activity
20132026
most citedThe COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies

1.2k citations · 9.4k across the 107 of their papers we have counts for

collaborators
Showing 2022Show all

12 papers · 1 filter

astro-ph.GA2022★ 16 cited

Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function

Juhan Kim, Jaehyun Lee, Clotilde Laigle +8

We investigate the impact of the surface brightness (SB) limit on the galaxy stellar mass functions (GSMFs) using mock surveys generated from the Horizon Run 5 (HR5) simulation. We…

astro-ph.IM2022★ 211 cited

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Shoko Jin, Scott C. Trager, Gavin B. Dalton +212

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree…

astro-ph.GA2022★ 193 cited

COSMOS2020: The Galaxy Stellar Mass Function: the assembly and star formation cessation of galaxies at

J. R. Weaver, I. Davidzon, S. Toft +30

How galaxies form, assemble, and cease their star-formation is a central question within the modern landscape of galaxy evolution studies. These processes are indelibly imprinted o…

astro-ph.GA2022

Evolution of Gas, and Star Formation from z = 0 to 5

Nick Scoville, Andreas Faisst, John Weaver +20

ALMA observations of the long wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming (SF) galaxies at z = 0.3 to 4.5. We determine the depend…

astro-ph.GA2022★ 13 cited

COSMOS-Web: An Overview of the JWST Cosmic Origins Survey

Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos +82

We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations…

astro-ph.GA2022★ 29 cited

COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys

I. Davidzon, K. Jegatheesan, O. Ilbert +16

We present a novel method to estimate galaxy physical properties from spectral energy distributions (SEDs), alternate to template fitting techniques and based on self-organizing ma…