Search Publications

A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67
DOI: 10.3847/1538-4357/ac90be Bibcode: 2022ApJ...938..118D

Magnier, Eugene A.; van Saders, Jennifer; García, Rafael A. +5 more

We present stellar rotation periods for late K- and early M-dwarf members of the 4 Gyr old open cluster M67 as calibrators for gyrochronology and tests of stellar spin-down models. Using Gaia EDR3 astrometry for cluster membership and Pan-STARRS (PS1) photometry for binary identification, we build this set of rotation periods from a campaign of mo…

2022 The Astrophysical Journal
Gaia 42
Stellar Abundance Maps of the Milky Way Disk
DOI: 10.3847/1538-4357/ac54ad Bibcode: 2022ApJ...928...23E

Hogg, David W.; Rix, Hans-Walter; Price-Whelan, Adrian M. +4 more

To understand the formation of the Milky Way's prominent bar it is important to know whether stars in the bar differ in the chemical element composition of their birth material as compared to disk stars. This requires stellar abundance measurements for large samples across the Milky Way's body. Such samples, e.g., luminous red giant stars observed…

2022 The Astrophysical Journal
Gaia 42
Direct-imaging Discovery and Dynamical Mass of a Substellar Companion Orbiting an Accelerating Hyades Sun-like Star with SCExAO/CHARIS
DOI: 10.3847/2041-8213/ac772f Bibcode: 2022ApJ...934L..18K

Currie, Thayne; Kwon, Jungmi; Tamura, Motohide +33 more

We present the direct-imaging discovery of a substellar companion in orbit around a Sun-like star member of the Hyades open cluster. So far, no other substellar companions have been unambiguously confirmed via direct imaging around main-sequence stars in Hyades. The star HIP 21152 is an accelerating star as identified by the astrometry from the Ga…

2022 The Astrophysical Journal
Gaia Hipparcos 41
A New Estimate of the Cosmic Star Formation Density from a Radio-selected Sample, and the Contribution of H-dark Galaxies at z ≥ 3
DOI: 10.3847/1538-4357/ac51ca Bibcode: 2022ApJ...927..204E

Bisigello, Laura; Pozzi, Francesca; Calura, Francesco +13 more

The star formation rate density (SFRD) history of the universe is well constrained up to redshift z ~ 2. At earlier cosmic epochs, the picture has been largely inferred from UV-selected galaxies (e.g., Lyman-break galaxies; LBGs). However, the inferred star formation rates of LBGs strongly depend on the assumed dust extinction correction, which is…

2022 The Astrophysical Journal
eHST 41
ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier That Validates 301 New Exoplanets
DOI: 10.3847/1538-4357/ac4399 Bibcode: 2022ApJ...926..120V

Jenkins, Jon M.; Caldwell, Douglas A.; Twicken, Joseph D. +10 more

The Kepler and Transiting Exoplanet Survey Satellite (TESS) missions have generated over 100,000 potential transit signals that must be processed in order to create a catalog of planet candidates. During the past few years, there has been a growing interest in using machine learning to analyze these data in search of new exoplanets. Different from…

2022 The Astrophysical Journal
Gaia 41
Characterizing Extreme Emission Line Galaxies. II. A Self-consistent Model of Their Ionizing Spectrum
DOI: 10.3847/1538-4357/ac8f2c Bibcode: 2022ApJ...938...16O

Skillman, Evan D.; Chisholm, John; Erb, Dawn K. +3 more

Observations of high-redshift galaxies (z > 5) have shown that these galaxies have extreme emission lines with equivalent widths much larger than their local star-forming counterparts. Extreme emission line galaxies (EELGs) in the nearby universe are likely analogs to galaxies during the Epoch of Reionization and provide nearby laboratories to …

2022 The Astrophysical Journal
eHST 40
Multipoint Interplanetary Coronal Mass Ejections Observed with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind, and STEREO-A
DOI: 10.3847/2041-8213/ac42d0 Bibcode: 2022ApJ...924L...6M

Möstl, Christian; Davies, Emma E.; Freiherr von Forstner, Johan L. +12 more

We report the result of the first search for multipoint in situ and imaging observations of interplanetary coronal mass ejections (ICMEs) starting with the first Solar Orbiter (SolO) data in 2020 April-2021 April. A data exploration analysis is performed including visualizations of the magnetic-field and plasma observations made by the five spacec…

2022 The Astrophysical Journal
BepiColombo SOHO SolarOrbiter 40
Early Results from GLASS-JWST. IV. Spatially Resolved Metallicity in a Low-mass z 3 Galaxy with NIRISS
DOI: 10.3847/2041-8213/ac959e Bibcode: 2022ApJ...938L..16W

Calabrò, Antonello; Castellano, Marco; Fontana, Adriano +19 more

We report the first gas-phase metallicity map of a distant galaxy measured with the James Webb Space Telescope (JWST). We use the NIRISS slitless spectroscopy acquired by the GLASS Early Release Science program to spatially resolve the rest-frame optical nebular emission lines in a gravitationally lensed galaxy at z = 3.06 behind the A2744 galaxy …

2022 The Astrophysical Journal
eHST JWST 40
The Physical Properties of Luminous z ≳ 8 Galaxies and Implications for the Cosmic Star Formation Rate Density from 0.35 deg2 of (Pure-)Parallel HST Observations
DOI: 10.3847/1538-4357/ac4803 Bibcode: 2022ApJ...927..236R

Treu, Tommaso; Trenti, Michele; Morishita, Takahiro +2 more

We present the largest systematic, Hubble Space Telescope (HST)-based search to date for luminous z ≳ 8 galaxy candidates using ~1267 arcmin2 of (pure-)parallel observations from a compilation of 288 random sightlines with Advanced Camera for Surveys and Wide Field Camera 3 observations, derived from the (Super)Brightest of Reionizing G…

2022 The Astrophysical Journal
eHST 40
Water and an Escaping Helium Tail Detected in the Hazy and Methane-depleted Atmosphere of HAT-P-18b from JWST NIRISS/SOSS
DOI: 10.3847/2041-8213/ac9977 Bibcode: 2022ApJ...940L..35F

Deming, Drake; Sing, David K.; Fu, Guangwei +11 more

JWST is here. The early release observation (ERO) program provides us with the first look at the scientific data and the spectral capabilities. One of the targets from the ERO is HAT-P-18b, an inflated Saturn-mass planet with an equilibrium temperature of ~850 K. We present the NIRISS/SOSS transmission spectrum of HAT-P-18b from 0.6 to 2.8 µ…

2022 The Astrophysical Journal
eHST JWST 39