. I. The Effect of the Group Environment on Star Formation in Spiral Galaxies.

Real- and redshift-space halo clustering in f(R) cosmologies (2017)
Journal Article
Arnalte-Mur, P., Hellwing, W., & Norberg, P. (2017). Real- and redshift-space halo clustering in f(R) cosmologies. Monthly Notices of the Royal Astronomical Society, 467(2), 1569-1585. https://doi.org/10.1093/mnras/stx196

We present two-point correlation function statistics of the mass and the haloes in the chameleon f(R) modified gravity scenario using a series of large-volume N-body simulations. Three distinct variations of f(R) are considered (F4, F5 and F6) and co... Read More about Real- and redshift-space halo clustering in f(R) cosmologies.

The evolution of the galaxy content of dark matter haloes (2016)
Journal Article
Contreras, S., Zehavi, I., Baugh, C., Padilla, N., & Norberg, P. (2017). The evolution of the galaxy content of dark matter haloes. Monthly Notices of the Royal Astronomical Society, 465(3), 2833-2848. https://doi.org/10.1093/mnras/stw2826

We use the halo occupation distribution (HOD) framework to characterize the predictions from two independent galaxy formation models for the galactic content of dark matter haloes and its evolution with redshift. Our galaxy samples correspond to a ra... Read More about The evolution of the galaxy content of dark matter haloes.

The SAMI Galaxy Survey: Spatially resolving the environmental quenching of star formation in GAMA galaxies (2016)
Journal Article
Schaefer, A., Croom, S., Allen, J., Brough, S., Medling, A., I.-t., H., …Wong, O. (2017). The SAMI Galaxy Survey: Spatially resolving the environmental quenching of star formation in GAMA galaxies. Monthly Notices of the Royal Astronomical Society, 464(1), 121-142. https://doi.org/10.1093/mnras/stw2289

We use data from the Sydney-AAO Multi-Object Integral Field Spectrograph (SAMI) Galaxy Survey and the Galaxy And Mass Assembly (GAMA) survey to investigate the spatially-resolved signatures of the environmental quenching of star formation in galaxies... Read More about The SAMI Galaxy Survey: Spatially resolving the environmental quenching of star formation in GAMA galaxies.

Galaxy And Mass Assembly (GAMA): detection of low-surface-brightness galaxies from SDSS data (2016)
Journal Article
Williams, R., Baldry, I., Kelvin, L., James, P., Driver, S., Prescott, M., …Wright, A. (2016). Galaxy And Mass Assembly (GAMA): detection of low-surface-brightness galaxies from SDSS data. Monthly Notices of the Royal Astronomical Society, 463(3), 2746-2755. https://doi.org/10.1093/mnras/stw2185

We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey (SDSS) data within the Galaxy And Mass Assembly (GAMA) equatorial fields. The search method consisted of masking objects detected with SDSS PHOTO, co... Read More about Galaxy And Mass Assembly (GAMA): detection of low-surface-brightness galaxies from SDSS data.

The faint end of the 250 μm luminosity function at z < 0.5 (2016)
Journal Article
Wang, L., Norberg, P., Bethermin, M., Bourne, N., Cooray, A., Cowley, W., …Viero, M. (2016). The faint end of the 250 μm luminosity function at z < 0.5. Astronomy & Astrophysics, 592, Article L5. https://doi.org/10.1051/0004-6361/201629076

Aims. We aim to study the 250 μm luminosity function (LF) down to much fainter luminosities than achieved by previous efforts. Methods. We developed a modified stacking method to reconstruct the 250 μm LF using optically selected galaxies from the SD... Read More about The faint end of the 250 μm luminosity function at z < 0.5.

Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 deg2 of KiDS weak lensing data (2016)
Journal Article
Brouwer, M., Cacciato, M., Dvornik, A., Eardley, L., Heymans, C., Hoekstra, H., …Valentijn, E. (2016). Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 deg2 of KiDS weak lensing data. Monthly Notices of the Royal Astronomical Society, 462(4), 4451-4463. https://doi.org/10.1093/mnras/stw1602

Galaxies and their dark matter haloes are part of a complex network of mass structures, collectively called the cosmic web. Using the tidal tensor prescription these structures can be classified into four cosmic environments: voids, sheets, filaments... Read More about Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 deg2 of KiDS weak lensing data.

Measuring galaxy environment with the synergy of future photometric and spectroscopic surveys (2016)
Journal Article
Cucciati, O., Marulli, F., Cimatti, A., Merson, A., Norberg, P., Pozzetti, L., …Branchini, E. (2016). Measuring galaxy environment with the synergy of future photometric and spectroscopic surveys. Monthly Notices of the Royal Astronomical Society, 462(2), 1786-1801. https://doi.org/10.1093/mnras/stw1729

We exploit the synergy between low-resolution spectroscopy and photometric redshifts to study environmental effects on galaxy evolution in slitless spectroscopic surveys from space. As a test case, we consider the future Euclid Deep survey (∼40 deg2)... Read More about Measuring galaxy environment with the synergy of future photometric and spectroscopic surveys.

GAMA/H-ATLAS: common star formation rate indicators and their dependence on galaxy physical parameters (2016)
Journal Article
Wang, L., Norberg, P., Gunawardhana, M., Heinis, S., Baldry, I., Bland-Hawthorn, J., …van der Werf, P. (2016). GAMA/H-ATLAS: common star formation rate indicators and their dependence on galaxy physical parameters. Monthly Notices of the Royal Astronomical Society, 461(2), 1898-1916. https://doi.org/10.1093/mnras/stw1450

We compare common star formation rate (SFR) indicators in the local Universe in the Galaxy and Mass Assembly (GAMA) equatorial fields (∼160 deg2), using ultraviolet (UV) photometry from GALEX, far-infrared and sub-millimetre (sub-mm) photometry from... Read More about GAMA/H-ATLAS: common star formation rate indicators and their dependence on galaxy physical parameters.

The evolution of the [O II], H β and [O III] emission line luminosity functions over the last nine billions years (2016)
Journal Article
Comparat, J., Zhu, G., Gonzalez-Perez, V., Norberg, P., Newman, J., Tresse, L., …Jullo, E. (2016). The evolution of the [O II], H β and [O III] emission line luminosity functions over the last nine billions years. Monthly Notices of the Royal Astronomical Society, 461(1), 1076-1087. https://doi.org/10.1093/mnras/stw1393

Emission line galaxies are one of the main tracers of the large-scale structure to be targeted by the next-generation dark energy surveys. To provide a better understanding of the properties and statistics of these galaxies, we have collected spectro... Read More about The evolution of the [O II], H β and [O III] emission line luminosity functions over the last nine billions years.

The Wide Area VISTA Extra-Galactic Survey (WAVES) (2016)
Book Chapter
Driver, S., Davies, L., Meyer, M., Power, C., Robotham, A., Baldry, I., …Norberg, P. (2016). The Wide Area VISTA Extra-Galactic Survey (WAVES). In N. R. Napolitano, G. Longo, M. Marconi, M. Paolillo, E. Iodice, & M. Capaccioli (Eds.), The Universe of Digital Sky Surveys (205-214). Springer Verlag. https://doi.org/10.1007/978-3-319-19330-4_32

The “Wide Area VISTA Extra-galactic Survey” (WAVES) is a 4MOST Consortium Design Reference Survey which will use the VISTA/4MOST facility to spectroscopically survey ∼2 million galaxies to rAB 

Modelling the number density of Hα emitters for future spectroscopic near-IR space missions (2016)
Journal Article
Pozzetti, L., Hirata, C., Geach, J., Cimatti, A., Baugh, C., Cucciati, O., …Shi, D. (2016). Modelling the number density of Hα emitters for future spectroscopic near-IR space missions. Astronomy & Astrophysics, 590, https://doi.org/10.1051/0004-6361/201527081

Context. The future space missions Euclid and WFIRST-AFTA will use the Hα emission line to measure the redshifts of tens of millions of galaxies. The Hα luminosity function at z> 0.7 is one of the major sources of uncertainty in forecasting cosmologi... Read More about Modelling the number density of Hα emitters for future spectroscopic near-IR space missions.

Galaxy And Mass Assembly (GAMA): Accurate Panchromatic Photometry from Optical Priors using LAMBDAR (2016)
Journal Article
Wright, A., Robotham, A., Bourne, N., Driver, S., Dunne, L., Maddox, S., …Wilkins, S. (2016). Galaxy And Mass Assembly (GAMA): Accurate Panchromatic Photometry from Optical Priors using LAMBDAR. Monthly Notices of the Royal Astronomical Society, 460(1), 765-801. https://doi.org/10.1093/mnras/stw832

We present the Lambda Adaptive Multi-Band Deblending Algorithm in R (LAMBDAR), a novel code for calculating matched aperture photometry across images that are neither pixel- nor PSF-matched, using prior aperture definitions derived from high-resoluti... Read More about Galaxy And Mass Assembly (GAMA): Accurate Panchromatic Photometry from Optical Priors using LAMBDAR.

ZENS. IV. Similar Morphological Changes Associated with Mass Quenching and Environment Quenching and the Relative Importance of Bulge Growth versus the Fading of Disks* (2016)
Journal Article
Carollo, C., Cibinel, A., Lilly, S., Pipino, A., Bonoli, S., Finoguenov, A., …Silverman, J. (2016). ZENS. IV. Similar Morphological Changes Associated with Mass Quenching and Environment Quenching and the Relative Importance of Bulge Growth versus the Fading of Disks*. Astrophysical Journal, 818(2), Article 180. https://doi.org/10.3847/0004-637x/818/2/180

We use the low-redshift Zurich Environmental Study (ZENS) catalog to study the dependence of the quenched satellite fraction at ${10}^{10.0}\;{M}_{\odot }\to {10}^{11.5}\;{M}_{\odot }$, and of the morphological mix of these quenched satellites, on th... Read More about ZENS. IV. Similar Morphological Changes Associated with Mass Quenching and Environment Quenching and the Relative Importance of Bulge Growth versus the Fading of Disks*.

Galaxy And Mass Assembly (GAMA): the stellar mass budget by galaxy type (2016)
Journal Article
Moffett, A., Ingarfield, S., Driver, S., Robotham, A., Kelvin, L., Lange, R., …Taylor, E. (2016). Galaxy And Mass Assembly (GAMA): the stellar mass budget by galaxy type. Monthly Notices of the Royal Astronomical Society, 457(2), 1308-1319. https://doi.org/10.1093/mnras/stv2883

We report an expanded sample of visual morphological classifications from the Galaxy and Mass Assembly survey phase two, which now includes 7556 objects (previously 3727 in phase one). We define a local (z < 0.06) sample and classify galaxies into E,... Read More about Galaxy And Mass Assembly (GAMA): the stellar mass budget by galaxy type.

Galaxy and mass assembly: Redshift space distortions from the clipped galaxy field (2016)
Journal Article
Simpson, F., Blake, C., Peacock, J., Baldry, I., Bland-Hawthorn, J., Heavens, A., …Norberg, P. (2016). Galaxy and mass assembly: Redshift space distortions from the clipped galaxy field. Physical Review D, 93(2), Article 023525. https://doi.org/10.1103/physrevd.93.023525

We present the first cosmological measurement derived from a galaxy density field subject to a “clipping” transformation. By enforcing an upper bound on the galaxy number density field in the galaxy and mass assembly survey (GAMA), contributions from... Read More about Galaxy and mass assembly: Redshift space distortions from the clipped galaxy field.

