Search Publications

Weak Mass Loss from the Red Supergiant Progenitor of the Type II SN 2021yja
DOI: 10.3847/1538-4357/ac75f0 Bibcode: 2022ApJ...935...31H

Kilpatrick, Charles D.; Foley, Ryan J.; Pan, Yen-Chen +56 more

We present high-cadence optical, ultraviolet (UV), and near-infrared data of the nearby (D ≈ 23 Mpc) Type II supernova (SN) 2021yja. Many Type II SNe show signs of interaction with circumstellar material (CSM) during the first few days after explosion, implying that their red supergiant (RSG) progenitors experience episodic or eruptive mass loss. …

2022 The Astrophysical Journal
eHST 33
Constraining Black Hole Natal Kicks with Astrometric Microlensing
DOI: 10.3847/1538-4357/ac66d6 Bibcode: 2022ApJ...930..159A

Andrews, Jeff J.; Kalogera, Vicky

Multiple pieces of evidence suggest that neutron stars receive large kicks when formed from the remnant of a collapsing star. However, the evidence for whether black holes (BHs) receive natal kicks is less clear, reliant on weak constraints from the analysis of BH X-ray binaries and massive runaway and walkaway stars. Here we show, for the first t…

2022 The Astrophysical Journal
Gaia 33
The Origin of Weakened Magnetic Braking in Old Solar Analogs
DOI: 10.3847/2041-8213/ac794d Bibcode: 2022ApJ...933L..17M

Ayres, Thomas R.; Kochukhov, Oleg; Stassun, Keivan G. +10 more

The rotation rates of main-sequence stars slow over time as they gradually lose angular momentum to their magnetized stellar winds. The rate of angular momentum loss depends on the strength and morphology of the magnetic field, the mass-loss rate, and the stellar rotation period, mass, and radius. Previous observations suggested a shift in magneti…

2022 The Astrophysical Journal
Gaia XMM-Newton 33
The Stellar Metallicities of Massive Quiescent Galaxies at 1.0 < z < 1.3 from KMOS + VANDELS
DOI: 10.3847/1538-4357/ac5b62 Bibcode: 2022ApJ...929..131C

Castellano, Marco; Hathi, Nimish P.; Pentericci, Laura +18 more

We present a rest-frame UV-optical (λ = 2500-6400 Å) stacked spectrum representative of massive quiescent galaxies at 1.0 < z < 1.3 with log(M */M ) > 10.8. The stack is constructed using VANDELS survey data, combined with new KMOS observations. We apply two independent full-spectral-fitting approaches, measuring a …

2022 The Astrophysical Journal
eHST 33
Sun-as-a-star Analyses of Various Solar Active Events Using Hα Spectral Images Taken by SMART/SDDI
DOI: 10.3847/1538-4357/ac9730 Bibcode: 2022ApJ...939...98O

Namekata, Kosuke; Ichimoto, Kiyoshi; Ishii, Takako T. +2 more

Sun-as-a-star analyses in which observational data is spatially integrated are useful for interpreting stellar data. For future applications to stellar observations, we performed Sun-as-a-star analyses of Hα spectra for various active events on the Sun, not only for flares and filament eruptions/surges on the solar disk, but also for eruptions of …

2022 The Astrophysical Journal
SOHO 32
ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z ≃ 0.5 - 6
DOI: 10.3847/1538-4357/ac6e3f Bibcode: 2022ApJ...932...77S

Pérez-González, Pablo G.; Koekemoer, Anton M.; Smail, Ian +25 more

We present an ALMA-Herschel joint analysis of sources detected by the ALMA Lensing Cluster Survey (ALCS) at 1.15 mm. Herschel/PACS and SPIRE data at 100-500 µm are deblended for 180 ALMA sources in 33 lensing cluster fields that are detected either securely (141 sources; in our main sample) or tentatively at S/N ≥ 4 with cross-matched HST/Sp…

2022 The Astrophysical Journal
Herschel eHST 32
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