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JWST lensed quasar dark matter survey - II. Strongest gravitational lensing limit on the dark matter free streaming length to date
DOI: 10.1093/mnras/stae2458 Bibcode: 2024MNRAS.535.1652K

Djorgovski, S. G.; Stern, D.; Treu, T. +20 more

This is the second in a series of papers in which we use JWST Mid Infrared Instrument multiband imaging to measure the warm dust emission in a sample of 31 multiply imaged quasars, to be used as a probe of the particle nature of dark matter. We present measurements of the relative magnifications of the strongly lensed warm dust emission in a sampl…

2024 Monthly Notices of the Royal Astronomical Society
JWST 12
The Sydney Radio Star Catalogue: Properties of radio stars at megahertz to gigahertz frequencies
DOI: 10.1017/pasa.2024.72 Bibcode: 2024PASA...41...84D

Stelzer, Beate; Das, Barnali; Pope, Benjamin J. S. +13 more

We present the Sydney Radio Star Catalogue, a new catalogue of stars detected at megahertz to gigahertz radio frequencies. It consists of 839 unique stars with 3 405 radio detections, more than doubling the previously known number of radio stars. We have included stars from large area searches for radio stars found using circular polarisation sear…

2024 Publications of the Astronomical Society of Australia
Gaia XMM-Newton 12
Discovery of a Metal-poor Red Giant Star with the Highest Ultralithium Enhancement
DOI: 10.3847/1538-4357/ad6004 Bibcode: 2024ApJ...973..125K

Beers, Timothy C.; Placco, Vinicius M.; Hansen, Terese T. +10 more

We present the discovery of 2MASS J05241392‑0336543 (hereafter J0524‑0336), a very metal-poor ([Fe/H] = ‑2.43 ± 0.16), highly r-process-enhanced ([Eu/Fe] = +1.34 ± 0.10) Milky Way halo field red giant star, with an ultrahigh Li abundance of A(Li, 3D, NLTE) = 6.15 ± 0.25 and [Li/Fe] = +7.64 ± 0.25, respectively. This makes J0524‑0336 the most lithi…

2024 The Astrophysical Journal
Gaia 12
Testing kinematic distances under a realistic Galactic potential: Investigating systematic errors in the kinematic distance method arising from a non-axisymmetric potential
DOI: 10.1051/0004-6361/202450000 Bibcode: 2024A&A...692A.216H

Glover, Simon C. O.; Klessen, Ralf S.; Vasiliev, Eugene +15 more

Context. Obtaining reliable distance estimates to gas clouds within the Milky Way is challenging in the absence of certain tracers. The kinematic distance approach has been used as an alternative, and it is derived from the assumption of circular trajectories around the Galactic centre. Consequently, significant errors are expected in regions wher…

2024 Astronomy and Astrophysics
Gaia 12
Keck and Hubble Observations Show that MOA-2008-BLG-379Lb is a Super-Jupiter Orbiting an M Dwarf
DOI: 10.3847/1538-3881/ad4880 Bibcode: 2024AJ....168...15B

Lu, Jessica R.; Beaulieu, Jean-Philippe; Bond, Ian A. +11 more

We present high angular resolution imaging that detects the MOA-2008-BLG-379L exoplanet host star using Keck adaptive optics and the Hubble Space Telescope. These observations reveal host star and planet masses of M host = 0.434 ± 0.065 M and m p = 2.44 ± 0.49 M Jupiter. They are located at a distanc…

2024 The Astronomical Journal
eHST 12
Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z = 3.95
DOI: 10.1051/0004-6361/202348351 Bibcode: 2024A&A...684A.196Z

Finoguenov, A.; Magnelli, B.; Daddi, E. +34 more

The study of distant galaxy groups and clusters at the peak epoch of star formation is limited by the lack of a statistically and homogeneously selected and spectroscopically confirmed sample. Recent discoveries of concentrated starburst activities in cluster cores have opened a new window to hunt for these structures based on their integrated IR …

2024 Astronomy and Astrophysics
Herschel 12
Using Solar Orbiter as an Upstream Solar Wind Monitor for Real Time Space Weather Predictions
DOI: 10.1029/2023SW003628 Bibcode: 2024SpWea..2203628L

Möstl, C.; Davies, J. A.; Horbury, T. S. +11 more

Coronal mass ejections (CMEs) can create significant disruption to human activities and systems on Earth, much of which can be mitigated with prior warning of the upstream solar wind conditions. However, it is currently extremely challenging to accurately predict the arrival time and internal structure of a CME from coronagraph images alone. In th…

2024 Space Weather
SolarOrbiter 12
X-Shooting ULLYSES: Massive stars at low metallicity: VII. Stellar and wind properties of B supergiants in the Small Magellanic Cloud
DOI: 10.1051/0004-6361/202450475 Bibcode: 2024A&A...692A..89B

van Loon, J. Th.; Crowther, P. A.; Mehner, A. +22 more

Context. With the aim of understanding massive stars and their feedback in the early epochs of our Universe, the ULLYSES and XShootU collaborations collected the biggest homogeneous dataset of high-quality hot star spectra at low metallicity. Within the rich "zoo" of massive star stellar types, B supergiants (BSGs) represent an important connectio…

2024 Astronomy and Astrophysics
eHST 12
HPIC: The Habitable Worlds Observatory Preliminary Input Catalog
DOI: 10.3847/1538-3881/ad25ec Bibcode: 2024AJ....167..139T

Tuchow, Noah W.; Stark, Christopher C.; Mamajek, Eric

The Habitable Worlds Observatory Preliminary Input Catalog (HPIC) is a list of ∼13,000 nearby bright stars that will be potential targets for the Habitable Worlds Observatory (HWO) in its search for Earth-sized planets around Sun-like stars. We construct this target list using the TESS and Gaia DR3 catalogs and develop an automated pipeline to com…

2024 The Astronomical Journal
Gaia 12
Circumstellar Interaction in the Ultraviolet Spectra of SN 2023ixf 14–66 Days After Explosion
DOI: 10.3847/2041-8213/ad7855 Bibcode: 2024ApJ...973L..47B

Filippenko, Alexei V.; Smith, Nathan; Sand, David J. +20 more

SN 2023ixf was discovered in M101 within a day of the explosion and rapidly classified as a Type II supernova with flash features. Here we present ultraviolet (UV) spectra obtained with the Hubble Space Telescope 14, 19, 24, and 66 days after the explosion. Interaction between the supernova ejecta and circumstellar material (CSM) is seen in the UV…

2024 The Astrophysical Journal
eHST 12