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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
SN 2018bsz: A Type I superluminous supernova with aspherical circumstellar material
DOI: 10.1051/0004-6361/202243256 Bibcode: 2022A&A...666A..30P

Spyromilio, J.; Gromadzki, M.; Galbany, L. +26 more

We present a spectroscopic analysis of the most nearby Type I superluminous supernova (SLSN-I), SN 2018bsz. The photometric evolution of SN 2018bsz has several surprising features, including an unusual pre-peak plateau and evidence for rapid formation of dust ≳200 d post-peak. We show here that the spectroscopic and polarimetric properties of SN 2…

2022 Astronomy and Astrophysics
eHST 32
How much hydrogen is in Type Ib and IIb supernova progenitors?
DOI: 10.1093/mnras/stac088 Bibcode: 2022MNRAS.511..691G

Arcavi, Iair; Gilkis, Avishai

Core-collapse supernovae showing little or no hydrogen (denoted by Type IIb and Ib, respectively) are the explosions of massive stars that have lost some or most of their outer envelopes. How they lose their mass is unclear, but it likely involves binary interaction. So far, seven progenitors of such supernovae have been identified in pre-explosio…

2022 Monthly Notices of the Royal Astronomical Society
eHST 32
NuSTAR Observations of 52 Compton-thick Active Galactic Nuclei Selected by the Swift/Burst Alert Telescope All-sky Hard X-Ray Survey
DOI: 10.3847/1538-4365/ac5f59 Bibcode: 2022ApJS..260...30T

Tanimoto, Atsushi; Ueda, Yoshihiro; Ricci, Claudio +2 more

We present systematic broadband X-ray spectral analysis of 52 Compton-thick ( $24\leqslant \mathrm{log}{N}_{{\rm{H}}}^{\mathrm{LOS}}/{\mathrm{cm}}^{-2}$ ) active galactic nucleus (CTAGN) candidates selected by the Swift/Burst Alert Telescope all-sky hard X-ray survey observed with Chandra, X-ray Multi-Mirror Mission-Newton (XMM-Newton), Swift/X-Ra…

2022 The Astrophysical Journal Supplement Series
Suzaku XMM-Newton 32
An early transition to magnetic supercriticality in star formation
DOI: 10.1038/s41586-021-04159-x Bibcode: 2022Natur.601...49C

Li, D.; Heiles, C.; Qian, L. +5 more

Magnetic fields have an important role in the evolution of interstellar medium and star formation1,2. As the only direct probe of interstellar field strength, credible Zeeman measurements remain sparse owing to the lack of suitable Zeeman probes, particularly for cold, molecular gas3. Here we report the detection of a magneti…

2022 Nature
Herschel 32
Exploring the dependence of hot Jupiter occurrence rates on stellar mass with TESS
DOI: 10.1093/mnras/stac2179 Bibcode: 2022MNRAS.516...75B

Kunimoto, M.; Beleznay, Maya

We present estimates for the occurrence rates of hot Jupiters around dwarf stars based on data from the Transiting Exoplanet Survey Satellite (TESS) Prime Mission. We take 97 hot Jupiters orbiting 198 721 AFG dwarf stars (ranging in mass from 0.8 to $2.3\, {\rm M}_{\odot }$) from an independent search for hot Jupiters using TESS Prime Mission data…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 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
Exoplanet X-ray irradiation and evaporation rates with eROSITA
DOI: 10.1051/0004-6361/202141097 Bibcode: 2022A&A...661A..23F

Schwope, A.; Poppenhaeger, K.; Ilic, N. +1 more

High-energy irradiation is a driver for atmospheric evaporation and mass loss in exoplanets. This work is based on data from eROSITA, the soft X-ray instrument on board the Spectrum Roentgen Gamma mission, as well as on archival data from other missions. We aim to characterise the high-energy environment of known exoplanets and estimate their mass…

2022 Astronomy and Astrophysics
Gaia XMM-Newton 32
The relativistic solar particle event on 28 October 2021: Evidence of particle acceleration within and escape from the solar corona
DOI: 10.1051/0004-6361/202243903 Bibcode: 2022A&A...663A.173K

Krucker, Säm; Dresing, Nina; Klein, Karl-Ludwig +6 more


Aims: We analyse particle, radio, and X-ray observations during the first relativistic proton event of solar cycle 25 detected on Earth. The aim is to gain insight into the relationship between relativistic solar particles detected in space and the processes of acceleration and propagation in solar eruptive events.
Methods: To this end, …

2022 Astronomy and Astrophysics
SOHO SolarOrbiter 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