Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation

Béthermin, M.; Daddi, E.; Magdis, G.; Lagos, C.; Sargent, M.; Albrecht, M.; Aussel, H.; Bertoldi, F.; Buat, V.; Galametz, M.; Heinis, S.; Ilbert, O.; Karim, A.; Koekemoer, A.; Lacey, C.; Le Floc'h, E.; Navarrete, F.; Pannella, M.; Schreiber, C.; Smolčić, V.; Symeonidis, M.; Viero, M.

doi:10.1051/0004-6361/201425031

The evolution of the stellar mass versus halo mass relationship (2015)
Journal Article
Mitchell, P. D., Lacey, C. G., Baugh, C. M., & Cole, S. (2016). The evolution of the stellar mass versus halo mass relationship. Monthly Notices of the Royal Astronomical Society, 456(2), 1459-1483. https://doi.org/10.1093/mnras/stv2741

We present an analysis of the predictions made by the GALFORM semi-analytic galaxy formation model for the evolution of the relationship between stellar mass and halo mass. We show that for the standard implementations of supernova feedback and gas r... Read More about The evolution of the stellar mass versus halo mass relationship.

Erratum: "HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies" (2015, ApJ, 812, 43) (2015)
Journal Article
Bussmann, R., Riechers, D., Fialkov, A., Scudder, J., Hayward, C., Cowley, W., …Wardlow, J. (2015). Erratum: "HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies" (2015, ApJ, 812, 43). Astrophysical Journal, 815(2), Article 135. https://doi.org/10.1088/0004-637x/815/2/135

The original published article omitted the final 6 panels of Figure 2. In addition, the original article included an older version of Figure 3 that does not have source labels shown in each panel.

A hybrid multiresolution scheme to efficiently model the structure of reionization on the largest scales (2015)
Journal Article
Kim, H., Wyithe, J., Park, J., Poole, G., Lacey, C., & Baugh, C. (2016). A hybrid multiresolution scheme to efficiently model the structure of reionization on the largest scales. Monthly Notices of the Royal Astronomical Society, 455(4), 4498-4511. https://doi.org/10.1093/mnras/stv2623

Redshifted 21-cm measurements of the structure of ionized regions that grow during reionization promise to provide a new probe of early galaxy and structure formation. One of the challenges of modelling reionization is to account both for the subhalo... Read More about A hybrid multiresolution scheme to efficiently model the structure of reionization on the largest scales.

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.

HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies (2015)
Journal Article
Bussmann, R., Riechers, D., Fialkov, A., Scudder, J., Hayward, C., Cowley, W., …Wardlow, J. (2015). HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies. Astrophysical Journal, 812(1), Article 43. https://doi.org/10.1088/0004-637x/812/1/43

The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-forming galaxies (DSFGs) over a wide range in redshift. A detailed understanding of these DSFGs is hampered by the limited spatial resolution of Hersch... Read More about HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies.

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.

A new methodology to test galaxy formation models using the dependence of clustering on stellar mass (2015)
Journal Article
Campbell, D., Baugh, C., Mitchell, P., Helly, J., Gonzalez-Perez, V., Lacey, C., …Farrow, D. (2015). A new methodology to test galaxy formation models using the dependence of clustering on stellar mass. Monthly Notices of the Royal Astronomical Society, 452(1), 852-871. https://doi.org/10.1093/mnras/stv1315

We present predictions for the two-point correlation function of galaxy clustering as a function of stellar mass, computed using two new versions of the GALFORM semi-analytic galaxy formation model. These models make use of a high resolution, large v... Read More about A new methodology to test galaxy formation models using the dependence of clustering on stellar mass.

The star formation and AGN luminosity relation: predictions from a semi-analytical model (2015)
Journal Article
Gutcke, T., Fanidakis, N., Macciò, A., & Lacey, C. (2015). The star formation and AGN luminosity relation: predictions from a semi-analytical model. Monthly Notices of the Royal Astronomical Society, 451(4), 3759-3767. https://doi.org/10.1093/mnras/stv1205

In a universe where active galactic nucleus (AGN) feedback regulates star formation in massive galaxies, a strong correlation between these two quantities is expected. If the gas causing star formation is also responsible for feeding the central blac... Read More about The star formation and AGN luminosity relation: predictions from a semi-analytical model.