Recovering dark-matter clustering from galaxies with Gaussianization (2016)
Journal Article
McCullagh, N., Neyrinck, M., Norberg, P., & Cole, S. (2016). Recovering dark-matter clustering from galaxies with Gaussianization. Monthly Notices of the Royal Astronomical Society, 457(4), 3652-3665. https://doi.org/10.1093/mnras/stw223

The Gaussianization transform has been proposed as a method to remove the issues of scale-dependent galaxy bias and non-linearity from galaxy clustering statistics, but these benefits have yet to be thoroughly tested for realistic galaxy samples. In... Read More about Recovering dark-matter clustering from galaxies with Gaussianization.

Galaxy And Mass Assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies (2016)
Journal Article
Prescott, M., Mauch, T., Jarvis, M., McAlpine, K., Smith, D., Fine, S., …Sadler, E. (2016). Galaxy And Mass Assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 457(1), 730-744. https://doi.org/10.1093/mnras/stv3020

Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies underpins our understanding of galaxy evolution over cosmic time. Radio continuum observations can provide key information on these two processes, in par... Read More about Galaxy And Mass Assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies.

The masses of satellites in GAMA galaxy groups from 100 square degrees of KiDS weak lensing data (2015)
Journal Article
Sifón, C., Cacciato, M., Hoekstra, H., Brouwer, M., van Uitert, E., Viola, M., …Kleijn, G. (2015). The masses of satellites in GAMA galaxy groups from 100 square degrees of KiDS weak lensing data. Monthly Notices of the Royal Astronomical Society, 454(4), 3938-3951. https://doi.org/10.1093/mnras/stv2051

We use the first 100 deg2 of overlap between the Kilo-Degree Survey and the Galaxy And Mass Assembly survey to determine the average galaxy halo mass of ∼10 000 spectroscopically confirmed satellite galaxies in massive (M > 1013 h−1 M⊙) galaxy groups... Read More about The masses of satellites in GAMA galaxy groups from 100 square degrees of KiDS weak lensing data.

Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget (2015)
Journal Article
Driver, S. P., Wright, A. H., Andrews, S. K., Davies, L. J., Kafle, P. R., Lange, R., …Williams, R. (2016). Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget. Monthly Notices of the Royal Astronomical Society, 455(4), 3911-3942. https://doi.org/10.1093/mnras/stv2505

We present the Galaxy And Mass Assembly (GAMA) Panchromatic Data Release (PDR) constituting over 230 deg2 of imaging with photometry in 21 bands extending from the far-UV to the far-IR. These data complement our spectroscopic campaign of over 300k ga... Read More about Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget.

Galaxy and mass assembly (GAMA): projected galaxy clustering (2015)
Journal Article
Farrow, D., Cole, S., Norberg, P., Metcalfe, N., Baldry, I., Bland-Hawthorn, J., …Sridhar, S. (2015). Galaxy and mass assembly (GAMA): projected galaxy clustering. Monthly Notices of the Royal Astronomical Society, 454(2), 2120-2145. https://doi.org/10.1093/mnras/stv2075

We measure the projected two-point correlation function of galaxies in the 180 deg2 equatorial regions of the GAMA II survey, for four different redshift slices between z = 0.0 and 0.5. To do this, we further develop the Cole method of producing suit... Read More about Galaxy and mass assembly (GAMA): projected galaxy clustering.

Galaxy And Mass Assembly (GAMA): the bright void galaxy population in the optical and mid-IR (2015)
Journal Article
Penny, S., Brown, M., Pimbblet, K., Cluver, M., Croton, D., Owers, M., …Rodrigues, M. (2015). Galaxy And Mass Assembly (GAMA): the bright void galaxy population in the optical and mid-IR. Monthly Notices of the Royal Astronomical Society, 453(4), 3519-3539. https://doi.org/10.1093/mnras/stv1926

We examine the properties of galaxies in the Galaxies and Mass Assembly (GAMA) survey located in voids with radii >10 h−1 Mpc. Utilizing the GAMA equatorial survey, 592 void galaxies are identified out to z ≈ 0.1 brighter than Mr = −18.4, our magnitu... Read More about Galaxy And Mass Assembly (GAMA): the bright void galaxy population in the optical and mid-IR.

Galaxy And Mass Assembly (GAMA): end of survey report and data release 2 (2015)
Journal Article
Liske, J., Baldry, I., Driver, S., Tuffs, R., Alpaslan, M., Andrae, E., …Wright, A. (2015). Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. Monthly Notices of the Royal Astronomical Society, 452(2), 2087-2126. https://doi.org/10.1093/mnras/stv1436

The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary spectroscopic surveys of low redshift galaxies. Covering an area of ∼286 deg2 (split among five survey regions) down to a limiting magnitude of r < 19.8 mag, we have collec... Read More about Galaxy And Mass Assembly (GAMA): end of survey report and data release 2.

Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies (2015)
Journal Article
Davies, L., Robotham, A., Driver, S., Alpaslan, M., Baldry, I., Bland-Hawthorn, J., …Smith, M. (2015). Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies. Monthly Notices of the Royal Astronomical Society, 452(1), 616-636. https://doi.org/10.1093/mnras/stv1241

The modification of star formation (SF) in galaxy interactions is a complex process, with SF observed to be both enhanced in major mergers and suppressed in minor pair interactions. Such changes likely to arise on short time-scales and be directly re... Read More about Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies.

Galaxy And Mass Assembly (GAMA): trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments (2015)
Journal Article
Alpaslan, M., Driver, S., Robotham, A., Obreschkow, D., Andrae, E., Cluver, M., …Tuffs, R. (2015). Galaxy And Mass Assembly (GAMA): trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments. Monthly Notices of the Royal Astronomical Society, 451(3), 3249-3268. https://doi.org/10.1093/mnras/stv1176

We explore trends in galaxy properties with Mpc-scale structures using catalogues of environment and large-scale structure from the Galaxy And Mass Assembly (GAMA) survey. Existing GAMA catalogues of large-scale structure, group, and pair membership... Read More about Galaxy And Mass Assembly (GAMA): trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments.

Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data (2015)
Journal Article
Viola, M., Cacciato, M., Brouwer, M., Kuijken, K., Hoekstra, H., Norberg, P., …Verdoes Kleijn, G. (2015). Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data. Monthly Notices of the Royal Astronomical Society, 452(4), 3529-3550. https://doi.org/10.1093/mnras/stv1447

The Kilo-Degree Survey is an optical wide-field survey designed to map the matter distribution in the Universe using weak gravitational lensing. In this paper, we use these data to measure the density profiles and masses of a sample of ∼1400 spectros... Read More about Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data.

The galaxy-dark matter halo connection: which galaxy properties are correlated with the host halo mass? (2015)
Journal Article
Contreras, S., Baugh, C., Norberg, P., & Padilla, N. (2015). The galaxy-dark matter halo connection: which galaxy properties are correlated with the host halo mass?. Monthly Notices of the Royal Astronomical Society, 452(2), 1861-1876. https://doi.org/10.1093/mnras/stv1438

We demonstrate how the properties of a galaxy depend on the mass of its host dark matter subhalo, using two independent models of galaxy formation. For the cases of stellar mass and black hole mass, the median property value displays a monotonic depe... Read More about The galaxy-dark matter halo connection: which galaxy properties are correlated with the host halo mass?.

Galaxy and Mass Assembly (GAMA): maximum-likelihood determination of the luminosity function and its evolution (2015)
Journal Article
Loveday, J., Norberg, P., Baldry, I., Bland-Hawthorn, J., Brough, S., Brown, M., …Phillipps, S. (2015). Galaxy and Mass Assembly (GAMA): maximum-likelihood determination of the luminosity function and its evolution. Monthly Notices of the Royal Astronomical Society, 451(2), 1540-1552. https://doi.org/10.1093/mnras/stv1013

We describe modifications to the joint stepwise maximum-likelihood method of Cole in order to simultaneously fit the Galaxy and Mass Assembly II galaxy luminosity function (LF), corrected for radial density variations, and its evolution with redshift... Read More about Galaxy and Mass Assembly (GAMA): maximum-likelihood determination of the luminosity function and its evolution.

Co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background (2015)
Journal Article
Wang, L., Viero, M., Ross, N., Asboth, V., Béthermin, M., Bock, J., …Zemcov, M. (2015). Co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background. Monthly Notices of the Royal Astronomical Society, 449(4), 4476-4493. https://doi.org/10.1093/mnras/stv559

We present the first cross-correlation measurement between Sloan Digital Sky Survey type 1 quasars and the cosmic infrared background (CIB) measured by Herschel. The quasars cover the redshift range 0.15 < z < 3.5 where most of the CIB originates. We... Read More about Co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background.

On optical mass estimation methods for galaxy groups (2015)
Journal Article
Pearson, R., Ponman, T., Norberg, P., Robotham, A., & Farr, W. (2015). On optical mass estimation methods for galaxy groups. Monthly Notices of the Royal Astronomical Society, 449(3), 3082-3106. https://doi.org/10.1093/mnras/stv463

We examine the performance of a variety of different estimators for the mass of galaxy groups, based on their galaxy distribution alone. We draw galaxies from the Sloan Digital Sky Survey for a set of groups and clusters for which hydrostatic mass es... Read More about On optical mass estimation methods for galaxy groups.

Galaxy And Mass Assembly (GAMA): the galaxy luminosity function within the cosmic web (2015)
Journal Article
Eardley, E., Peacock, J., McNaught-Roberts, T., Heymans, C., Norberg, P., Alpaslan, M., …Robotham, A. (2015). Galaxy And Mass Assembly (GAMA): the galaxy luminosity function within the cosmic web. Monthly Notices of the Royal Astronomical Society, 448(4), 3665-3678. https://doi.org/10.1093/mnras/stv237

We investigate the dependence of the galaxy luminosity function on geometric environment within the Galaxy And Mass Assembly (GAMA) survey. The tidal tensor prescription, based on the Hessian of the pseudo-gravitational potential, is used to classify... Read More about Galaxy And Mass Assembly (GAMA): the galaxy luminosity function within the cosmic web.

Galaxy And Mass Assembly (GAMA): mass-size relations of z < 0.1 galaxies subdivided by Sérsic index, colour and morphology (2015)
Journal Article
Lange, R., Driver, S., Robotham, A., Kelvin, L., Graham, A., Alpaslan, M., …Wilkins, S. (2015). Galaxy And Mass Assembly (GAMA): mass-size relations of z < 0.1 galaxies subdivided by Sérsic index, colour and morphology. Monthly Notices of the Royal Astronomical Society, 447(3), 2603-2630. https://doi.org/10.1093/mnras/stu2467

We use data from the Galaxy And Mass Assembly (GAMA) survey in the redshift range 0.01 < z < 0.1 (8399 galaxies in g to Ks bands) to derive the stellar mass–half-light radius relations for various divisions of ‘early’- and ‘late’-type samples. We fin... Read More about Galaxy And Mass Assembly (GAMA): mass-size relations of z < 0.1 galaxies subdivided by Sérsic index, colour and morphology.

Galaxy And Mass Assembly (GAMA): bivariate functions of Hα star-forming galaxies (2015)
Journal Article
Gunawardhana, M., Hopkins, A., Taylor, E., Bland-Hawthorn, J., Norberg, P., Baldry, I., …Robotham, A. (2015). Galaxy And Mass Assembly (GAMA): bivariate functions of Hα star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 447(1), 875-901. https://doi.org/10.1093/mnras/stu2232

We present bivariate luminosity and stellar mass functions of Hα star-forming galaxies drawn from the Galaxy And Mass Assembly (GAMA) survey. While optically deep spectroscopic observations of GAMA over a wide sky area enable the detection of a large... Read More about Galaxy And Mass Assembly (GAMA): bivariate functions of Hα star-forming galaxies.

