Search Publications

Panic! at the Disks: First Rest-frame Optical Observations of Galaxy Structure at z > 3 with JWST in the SMACS 0723 Field
DOI: 10.3847/2041-8213/ac947c Bibcode: 2022ApJ...938L...2F

Wilkins, Stephen M.; Broadhurst, Tom; Frye, Brenda L. +13 more

We present early results regarding the morphological and structural properties of galaxies seen with the James Webb Space Telescope (JWST) at z > 3 in the Early Release Observations toward the SMACS 0723 cluster field. Using JWST we investigate, for the first time, the optical morphologies of a significant number of z > 3 galaxies with accur…

2022 The Astrophysical Journal
eHST JWST 125
A New Census of the 0.2 < z < 3.0 Universe. II. The Star-forming Sequence
DOI: 10.3847/1538-4357/ac887d Bibcode: 2022ApJ...936..165L

Franx, Marijn; van Dokkum, Pieter; Conroy, Charlie +6 more

We use the panchromatic spectral energy distribution (SED)-fitting code Prospector to measure the galaxy logM*-logSFR relationship (the star-forming sequence) across 0.2 < z < 3.0 using the COSMOS-2015 and 3D-HST UV-IR photometric catalogs. We demonstrate that the chosen method of identifying star-forming galaxies introduces a systematic unc…

2022 The Astrophysical Journal
eHST 123
Cluster Cepheids with High Precision Gaia Parallaxes, Low Zero-point Uncertainties, and Hubble Space Telescope Photometry
DOI: 10.3847/1538-4357/ac8f24 Bibcode: 2022ApJ...938...36R

Casertano, Stefano; Riess, Adam G.; Breuval, Louise +7 more

We present Hubble Space Telescope (HST) photometry of 17 Cepheids in open clusters and their cluster mean parallaxes from Gaia EDR3. These parallaxes are more precise than those from individual Cepheids (G < 8 mag) previously used to measure the Hubble constant because they are derived from an average of >300 stars per cluster. Cluster paral…

2022 The Astrophysical Journal
Gaia eHST 120
The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration Systematic Uncertainty
DOI: 10.3847/1538-4357/ac8bcc Bibcode: 2022ApJ...938..111B

Riess, Adam; Scolnic, Dan; Brout, Dillon +9 more

We present a recalibration of the photometric systems in the Pantheon+ sample of Type Ia supernovae (SNe Ia) including those in the SH0ES distance-ladder measurement of H 0. We utilize the large and uniform sky coverage of the public Pan-STARRS stellar photometry catalog to cross calibrate against tertiary standards released by individu…

2022 The Astrophysical Journal
eHST 118
The Exploration of Local VolumE Satellites (ELVES) Survey: A Nearly Volume-limited Sample of Nearby Dwarf Satellite Systems
DOI: 10.3847/1538-4357/ac6fd7 Bibcode: 2022ApJ...933...47C

Greene, Jenny E.; Beaton, Rachael L.; Danieli, Shany +2 more

We present the final sample of the Exploration of Local VolumE Satellites (ELVES) survey, a survey of the dwarf satellites of a nearly volume-limited sample of Milky Way (MW)-like hosts in the Local Volume. Hosts are selected simply via a cut in luminosity ( ${M}_{{K}_{s}}\lt -22.1$ mag) and distance (D < 12 Mpc). We cataloged the satellites of…

2022 The Astrophysical Journal
Gaia 115
A Census of the Bright z = 8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields
DOI: 10.3847/1538-4357/ac3aed Bibcode: 2022ApJ...928...52F

Papovich, Casey; Finkelstein, Steven L.; Dickinson, Mark +21 more

We present the results from a new search for candidate galaxies at z ≈ 8.5-11 discovered over the 850 arcmin2 area probed by the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS). We use a photometric-redshift selection including both Hubble and Spitzer Space Telescope photometry to robustly identify galaxies in t…

2022 The Astrophysical Journal
eHST 110
A First Look at the Abundance Pattern-O/H, C/O, and Ne/O-in z > 7 Galaxies with JWST/NIRSpec
DOI: 10.3847/2041-8213/ac9ab2 Bibcode: 2022ApJ...940L..23A

Finkelstein, Steven L.; Arrabal Haro, Pablo; Dickinson, Mark +9 more

We analyze the rest-frame near-UV and optical nebular spectra of three z > 7 galaxies from the Early Release Observations taken with the Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope (JWST). These three high-z galaxies show the detection of several strong emission nebular lines, including the temperature-sensitive [O II…

2022 The Astrophysical Journal
JWST 103
A Highly Settled Disk around Oph163131
DOI: 10.3847/1538-4357/ac5fae Bibcode: 2022ApJ...930...11V

Pinte, C.; Ménard, F.; Duchêne, G. +10 more

High dust density in the midplane of protoplanetary disks is favorable for efficient grain growth and can allow fast formation of planetesimals and planets, before disks dissipate. Vertical settling and dust trapping in pressure maxima are two mechanisms allowing dust to concentrate in geometrically thin and high-density regions. In this work, we …

2022 The Astrophysical Journal
eHST 99
The Poor Old Heart of the Milky Way
DOI: 10.3847/1538-4357/ac9e01 Bibcode: 2022ApJ...941...45R

Xiang, Maosheng; Conroy, Charlie; Hogg, David W. +9 more

Our Milky Way should host an ancient, metal-poor, and centrally concentrated stellar population, which reflects the star formation and enrichment in the few most massive progenitors that coalesced at high redshift to form the proto-Galaxy. While metal-poor stars are known to reside in the inner few kiloparsecs of our Galaxy, current data do not ye…

2022 The Astrophysical Journal
Gaia 98
Proper Motions, Orbits, and Tidal Influences of Milky Way Dwarf Spheroidal Galaxies
DOI: 10.3847/1538-4357/ac997b Bibcode: 2022ApJ...940..136P

Erkal, Denis; Li, Ting S.; Pace, Andrew B.

We combine Gaia early data release 3 astrometry with accurate photometry and utilize a probabilistic mixture model to measure the systemic proper motion of 52 dwarf spheroidal (dSph) satellite galaxies of the Milky Way (MW). For the 46 dSphs with literature line-of-sight velocities we compute orbits in both a MW and a combined MW + Large Magellani…

2022 The Astrophysical Journal
Gaia 97