activity
19972021
most citedGalaxy Luminosity Functions to z~1: DEEP2 vs. COMBO-17 and Implications for Red Galaxy Formation

1.1k citations · 5k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2021★ 14 cited

Supernovae Shock Breakout/Emergence Detection Predictions for a Wide-Field X-ray Survey

Amanda J. Bayless, Chris Fryer, Peter J. Brown +7

There are currently many large-field surveys operational and planned including the powerful Vera C. Rubin Observatory Legacy Survey of Space and Time. These surveys will increase t…

astro-ph.CO2013★ 42 cited

X-Ray Groups of Galaxies in the Aegis Deep and Wide Fields

G. Erfanianfar, A. Finoguenov, M. Tanaka +19

We present the results of a search for extended X-ray sources and their corresponding galaxy groups from 800-ks Chandra coverage of the All-wavelength Extended Groth Strip Internat…

astro-ph.CO2013★ 78 cited

Towards a resolved Kennicutt-Schmidt law at high redshift

J. Freundlich, F. Combes, L. J. Tacconi +16

Massive galaxies in the distant Universe form stars at much higher rates than today. Although direct resolution of the star forming regions of these galaxies is still a challenge,…

astro-ph.GA2012★ 242 cited

The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5<z< 0.8 in the DEEP2/AEGIS Survey

Edmond Cheung, S. M. Faber, David C. Koo +25

The shutdown of star formation in galaxies is generally termed `quenching'. Although quenching may occur through a variety of processes, the exact mechanism(s) that is in fact resp…

astro-ph.CO2011★ 293 cited

The metallicity dependence of the CO {\rightarrow} H_2 conversion factor in z>1 star forming galaxies

R. Genzel, L. J. Tacconi, F. Combes +20

We use the first systematic samples of CO millimeter emission in z>1 'main-sequence' star forming galaxies (SFGs) to study the metallicity dependence of the conversion factor αCO,…

astro-ph.CO2010★ 957 cited

A Study of the Gas-Star Formation Relation over Cosmic Time

R. Genzel, L. J. Tacconi, J. Gracia-Carpio +19

We use the first systematic data sets of CO molecular line emission in z~1-3 normal star forming galaxies for a comparison of the dependence of galaxy-averaged star formation rates…