The SAMI Galaxy Survey: Early Data Release (2015)
Journal Article
Allen, J., Croom, S., Konstantopoulos, I., Bryant, J., Sharp, R., Cecil, G., …Walcher, C. (2015). The SAMI Galaxy Survey: Early Data Release. Monthly Notices of the Royal Astronomical Society, 446(2), 1567-1583. https://doi.org/10.1093/mnras/stu2057

We present the Early Data Release of the Sydney–AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey. The SAMI Galaxy Survey is an ongoing integral field spectroscopic survey of ∼3400 low-redshift (z < 0.12) galaxies, covering galaxies i... Read More about The SAMI Galaxy Survey: Early Data Release.

Galaxy And Mass Assembly (GAMA): deconstructing bimodality - I. Red ones and blue ones (2015)
Journal Article
Taylor, E., Hopkins, A., Baldry, I., Bland-Hawthorn, J., Brown, M., Colless, M., …Loveday, J. (2015). Galaxy And Mass Assembly (GAMA): deconstructing bimodality - I. Red ones and blue ones. Monthly Notices of the Royal Astronomical Society, 446(2), 2144-2185. https://doi.org/10.1093/mnras/stu1900

We measure the mass functions for generically red and blue galaxies, using a z < 0.12 sample of log M* > 8.7 field galaxies from the Galaxy And Mass Assembly (GAMA) survey. Our motivation is that, as we show, the dominant uncertainty in existing meas... Read More about Galaxy And Mass Assembly (GAMA): deconstructing bimodality - I. Red ones and blue ones.

Galaxy And Mass Assembly (GAMA): the halo mass of galaxy groups from maximum-likelihood weak lensing (2014)
Journal Article
Han, J., Eke, V., Frenk, C., Mandelbaum, R., Norberg, P., Schneider, M., …Robotham, A. (2015). Galaxy And Mass Assembly (GAMA): the halo mass of galaxy groups from maximum-likelihood weak lensing. Monthly Notices of the Royal Astronomical Society, 446(2), 1356-1379. https://doi.org/10.1093/mnras/stu2178

We present a maximum-likelihood weak-lensing analysis of the mass distribution in optically selected spectroscopic Galaxy Groups (G3Cv5) in the Galaxy And Mass Assembly (GAMA) survey, using background Sloan Digital Sky Survey (SDSS) photometric galax... Read More about Galaxy And Mass Assembly (GAMA): the halo mass of galaxy groups from maximum-likelihood weak lensing.

Galaxy And Mass Assembly (GAMA): the dependence of the galaxy luminosity function on environment, redshift and colour (2014)
Journal Article
McNaught-Roberts, T., Norberg, P., Baugh, C., Lacey, C., Loveday, J., Peacock, J., …Vázquez-Mata, J. (2014). Galaxy And Mass Assembly (GAMA): the dependence of the galaxy luminosity function on environment, redshift and colour. Monthly Notices of the Royal Astronomical Society, 445(2), 2125-2145. https://doi.org/10.1093/mnras/stu1886

We use 80 922 galaxies in the Galaxy And Mass Assembly (GAMA) survey to measure the galaxy luminosity function (LF) in different environments over the redshift range 0.04 < z < 0.26. The depth and size of GAMA allows us to define samples split by col... Read More about Galaxy And Mass Assembly (GAMA): the dependence of the galaxy luminosity function on environment, redshift and colour.

Galaxy And Mass Assembly (GAMA): AUTOZ spectral redshift measurements, confidence and errors (2014)
Journal Article
Baldry, I., Alpaslan, M., Bauer, A., Bland-Hawthorn, J., Brough, S., Cluver, M., …Taylor, E. (2014). Galaxy And Mass Assembly (GAMA): AUTOZ spectral redshift measurements, confidence and errors. Monthly Notices of the Royal Astronomical Society, 441(3), 2440-2451. https://doi.org/10.1093/mnras/stu727

The Galaxy And Mass Assembly (GAMA) survey has obtained spectra of over 230 000 targets using the Anglo-Australian Telescope. To homogenize the redshift measurements and improve the reliability, a fully automatic redshift code was developed (AUTOZ).... Read More about Galaxy And Mass Assembly (GAMA): AUTOZ spectral redshift measurements, confidence and errors.

The ALHAMBRA survey: evolution of galaxy clustering since z ~ 1 (2014)
Journal Article
Arnalte-Mur, P., Martínez, V., Norberg, P., Fernández-Soto, A., Ascaso, B., Merson, A., …Quintana, J. (2014). The ALHAMBRA survey: evolution of galaxy clustering since z ~ 1. Monthly Notices of the Royal Astronomical Society, 441(2), 1783-1801. https://doi.org/10.1093/mnras/stu681

We study the clustering of galaxies as function of luminosity and redshift in the range 0.35 < z < 1.25 using data from the Advanced Large Homogeneous Area Medium-Band Redshift Astronomical (ALHAMBRA) survey. The ALHAMBRA data used in this work cover... Read More about The ALHAMBRA survey: evolution of galaxy clustering since z ~ 1.

Galaxy and Mass Assembly (GAMA): fine filaments of galaxies detected within voids (2014)
Journal Article
Alpaslan, M., Robotham, A., Obreschkow, D., Penny, S., Driver, S., Norberg, P., …Pimbblet, K. (2014). Galaxy and Mass Assembly (GAMA): fine filaments of galaxies detected within voids. Monthly Notices of the Royal Astronomical Society: Letters, 440(1), L106-L110. https://doi.org/10.1093/mnrasl/slu019

Based on data from the Galaxy and Mass Assembly (GAMA) survey, we report on the discovery of structures that we refer to as ‘tendrils’ of galaxies: coherent, thin chains of galaxies that are rooted in filaments and terminate in neighbouring filaments... Read More about Galaxy and Mass Assembly (GAMA): fine filaments of galaxies detected within voids.

Galaxy and Mass Assembly: the evolution of bias in the radio source population to z∼1.5 (2014)
Journal Article
Lindsay, S., Jarvis, M., Santos, M., Brown, M., Croom, S., Driver, S., …Robotham, A. (2014). Galaxy and Mass Assembly: the evolution of bias in the radio source population to z∼1.5. Monthly Notices of the Royal Astronomical Society, 440(2), 1527-1541. https://doi.org/10.1093/mnras/stu354

We present a large-scale clustering analysis of radio galaxies in the Very Large Array Faint Images of the Radio Sky at Twenty-cm survey over the Galaxy and Mass Assembly (GAMA) survey area, limited to S1.4 GHz > 1 mJy with spectroscopic and photomet... Read More about Galaxy and Mass Assembly: the evolution of bias in the radio source population to z∼1.5.

Galaxy And Mass Assembly (GAMA): ugrizYJHK Sérsic luminosity functions and the cosmic spectral energy distribution by Hubble type (2014)
Journal Article
Kelvin, L., Driver, S., Robotham, A., Graham, A., Phillipps, S., Agius, N., …Tuffs, R. (2014). Galaxy And Mass Assembly (GAMA): ugrizYJHK Sérsic luminosity functions and the cosmic spectral energy distribution by Hubble type. Monthly Notices of the Royal Astronomical Society, 439(2), 1245-1269. https://doi.org/10.1093/mnras/stt2391

We report the morphological classification of 3727 galaxies from the Galaxy and Mass Assembly survey with Mr < −17.4 mag and in the redshift range 0.025 < z < 0.06 (2.1 × 105 Mpc3) into E, S0-Sa, SB0-SBa, Sab-Scd, SBab-SBcd, Sd-Irr and little blue sp... Read More about Galaxy And Mass Assembly (GAMA): ugrizYJHK Sérsic luminosity functions and the cosmic spectral energy distribution by Hubble type.

Galaxy and Mass Assembly (GAMA): Mid-infrared Properties and Empirical Relations from WISE (2014)
Journal Article
Cluver, M., Jarrett, T., Hopkins, A., Driver, S., Liske, J., Gunawardhana, M., …Wilkins, S. (2014). Galaxy and Mass Assembly (GAMA): Mid-infrared Properties and Empirical Relations from WISE. Astrophysical Journal, 782(2), Article 90. https://doi.org/10.1088/0004-637x/782/2/90

The Galaxy And Mass Assembly (GAMA) survey furnishes a deep redshift catalog that, when combined with the Wide-field Infrared Survey Explorer (WISE), allows us to explore for the first time the mid-infrared properties of >110, 000 galaxies over 120 d... Read More about Galaxy and Mass Assembly (GAMA): Mid-infrared Properties and Empirical Relations from WISE.

Galaxy And Mass Assembly (GAMA): the large-scale structure of galaxies and comparison to mock universes (2014)
Journal Article
Alpaslan, M., Robotham, A., Driver, S., Norberg, P., Baldry, I., Bauer, A., …Pimbblet, K. (2014). Galaxy And Mass Assembly (GAMA): the large-scale structure of galaxies and comparison to mock universes. Monthly Notices of the Royal Astronomical Society, 438(1), 177-194. https://doi.org/10.1093/mnras/stt2136

From a volume-limited sample of 45 542 galaxies and 6000 groups with z ≤ 0.213, we use an adapted minimal spanning tree algorithm to identify and classify large-scale structures within the Galaxy And Mass Assembly (GAMA) survey. Using galaxy groups,... Read More about Galaxy And Mass Assembly (GAMA): the large-scale structure of galaxies and comparison to mock universes.

The Pan-STARRS1 Medium-Deep Survey: The Role of Galaxy Group Environment in the Star Formation Rate versus Stellar Mass Relation and Quiescent Fraction out to z ~ 0.8 (2014)
Journal Article
Lin, L., Jian, H., Foucaud, S., Norberg, P., Bower, R., Cole, S., …Waters, C. (2014). The Pan-STARRS1 Medium-Deep Survey: The Role of Galaxy Group Environment in the Star Formation Rate versus Stellar Mass Relation and Quiescent Fraction out to z ~ 0.8. Astrophysical Journal, 782(1), Article 33. https://doi.org/10.1088/0004-637x/782/1/33

Using a large optically selected sample of field and group galaxies drawn from the Pan-STARRS1 Medium-Deep Survey (PS1/MDS), we present a detailed analysis of the specific star formation rate (SSFR)—stellar mass (M *) relation, as well as the quiesce... Read More about The Pan-STARRS1 Medium-Deep Survey: The Role of Galaxy Group Environment in the Star Formation Rate versus Stellar Mass Relation and Quiescent Fraction out to z ~ 0.8.

Pan-STARRS1: Galaxy clustering in the Small Area Survey 2 (2014)
Journal Article
Farrow, D. J., Cole, S., Metcalfe, N., Draper, P., Norberg, P., Foucaud, S., …Waters, C. (2014). Pan-STARRS1: Galaxy clustering in the Small Area Survey 2. Monthly Notices of the Royal Astronomical Society, 437(1), 748-770. https://doi.org/10.1093/mnras/stt1933

The Panoramic Survey Telescope and Rapid Response System 1 survey is currently obtaining imaging in five bands (gP1, rP1, iP1, zP1 and yP1) for the 3π steradian survey, one of the largest optical surveys ever conducted. The finished survey will have... Read More about Pan-STARRS1: Galaxy clustering in the Small Area Survey 2.

Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure (2013)
Journal Article
Blake, C., Baldry, I., Bland-Hawthorn, J., Christodoulou, L., Colless, M., Conselice, C., …Robotham, A. (2013). Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure. Monthly Notices of the Royal Astronomical Society, 436(4), 3089-3105. https://doi.org/10.1093/mnras/stt1791

We present the first application of a ‘multiple-tracer’ redshift-space distortion (RSD) analysis to an observational galaxy sample, using data from the Galaxy and Mass Assembly (GAMA) survey. Our data set is an r < 19.8 magnitude-limited sample of 17... Read More about Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure.

The Zurich Environmental Study of Galaxies in Groups along the Cosmic Web. III. Galaxy Photometric Measurements and the Spatially Resolved Color Properties of Early- and Late-type Satellites in Diverse Environments (2013)
Journal Article
Cibinel, A., Carollo, C., Lilly, S., Bonoli, S., Miniati, F., Pipino, A., …Rudick, C. (2013). The Zurich Environmental Study of Galaxies in Groups along the Cosmic Web. III. Galaxy Photometric Measurements and the Spatially Resolved Color Properties of Early- and Late-type Satellites in Diverse Environments. Astrophysical Journal, 777(2), Article 116. https://doi.org/10.1088/0004-637x/777/2/116

We present photometric measurements for the galaxies—and when possible their bulges and disks—in the 0.05 < z < 0.0585 groups of the Zurich Environmental Study (ZENS); these measurements include (B – I) colors, color gradients and maps, color dispers... Read More about The Zurich Environmental Study of Galaxies in Groups along the Cosmic Web. III. Galaxy Photometric Measurements and the Spatially Resolved Color Properties of Early- and Late-type Satellites in Diverse Environments.

Galaxy And Mass Assembly: resolving the role of environment in galaxy evolution (2013)
Journal Article
Brough, S., Croom, S., Sharp, R., Hopkins, A., Taylor, E., Baldry, I., …Prescott, M. (2013). Galaxy And Mass Assembly: resolving the role of environment in galaxy evolution. Monthly Notices of the Royal Astronomical Society, 435(4), 2903-2917. https://doi.org/10.1093/mnras/stt1489

We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the SPIRAL optical integral field unit (IFU) on the Anglo-Australian Telescope. The galaxies are selected to have a narrow range in stellar mass (6 × 109... Read More about Galaxy And Mass Assembly: resolving the role of environment in galaxy evolution.

The Pan-STARRS1 Small Area Survey 2 (2013)
Journal Article
Metcalfe, N., Farrow, D., Cole, S., Draper, P., Norberg, P., Burgett, W., …Waters, C. (2013). The Pan-STARRS1 Small Area Survey 2. Monthly Notices of the Royal Astronomical Society, 435(3), 1825-1839. https://doi.org/10.1093/mnras/stt1343

The Panoramic Survey Telescope and Rapid Response System 1 (Pan-STARRS1) survey is acquiring multi-epoch imaging in five bands (gP1, rP1, iP1, zP1, yP1) over the entire sky north of declination −30° (the 3π survey). In 2011 July a test area of about... Read More about The Pan-STARRS1 Small Area Survey 2.

The Zurich Environmental Study of Galaxies in Groups along the Cosmic Web. I. Which Environment Affects Galaxy Evolution? (2013)
Journal Article
Carollo, C., Cibinel, A., Lilly, S., Miniati, F., Norberg, P., Silverman, J., …Rudick, C. (2013). The Zurich Environmental Study of Galaxies in Groups along the Cosmic Web. I. Which Environment Affects Galaxy Evolution?. Astrophysical Journal, 776(2), Article 71. https://doi.org/10.1088/0004-637x/776/2/71

The Zurich Environmental Study (ZENS) is based on a sample of ~1500 galaxy members of 141 groups in the mass range ~1012.5-14.5 M ☉ within the narrow redshift range 0.05 < z < 0.0585. ZENS adopts novel approaches, described here, to quantify four dif... Read More about The Zurich Environmental Study of Galaxies in Groups along the Cosmic Web. I. Which Environment Affects Galaxy Evolution?.

The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. II. Galaxy Structural Measurements and the Concentration of Morphologically Classified Satellites in Diverse Environments (2013)
Journal Article
Cibinel, A., Carollo, C., Lilly, S., Miniati, F., Silverman, J., van Gorkom, J., …Rudick, C. (2013). The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. II. Galaxy Structural Measurements and the Concentration of Morphologically Classified Satellites in Diverse Environments. Astrophysical Journal, 776(2), Article 72. https://doi.org/10.1088/0004-637x/776/2/72

We present structural measurements for the galaxies in the 0.05 < z < 0.0585 groups of the Zurich Environmental Study, aimed at establishing how galaxy properties depend on four environmental parameters: group halo mass (M GROUP), group-centric dista... Read More about The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. II. Galaxy Structural Measurements and the Concentration of Morphologically Classified Satellites in Diverse Environments.

Galaxy And Mass Assembly (GAMA): linking star formation histories and stellar mass growth (2013)
Journal Article
Bauer, A., Hopkins, A., Gunawardhana, M., Taylor, E., Baldry, I., Bamford, S., …Sharp, R. (2013). Galaxy And Mass Assembly (GAMA): linking star formation histories and stellar mass growth. Monthly Notices of the Royal Astronomical Society, 434(1), 209-221. https://doi.org/10.1093/mnras/stt1011

We present evidence for stochastic star formation histories in low-mass (M* < 1010 M⊙) galaxies from observations within the Galaxy And Mass Assembly (GAMA) survey. For ∼73 000 galaxies between 0.05 < z < 0.32, we calculate star formation rates (SFR)... Read More about Galaxy And Mass Assembly (GAMA): linking star formation histories and stellar mass growth.

Galaxy And Mass Assembly (GAMA): galaxy radial alignments in GAMA groups (2013)
Journal Article
Schneider, M. D., Cole, S., Frenk, C. S., Kelvin, L., Mandelbaum, R., Norberg, P., …Robotham, A. (2013). Galaxy And Mass Assembly (GAMA): galaxy radial alignments in GAMA groups. Monthly Notices of the Royal Astronomical Society, 433(4), 2727-2738. https://doi.org/10.1093/mnras/stt855

We constrain the distributions of projected radial alignment angles of satellite galaxy shapes within the Galaxy And Mass Assembly survey group catalogue. We identify the galaxy groups using spectroscopic redshifts and measure galaxy projected ellipt... Read More about Galaxy And Mass Assembly (GAMA): galaxy radial alignments in GAMA groups.

Galaxy And Mass Assembly: evolution of the Hα luminosity function and star formation rate density up to z < 0.35 (2013)
Journal Article
Gunawardhana, M., Hopkins, A., Bland-Hawthorn, J., Brough, S., Sharp, R., Loveday, J., …Wang, L. (2013). Galaxy And Mass Assembly: evolution of the Hα luminosity function and star formation rate density up to z < 0.35. Monthly Notices of the Royal Astronomical Society, 433(4), 2764-2789. https://doi.org/10.1093/mnras/stt890

Measurements of the low-z Hα luminosity function, Φ, have a large dispersion in the local number density of sources (∼0.5–1 Mpc−3 dex−1), and correspondingly in the star formation rate density (SFRD). The possible causes for these discrepancies inclu... Read More about Galaxy And Mass Assembly: evolution of the Hα luminosity function and star formation rate density up to z < 0.35.

How robust are predictions of galaxy clustering? (2013)
Journal Article
Contreras, S., Baugh, C., Norberg, P., & Padilla, N. (2013). How robust are predictions of galaxy clustering?. Monthly Notices of the Royal Astronomical Society, 432(4), 2717-2730. https://doi.org/10.1093/mnras/stt629

We use the Millennium Simulation data base to compare how different versions of the Durham and Munich semi-analytical galaxy formation models populate dark matter haloes with galaxies. The models follow the same physical processes but differ in how t... Read More about How robust are predictions of galaxy clustering?.

Galaxy And Mass Assembly (GAMA): the life and times of L★ galaxies (2013)
Journal Article
Robotham, A., Liske, J., Driver, S., Sansom, A., Baldry, I., Bauer, A., …Tuffs, R. (2013). Galaxy And Mass Assembly (GAMA): the life and times of L★ galaxies. Monthly Notices of the Royal Astronomical Society, 431(1), 167-193. https://doi.org/10.1093/mnras/stt156

In this work, we investigate in detail the effects the local environment (groups and pairs) has on galaxies with stellar mass similar to the Milky Way (L* galaxies). A volume limited sample of 6150 galaxies are visually classified to determine the em... Read More about Galaxy And Mass Assembly (GAMA): the life and times of L★ galaxies.

Galaxy And Mass Assembly (GAMA) : The M-Z relation for galaxy groups. (2013)
Journal Article
Lara-López, M., Hopkins, A., Robotham, A., Owers, M., Colless, M., Brough, S., …Thomas, D. (2013). Galaxy And Mass Assembly (GAMA) : The M-Z relation for galaxy groups. Astronomical Notes, 334(4-5), 466-469. https://doi.org/10.1002/asna.201211882

Galaxy And Mass Assembly (GAMA): spectroscopic analysis (2013)
Journal Article
Hopkins, A., Driver, S., Brough, S., Owers, M., Bauer, A., Gunawardhana, M., …Wilkins, S. (2013). Galaxy And Mass Assembly (GAMA): spectroscopic analysis. Monthly Notices of the Royal Astronomical Society, 430(3), 2047-2066. https://doi.org/10.1093/mnras/stt030

The Galaxy And Mass Assembly (GAMA) survey is a multiwavelength photometric and spectroscopic survey, using the AAOmega spectrograph on the Anglo-Australian Telescope to obtain spectra for up to ∼300 000 galaxies over 280 deg2, to a limiting magnitud... Read More about Galaxy And Mass Assembly (GAMA): spectroscopic analysis.

GAMA/H-ATLAS: The Dust Opacity-Stellar Mass Surface Density Relation for Spiral Galaxies (2013)
Journal Article
Grootes, M., Tuffs, R., Popescu, C., Pastrav, B., Andrae, E., Gunawardhana, M., …Valiante, E. (2013). GAMA/H-ATLAS: The Dust Opacity-Stellar Mass Surface Density Relation for Spiral Galaxies. Astrophysical Journal, 766(1), Article 59. https://doi.org/10.1088/0004-637x/766/1/59

We report the discovery of a well-defined correlation between B-band face-on central optical depth due to dust, τ f/B, and the stellar mass surface density, μ∗, of nearby (z

Lightcone mock catalogues from semi-analytic models of galaxy formation - I. Construction and application to the BzK colour selection (2013)
Journal Article
Merson, A., Baugh, C., Helly, J., Gonzalez-Perez, V., Cole, S., Bielby, R., …Lagos, C. D. P. (2013). Lightcone mock catalogues from semi-analytic models of galaxy formation - I. Construction and application to the BzK colour selection. Monthly Notices of the Royal Astronomical Society, 429(1), 556-578. https://doi.org/10.1093/mnras/sts355

We introduce a method for constructing end-to-end mock galaxy catalogues using a semi-analytical model of galaxy formation, applied to the halo merger trees extracted from a cosmological N-body simulation. The mocks that we construct are lightcone ca... Read More about Lightcone mock catalogues from semi-analytic models of galaxy formation - I. Construction and application to the BzK colour selection.

Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm (2012)
Journal Article
Driver, S., Robotham, A., Kelvin, L., Alpaslan, M., Baldry, I., Bamford, S., …Wilkins, S. (2012). Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm. Monthly Notices of the Royal Astronomical Society, 427(4), 3244-3264. https://doi.org/10.1111/j.1365-2966.2012.22036.x

We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z < 0.1) galaxy luminosity functions in FUV, NUV, ugr... Read More about Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm.

