442 citations · 2.1k across the 21 of their papers we have counts for
22 papers
Quantifying the inside-out formation of disk galaxies at
Laura DeGroot, Swara Ravindaranath, Karmellah Buttler +1
We examine the properties of galaxies at in the Extended Groth Strip (EGS) field to explore inside-out disk growth. We take advantage of the high-resolution James…
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…
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…
The UV luminosity function at 0.6 < z < 1 from UVCANDELS
Lei Sun, Xin Wang, Harry I. Teplitz +75
UVCANDELS is a HST Cycle-26 Treasury Program awarded 164 orbits of primary ultraviolet (UV) F275W imaging and coordinated parallel optical F435W imaging in four CANDELS fields: GOO…
The Lyman Continuum Escape Fraction of Star-forming Galaxies at from UVCANDELS
Xin Wang, Harry I. Teplitz, Brent M. Smith +74
The UltraViolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) survey is a Hubble Space Telescope (HST) Cycle-26 Treasury Program,…
The MOSDEF Survey: Probing Resolved Stellar Populations at Using a New Bayesian-defined Morphology Metric Called Patchiness
Tara Fetherolf, Naveen A. Reddy, Alice E. Shapley +12
We define a new morphology metric called "patchiness" () that is sensitive to deviations from the average of a resolved distribution, does not require the galaxy center to be de…