activity
20122026
most citedA CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars

365 citations · 3.9k across the 78 of their papers we have counts for

collaborators
Showing 2020Show all

5 papers · 1 filter

astro-ph.GA2020★ 26 cited

JWST/MIRI Simulated Imaging: Insights into Obscured Star-Formation and AGN for Distant Galaxies in Deep Surveys

Guang Yang, Casey Papovich, Micaela B. Bagley +13

The JWST MIRI instrument will revolutionize extragalactic astronomy with unprecedented sensitivity and angular resolution in mid-IR. Here, we assess the potential of MIRI photometr…

astro-ph.GA2020★ 77 cited

CLEAR: The Gas-Phase Metallicity Gradients of Star-Forming Galaxies at 0.6 < z < 2.6

Raymond C. Simons, Casey Papovich, Ivelina Momcheva +11

We report on the gas-phase metallicity gradients of a sample of 264 star-forming galaxies at 0.6 < z < 2.6, measured through deep near-infrared Hubble Space Telescope slitless spec…

astro-ph.GA2020★ 143 cited

Texas Spectroscopic Search for Ly Emission at the End of Reionization III. the Ly Equivalent-width Distribution and Ionized Structures at

Intae Jung, Steven L. Finkelstein, Mark Dickinson +11

Ly emission from galaxies can be utilized to characterize the ionization state in the intergalactic medium (IGM). We report our search for Ly emission at using a compre…

astro-ph.GA2020★ 24 cited

CLEAR: Paschen- Star Formation Rates and Dust Attenuation of Low Redshift Galaxies

Nikko J. Cleri, Jonathan R. Trump, Bren E. Backhaus +12

We use \Pab\ (1282~nm) observations from the Hubble Space Telescope ($\HST$) G141 grism to study the star-formation and dust attenuation properties of a sample of 29 low-redshift (…

astro-ph.GA2020★ 59 cited

CLEAR II: Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift

Vicente Estrada-Carpenter, Casey Papovich, Ivelina Momcheva +11

The origin of the correlations between mass, morphology, quenched fraction, and formation history in galaxies is difficult to define, primarily due to the uncertainties in galaxy s…