papers

Publications (36)

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.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.GA2016

Breaking the Curve with CANDELS: A Bayesian Approach to Reveal the Non-Universality of the Dust-Attenuation Law at High Redshift

Brett Salmon, Casey Papovich, James Long +13

Dust attenuation affects nearly all observational aspects of galaxy evolution, yet very little is known about the form of the dust-attenuation law in the distant Universe. Here, we…

astro-ph.GA2026

Resolving galaxy formation in the early Universe with BonFIRE and CampFIRE

Jenna Samuel, Michael Boylan-Kolchin, Robert Feldmann +16

The abundance and rapid growth of galaxies at cosmic dawn revealed by the James Webb Space Telescope challenges models of galaxy formation, motivating new simulations to uncover th…

astro-ph.GA2025

Mysteries of Capotauro: investigating the puzzling nature of an extreme F356W-dropout

Giovanni Gandolfi, Giulia Rodighiero, Marco Castellano +38

JWST has uncovered a diverse population of extreme near-infrared dropouts, including ultra high-redshift () galaxy candidates, dust-obscured galaxies challenging dust product…

astro-ph.GA2025

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.GA2026

Near-infrared emission line diagnostics for AGN from the local Universe to redshift 3

Antonello Calabrò, Laura Pentericci, Anna Feltre +35

Optical rest-frame spectroscopic diagnostics are usually employed to distinguish between star formation and AGN-powered emission. However, this method is biased against dusty sourc…

astro-ph2008

The Expected Detection of Dust Emission from High-Redshift Lyman Alpha Galaxies

Steven Finkelstein, Sangeeta Malhotra, James Rhoads +2

Recent results have shown that a substantial fraction of high-redshift Lyman alpha galaxies contain considerable amounts of dust. This implies that Lyman alpha galaxies are not pri…

astro-ph.GA2019

Lyman continuum observations across cosmic time: recent developments, future requirements

Stephan R. McCandliss, Daniela Calzetti, Henry C. Ferguson +19

Quantifying the physical conditions that allow radiation emitted shortward of the hydrogen ionization edge at 911.7 Ã to escape the first collapsed objects and ultimately reionize…

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.GA2023

CEERS: 7.7 m PAH Star Formation Rate Calibration with JWST MIRI

Kaila Ronayne, Casey Papovich, Guang Yang +33

We test the relationship between UV-derived star formation rates (SFRs) and the 7.7 m polycyclic aromatic hydrocarbon (PAH) luminosities from the integrated emission of galaxie…

astro-ph.CO2009

Paschen-alpha Emission in the Gravitationally Lensed Galaxy SMM J163554.2+661225

Casey Papovich, Gregory Rudnick, Jane Rigby +5

We report the detection of the Paschen-alpha emission line in the z=2.515 galaxy SMM J163554.2+661225 using Spitzer spectroscopy. SMM J163554.2+661225 is a sub-millimeter-selected…

astro-ph.GA2017

UVUDF: UV Luminosity Functions at the cosmic high-noon

Vihang Mehta, Claudia Scarlata, Marc Rafelski +14

We present the rest-1500Ã UV luminosity functions (LF) for star-forming galaxies during the cosmic \textit{high noon} -- the peak of cosmic star formation rate at . We use…

astro-ph.IM2019

Another Servicing Mission to Extend Hubble Space Telescope's Science past the Next Decade

Mercedes López-Morales, Kevin France, Francesco R. Ferraro +17

The Hubble Space Telescope has produced astonishing science over the past thirty years. Hubble's productivity can continue to soar for years to come provided some worn out componen…

astro-ph.GA2019

Cosmic Dawn and Reionization: Astrophysics in the Final Frontier

Asantha Cooray, James Aguirre, Yacine Ali-Haimoud +71

The cosmic dawn and epoch of reionization mark the time period in the universe when stars, galaxies, and blackhole seeds first formed and the intergalactic medium changed from neut…

astro-ph.CO2012

Metallicities of Emission-Line Galaxies from HST ACS PEARS and HST WFC3 ERS Grism Spectroscopy at 0.6 < z < 2.4

Lifang Xia, Sangeeta Malhotra, James Rhoads +9

Galaxies selected on the basis of their emission line strength show low metallicities, regardless of their redshifts. We conclude this from a sample of faint galaxies at redshifts…

astro-ph.GA2019

Astro2020 Science White Paper: Synergies Between Galaxy Surveys and Reionization Measurements

Steven Furlanetto, Adam Beardsley, Chris L. Carilli +47

The early phases of galaxy formation constitute one of the most exciting frontiers in astrophysics. It is during this era that the first luminous sources reionize the intergalactic…

astro-ph.GA2018

CLEAR I: Ages and Metallicities of Quiescent Galaxies at Derived from Deep Hubble Space Telescope Grism Data

Vicente Estrada-Carpenter, Casey Papovich, Ivelina Momcheva +14

We use deep \textit{Hubble Space Telescope} spectroscopy to constrain the metallicities and (\editone{light-weighted}) ages of massive () galaxies sel…

astro-ph.CO2019

Astro2020 Science White Paper: A proposal to exploit galaxy-21cm synergies to shed light on the Epoch of Reionization