Galaxy And Mass Assembly (GAMA): the mass-metallicity relationship (2012)
Journal Article
Foster, C., Hopkins, A., Gunawardhana, M., Lara-López, M., Sharp, R., Steele, O., …Wijesinghe, D. (2012). Galaxy And Mass Assembly (GAMA): the mass-metallicity relationship. Astronomy & Astrophysics, 547, https://doi.org/10.1051/0004-6361/201220050

Herschel-ATLAS/GAMA : spatial clustering of low-redshift submm galaxies (2012)
Journal Article
van Kampen, E., Smith, D., Maddox, S., Hopkins, A., Valtchanov, I., Peacock, J., …Tuffs, R. (2012). Herschel-ATLAS/GAMA : spatial clustering of low-redshift submm galaxies. Monthly Notices of the Royal Astronomical Society, 426(4), 3455-3463. https://doi.org/10.1111/j.1365-2966.2012.21949.x

We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 μm in the Herschel-ATLAS science demonstration phase field. We selected a sample for which we have high-quality spectroscopic redshifts, obtained from... Read More about Herschel-ATLAS/GAMA : spatial clustering of low-redshift submm galaxies.

Galaxy And Mass Assembly (GAMA) : estimating galaxy group masses via caustic analysis (2012)
Journal Article
Alpaslan, M., Robotham, A., Driver, S., Norberg, P., Peacock, J., Baldry, I., …Pimbblet, K. (2012). Galaxy And Mass Assembly (GAMA) : estimating galaxy group masses via caustic analysis. Monthly Notices of the Royal Astronomical Society, 426(4), 2832-2846. https://doi.org/10.1111/j.1365-2966.2012.21020.x

We have generated complementary halo mass estimates for all the groups in the Galaxy And Mass Assembly Galaxy Group Catalogue (GAMA G3Cv1) using a modified caustic mass estimation algorithm, originally developed by Diaferio & Geller. We calibrate the... Read More about Galaxy And Mass Assembly (GAMA) : estimating galaxy group masses via caustic analysis.

Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts (2012)
Journal Article
Christodoulou, L., Eminian, C., Loveday, J., Norberg, P., Baldry, I., Hurley, P., …Wijesinghe, D. (2012). Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts. Monthly Notices of the Royal Astronomical Society, 425(2), 1527-1548. https://doi.org/10.1111/j.1365-2966.2012.21434.x

We measure the two-point angular correlation function of a sample of 4289 223 galaxies with r < 19.4 mag from the Sloan Digital Sky Survey (SDSS) as a function of photometric redshift, absolute magnitude and colour down to Mr − 5 log h = −14 mag. Pho... Read More about Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts.

Galaxy And Mass Assembly (GAMA) : in search of Milky Way Magellanic Cloud analogues (2012)
Journal Article
Robotham, A., Baldry, I., Bland-Hawthorn, J., Driver, S., Loveday, J., Norberg, P., …Staveley-Smith, L. (2012). Galaxy And Mass Assembly (GAMA) : in search of Milky Way Magellanic Cloud analogues. Monthly Notices of the Royal Astronomical Society, 424(2), 1448-1453. https://doi.org/10.1111/j.1365-2966.2012.21332.x

Analysing all Galaxy And Mass Assembly (GAMA) galaxies within a factor of 2 (±0.3 dex) of the stellar mass of the Milky Way (MW), there is a 11.9 per cent chance that one of these galaxies will have a close companion (within a projected separation of... Read More about Galaxy And Mass Assembly (GAMA) : in search of Milky Way Magellanic Cloud analogues.

Galaxy And Mass Assembly (GAMA) : galaxy environments and star formation rate variations (2012)
Journal Article
Wijesinghe, D., Hopkins, A., Brough, S., Taylor, E., Norberg, P., Bauer, A., …Tuffs, R. (2012). Galaxy And Mass Assembly (GAMA) : galaxy environments and star formation rate variations. Monthly Notices of the Royal Astronomical Society, 423(4), 3679-3691. https://doi.org/10.1111/j.1365-2966.2012.21164.x

We present a detailed investigation into the effects of galaxy environment on their star formation rates (SFRs) using galaxies observed in the Galaxy And Mass Assembly (GAMA) survey. We use three independent volume-limited samples of galaxies within... Read More about Galaxy And Mass Assembly (GAMA) : galaxy environments and star formation rate variations.

Herschel-ATLAS/GAMA : a census of dust in optically selected galaxies from stacking at submillimetre wavelengths (2012)
Journal Article
Bourne, N., Maddox, S., Dunne, L., Auld, R., Baes, M., Baldry, I., …Temi, P. (2012). Herschel-ATLAS/GAMA : a census of dust in optically selected galaxies from stacking at submillimetre wavelengths. Monthly Notices of the Royal Astronomical Society, 421(4), 3027-3059. https://doi.org/10.1111/j.1365-2966.2012.20528.x

We use the Herschel‐ATLAS survey to conduct the first large‐scale statistical study of the submillimetre properties of optically selected galaxies. Using ∼80 000 r‐band selected galaxies from 126  deg2 of the GAMA survey, we stack into submillimetre... Read More about Herschel-ATLAS/GAMA : a census of dust in optically selected galaxies from stacking at submillimetre wavelengths.

Galaxy And Mass Assembly (GAMA) : structural investigation of galaxies via model analysis (2012)
Journal Article
Kelvin, L., Driver, S., Robotham, A., Hill, D., Alpaslan, M., Baldry, I., …Tuffs, R. (2012). Galaxy And Mass Assembly (GAMA) : structural investigation of galaxies via model analysis. Monthly Notices of the Royal Astronomical Society, 421(2), 1007-1039. https://doi.org/10.1111/j.1365-2966.2012.20355.x

We present single-Sérsic two-dimensional (2D) model fits to 167 600 galaxies modelled independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital Sky Survey Data Release Seven (SDSS DR7) and UKIRT Infrared Deep Sky Survey Large Area Sur... Read More about Galaxy And Mass Assembly (GAMA) : structural investigation of galaxies via model analysis.

Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06 (2012)
Journal Article
Baldry, I., Driver, S., Loveday, J., Taylor, E., Kelvin, L., Liske, J., …Tuffs, R. (2012). Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06. Monthly Notices of the Royal Astronomical Society, 421(1), 621-634. https://doi.org/10.1111/j.1365-2966.2012.20340.x

We determine the low-redshift field galaxy stellar mass function (GSMF) using an area of 143 deg2 from the first three years of the Galaxy And Mass Assembly (GAMA) survey. The magnitude limits of this redshift survey are r < 19.4 mag over two-thirds... Read More about Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06.

Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions (2012)
Journal Article
Loveday, J., Norberg, P., Baldry, I., Driver, S., Hopkins, A., Peacock, J., …Wijesinghe, D. (2012). Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions. Monthly Notices of the Royal Astronomical Society, 420(2), 1239-1262. https://doi.org/10.1111/j.1365-2966.2011.20111.x

Galaxy and Mass Assembly (GAMA) is a project to study galaxy formation and evolution, combining imaging data from ultraviolet to radio with spectroscopic data from the AAOmega spectrograph on the Anglo-Australian Telescope. Using data from Phase 1 of... Read More about Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions.

Herschel-ATLAS/GAMA : dusty early-type galaxies and passive spirals (2012)
Journal Article
Rowlands, K., Dunne, L., Maddox, S., Bourne, N., Gomez, H., Kaviraj, S., …Tuffs, R. (2012). Herschel-ATLAS/GAMA : dusty early-type galaxies and passive spirals. Monthly Notices of the Royal Astronomical Society, 419(3), 2545-2578. https://doi.org/10.1111/j.1365-2966.2011.19905.x

We present the dust properties and star formation histories of local submillimetre-selected galaxies, classified by optical morphology. Most of the galaxies are late types and very few are early types. The early-type galaxies (ETGs) that are detected... Read More about Herschel-ATLAS/GAMA : dusty early-type galaxies and passive spirals.

Statistical analysis of galaxy surveys - IV. An objective way to quantify the impact of superstructures on galaxy clustering statistics (2011)
Journal Article
Norberg, P., Gaztañaga, E., Baugh, C., & Croton, D. (2011). Statistical analysis of galaxy surveys - IV. An objective way to quantify the impact of superstructures on galaxy clustering statistics. Monthly Notices of the Royal Astronomical Society, 418(4), 2435-2450. https://doi.org/10.1111/j.1365-2966.2011.19636.x

Galaxy And Mass Assembly (GAMA): stellar mass estimates (2011)
Journal Article
Taylor, E., Hopkins, A., Baldry, I., Brown, M., Driver, S., Kelvin, L., …Wijesinghe, D. (2011). Galaxy And Mass Assembly (GAMA): stellar mass estimates. Monthly Notices of the Royal Astronomical Society, 418, 1587-1620. https://doi.org/10.1111/j.1365-2966.2011.19536.x

The environment and characteristics of low-redshift galaxies detected by the Herschel-ATLAS (2011)
Journal Article
Dariush, A., Cortese, L., Eales, S., Pascale, E., Smith, M., Dunne, L., …van der Werf, P. (2011). The environment and characteristics of low-redshift galaxies detected by the Herschel-ATLAS. Monthly Notices of the Royal Astronomical Society, 418, 64-73. https://doi.org/10.1111/j.1365-2966.2011.19340.x

Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G$^3$Cv1) (2011)
Journal Article
Robotham, A., Norberg, P., Driver, S., Baldry, I., Bamford, S., Hopkins, A., …Wijesinghe, D. (2011). Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G$^3$Cv1). Monthly Notices of the Royal Astronomical Society, 416(4), 2640-2668. https://doi.org/10.1111/j.1365-2966.2011.19217.x

Galaxy and Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxies (2011)
Journal Article
Prescott, M., Baldry, I., James, P., Bamford, S., Bland-Hawthorn, J., Brough, S., …Wijesinghe, D. (2011). Galaxy and Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxies. Monthly Notices of the Royal Astronomical Society, 417, 1374-1386. https://doi.org/10.1111/j.1365-2966.2011.19353.x

Herschel-ATLAS: counterparts from the ultraviolet-near-infrared in the science demonstration phase catalogue (2011)
Journal Article
Smith, D., Dunne, L., Maddox, S., Eales, S., Bonfield, D., Jarvis, M., …van Kampen, E. (2011). Herschel-ATLAS: counterparts from the ultraviolet-near-infrared in the science demonstration phase catalogue. Monthly Notices of the Royal Astronomical Society, 416, 857-872. https://doi.org/10.1111/j.1365-2966.2011.18827.x

Galaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass function (2011)
Journal Article
Gunawardhana, M., Hopkins, A., Sharp, R., Brough, S., Taylor, E., Bland-Hawthorn, J., …van Kampen, E. (2011). Galaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass function. Monthly Notices of the Royal Astronomical Society, 415, 1647-1662. https://doi.org/10.1111/j.1365-2966.2011.18800.x

GAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxies (2011)
Journal Article
Wijesinghe, D., da Cunha, E., Hopkins, A., Dunne, L., Sharp, R., Gunawardhana, M., …van der Werf, P. (2011). GAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxies. Monthly Notices of the Royal Astronomical Society, 415, 1002-1012. https://doi.org/10.1111/j.1365-2966.2011.18615.x

