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JWST's PEARLS: Mothra, a new kaiju star at z = 2.091 extremely magnified by MACS0416, and implications for dark matter models
DOI: 10.1051/0004-6361/202347556 Bibcode: 2023A&A...679A..31D

Grogin, Norman A.; Koekemoer, Anton M.; Pirzkal, Nor +28 more

We report the discovery of Mothra, an extremely magnified monster star, likely a binary system of two supergiant stars, in one of the strongly lensed galaxies behind the galaxy cluster MACS J0416.1−2403. Mothra is in a galaxy with spectroscopic redshift z = 2.091 in a portion of the galaxy that is parsecs away from the cluster caustic. The binary …

2023 Astronomy and Astrophysics
eHST JWST 33
Stepped partially acoustic dark matter, large scale structure, and the Hubble tension
DOI: 10.1007/JHEP06(2023)012 Bibcode: 2023JHEP...06..012B

Marques-Tavares, Gustavo; Buen-Abad, Manuel A.; Chacko, Zackaria +2 more

We propose a new interacting dark sector model, Stepped Partially Acoustic Dark Matter (SPartAcous), that can simultaneously address the two most important tensions in current cosmological data, the H0 and S8 problems. As in the Partially Acoustic Dark Matter (PAcDM) scenario, this model features a subcomponent of dark matter…

2023 Journal of High Energy Physics
Gaia 33
The Physical Drivers and Observational Tracers of CO-to-H2 Conversion Factor Variations in Nearby Barred Galaxy Centers
DOI: 10.3847/1538-4357/accb86 Bibcode: 2023ApJ...950..119T

Sandstrom, Karin M.; Bolatto, Alberto D.; Leroy, Adam K. +24 more

The CO-to-H2 conversion factor (α CO) is central to measuring the amount and properties of molecular gas. It is known to vary with environmental conditions, and previous studies have revealed lower α CO in the centers of some barred galaxies on kiloparsec scales. To unveil the physical drivers of such variations, w…

2023 The Astrophysical Journal
Herschel 33
Localizing Sources of Variability in Crowded TESS Photometry
DOI: 10.3847/1538-3881/acb20c Bibcode: 2023AJ....165..141H

Bell, Keaton J.; Higgins, Michael E.

The Transiting Exoplanet Survey Satellite (TESS) has an exceptionally large plate scale of 21″ px-1, causing most TESS light curves to record the blended light of multiple stars. This creates a danger of misattributing variability observed by TESS to the wrong source, which would invalidate any analysis. We developed a method that can l…

2023 The Astronomical Journal
Gaia 33
JWST/NIRSpec Measurements of the Relationships between Nebular Emission-line Ratios and Stellar Mass at z 3-6
DOI: 10.3847/2041-8213/acd939 Bibcode: 2023ApJ...950L...1S

Shapley, Alice E.; Reddy, Naveen A.; Sanders, Ryan L. +2 more

We analyze the rest-optical emission-line ratios of star-forming galaxies at 2.7 ≤ z < 6.5 drawn from the Cosmic Evolution Early Release Science (CEERS) Survey and their relationships with stellar mass (M *). Our analysis includes both line ratios based on the [N II] λ6583 feature ([N II] λ6583/Hα, ([O III] λ5007/Hβ)/([N II] λ6583/Hα…

2023 The Astrophysical Journal
eHST JWST 33
The distribution of CO2 on Europa indicates an internal source of carbon
DOI: 10.1126/science.adg4155 Bibcode: 2023Sci...381.1308T

Brown, Michael E.; Trumbo, Samantha K.

Jupiter’s moon Europa has a subsurface ocean, the chemistry of which is largely unknown. Carbon dioxide (CO2) has previously been detected on the surface of Europa, but it was not possible to determine whether it originated from subsurface ocean chemistry, was delivered by impacts, or was produced on the surface by radiation processing …

2023 Science
JWST 33
Significance mode analysis (SigMA) for hierarchical structures. An application to the Sco-Cen OB association
DOI: 10.1051/0004-6361/202243690 Bibcode: 2023A&A...677A..59R

Meingast, Stefan; Alves, João; Großschedl, Josefa E. +3 more

We present a new clustering method, significance mode analysis (SigMA), for extracting co-spatial and co-moving stellar populations from large-scale surveys such as ESA Gaia. The method studies the topological properties of the density field in the multidimensional phase space. We validated SigMA on simulated clusters and find that it outperforms …

2023 Astronomy and Astrophysics
Gaia 33
High-frequency Decayless Waves with Significant Energy in Solar Orbiter/EUI Observations
DOI: 10.3847/1538-4357/acb26a Bibcode: 2023ApJ...946...36P

Van Doorsselaere, Tom; Berghmans, David; Petrova, Elena +1 more

High-frequency wave phenomena present a great deal of interest as one of the possible candidates to contribute to the energy input required to heat the corona as a part of the alternating current heating theory. However, the resolution of imaging instruments up until the Solar Orbiter has made it impossible to resolve the necessary time and spatia…

2023 The Astrophysical Journal
SolarOrbiter 33
A catalogue of cataclysmic variables from 20 yr of the Sloan Digital Sky Survey with new classifications, periods, trends, and oddities
DOI: 10.1093/mnras/stad2018 Bibcode: 2023MNRAS.524.4867I

Thorstensen, John R.; Breedt, Elmé; Gänsicke, Boris T. +7 more

We present a catalogue of 507 cataclysmic variables (CVs) observed in SDSS I to IV including 70 new classifications collated from multiple archival data sets. This represents the largest sample of CVs with high-quality and homogeneous optical spectroscopy. We have used this sample to derive unbiased space densities and period distributions for the…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 33
Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-dwarf Companion in the Hyades
DOI: 10.3847/1538-3881/aca408 Bibcode: 2023AJ....165...39F

Magnier, Eugene A.; Jensen-Clem, Rebecca; Crepp, Justin R. +28 more

Benchmark brown dwarf companions with well-determined ages and model-independent masses are powerful tools to test substellar evolutionary models and probe the formation of giant planets and brown dwarfs. Here, we report the independent discovery of HIP 21152 B, the first imaged brown dwarf companion in the Hyades, and conduct a comprehensive orbi…

2023 The Astronomical Journal
Gaia Hipparcos 33