Constraining the properties of AGN host galaxies with spectral energy distribution modelling (2015)
Journal Article
Ciesla, L., Charmandaris, V., Georgakakis, A., Bernhard, E., Mitchell, P., Buat, V., …Xilouris, M. (2015). Constraining the properties of AGN host galaxies with spectral energy distribution modelling. Astronomy & Astrophysics, 576, Article A10. https://doi.org/10.1051/0004-6361/201425252

Detailed studies of the spectral energy distribution (SED) of normal galaxies have increasingly been used to understand the physical mechanism dominating their integrated emission, mainly owing to the availability of high quality multi-wavelength dat... Read More about Constraining the properties of AGN host galaxies with spectral energy distribution modelling.

The 0.1 < z < 1.65 evolution of the bright end of the OII luminosity function (2015)
Journal Article
Comparat, J., Richard, J., Kneib, J., Ilbert, O., Gonzalez-Perez, V., Tresse, L., …Zou, H. (2015). The 0.1 < z < 1.65 evolution of the bright end of the OII luminosity function. Astronomy & Astrophysics, 575, Article A40. https://doi.org/10.1051/0004-6361/201424767

We present the [Oii] (λλ3729,3726) luminosity function measured in the redshift range 0.1

The origin of the atomic and molecular gas contents of early-type galaxies - II. Misaligned gas accretion (2015)
Journal Article
Lagos, C. D. P., Padilla, N., Davis, T., Lacey, C., Baugh, C., Gonzalez-Perez, V., …Contreras, S. (2015). The origin of the atomic and molecular gas contents of early-type galaxies - II. Misaligned gas accretion. Monthly Notices of the Royal Astronomical Society, 448(2), 1271-1287. https://doi.org/10.1093/mnras/stu2763

We study the origin of the wide distribution of angles between the angular momenta of the stellar and gas components, αG, S, in early-type galaxies (ETGs). We use the GALFORM model of galaxy formation, set in the Λ cold dark matter framework, and cou... Read More about The origin of the atomic and molecular gas contents of early-type galaxies - II. Misaligned gas accretion.

The environments of Ly α blobs I: Wide-field Ly α imaging of TN J1338-1942, a powerful radio galaxy at z ≃ 4.1 associated with a giant Ly α nebula (2015)
Journal Article
Saito, T., Matsuda, Y., Lacey, C., Smail, I., Orsi, A., Baugh, C., …Taniguchi, Y. (2015). The environments of Ly α blobs I: Wide-field Ly α imaging of TN J1338-1942, a powerful radio galaxy at z ≃ 4.1 associated with a giant Ly α nebula. Monthly Notices of the Royal Astronomical Society, 447(4), 3069-3086. https://doi.org/10.1093/mnras/stu2538

We exploit wide-field Ly α imaging with Subaru to probe the environment around TN J1338−1942, a powerful radio galaxy with a > 100 kpc Ly α halo at z = 4.11. We used a sample of Ly α emitters (LAEs) down to log (LLyα[ erg s−1]) ∼ 42.8 to measure the... Read More about The environments of Ly α blobs I: Wide-field Ly α imaging of TN J1338-1942, a powerful radio galaxy at z ≃ 4.1 associated with a giant Ly α nebula.

Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation (2015)
Journal Article
Béthermin, M., Daddi, E., Magdis, G., Lagos, C., Sargent, M., Albrecht, M., …Viero, M. (2015). Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation. Astronomy & Astrophysics, 573, Article A113. https://doi.org/10.1051/0004-6361/201425031

We aim to measure the average dust and molecular gas content of massive star-forming galaxies (>3 × 1010M⊙) up to z = 4 in the COSMOS field to determine if the intense star formation observed at high redshift is induced by major mergers or is caused... Read More about Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation.

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