Search Publications

COSMOS2020: A Panchromatic View of the Universe to z∼10 from Two Complementary Catalogs
DOI: 10.3847/1538-4365/ac3078 Bibcode: 2022ApJS..258...11W

Aussel, H.; Sanders, D. B.; Ilbert, O. +55 more

The Cosmic Evolution Survey (COSMOS) has become a cornerstone of extragalactic astronomy. Since the last public catalog in 2015, a wealth of new imaging and spectroscopic data have been collected in the COSMOS field. This paper describes the collection, processing, and analysis of these new imaging data to produce a new reference photometric redsh…

2022 The Astrophysical Journal Supplement Series
Gaia eHST 354
GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with 4,000,000 Galaxies at z 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10
DOI: 10.3847/1538-4365/ac3dfc Bibcode: 2022ApJS..259...20H

Ono, Yoshiaki; Ouchi, Masami; Willott, Chris J. +16 more

We present new measurements of rest-UV luminosity functions and angular correlation functions from 4,100,221 galaxies at z ~ 2-7 identified in the Subaru/Hyper Suprime-Cam survey and CFHT Large Area U-band Survey. The obtained luminosity functions at z ~ 4-7 cover a very wide UV luminosity range of ~ $0.002\mbox{--}2000{L}_{\mathrm{UV}}^{* }$ comb…

2022 The Astrophysical Journal Supplement Series
eHST 184
The Low-redshift Lyman Continuum Survey. I. New, Diverse Local Lyman Continuum Emitters
DOI: 10.3847/1538-4365/ac5331 Bibcode: 2022ApJS..260....1F

Papovich, Casey; Finkelstein, Steven L.; Santini, Paola +44 more

The origins of Lyman continuum (LyC) photons responsible for the reionization of the universe are as of yet unknown and highly contested. Detecting LyC photons from the Epoch of Reionization is not possible due to absorption by the intergalactic medium, which has prompted the development of several indirect diagnostics to infer the rate at which g…

2022 The Astrophysical Journal Supplement Series
eHST 151
The PHANGS-HST Survey: Physics at High Angular Resolution in Nearby Galaxies with the Hubble Space Telescope
DOI: 10.3847/1538-4365/ac1fe5 Bibcode: 2022ApJS..258...10L

White, Richard L.; Henshaw, Jonathan D.; Kruijssen, J. M. Diederik +52 more

The PHANGS program is building the first data set to enable the multiphase, multiscale study of star formation across the nearby spiral galaxy population. This effort is enabled by large survey programs with the Atacama Large Millimeter/submillimeter Array (ALMA), MUSE on the Very Large Telescope, and the Hubble Space Telescope (HST), with which w…

2022 The Astrophysical Journal Supplement Series
Gaia eHST 112
The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas
DOI: 10.3847/1538-4365/ac6c03 Bibcode: 2022ApJS..261...31B

Ouchi, Masami; Kewley, Lisa J.; Ravindranath, Swara +46 more

Far-ultraviolet (FUV; ~1200-2000 Å) spectra are fundamental to our understanding of star-forming galaxies, providing a unique window on massive stellar populations, chemical evolution, feedback processes, and reionization. The launch of the James Webb Space Telescope will soon usher in a new era, pushing the UV spectroscopic frontier to higher red…

2022 The Astrophysical Journal Supplement Series
IUE eHST 86
Five Key Exoplanet Questions Answered via the Analysis of 25 Hot-Jupiter Atmospheres in Eclipse
DOI: 10.3847/1538-4365/ac5cc2 Bibcode: 2022ApJS..260....3C

Tsiaras, A.; Waldmann, I. P.; Tinetti, G. +11 more

Population studies of exoplanets are key to unlocking their statistical properties. So far, the inferred properties have been mostly limited to planetary, orbital, and stellar parameters extracted from, e.g., Kepler, radial velocity, and Gaia data. More recently an increasing number of exoplanet atmospheres have been observed in detail from space …

2022 The Astrophysical Journal Supplement Series
eHST 74
ALMA Lensing Cluster Survey: Hubble Space Telescope and Spitzer Photometry of 33 Lensed Fields Built with CHArGE
DOI: 10.3847/1538-4365/ac9909 Bibcode: 2022ApJS..263...38K

Magdis, G. E.; Wang, T.; Bauer, F. E. +30 more

We present a set of multiwavelength mosaics and photometric catalogs in the Atacama Large Millimeter/submillimeter Array (ALMA) lensing cluster survey fields. The catalogs were built by the reprocessing of archival data from the Complete Hubble Archive for Galaxy Evolution compilation, taken by the Hubble Space Telescope (HST) in the Reionization …

2022 The Astrophysical Journal Supplement Series
Gaia eHST 60
The R-process Alliance: A Nearly Complete R-process Abundance Template Derived from Ultraviolet Spectroscopy of the R-process-enhanced Metal-poor Star HD 222925
DOI: 10.3847/1538-4365/ac5cbc Bibcode: 2022ApJS..260...27R

Beers, Timothy C.; Placco, Vinicius M.; Hattori, Kohei +9 more

We present a nearly complete rapid neutron-capture process (r-process) chemical inventory of the metal-poor ([Fe/H] = -1.46 ± 0.10) r-process-enhanced ([Eu/Fe] = +1.32 ± 0.08) halo star HD 222925. This abundance set is the most complete for any object beyond the solar system, with a total of 63 metals detected and seven with upper limits. It compr…

2022 The Astrophysical Journal Supplement Series
Gaia eHST 50
BASS. XXI. The Data Release 2 Overview
DOI: 10.3847/1538-4365/ac6c8f Bibcode: 2022ApJS..261....1K

Lamperti, Isabella; Cenko, S. Bradley; Schawinski, Kevin +24 more

The BAT AGN Spectroscopic Survey (BASS) is designed to provide a highly complete census of the key physical parameters of the supermassive black holes (SMBHs) that power local active galactic nuclei (AGNs) (z ≲ 0.3), including their bolometric luminosity (L bol), black hole (BH) mass (M BH), accretion rates (L bol/…

2022 The Astrophysical Journal Supplement Series
eHST 47
CLASSY. II. A Technical Overview of the COS Legacy Archive Spectroscopic Survey
DOI: 10.3847/1538-4365/ac8008 Bibcode: 2022ApJS..262...37J

Ouchi, Masami; Kewley, Lisa J.; Ravindranath, Swara +43 more

The COS Legacy Archive Spectroscopic SurveY (CLASSY) is designed to provide the community with a spectral atlas of 45 nearby star-forming galaxies that were chosen to cover similar properties to those seen at high z (z > 6). The prime high-level science product of CLASSY is accurately coadded UV spectra, ranging from ~1000 to 2000 Å, derived fr…

2022 The Astrophysical Journal Supplement Series
eHST 33