most citedAre high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties

113 citations · 258 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA201739 cited

An alternate approach to measure specific star formation rates at 2<z<7

Iary Davidzon, Olivier Ilbert, Andreas L. Faisst +2

We trace the specific star formation rate (sSFR) of massive star-forming galaxies () from to 7. Our method is substantially different…

astro-ph.GA201744 cited

Predicting Hα emission line galaxy counts for future galaxy redshift surveys

Alexander Merson, Yun Wang, Andrew Benson +4

Knowledge of the number density of H emitting galaxies is vital for assessing the scientific impact of the Euclid and WFIRST missions. In this work we present predictions from a…

astro-ph.GA2017113 cited

Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties

Andreas L. Faisst, Peter L. Capak, Lin Yan +6

Recent studies have found a significant evolution and scatter in the IRX- relation at z > 4, suggesting different dust properties of these galaxies. The total far-infrared (FIR)…

astro-ph.GA201762 cited

Dust Properties of [CII] Detected z 5.5 Galaxies: New HST/WFC3 Near-IR Observations

Ivana Barišić, Andreas L. Faisst, Peter L. Capak +7

We examine the rest-frame ultra-violet (UV) properties of 10 [CII]detected galaxies at in COSMOS using new HST/WFC3 near-infrared imaging. Toget…

astro-ph.GA2016

Effects of Local Environment and Stellar Mass on Galaxy Quenching out to z~3

Behnam Darvish, Bahram Mobasher, David Sobral +4

We study the effects of local environment and stellar mass on galaxy properties using a mass complete sample of quiescent and star-forming systems in the COSMOS field at $z\lesssim…