Anne Hutter, Pratika Dayal, Sangeeta Malhotra +26

This white paper highlights the crucial and urgent synergies required between WFIRST, Subaru Hyper Suprime-Cam or other >25m-class telescopes galaxy observations and SKA 21cm measu…

astro-ph.CO2013

Galaxy redshift surveys with sparse sampling

Chi-Ting Chiang, Philipp Wullstein, Donghui Jeong +16

Survey observations of the three-dimensional locations of galaxies are a powerful approach to measure the distribution of matter in the universe, which can be used to learn about t…

astro-ph.CO2015

Ultraviolet Luminosity Density of the Universe During the Epoch of Reionization

Ketron Mitchell-Wynne, Asantha Cooray, Yan Gong +9

The spatial fluctuations of the extragalactic background light trace the total emission from all stars and galaxies in the Universe. A multi-wavelength study can be used to measure…

astro-ph.GA2021

HETDEX [OIII] Emitters I: A spectroscopically selected low-redshift population of low-mass, low-metallicity galaxies

Briana Indahl, Greg Zeimann, Gary J. Hill +16

We assemble a sample of 17 low metallicity (7.45 < log(O/H)+12 < 8.12) galaxies with z < 0.1 found spectroscopically, without photometric pre-selection, in early data from the Hobb…

astro-ph.GA2024

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,…

astro-ph.HE2023

Roman CCS White Paper: Identifying high-redshift pair-instability supernovae by adding sparse F213 filter observations

Takashi Moriya, Ori D. Fox, Robert Quimby +22

Pair-instability supernovae (PISNe) are explosions of very massive stars that may have played a critical role in the chemical evolution and reionization of the early Universe. In o…

astro-ph.GA2014

Herschel Extreme Lensing Line Observations: Dynamics of two strongly lensed star forming galaxies near redshift z = 2

James E. Rhoads, Sangeeta Malhotra, Sahar Allam +11

We report on two regularly rotating galaxies at redshift z=2, using high resolution spectra of the bright [CII] 158 micron emission line from the HIFI instrument on the Herschel Sp…

astro-ph.GA2018

The Spitzer-HETDEX Exploratory Large Area Survey II: Dark Energy Camera and Spitzer/IRAC Multiwavelength Catalog

Isak Wold, Lalitwadee Kawinwanichakij, Matthew Stevans +15

We present the -band Dark Energy Camera (DECam) plus 3.6 and 4.5 m IRAC catalogs for the Spitzer/HETDEX Exploratory Large-Area (SHELA) survey. SHELA covers deg$…

astro-ph.GA2018

Spectrophotometric Redshifts In The Faint Infrared Grism Survey: Finding Overdensities Of Faint Galaxies

John Pharo, Sangeeta Malhotra, James Rhoads +19

We improve the accuracy of photometric redshifts by including low-resolution spectral data from the G102 grism on the Hubble Space Telescope, which assists in redshift determinatio…

astro-ph.GA2024

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…

astro-ph.GA2023

The Spitzer-HETDEX Exploratory Large Area Survey. IV. Model-Based Multi-wavelength Photometric Catalog

Gene C. K. Leung, Steven Finkelstein, John Weaver +11

We present a 0.3--4.5 m 16-band photometric catalog for the Spitzer/HETDEX Exploratory Large-Area (SHELA) survey. SHELA covers a deg field within the footprint of…

astro-ph.GA2021

The mass-metallicity relation at z~1-2 and its dependence on star formation rate

Alaina Henry, Marc Rafelski, Ben Sunnquist +24

We present a new measurement of the gas-phase mass-metallicity relation (MZR), and its dependence on star formation rates (SFRs) at 1.3 < z < 2.3. Our sample comprises 1056 galaxie…

astro-ph.GA2017

First Spectroscopic Confirmations of z ~ 7.0 Lya Emitting Galaxies in the LAGER Survey

Weida Hu, Junxian Wang, Zhenya Zheng +16

Narrowband imaging is a highly successful approach for finding large numbers of high redshift Lya emitting galaxies (LAEs) up to z~6.6. However, at z>~7 there are as yet only 3 nar…

astro-ph.IM2019

The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s

Rachel Akeson, Lee Armus, Etienne Bachelet +103

The Wide Field Infrared Survey Telescope (WFIRST) is a 2.4m space telescope with a 0.281 deg^2 field of view for near-IR imaging and slitless spectroscopy and a coronagraph designe…

astro-ph.GA2016

Large Molecular Gas Reservoirs in Ancestors of Milky Way-Mass Galaxies 9 Billion Years Ago

Casey Papovich, Ivo Labbé, Karl Glazebrook +10

The gas accretion and star-formation histories of galaxies like the Milky Way remain an outstanding problem in astrophysics. Observations show that 8 billion years ago, the progeni…

astro-ph.GA2026

The Growth of Dust in Galaxies in the First Billion Years with Applications to Blue Monsters

Desika Narayanan, Paul Torrey, Daniel Stark +9

A combination of JWST observations at z~12-14 and ALMA observations of extremely dust-rich systems at z~6 has demonstrated that dust grows extremely fast in the early Universe, wit…

astro-ph.GA2023

Identifying Active Galactic Nuclei at from the HETDEX Survey Using Machine Learning

Valentina Tardugno Poleo, Steven Finkelstein, Gene C. K. Leung +9

We used data from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) to study the incidence of AGN in continuum-selected galaxies at . From optical and infrared ima…

astro-ph.GA2019

Taking Census of Massive, Star-Forming Galaxies formed <1 Gyr After the Big Bang

Caitlin M. Casey, Peter Capak, Johannes Staguhn +24

Two decades of effort have been poured into both single-dish and interferometric millimeter-wave surveys of the sky to infer the volume density of dusty star-forming galaxies (DSFG…