Galaxy and Mass Assembly (GAMA): galaxies at the faint end of the H$\alpha$ luminosity function (2011)
Journal Article
Brough, S., Hopkins, A., Sharp, R., Gunawardhana, M., Wijesinghe, D., Robotham, A., …van Kampen, E. (2011). Galaxy and Mass Assembly (GAMA): galaxies at the faint end of the H$\alpha$ luminosity function. Monthly Notices of the Royal Astronomical Society, 413, 1236-1243. https://doi.org/10.1111/j.1365-2966.2011.18210.x

Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release (2011)
Journal Article
Driver, S., Hill, D., Kelvin, L., Robotham, A., Liske, J., Norberg, P., …Warren, S. (2011). Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release. Monthly Notices of the Royal Astronomical Society, 413(2), 971-995. https://doi.org/10.1111/j.1365-2966.2010.18188.x

Galaxy and Mass Assembly: FUV, NUV, ugrizYJHK Petrosian, Kron and Sérsic photometry (2011)
Journal Article
Hill, D., Kelvin, L., Driver, S., Robotham, A., Cameron, E., Cross, N., …van Kampen, E. (2011). Galaxy and Mass Assembly: FUV, NUV, ugrizYJHK Petrosian, Kron and Sérsic photometry. Monthly Notices of the Royal Astronomical Society, 412, 765-799. https://doi.org/10.1111/j.1365-2966.2010.17950.x

Which haloes host Herschel-ATLAS galaxies in the local Universe? (2011)
Journal Article
Guo, Q., Cole, S., Lacey, C., Baugh, C., Frenk, C., Norberg, P., …van Kampen, E. (2011). Which haloes host Herschel-ATLAS galaxies in the local Universe?. Monthly Notices of the Royal Astronomical Society, 412(4), 2277-2285. https://doi.org/10.1111/j.1365-2966.2010.18051.x

We measure the projected cross-correlation between low-redshift (z < 0.5) far-infrared selected galaxies in the science demonstration phase (SDP) field of the Herschel-ATLAS (H-ATLAS) survey and optically selected galaxies from the Galaxy and Mass As... Read More about Which haloes host Herschel-ATLAS galaxies in the local Universe?.

Galaxy and mass assembly (GAMA): dust obscuration in galaxies and their recent star formation histories (2011)
Journal Article
Wijesinghe, D., Hopkins, A., Sharp, R., Gunawardhana, M., Brough, S., Sadler, E., …Thomas, D. (2011). Galaxy and mass assembly (GAMA): dust obscuration in galaxies and their recent star formation histories. Monthly Notices of the Royal Astronomical Society, 410, 2291-2301. https://doi.org/10.1111/j.1365-2966.2010.17599.x

Herschel-ATLAS: far-infrared properties of radio-selected galaxies (2010)
Journal Article
Hardcastle, M., Virdee, J., Jarvis, M., Bonfield, D., Dunne, L., Rawlings, S., …van Kampen, E. (2010). Herschel-ATLAS: far-infrared properties of radio-selected galaxies. Monthly Notices of the Royal Astronomical Society, 409, 122-131. https://doi.org/10.1111/j.1365-2966.2010.17791.x

Herschel-ATLAS: the far-infrared-radio correlation at z \lt 0.5 (2010)
Journal Article
Jarvis, M., Smith, D., Bonfield, D., Hardcastle, M., Falder, J., Stevens, J., …White, G. (2010). Herschel-ATLAS: the far-infrared-radio correlation at z \lt 0.5. Monthly Notices of the Royal Astronomical Society, 409, 92-101. https://doi.org/10.1111/j.1365-2966.2010.17772.x

Herschel-ATLAS: Evolution of the 250 \microm luminosity function out to z = 0.5 (2010)
Journal Article
Dye, S., Dunne, L., Eales, S., Smith, D., Amblard, A., Auld, R., …Verma, A. (2010). Herschel-ATLAS: Evolution of the 250 \microm luminosity function out to z = 0.5. Astronomy & Astrophysics, 518, https://doi.org/10.1051/0004-6361/201014614

Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours (2010)
Journal Article
Amblard, A., Cooray, A., Serra, P., Temi, P., Barton, E., Negrello, M., …Vlahakis, C. (2010). Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours. Astronomy & Astrophysics, 518, https://doi.org/10.1051/0004-6361/201014586

Galaxy And Mass Assembly (GAMA): the input catalogue and star-galaxy separation (2010)
Journal Article
Baldry, I., Robotham, A., Hill, D., Driver, S., Liske, J., Norberg, P., …Tuffs, R. (2010). Galaxy And Mass Assembly (GAMA): the input catalogue and star-galaxy separation. Monthly Notices of the Royal Astronomical Society, 404, 86-100. https://doi.org/10.1111/j.1365-2966.2010.16282.x

Galaxy and Mass Assembly (GAMA): Optimal Tiling of Dense Surveys with a Multi-Object Spectrograph (2010)
Journal Article
Robotham, A., Driver, S., Norberg, P., Baldry, I., Bamford, S., Hopkins, A., …Tuffs, R. (2010). Galaxy and Mass Assembly (GAMA): Optimal Tiling of Dense Surveys with a Multi-Object Spectrograph. Publications of the Astronomical Society of Australia, 27, 76-90. https://doi.org/10.1071/as09053

Statistical analysis of galaxy surveys - I. Robust error estimation for two-point clustering statistics (2009)
Journal Article
Norberg, P., Baugh, C., Gaztañaga, E., & Croton, D. (2009). Statistical analysis of galaxy surveys - I. Robust error estimation for two-point clustering statistics. Monthly Notices of the Royal Astronomical Society, 396(1), 19-38. https://doi.org/10.1111/j.1365-2966.2009.14389.x

The real-space clustering of luminous red galaxies around z < 0.6 quasars in the Sloan Digital Sky Survey (2009)
Journal Article
Padmanabhan, N., White, M., Norberg, P., & Porciani, C. (2009). The real-space clustering of luminous red galaxies around z < 0.6 quasars in the Sloan Digital Sky Survey. Monthly Notices of the Royal Astronomical Society, 397(4), 1862-1875. https://doi.org/10.1111/j.1365-2966.2008.14071.x

The anisotropic distribution of satellite galaxies (2008)
Journal Article
Bailin, J., Power, C., Norberg, P., Zaritsky, D., & Gibson, B. (2008). The anisotropic distribution of satellite galaxies. Monthly Notices of the Royal Astronomical Society, 390, 1133-1156. https://doi.org/10.1111/j.1365-2966.2008.13828.x

Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment? (2008)
Journal Article
Tinker, J., Conroy, C., Norberg, P., Patiri, S., Weinberg, D., & Warren, M. (2008). Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment?. Astrophysical Journal, 686, 53-71. https://doi.org/10.1086/589983

Massive dark matter haloes around bright isolated galaxies in the 2dFGRS (2008)
Journal Article
Norberg, P., Frenk, C., & Cole, S. (2008). Massive dark matter haloes around bright isolated galaxies in the 2dFGRS. Monthly Notices of the Royal Astronomical Society, 383, 646-662. https://doi.org/10.1111/j.1365-2966.2007.12583.x

Statistical analysis of galaxy surveys - III. The non-linear clustering of red and blue galaxies in the 2dFGRS (2007)
Journal Article
Croton, D., Norberg, P., Gaztañaga, E., & Baugh, C. (2007). Statistical analysis of galaxy surveys - III. The non-linear clustering of red and blue galaxies in the 2dFGRS. Monthly Notices of the Royal Astronomical Society, 379, 1562-1570. https://doi.org/10.1111/j.1365-2966.2007.12035.x

On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion (2007)
Journal Article
Tinker, J., Norberg, P., Weinberg, D., & Warren, M. (2007). On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion. Astrophysical Journal, 659, 877-889. https://doi.org/10.1086/511967

Can a large-scale structure probe cosmic microwave background-constrained non-Gaussianity? (2007)
Journal Article
Kang, X., Norberg, P., & Silk, J. (2007). Can a large-scale structure probe cosmic microwave background-constrained non-Gaussianity?. Monthly Notices of the Royal Astronomical Society, 376, 343-347. https://doi.org/10.1111/j.1365-2966.2007.11435.x

Luminosity- and redshift-dependent quasar clustering (2006)
Journal Article
Porciani, C., & Norberg, P. (2006). Luminosity- and redshift-dependent quasar clustering. Monthly Notices of the Royal Astronomical Society, 371, 1824-1834. https://doi.org/10.1111/j.1365-2966.2006.10813.x

Cosmological parameters from cosmic microwave background measurements and the final 2dF Galaxy Redshift Survey power spectrum (2006)
Journal Article
Sanchez, A., Baugh, C., Percival, W., Peacock, J., Padilla, N., Cole, S., …Norberg, P. (2006). Cosmological parameters from cosmic microwave background measurements and the final 2dF Galaxy Redshift Survey power spectrum. Monthly Notices of the Royal Astronomical Society, 366(1), 189-207. https://doi.org/10.1111/j.1365-2966.2005.09833.x

We derive constraints on cosmological parameters using the power spectrum of galaxy clustering measured from the final 2dF Galaxy Redshift Survey (2dFGRS) and a compilation of measurements of the temperature power spectrum and temperature–polarizatio... Read More about Cosmological parameters from cosmic microwave background measurements and the final 2dF Galaxy Redshift Survey power spectrum.

Statistical analysis of galaxy surveys - II. The three-point galaxy correlation function measured from the 2dFGRS (2005)
Journal Article
Gaztañaga, E., Norberg, P., Baugh, C., & Croton, D. (2005). Statistical analysis of galaxy surveys - II. The three-point galaxy correlation function measured from the 2dFGRS. Monthly Notices of the Royal Astronomical Society, 364, 620-634. https://doi.org/10.1111/j.1365-2966.2005.09583.x

The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey (2005)
Journal Article
Hilton, M., Collins, C., De Propris, R., Baldry, I., Baugh, C., Bland-Hawthorn, J., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey. Monthly Notices of the Royal Astronomical Society, 363(2), 661-674. https://doi.org/10.1111/j.1365-2966.2005.09470.x

The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and the Two-degree Field Galaxy Redshift Survey (2dFGRS), respectively, comprise the largest, homogeneous X-ray selected cluster catalogue and completed g... Read More about The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey.

The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications (2005)
Journal Article
Cole, S., Percival, W., Peacock, J., Norberg, P., Baugh, C., Frenk, C., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications. Monthly Notices of the Royal Astronomical Society, 362(2), 505-534. https://doi.org/10.1111/j.1365-2966.2005.09318.x

We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a direct Fourier method. The sample used comprises 221 414 galaxies with measured redshifts. We investigate in detail the modelling of the sample selecti... Read More about The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications.

The abundance and radial distribution of satellite galaxies (2005)
Journal Article
van den Bosch, F., Yang, X., Mo, H., & Norberg, P. (2005). The abundance and radial distribution of satellite galaxies. Monthly Notices of the Royal Astronomical Society, 356, 1233-1248. https://doi.org/10.1111/j.1365-2966.2004.08407.x

The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations (2005)
Journal Article
Wild, V., Peacock, J., Lahav, O., Conway, E., Maddox, S., Baldry, I., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations. Monthly Notices of the Royal Astronomical Society, 356(1), 247-269. https://doi.org/10.1111/j.1365-2966.2004.08447.x

It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complicates the inference of cosmological parameters from galaxy redshift surveys, and is a challenge to theories of galaxy formation and evolution. In this p... Read More about The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations.

