Outputs (162)

Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to 108M⊙ (2016)
Journal Article
Contini, T., Epinat, B., Bouché, N., Brinchmann, J., Boogaard, L., Ventou, E., …Soucail, G. (2016). Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to 108M⊙. Astronomy & Astrophysics, 591, Article A49. https://doi.org/10.1051/0004-6361/201527866

Aims. Whereas the evolution of gas kinematics of massive galaxies is now relatively well established up to redshift z ~ 3, little is known about the kinematics of lower mass (M⋆≤ 1010M⊙) galaxies. We use MUSE, a powerful wide-field, optical integral-... Read More about Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to 108M⊙.

Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2–3 (2016)
Journal Article
Kato, Y., Matsuda, Y., Smail, I., Swinbank, A., Hatsukade, B., Umehata, H., …Hayashino, T. (2016). Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2–3. Monthly Notices of the Royal Astronomical Society, 460(4), 3861-3872. https://doi.org/10.1093/mnras/stw1237

We present a Herschel/SPIRE survey of three protoclusters at z = 2 − 3 (2QZCluster, HS1700, SSA22). Based on the SPIRE colours (S350/S250 and S500/S350) of 250 μm sources, we selected high redshift dusty star-forming galaxies potentially associated w... Read More about Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2–3.

Optical emission line nebulae in galaxy cluster cores 1: the morphological, kinematic and spectral properties of the sample (2016)
Journal Article
Hamer, S., Edge, A., Swinbank, A., Wilman, R., Combes, F., Salomé, P., …Bremer, M. (2016). Optical emission line nebulae in galaxy cluster cores 1: the morphological, kinematic and spectral properties of the sample. Monthly Notices of the Royal Astronomical Society, 460(2), 1758-1789. https://doi.org/10.1093/mnras/stw1054

We present an Integral Field Unit survey of 73 galaxy clusters and groups with the VIsible Multi Object Spectrograph on the Very Large Telescope. We exploit the data to determine the H α gas dynamics on kpc scales to study the feedback processes occu... Read More about Optical emission line nebulae in galaxy cluster cores 1: the morphological, kinematic and spectral properties of the sample.

The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s (2016)
Journal Article
Johnson, H., Harrison, C., Swinbank, A., Bower, R., Smail, I., Koyama, Y., & Geach, J. (2016). The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s. Monthly Notices of the Royal Astronomical Society, 460(1), 1059-1076. https://doi.org/10.1093/mnras/stw1030

To investigate what drives the reversal of the morphology–density relation at intermediate/high redshift, we present a multiwavelength analysis of 27 dusty starburst galaxies in the massive cluster Cl 0024+17 at z = 0.4. We combine Hα dynamical maps... Read More about The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s.

The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1 (2016)
Journal Article
Tiley, A., Stott, J., Swinbank, A., Bureau, M., Harrison, C., Bower, R., …Best, P. (2016). The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1. Monthly Notices of the Royal Astronomical Society, 460(1), 103-129. https://doi.org/10.1093/mnras/stw936

We present the stellar mass (M*), and K-corrected K-band absolute magnitude (MK) Tully–Fisher relations (TFRs) for subsamples of the 584 galaxies spatially resolved in H α emission by the KMOS Redshift One Spectroscopic Survey (KROSS). We model the v... Read More about The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1.

The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field (2016)
Journal Article
Chen, C., Smail, I., Ivison, R., Arumugam, V., Almaini, O., Conselice, C., …Zavala, J. (2016). The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field. Astrophysical Journal, 820(2), Article 82. https://doi.org/10.3847/0004-637x/820/2/82

We present multiwavelength identifications for the counterparts of 1088 submillimeter sources detected at 850 μm in the SCUBA-2 Cosmology Legacy Survey study of the UKIRT Infrared Deep Sky Survey-Ultra-Deep Survey (UDS) field. By utilizing an Atacama... Read More about The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field.

The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies (2016)
Journal Article
Stott, J., Swinbank, A., Johnson, H., Tiley, A., Magdis, G., Bower, R., …Cirasuolo, M. (2016). The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 457(2), 1888-1904. https://doi.org/10.1093/mnras/stw129

The KMOS Redshift One Spectroscopic Survey (KROSS) is an ESO-guaranteed time survey of 795 typical star-forming galaxies in the redshift range z = 0.8–1.0 with the KMOS instrument on the Very Large Telescope. In this paper, we present resolved kinema... Read More about The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies.

KROSS: mapping the Hα emission across the star formation sequence at z ≈ 1 (2016)
Journal Article
Magdis, G., Bureau, M., Stott, J., Tiley, A., Swinbank, A., Bower, R., …Sharples, R. (2016). KROSS: mapping the Hα emission across the star formation sequence at z ≈ 1. Monthly Notices of the Royal Astronomical Society, 456(4), 4533-4541. https://doi.org/10.1093/mnras/stv2931

We present first results from the KMOS (K-band Multi-Object Spectrograph) Redshift One Spectroscopic Survey, an ongoing large kinematical survey of a thousand, z ∼ 1 star-forming galaxies, with VLT KMOS. Out of the targeted galaxies (∼500 so far), we... Read More about KROSS: mapping the Hα emission across the star formation sequence at z ≈ 1.

The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionized outflows in the host galaxies of X-ray AGN (2015)
Journal Article
Harrison, C., Alexander, D., Mullaney, J., Stott, J., Swinbank, A., Arumugam, V., …Sharples, R. (2016). The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionized outflows in the host galaxies of X-ray AGN. Monthly Notices of the Royal Astronomical Society, 456(2), 1195-1220. https://doi.org/10.1093/mnras/stv2727

We present the first results from the KMOS (K-band Multi-Object Spectrograph) AGN (active galactic nuclei) Survey at High redshift (KASHz), a VLT/KMOS integral-field spectroscopic (IFS) survey of z ≳ 0.6 AGN. We present galaxy-integrated spectra of 8... Read More about The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionized outflows in the host galaxies of X-ray AGN.

HSIM: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT (2015)
Journal Article
Zieleniewski, S., Thatte, N., Kendrew, S., Houghton, R., Swinbank, A., Tecza, M., …Fusco, T. (2015). HSIM: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT. Monthly Notices of the Royal Astronomical Society, 453(4), 3754-3765. https://doi.org/10.1093/mnras/stv1860

We present hsim: a dedicated pipeline for simulating observations with the High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) on the European Extremely Large Telescope. hsim takes high spectral and spat... Read More about HSIM: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT.