Search Publications

The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates
DOI: 10.3847/1538-4365/ab23f2 Bibcode: 2019ApJS..243...22B

Barro, Guillermo; Pérez-González, Pablo G.; Castellano, Marco +52 more

We present a WFC3 F160W (H-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts, and stellar parameters derived from the analysis of the multiwavelength data. The catalog contains 35,445 sources over the 171 arcmin2 of the CANDELS F160W mosaic…

2019 The Astrophysical Journal Supplement Series
Herschel eHST 161
The Hubble Legacy Field GOODS-S Photometric Catalog
DOI: 10.3847/1538-4365/ab3853 Bibcode: 2019ApJS..244...16W

Franx, Marijn; Mowla, Lamiya; Labbé, Ivo +12 more

This manuscript describes the public release of the Hubble Legacy Fields (HLF) project photometric catalog for the extended GOODS-South region from the Hubble Space Telescope (HST) archival program AR-13252. The analysis is based on the version 2.0 HLF data release that now includes all ultraviolet (UV) imaging, combining three major UV surveys. T…

2019 The Astrophysical Journal Supplement Series
Gaia eHST 119
Microlensing Optical Depth and Event Rate toward the Galactic Bulge from 8 yr of OGLE-IV Observations
DOI: 10.3847/1538-4365/ab426b Bibcode: 2019ApJS..244...29M

Udalski, Andrzej; Mróz, Przemek; Szymański, Michał K. +9 more

The number and properties of observed gravitational microlensing events depend on the distribution and kinematics of stars and other compact objects along the line of sight. In particular, precise measurements of the microlensing optical depth and event rate toward the Galactic bulge enable strict tests of competing models of the Milky Way. Previo…

2019 The Astrophysical Journal Supplement Series
Gaia eHST 89
Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS). I. Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation Properties for ∼700 Galaxies at z = 0.5-6
DOI: 10.3847/1538-4365/ab42da Bibcode: 2019ApJS..244...40L

Bondi, M.; Magnelli, B.; Vaccari, M. +21 more

The rich information on (sub)millimeter dust continuum emission from distant galaxies in the public Atacama Large Millimeter/submillimeter Array (ALMA) archive is contained in thousands of inhomogeneous observations from individual PI-led programs. To increase the usability of these data for studies deepening our understanding of galaxy evolution,…

2019 The Astrophysical Journal Supplement Series
Herschel eHST 86
Rates and Properties of Supernovae Strongly Gravitationally Lensed by Elliptical Galaxies in Time-domain Imaging Surveys
DOI: 10.3847/1538-4365/ab1fe0 Bibcode: 2019ApJS..243....6G

Nugent, Peter E.; Goobar, Ariel; Goldstein, Daniel A.

Supernovae that are strongly gravitationally lensed (gLSNe) by elliptical galaxies are powerful probes of astrophysics and cosmology that will be discovered systematically by wide-field, high-cadence imaging surveys such as the Zwicky Transient Facility (ZTF) and the Large Synoptic Survey Telescope (LSST). Here we use pixel-level simulations that …

2019 The Astrophysical Journal Supplement Series
eHST 82
The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z ≃ 1
DOI: 10.3847/1538-4365/aafad2 Bibcode: 2019ApJS..240...33G

Chambers, Kenneth C.; Magnier, Eugene; Wright, Edward L. +23 more

We present the Massive and Distant Clusters of WISE Survey (MaDCoWS), a search for galaxy clusters at 0.7 ≲ z ≲ 1.5 based upon data from the Wide-field Infrared Survey Explorer (WISE) mission. MaDCoWS is the first cluster survey capable of discovering massive clusters at these redshifts over the full extragalactic sky. The search is divided into t…

2019 The Astrophysical Journal Supplement Series
eHST 79
Col-OSSOS: The Colors of the Outer Solar System Origins Survey
DOI: 10.3847/1538-4365/ab2194 Bibcode: 2019ApJS..243...12S

Wang, Shiang-Yu; Marsset, Michaël; Fraser, Wesley C. +15 more

The Colours of the Outer Solar System Origins Survey is acquiring near-simultaneous g, r, and J photometry of unprecedented precision with the Gemini North Telescope, targeting nearly 100 trans-Neptunian objects (TNOs) brighter than m r = 23.6 mag discovered in the Outer Solar System Origins Survey. Combining the optical and near-infr…

2019 The Astrophysical Journal Supplement Series
eHST 47
Transition Probabilities of Sc I and Sc II and Scandium Abundances in the Sun, Arcturus, and HD 84937
DOI: 10.3847/1538-4365/ab08ef Bibcode: 2019ApJS..241...21L

Sneden, C.; Wood, M. P.; Lawler, J. E. +3 more

New branching fraction (BF) measurements for lines of Sc I and Sc II from 24 Fourier transform spectra calibrated using standard lamps and the Ar branching ratio method are reported. The BFs for 259 lines are converted to absolute atomic transition probabilities using published radiative lifetimes from laser-induced fluorescence measurements. Deta…

2019 The Astrophysical Journal Supplement Series
eHST 43
A Census of Early-phase High-mass Star Formation in the Central Molecular Zone
DOI: 10.3847/1538-4365/ab4258 Bibcode: 2019ApJS..244...35L

Ott, Jürgen; Lu, Xing; Henshaw, Jonathan D. +13 more

We present new observations of the C-band continuum emission and masers to assess high-mass (>8 {M}) star formation at early evolutionary phases in the inner 200 pc of the Central Molecular Zone (CMZ) of the Galaxy. The continuum observation is complete to free-free emission from stars above 10-11 {M} in 91% of the cov…

2019 The Astrophysical Journal Supplement Series
Gaia eHST 41
Subpercent Photometry: Faint DA White Dwarf Spectrophotometric Standards for Astrophysical Observatories
DOI: 10.3847/1538-4365/ab0557 Bibcode: 2019ApJS..241...20N

Rest, Armin; Matheson, Thomas; Points, Sean +18 more

We have established a network of 19 faint (16.5 mag < V < 19 mag) northern and equatorial DA white dwarfs (WDs) as spectrophotometric standards for present and future wide-field observatories. Our analysis infers spectral energy distribution (SED) models for the stars that are tied to the three CALSPEC primary standards. Our SED models are c…

2019 The Astrophysical Journal Supplement Series
Gaia eHST 39