Search Publications

Surface Brightness Profile of Lyman-α Halos out to 320 kpc in HETDEX
DOI: 10.3847/1538-4357/ac5cb8 Bibcode: 2022ApJ...929...90L

Ouchi, Masami; Finkelstein, Steven L.; Schneider, Donald P. +18 more

We present the median-stacked Lyman-α (Lyα) surface brightness profiles of 968 spectroscopically selected Lyα emitting galaxies (LAEs) at redshifts 1.9 < z < 3.5 in the early data of the Hobby-Eberly Telescope Dark Energy Experiment. The selected LAEs are high-confidence Lyα detections with high signal-to-noise ratios observed with good seei…

2022 The Astrophysical Journal
Gaia 32
A New Era of Intracluster Light Studies with JWST
DOI: 10.3847/2041-8213/ac98c5 Bibcode: 2022ApJ...940L..51M

Trujillo, Ignacio; Montes, Mireia

Still largely unexplored, the diffuse light in clusters of galaxies traces the past and ongoing buildup of these massive structures. Here we present the first comprehensive study of the intracluster light (ICL) of the cluster SMACS J0723.3-7327 (z = 0.39) using the JWST Early Release Observations. These deep and high spatial resolution images allo…

2022 The Astrophysical Journal
JWST 31
The Complexity of the Cetus Stream Unveiled from the Fusion of STREAMFINDER and StarGO
DOI: 10.3847/1538-4357/ac616f Bibcode: 2022ApJ...930..103Y

Huang, Yang; Chang, Jiang; Sestito, Federico +16 more

We combine the power of two stream-searching tools, STREAMFINDER and StarGO applied to the Gaia EDR3 data, to detect stellar debris belonging to the Cetus stream system that forms a complex, nearly polar structure around the Milky Way. In this work, we find the southern extensions of the northern Cetus stream as the Palca stream and a new southern…

2022 The Astrophysical Journal
Gaia 31
A Speed Bump: SN 2021aefx Shows that Doppler Shift Alone Can Explain Early Excess Blue Flux in Some Type Ia Supernovae
DOI: 10.3847/2041-8213/ac7235 Bibcode: 2022ApJ...932L...2A

Suntzeff, N. B.; Galbany, L.; Brown, P. J. +17 more

We present early-time photometric and spectroscopic observations of the Type Ia supernova (SN Ia) 2021aefx. The early-time u-band light curve shows an excess flux when compared to normal SNe Ia. We suggest that the early excess blue flux may be due to a rapid change in spectral velocity in the first few days post explosion, produced by the emissio…

2022 The Astrophysical Journal
eHST 31
Direct Constraints on the Extremely Metal-poor Massive Stars Underlying Nebular C IV Emission from Ultra-deep HST/COS Ultraviolet Spectroscopy
DOI: 10.3847/1538-4357/ac5d38 Bibcode: 2022ApJ...930..105S

Charlot, Stéphane; Chevallard, Jacopo; Sanders, Ryan L. +8 more

Metal-poor nearby galaxies hosting massive stars have a fundamental role to play in our understanding of both high-redshift galaxies and low-metallicity stellar populations. But while much attention has been focused on their bright nebular gas emission, the massive stars that power it remain challenging to constrain. Here we present exceptionally …

2022 The Astrophysical Journal
eHST 31
HST Strong-lensing Model for the First JWST Galaxy Cluster SMACS J0723.3-7327
DOI: 10.3847/1538-4357/ac8ff1 Bibcode: 2022ApJ...938...14G

Zitrin, Adi; Furtak, Lukas J.; Meena, Ashish K. +1 more

On 2022 July 8, NASA shared (https://www.nasa.gov/feature/goddard/2022/nasa-shares-list-of-cosmic-targets-for-webb-telescope-s-first-images) the list of five public showcase targets that have been observed with the new James Webb Space Telescope (JWST) and whose data-at the time of writing-are expected to be released to the public around Tuesday, …

2022 The Astrophysical Journal
eHST 31
Early JWST Imaging Reveals Strong Optical and NIR Color Gradients in Galaxies at z 2 Driven Mostly by Dust
DOI: 10.3847/2041-8213/aca675 Bibcode: 2022ApJ...941L..37M

van Dokkum, Pieter; Heintz, Kasper E.; Bezanson, Rachel +7 more

Recent studies have shown that galaxies at cosmic noon are redder in the center and bluer in the outskirts, mirroring results in the local universe. These color gradients could be caused by gradients in either the stellar age or dust opacity; however, distinguishing between these two causes is impossible with rest-frame optical photometry alone. H…

2022 The Astrophysical Journal
eHST JWST 31
Discovery of a Double-detonation Thermonuclear Supernova Progenitor
DOI: 10.3847/2041-8213/ac48f1 Bibcode: 2022ApJ...925L..12K

Green, Matthew J.; Rusholme, Ben; Bellm, Eric C. +12 more

We present the discovery of a new double-detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with a P orb = 76.34179(2) minutes orbital period. Spectroscopic observations are consistent with an sdB star during helium core burning residing on the extreme horizontal branch. Chimera light c…

2022 The Astrophysical Journal
Gaia 31
Constraints on the Spindown of Fully Convective M Dwarfs Using Wide Field Binaries
DOI: 10.3847/1538-4357/ac7da8 Bibcode: 2022ApJ...936..109P

Winters, Jennifer G.; Irwin, Jonathan M.; Charbonneau, David +1 more

M dwarfs remain active over longer timescales than their Sunlike counterparts, with potentially devastating implications for the atmospheres of their planets. However, the age at which fully convective M dwarfs transition from active and rapidly rotating to quiescent and slowly rotating is poorly understood, as these stars remain rapidly rotating …

2022 The Astrophysical Journal
Gaia 30
GOALS-JWST: Resolving the Circumnuclear Gas Dynamics in NGC 7469 in the Mid-infrared
DOI: 10.3847/2041-8213/ac961c Bibcode: 2022ApJ...940L...5U

Inami, Hanae; Böker, Torsten; Law, David R. +35 more

The nearby, luminous infrared galaxy NGC 7469 hosts a Seyfert nucleus with a circumnuclear star-forming ring and is thus the ideal local laboratory for investigating the starburst-AGN (active galactic nucleus) connection in detail. We present integral-field observations of the central 1.3 kpc region in NGC 7469 obtained with the JWST Mid-InfraRed …

2022 The Astrophysical Journal
JWST 30