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19932026
most citedThe Spectral Energy Distribution of Fermi bright blazars

1k citations · 12.5k across the 215 of their papers we have counts for

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Showing 2024Show all

7 papers · 1 filter

astro-ph.GA2024

Deep Swift/UVOT Observations of GOODS-N and the Evolution of the Ultraviolet Luminosity Function at 0.2<z<1.2

Alexander Belles, Caryl Gronwall, Michael H. Siegel +2

We present Swift Ultraviolet Optical Telescope (UVOT) observations of the deep field GOODS-N in four near-UV filters. A catalog of detected galaxies is reported, which will be used…

astro-ph.GA2024★ 5 cited

Quenching of Galaxies at Cosmic Noon: Understanding the Effect of Environment

Akriti Singh, Lucia Guaita, Pascale Hibon +16

The aim of this study is to identify quiescent galaxies in the 2-deg COSMOS field at and analyze their environment. Using data from the ODIN survey and COSMOS2020…

astro-ph.GA2024

ODIN: Strong Clustering of Protoclusters at Cosmic Noon

Vandana Ramakrishnan, Kyoung-Soo Lee, Nicole Firestone +15

The One-hundred-deg DECam Imaging in Narrowbands (ODIN) survey is carrying out a systematic search for protoclusters during Cosmic Noon, using Ly-emitting galaxies (LAEs) as…

astro-ph.GA2024

UVCANDELS: Catalogs of photometric redshifts and galaxy physical properties

Vihang Mehta, Marc Rafelski, Ben Sunnquist +76

The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep HST F275W and F435W imaging over four CANDELS…

astro-ph.GA2024★ 7 cited

Galaxy populations in protoclusters at cosmic noon

Moira Andrews, M. Celeste Artale, Ankit Kumar +20

We investigate the physical properties and redshift evolution of simulated galaxies residing in protoclusters at cosmic noon, to understand the influence of the environment on gala…

astro-ph.GA2024★ 1 cited

ODIN: Identifying Protoclusters and Cosmic Filaments Traced by Ly-emitting Galaxies

Vandana Ramakrishnan, Kyoung-Soo Lee, Maria Celeste Artale +22

To understand the formation and evolution of massive cosmic structures, studying them at high redshift, in the epoch when they formed the majority of their mass is essential. The O…