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20142026
most citedThe Frontier Fields: Survey Design

635 citations · 1.4k across the 25 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

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

UVCANDELS: The role of dust on the stellar mass-size relation of disk galaxies at 0.5 3.0

Kalina V. Nedkova, Marc Rafelski, Harry I. Teplitz +30

We use the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey fields (UVCANDELS) to measure half-light radii in the rest-frame far-UV for $\s…

astro-ph.GA2024★ 4 cited

Galaxy Rest-Frame UV Colors at z ~ 2-4 with HST UVCANDELS

Alexa Morales, Steven Finkelstein, Micaela Bagley +13

We present an analysis of rest-frame UV colors of 17,243 galaxies at in the HST UVCANDELS fields: GOODS-N, GOODS-S, COSMOS, and EGS. Here, we study the rest-frame UV spe…

astro-ph.EP2024

JWST/NIRCam Detection of the Fomalhaut C Debris Disk in Scattered Light

Kellen Lawson, Joshua E. Schlieder, Jarron M. Leisenring +20

Observations of debris disks offer important insights into the formation and evolution of planetary systems. Though M dwarfs make up approximately 80% of nearby stars, very few M-d…

astro-ph.GA2024

WFC3 Infrared Spectroscopic Parallel (WISP) Survey: Photometric and Emission Line Data Release

A. J. Battisti, M. B. Bagley, M. Rafelski +21

We present reduced images and catalogues of photometric and emission line data (230,000 and 8,000 sources, respectively) for the WFC3 Infrared Spectroscopic Parallel (W…

astro-ph.GA2024

Lyman Continuum Emission from AGN at 2.3z3.7 in the UVCANDELS Fields

Brent M. Smith, Rogier A. Windhorst, Harry Teplitz +19

We present the results of our search for Lyman continuum (LyC) emitting AGN at redshifts 2.3z4.9 from HST WFC3 F275W observations in the UVCANDELS fields. We al…