activity
20062022
most citedThe Cosmic Evolution Survey (COSMOS) -- Overview

2k citations · 3k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2022★ 6 cited

ALPINE: A Large Survey to Understand Teenage Galaxies

A. L. Faisst, L. Yan, M. Béthermin +13

A multiwavelength study of galaxies is important to understand their formation and evolution. Only in the recent past, thanks to the Atacama Large (Sub) Millimeter Array (ALMA), we…

astro-ph.GA2021★ 14 cited

Ionizing radiation from AGNs at z>3.3 with the Subaru Hyper Suprime-Cam Survey and the CFHT Large Area U-band Deep Survey (CLAUDS)

Ikuru Iwata, Marcin Sawicki, Akio K. Inoue +8

We use deep and wide imaging data from the CFHT Large Area U-band Deep Survey (CLAUDS) and the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) to constrain the ionizing radiat…

astro-ph.GA2019★ 113 cited

The CFHT Large Area U-band Deep Survey (CLAUDS)

Marcin Sawicki, Stephane Arnouts, Jiasheng Huang +37

The CFHT Large Area U-band Deep Survey (CLAUDS) uses data taken with the MegaCam mosaic imager on CFHT to produce images of 18.60 deg2 with median seeing of FWHM=0.92 arcsec and to…

astro-ph.GA2016★ 105 cited

Gas Fraction and Depletion Time of Massive Star Forming Galaxies at z~3.2: No Change in Global Star Formation Process out to z>3

E. Schinnerer, B. Groves, M. T. Sargent +8

The observed evolution of the gas fraction and its associated depletion time in main sequence (MS) galaxies provides insights on how star formation proceeds over cosmic time. We re…

astro-ph2008★ 191 cited

Photometric redshifts in the SWIRE Survey

Michael Rowan-Robinson, Tom Babbedge, Seb Oliver +14

We present the SWIRE Photometric Redshift Catalogue, 1025119 redshifts of unprecedented reliability and accuracy. Our method is based on fixed galaxy and QSO templates applied to d…

astro-ph2006★ 151 cited

Photometric Redshifts of Galaxies in COSMOS

B. Mobasher, P. Capak, N. Z. Scoville +26

We measure photometric redshifts and spectral types for galaxies in the COSMOS survey. We use template fitting technique combined with luminosity function priors and with the optio…