The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type (2005)
Journal Article
Croton, D., Farrar, G., Norberg, P., Colless, M., Peacock, J., Baldry, I., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type. Monthly Notices of the Royal Astronomical Society, 356(3), 1155-1167. https://doi.org/10.1111/j.1365-2966.2004.08546.x

We use the 2dF Galaxy Redshift Survey to measure the dependence of the bJ-band galaxy luminosity function on large-scale environment, defined by density contrast in spheres of radius 8 h−1 Mpc, and on spectral type, determined from principal componen... Read More about The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type.

The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type (2005)
Journal Article
Conway, E., Maddox, S., Wild, V., Peacock, J., Hawkins, E., Norberg, P., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type. Monthly Notices of the Royal Astronomical Society, 356(2), 456-474. https://doi.org/10.1111/j.1365-2966.2004.08446.x

We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) – as defined by the η parameter of Madgwick et al., which quantifies the spectral type of galaxies in the survey... Read More about The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type.

Cosmic evolution of quasar clustering: implications for the host haloes (2004)
Journal Article
Porciani, C., Magliocchetti, M., & Norberg, P. (2004). Cosmic evolution of quasar clustering: implications for the host haloes. Monthly Notices of the Royal Astronomical Society, 355, 1010-1030. https://doi.org/10.1111/j.1365-2966.2004.08408.x

The 2dF Galaxy Redshift Survey: the local E+A galaxy population (2004)
Journal Article
Blake, C., Pracy, M., Couch, W., Bekki, K., Lewis, I., Glazebrook, K., …Taylor, K. (2004). The 2dF Galaxy Redshift Survey: the local E+A galaxy population. Monthly Notices of the Royal Astronomical Society, 355(3), 713-727. https://doi.org/10.1111/j.1365-2966.2004.08351.x

We select a sample of low-redshift (z∼ 0.1) E+A galaxies from the 2dF Galaxy Redshift Survey (2dFGRS). The spectra of these objects are defined by strong hydrogen Balmer absorption lines (Hδ, Hγ, Hβ) combined with a lack of [O ii] 3727-Å emission, to... Read More about The 2dF Galaxy Redshift Survey: the local E+A galaxy population.

Galaxy groups in the two-degree field Galaxy Redshift Survey: the luminous content of the groups (2004)
Journal Article
Eke, V., Frenk, C., Baugh, C., Cole, S., Norberg, P., Peacock, J., …Taylor, K. (2004). Galaxy groups in the two-degree field Galaxy Redshift Survey: the luminous content of the groups. Monthly Notices of the Royal Astronomical Society, 355(3), 769-784. https://doi.org/10.1111/j.1365-2966.2004.08354.x

The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catalogue of 29 000 objects is used to study the luminous content of galaxy systems of various sizes. Mock galaxy catalogues constructed from cosmological... Read More about Galaxy groups in the two-degree field Galaxy Redshift Survey: the luminous content of the groups.

The 2dF Galaxy Redshift Survey: spherical harmonics analysis of fluctuations in the final catalogue (2004)
Journal Article
Percival, W., Burkey, D., Heavens, A., Taylor, A., Cole, S., Peacock, J., …Taylor, K. (2004). The 2dF Galaxy Redshift Survey: spherical harmonics analysis of fluctuations in the final catalogue. Monthly Notices of the Royal Astronomical Society, 353(4), 1201-1218. https://doi.org/10.1111/j.1365-2966.2004.08146.x

We present the result of a decomposition of the 2dF Galaxy Redshift Survey (2dFGRS) galaxy overdensity field into an orthonormal basis of spherical harmonics and spherical Bessel functions. Galaxies are expected to directly follow the bulk motion of... Read More about The 2dF Galaxy Redshift Survey: spherical harmonics analysis of fluctuations in the final catalogue.

Probing dark matter haloes with satellite kinematics (2004)
Journal Article
van den Bosch, F., Norberg, P., Mo, H., & Yang, X. (2004). Probing dark matter haloes with satellite kinematics. Monthly Notices of the Royal Astronomical Society, 352, 1302-1314. https://doi.org/10.1111/j.1365-2966.2004.08021.x

The 2dF Galaxy Redshift Survey: Wiener reconstruction of the cosmic web. (2004)
Journal Article
Erdoğdu, P., Lahav, O., Zaroubi, S., Efstathiou, G., Moody, S., Peacock, J., …Taylor, K. (2004). The 2dF Galaxy Redshift Survey: Wiener reconstruction of the cosmic web. Monthly Notices of the Royal Astronomical Society, 352(3), 939-960. https://doi.org/10.1111/j.1365-2966.2004.07984.x

We reconstruct the underlying density field of the Two-degree Field Galaxy Redshift Survey (2dFGRS) for the redshift range 0.035 < z < 0.200 using the Wiener filtering method. The Wiener filter suppresses shot noise and accounts for selection and inc... Read More about The 2dF Galaxy Redshift Survey: Wiener reconstruction of the cosmic web..

The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models (2004)
Journal Article
Croton, D., Colless, M., Gaztañaga, E., Baugh, C., Norberg, P., Baldry, I., …Taylor, K. (2004). The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models. Monthly Notices of the Royal Astronomical Society, 352(3), 828-836. https://doi.org/10.1111/j.1365-2966.2004.07968.x

We measure the redshift-space reduced void probability function (VPF) for 2dFGRS volume-limited galaxy samples covering the absolute magnitude range M b JGraphic−5 log10h=−18 to −22. Theoretically, the VPF connects the distribution of voids to the mo... Read More about The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models.

The 2dF Galaxy Redshift Survey: higher-order galaxy correlation functions (2004)
Journal Article
Croton, D., Gaztañaga, E., Baugh, C., Norberg, P., Colless, M., Baldry, I., …Taylor, K. (2004). The 2dF Galaxy Redshift Survey: higher-order galaxy correlation functions. Monthly Notices of the Royal Astronomical Society, 352(4), 1232-1244. https://doi.org/10.1111/j.1365-2966.2004.08017.x

We measure moments of the galaxy count probability distribution function in the Two-degree Field Galaxy Redshift Survey (2dFGRS). The survey is divided into volume-limited subsamples in order to examine the dependence of the higher-order clustering o... Read More about The 2dF Galaxy Redshift Survey: higher-order galaxy correlation functions.

Substructure analysis of selected low-richness 2dFGRS clusters of galaxies (2004)
Journal Article
Burgett, W. S., Vick, M. M., Davis, D. S., Colless, M., De Propris, R., Baldry, I., …Taylor, K. (2004). Substructure analysis of selected low-richness 2dFGRS clusters of galaxies. Monthly Notices of the Royal Astronomical Society, 352(2), 605-654. https://doi.org/10.1111/j.1365-2966.2004.07952.x

Complementary one-, two- and three-dimensional tests for detecting the presence of substructure in clusters of galaxies are applied to recently obtained data from the 2dF Galaxy Redshift Survey. The sample of 25 clusters used in this study includes 1... Read More about Substructure analysis of selected low-richness 2dFGRS clusters of galaxies.

The 2dF Galaxy Redshift Survey: the clustering of galaxy groups (2004)
Journal Article
Padilla, N., Baugh, C., Eke, V., Norberg, P., Cole, S., Frenk, C., …Taylor, K. (2004). The 2dF Galaxy Redshift Survey: the clustering of galaxy groups. Monthly Notices of the Royal Astronomical Society, 352(1), 211-225. https://doi.org/10.1111/j.1365-2966.2004.07911.x

We measure the clustering of galaxy groups in the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) catalogue. The 2PIGG sample has 28 877 groups with at least two members. The clustering amplitude of the full 2PIGG catalogue is weaker than that of 2d... Read More about The 2dF Galaxy Redshift Survey: the clustering of galaxy groups.

The 2dF Galaxy Redshift Survey: the blue galaxy fraction and implications for the Butcher-Oemler effect (2004)
Journal Article
De Propris, R., Colless, M., Peacock, J., Couch, W., Driver, S., Balogh, M., …Taylor, K. (2004). The 2dF Galaxy Redshift Survey: the blue galaxy fraction and implications for the Butcher-Oemler effect. Monthly Notices of the Royal Astronomical Society, 351(1), 125-132. https://doi.org/10.1111/j.1365-2966.2004.07756.x

We derive the fraction of blue galaxies in a sample of clusters at z < 0.11 and the general field at the same redshift. The value of the blue fraction is observed to depend on the luminosity limit adopted, cluster-centric radius and, more generally,... Read More about The 2dF Galaxy Redshift Survey: the blue galaxy fraction and implications for the Butcher-Oemler effect.

The 2dF galaxy redshift survey: clustering properties of radio galaxies (2004)
Journal Article
Magliocchetti, M., Maddox, S., Hawkins, E., Peacock, J., Bland-Hawthorn, J., Bridges, T., …Taylor, K. (2004). The 2dF galaxy redshift survey: clustering properties of radio galaxies. Monthly Notices of the Royal Astronomical Society, 350, 1485-1494. https://doi.org/10.1111/j.1365-2966.2004.07751.x

The 2dF Galaxy Redshift Survey: hierarchical galaxy clustering (2004)
Journal Article
Baugh, C., Croton, D., Gaztañaga, E., Norberg, P., Colless, M., Baldry, I., …Taylor, K. (2004). The 2dF Galaxy Redshift Survey: hierarchical galaxy clustering. Monthly Notices of the Royal Astronomical Society, 351(2), L44-L48. https://doi.org/10.1111/j.1365-2966.2004.07962.x

We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothesis: namely, that the p-point galaxy correlation functions can be written in terms of the two-point correlation function or variance. This scaling is... Read More about The 2dF Galaxy Redshift Survey: hierarchical galaxy clustering.

The Millennium Galaxy Catalogue: the photometric accuracy, completeness and contamination of the 2dFGRS and SDSS-EDR/DR1 data sets (2004)
Journal Article
Cross, N., Driver, S., Liske, J., Lemon, D., Peacock, J., Cole, S., …Sutherland, W. (2004). The Millennium Galaxy Catalogue: the photometric accuracy, completeness and contamination of the 2dFGRS and SDSS-EDR/DR1 data sets. Monthly Notices of the Royal Astronomical Society, 349, 576-594. https://doi.org/10.1111/j.1365-2966.2004.07527.x

Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS (2004)
Journal Article
Baugh, C., Bower, R., Cole, S., Eke, V., Baldry, I., Balogh, M., …Taylor, K. (2004). Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS. Monthly Notices of the Royal Astronomical Society, 348(4), 1355-1372. https://doi.org/10.1111/j.1365-2966.2004.07453.x

We analyse the observed correlation between galaxy environment and Hα emission-line strength, using volume-limited samples and group catalogues of 24 968 galaxies at 0.05

Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue (2004)
Journal Article
Eke, V., Baugh, C., Cole, S., Frenk, C., Norberg, P., Peacock, J., …Sutherland, W. (2004). Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue. Monthly Notices of the Royal Astronomical Society, 348(3), 866-878. https://doi.org/10.1111/j.1365-2966.2004.07408.x

The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2dFGRS) is described. Groups are identified by means of a friends-of-friends percolation algorithm which has been thoroughly tested on mock versions of... Read More about Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue.

