Search Publications

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
Short GRB Host Galaxies. I. Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets
DOI: 10.3847/1538-4357/ac91d0 Bibcode: 2022ApJ...940...56F

Kilpatrick, Charles D.; Smith, Nathan; Andrews, Jennifer +25 more

We present a comprehensive optical and near-infrared census of the fields of 90 short gamma-ray bursts (GRBs) discovered in 2005-2021, constituting all short GRBs for which host galaxy associations are feasible (≈60% of the total Swift short GRB population). We contribute 274 new multi-band imaging observations across 58 distinct GRBs and 26 spect…

2022 The Astrophysical Journal
Gaia eHST 97
Searching for Extremely Blue UV Continuum Slopes at z = 7-11 in JWST/NIRCam Imaging: Implications for Stellar Metallicity and Ionizing Photon Escape in Early Galaxies
DOI: 10.3847/1538-4357/aca522 Bibcode: 2022ApJ...941..153T

Charlot, Stéphane; Chen, Zuyi; Stark, Daniel P. +4 more

The ultraviolet (UV) continuum slope (β, where f λ ∝ λ β ) of galaxies is sensitive to a variety of properties, from the metallicity and age of the stellar population to dust attenuation throughout the galaxy. Considerable attention has focused on identifying reionization-era galaxies with very blue UV slopes (β < -3). …

2022 The Astrophysical Journal
eHST JWST 96
Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant
DOI: 10.3847/1538-4357/ac68df Bibcode: 2022ApJ...932...15A

Riess, Adam G.; Yuan, Wenlong; Anand, Gagandeep S. +2 more

The tip of the red giant branch has been used to measure distances to 500 nearby galaxies with the Hubble Space Telescope (HST) which are available in the Color-Magnitude Diagrams and Tip of the Red Giant Branch (CMDs/TRGB) catalog on the Extragalactic Distance Database (EDD). Our established methods are employed to perform an independent reductio…

2022 The Astrophysical Journal
eHST 96
z 2-9 Galaxies Magnified by the Hubble Frontier Field Clusters. II. Luminosity Functions and Constraints on a Faint-end Turnover
DOI: 10.3847/1538-4357/ac86d1 Bibcode: 2022ApJ...940...55B

Bouwens, R. J.; Oesch, P.; Illingworth, G. +2 more

We present new determinations of the rest-UV luminosity functions (LFs) at z = 2-9 to extremely low luminosities (>-14 mag) from a sample of >2500 lensed galaxies found behind the Hubble Frontier Fields (HFF) clusters. For the first time, we present faint-end slope results from lensed samples that are fully consistent with blank-field result…

2022 The Astrophysical Journal
eHST 95
The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age
DOI: 10.3847/1538-3881/ac51e3 Bibcode: 2022AJ....163..179P

Owen, James E.; Howard, Andrew W.; Petigura, Erik A. +10 more

In 2017, the California-Kepler Survey (CKS) published its first data release (DR1) of high-resolution optical spectra of 1305 planet hosts. Refined CKS planet radii revealed that small planets are bifurcated into two distinct populations, super-Earths (smaller than 1.5 R ) and sub-Neptunes (between 2.0 and 4.0 R ), with few…

2022 The Astronomical Journal
Gaia 95
A Search for H-Dropout Lyman Break Galaxies at z 12-16
DOI: 10.3847/1538-4357/ac53a9 Bibcode: 2022ApJ...929....1H

Koekemoer, Anton M.; Yung, L. Y. Aaron; Harikane, Yuichi +11 more

We present two bright galaxy candidates at z ~ 12-13 identified in our H-dropout Lyman break selection with 2.3 deg2 near-infrared deep imaging data. These galaxy candidates, selected after careful screening of foreground interlopers, have spectral energy distributions showing a sharp discontinuity around 1.7 µm, a flat continuum …

2022 The Astrophysical Journal
Herschel eHST 95
Extreme solar events
DOI: 10.1007/s41116-022-00033-8 Bibcode: 2022LRSP...19....2C

Shibata, Kazunari; Schrijver, Carolus J.; Usoskin, Ilya G. +1 more

We trace the evolution of research on extreme solar and solar-terrestrial events from the 1859 Carrington event to the rapid development of the last twenty years. Our focus is on the largest observed/inferred/theoretical cases of sunspot groups, flares on the Sun and Sun-like stars, coronal mass ejections, solar proton events, and geomagnetic stor…

2022 Living Reviews in Solar Physics
Gaia 94
SDSS-IV MaNGA: pyPipe3D Analysis Release for 10,000 Galaxies
DOI: 10.3847/1538-4365/ac7b8f Bibcode: 2022ApJS..262...36S

Bruzual, Gustavo; Sánchez, S. F.; Barrera-Ballesteros, J. K. +12 more

We present here the analysis performed using the pyPipe3D pipeline for the final MaNGA data set included in the Sloan Digital Sky Survey data release 17. This data set comprises more than 10,000 individual data cubes, being the integral field spectroscopic (IFS) galaxy survey with the largest number of galaxies. pyPipe3D processes the IFS data cub…

2022 The Astrophysical Journal Supplement Series
Gaia 94
The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds
DOI: 10.1051/0004-6361/202142742 Bibcode: 2022A&A...663A..36B

Sana, Hugues; Vink, Jorick S.; Kaper, Lex +17 more

Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive stars, including the most massive stars known. The strong stellar winds of these very luminous stars impact their evolution and the surrounding environment. We currently lack detailed knowledge of the wind structure that is needed to quantify this i…

2022 Astronomy and Astrophysics
eHST 92