activity
19972021
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 24.5k across the 211 of their papers we have counts for

collaborators

208 papers

astro-ph.GA2021★ 7 cited

Molecular Gas Excitation of the Massive Dusty Starburst CRLE and the Main-Sequence Galaxy HZ10 at z=5.7 in the COSMOS Field

Daniel Vieira, Dominik A. Riechers, Riccardo Pavesi +4

We report CO(54) and CO(65) line observations in the dusty starbursting galaxy CRLE () and the main-sequence (MS) galaxy HZ10 () wit…

astro-ph.GA2021★ 13 cited

The Physical Drivers of the Luminosity-Weighted Dust Temperatures in High-Redshift Galaxies

Anne D. Burnham, Caitlin M. Casey, Jorge A. Zavala +7

The underlying distribution of galaxies' dust SEDs (i.e., their spectra re-radiated by dust from rest-frame 3m-3mm) remains relatively unconstrained due to a dearth of FIR…

astro-ph.GA2020★ 27 cited

Dependence of the IRX- dust attenuation relation on metallicity and environment

Irene Shivaei, Behnam Darvish, Zahra Sattari +4

We use a sample of star-forming field and protocluster galaxies at z=2.0-2.5 with Keck/MOSFIRE K-band spectra, a wealth of rest-frame UV photometry, and Spitzer/MIPS and Herschel/P…

astro-ph.GA2020★ 99 cited

ALMA Characterises the Dust Temperature of z ~ 5.5 Star-Forming Galaxies

Andreas L. Faisst, Yoshinobu Fudamoto, Pascal A. Oesch +4

The infrared spectral energy distributions (SEDs) of main-sequence galaxies in the early universe (z > 4) is currently unconstrained as infrared continuum observations are time con…

astro-ph.GA2020★ 23 cited

S2COSMOS: Evolution of Gas Mass with Redshift Using Dust Emission

Jenifer S. Millard, Stephen A. Eales, M. W. L. Smith +15

We investigate the evolution of the gas mass fraction for galaxies in the COSMOS field using submillimetre emission from dust at 850m. We use stacking methodologies on the 850$μ…

astro-ph.GA2020★ 40 cited

Spectroscopic Confirmation of a Coma Cluster Progenitor at z ~ 2.2

Behnam Darvish, Nick Z. Scoville, Christopher Martin +17

We report the spectroscopic confirmation of a new protocluster in the COSMOS field at 2.2, COSMOS Cluster 2.2 (CC2.2), originally identified as an overdensity of narrowb…