Identifying groups and clusters in the 2dFGRS (2003)
Journal Article
Norberg, P., Eke, V., & Team, T. 2. (2003). Identifying groups and clusters in the 2dFGRS. Astrophysics and Space Science, 285, 205-209. https://doi.org/10.1023/a%3A1024650902547

The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe (2003)
Journal Article
Hawkins, E., Maddox, S., Cole, S., Lahav, O., Madgwick, D., Norberg, P., …Taylor, K. (2003). The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe. Monthly Notices of the Royal Astronomical Society, 346(1), 78-96. https://doi.org/10.1046/j.1365-2966.2003.07063.x

We present a detailed analysis of the two-point correlation function, ξ(σ, π), from the 2dF Galaxy Redshift Survey (2dFGRS). The large size of the catalogue, which contains ∼220 000 redshifts, allows us to make high-precision measurements of various... Read More about The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe.

The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type (2003)
Journal Article
Madgwick, D., Hawkins, E., Lahav, O., Maddox, S., Norberg, P., Peacock, J., …Taylor, K. (2003). The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type. Monthly Notices of the Royal Astronomical Society, 344(3), 847-856. https://doi.org/10.1046/j.1365-8711.2003.06861.x

We have calculated the two-point correlation functions in redshift space, ξ(σ, π), for galaxies of different spectral types in the 2dF Galaxy Redshift Survey. Using these correlation functions, we are able to estimate values of the linear redshift-sp... Read More about The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type.

The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies. (2003)
Journal Article
De Propris, R., Colless, M., Driver, S., Couch, W., Peacock, J., Baldry, I., …Taylor, K. (2003). The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies. Monthly Notices of the Royal Astronomical Society, 342(3), 725-737. https://doi.org/10.1046/j.1365-8711.2003.06510.x

We have determined the composite luminosity function (LF) for galaxies in 60 clusters from the 2dF Galaxy Redshift Survey. The LF spans the range −22.5 < Mmath image < −15, and is well fitted by a Schechter function with M*math image=−20.07 ± 0.07 an... Read More about The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies..

Parameter constraints for flat cosmologies from cosmic microwave background and 2dFGRS power spectra (2002)
Journal Article
Percival, W., Sutherland, W., Peacock, J., Baugh, C., Bland-Hawthorn, J., Bridges, T., …Taylor, K. (2002). Parameter constraints for flat cosmologies from cosmic microwave background and 2dFGRS power spectra. Monthly Notices of the Royal Astronomical Society, 337, 1068-1080. https://doi.org/10.1046/j.1365-8711.2002.06001.x

The 2dF Galaxy Redshift Survey: the b_J-band galaxy luminosity function and survey selection function (2002)
Journal Article
Norberg, P., Cole, S., Baugh, C., Frenk, C., Baldry, I., Bland-Hawthorn, J., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: the b_J-band galaxy luminosity function and survey selection function. Monthly Notices of the Royal Astronomical Society, 336, 907-931. https://doi.org/10.1046/j.1365-8711.2002.05831.x

The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe (2002)
Journal Article
Verde, L., Heavens, A., Percival, W., Matarrese, S., Baugh, C., Bland-Hawthorn, J., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe. Monthly Notices of the Royal Astronomical Society, 335(2), 432-440. https://doi.org/10.1046/j.1365-8711.2002.05620.x

We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias parameter of the galaxies. This parameter quantifies the strength of clustering of the galaxies relative to the mass in the Universe. By analysing 80... Read More about The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe.

Shape Alignments of Satellite Galaxies (2002)
Journal Article
Bernstein, G., & Norberg, P. (2002). Shape Alignments of Satellite Galaxies. Astronomical Journal, 124, 733-736. https://doi.org/10.1086/341383

The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters (2002)
Journal Article
Lewis, I., Balogh, M., De Propris, R., Couch, W., Bower, R., Offer, A., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters. Monthly Notices of the Royal Astronomical Society, 334(3), 673-683. https://doi.org/10.1046/j.1365-8711.2002.05558.x

We have measured the equivalent width of the Hα emission line for 11 006 galaxies brighter than Mb=−19 (ΩΛ= 0.7, Ωm= 0.3, H0= 70 km s−1 Mpc−1) at 0.05 < z < 0.1 in the 2dF Galaxy Redshift Survey (2dFGRS), in the fields of 17 known galaxy clusters. Th... Read More about The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters.

New Upper Limit on the Total Neutrino Mass from the 2 Degree Field Galaxy Redshift Survey (2002)
Journal Article
Elgarøy, &., !and, .., !, ,. O., rcival, W., Peacock, J., Madgwick, D., …Taylor, K. (2002). New Upper Limit on the Total Neutrino Mass from the 2 Degree Field Galaxy Redshift Survey. Physical Review Letters, 89(6), 061301-+. https://doi.org/10.1103/physrevlett.89.061301

The 2dF Galaxy Redshift Survey: the amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing (2002)
Journal Article
Lahav, O., Bridle, S., Percival, W., Peacock, J., Efstathiou, G., Baugh, C., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: the amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing. Monthly Notices of the Royal Astronomical Society, 333(4), 961-968. https://doi.org/10.1046/j.1365-8711.2002.05485.x

We compare the amplitudes of fluctuations probed by the 2dF Galaxy Redshift Survey (2dFGRS) and by the latest measurements of the cosmic microwave background (CMB) anisotropies. By combining the 2dFGRS and CMB data, we find the linear-theory rms mass... Read More about The 2dF Galaxy Redshift Survey: the amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing.

The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type. (2002)
Journal Article
Madgwick, D., Lahav, O., Baldry, I., Baugh, C., Bland-Hawthorn, J., Bridges, T., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type. Monthly Notices of the Royal Astronomical Society, 333(1), 133-144. https://doi.org/10.1046/j.1365-8711.2002.05393.x

We calculate the optical bJ luminosity function (LF) of the 2dF Galaxy Redshift Survey (2dFGRS) for different subsets defined by their spectral properties. These spectrally selected subsets are defined using a new parameter, η, which is a linear comb... Read More about The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type..

The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type (2002)
Journal Article
Norberg, P., Baugh, C., Hawkins, E., Maddox, S., Madgwick, D., Lahav, O., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type. Monthly Notices of the Royal Astronomical Society, 332(4), 827-838. https://doi.org/10.1046/j.1365-8711.2002.05348.x

We investigate the dependence of galaxy clustering on luminosity and spectral type using the 2dF Galaxy Redshift Survey (2dFGRS). Spectral types are assigned using the principal-component analysis of Madgwick et al. We divide the sample into two broa... Read More about The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type.

The 2dF Galaxy Redshift Survey: Constraints on Cosmic Star Formation History from the Cosmic Spectrum. (2002)
Journal Article
Baldry, I. K., Glazebrook, K., Baugh, C. M., Bland-Hawthorn, J., Bridges, T., Cannon, R., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: Constraints on Cosmic Star Formation History from the Cosmic Spectrum. Astrophysical Journal, 569(2), 582-594. https://doi.org/10.1086/339477

We present the first results on the history of star formation in the universe based on the "cosmic spectrum," in particular the volume-averaged, luminosity-weighted, stellar absorption-line spectrum of present-day galaxies from the 2dF Galaxy Redshif... Read More about The 2dF Galaxy Redshift Survey: Constraints on Cosmic Star Formation History from the Cosmic Spectrum..

Evidence for a non-zero $\Lambda$ and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and cosmic microwave background anisotropies (2002)
Journal Article
Efstathiou, G., Moody, S., Peacock, J., Percival, W., Baugh, C., Bland-Hawthorn, J., …Taylor, K. (2002). Evidence for a non-zero $\Lambda$ and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and cosmic microwave background anisotropies. Monthly Notices of the Royal Astronomical Society, 330, L29-L35. https://doi.org/10.1046/j.1365-8711.2002.05215.x

The 2dF Galaxy Redshift Survey: a targeted study of catalogued clusters of galaxies (2002)
Journal Article
De Propris, R., Couch, W., Colless, M., Dalton, G., Collins, C., Baugh, C., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: a targeted study of catalogued clusters of galaxies. Monthly Notices of the Royal Astronomical Society, 329, 87-101. https://doi.org/10.1046/j.1365-8711.2002.04958.x

Radio sources in the 2dF Galaxy Redshift Survey - II. Local radio luminosity functions for AGN and star-forming galaxies at 1.4 GHz (2002)
Journal Article
Sadler, E., Jackson, C., Cannon, R., McIntyre, V., Murphy, T., Bland-Hawthorn, J., …Taylor, K. (2002). Radio sources in the 2dF Galaxy Redshift Survey - II. Local radio luminosity functions for AGN and star-forming galaxies at 1.4 GHz. Monthly Notices of the Royal Astronomical Society, 329, 227-245. https://doi.org/10.1046/j.1365-8711.2002.04998.x

The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe (2001)
Journal Article
Percival, W., Baugh, C., Bland-Hawthorn, J., Bridges, T., Cannon, R., Cole, S., …Taylor, K. (2001). The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe. Monthly Notices of the Royal Astronomical Society, 327(4), 1297-1306. https://doi.org/10.1046/j.1365-8711.2001.04827.x

The 2dF Galaxy Redshift Survey has now measured in excess of 160-000 galaxy redshifts. This paper presents the power spectrum of the galaxy distribution, calculated using a direct Fourier transform based technique. We argue that, within the k-space r... Read More about The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe.

The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering (2001)
Journal Article
Norberg, P., Baugh, C., Hawkins, E., Maddox, S., Peacock, J., Cole, S., …Taylor, K. (2001). The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering. Monthly Notices of the Royal Astronomical Society, 328(1), 64-70. https://doi.org/10.1046/j.1365-8711.2001.04839.x

We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the Anglo-Australian two degree field galaxy redshift survey (2dFGRS). The 2dFGRS is over an order of magnitude larger than previous redshift surveys use... Read More about The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering.

The 2dF galaxy redshift survey: near-infrared galaxy luminosity functions (2001)
Journal Article
Cole, S., Norberg, P., Baugh, C., Frenk, C., Bland-Hawthorn, J., Bridges, T., …Taylor, K. (2001). The 2dF galaxy redshift survey: near-infrared galaxy luminosity functions. Monthly Notices of the Royal Astronomical Society, 326(1), 255-273. https://doi.org/10.1046/j.1365-8711.2001.04591.x

We combine the Two Micron All Sky Survey (2MASS) Extended Source Catalogue and the 2dF Galaxy Redshift Survey to produce an infrared selected galaxy catalogue with 17 173 measured redshifts. We use this extensive data set to estimate the galaxy lumin... Read More about The 2dF galaxy redshift survey: near-infrared galaxy luminosity functions.

The 2dF Galaxy Redshift Survey: the number and luminosity density of galaxies (2001)
Journal Article
Cross, N., Driver, S., Couch, W., Baugh, C., Bland-Hawthorn, J., Bridges, T., …Taylor, K. (2001). The 2dF Galaxy Redshift Survey: the number and luminosity density of galaxies. Monthly Notices of the Royal Astronomical Society, 324(4), 825-841. https://doi.org/10.1046/j.1365-8711.2001.04254.x

We present the bivariate brightness distribution (BBD) for the 2dF Galaxy Redshift Survey (2dFGRS) based on a preliminary subsample of 45 000 galaxies. The BBD is an extension of the galaxy luminosity function, incorporating surface brightness inform... Read More about The 2dF Galaxy Redshift Survey: the number and luminosity density of galaxies.

A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey (2001)
Journal Article
Peacock, J., Cole, S., Norberg, P., Baugh, C., Bland-Hawthorn, J., Bridges, T., …Taylor, K. (2001). A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey. Nature, 410(6825), 169-173

On the formation of massive stars by accretion (2000)
Journal Article
Norberg, P., & Maeder, A. (2000). On the formation of massive stars by accretion. Astronomy and Astrophysics, 359, 1025-1034