papers

Publications (9)

astro-ph.CO2012

Evolution of the Quasar Luminosity Function Over 3 < z < 5 in the COSMOS Survey Field

Daniel Masters, Peter Capak, Mara Salvato +10

We investigate the high-redshift quasar luminosity function (QLF) down to an apparent magnitude of I(AB) = 25 in the Cosmic Evolution Survey (COSMOS). Careful analysis of the exten…

astro-ph.GA2022

CLEAR: The Ionization and Chemical-Enrichment Properties of Galaxies at 1.1 < z < 2.3

Casey Papovich, Raymond C. Simons, Vicente Estrada-Carpenter +15

We use deep spectroscopy from the Hubble Space Telescope (HST) Wide-Field-Camera 3 (WFC3) IR grisms combined with broad-band photometry to study the stellar populations, gas ioniza…

astro-ph.GA2020

The Sloan Digital Sky Survey Reverberation Mapping Project: Photometric g and i Light Curves

K. Kinemuchi, Patrick B. Hall, Ian McGreer +28

The Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) program monitors 849 active galactic nuclei (AGN) both spectroscopically and photometrically. The photometric observati…

astro-ph.CO2014

Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS : Searching for Prompt Explosions in the Early Universe

Steven A. Rodney, Adam G. Riess, Louis-Gregory Strolger +35

The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) was a multi-cycle treasury program on the Hubble Space Telescope (HST) that surveyed a total area of ~0…

astro-ph.GA2023

CEERS MIRI Imaging: Data Reduction and Quality Assessment

Guang Yang, Casey Papovich, Micaela Bagley +35

The Cosmic Evolution Early Release Science Survey (CEERS), targeting the Extended Groth Strip extragalactic field, is one of the JWST Director's Discretionary Early Release Science…

astro-ph.GA2014

HST Emission Line Galaxies at z ~ 2: The Mystery of Neon

Gregory Zeimann, Robin Ciardullo, Henry Gebhardt +6

We use near-IR grism spectroscopy from the Hubble Space Telescope to examine the strength of [Ne~III] 3869 relative to H-beta, [O~II] 3727 and [O~III] 5007 in 236 low mass (7.5 < l…