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The SRG/eROSITA all-sky survey. First X-ray catalogues and data release of the western Galactic hemisphere
DOI: 10.1051/0004-6361/202347165 Bibcode: 2024A&A...682A..34M

Zhang, X.; Haberl, F.; Burwitz, V. +142 more

The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite began surveying the sky in December 2019, with the aim of producing all-sky X-ray source lists and sky maps of an unprecedented depth. Here we present catalogues of both point-like and extended sources using the data acquired in the first six months of survey operations…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 197
An Updated Mass-Radius Analysis of the 2017-2018 NICER Data Set of PSR J0030+0451
DOI: 10.3847/1538-4357/acfb83 Bibcode: 2024ApJ...961...62V

Chakrabarty, Deepto; Bogdanov, Slavko; Salmi, Tuomo +12 more

In 2019 the NICER collaboration published the first mass and radius inferred for PSR J0030+0451, thanks to NICER observations, and consequent constraints on the equation of state characterizing dense matter. Two independent analyses found a mass of ~1.3-1.4 M and a radius of ~13 km. They also both found that the hot spots were all loc…

2024 The Astrophysical Journal
XMM-Newton 102
A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437–4715
DOI: 10.3847/2041-8213/ad5a6f Bibcode: 2024ApJ...971L..20C

Remillard, Ronald A.; Bogdanov, Slavko; Salmi, Tuomo +17 more

We report Bayesian inference of the mass, radius, and hot X-ray emitting region properties—using data from the Neutron Star Interior Composition ExploreR (NICER)—for the brightest rotation-powered millisecond X-ray pulsar, PSR J0437‑4715. Our modeling is conditional on informative tight priors on mass, distance, and binary inclination obtained fro…

2024 The Astrophysical Journal
XMM-Newton 96
ULTRASAT: A Wide-field Time-domain UV Space Telescope
DOI: 10.3847/1538-4357/ad2704 Bibcode: 2024ApJ...964...74S

Mazeh, T.; Gal-Yam, A.; Tal-Or, L. +41 more

The Ultraviolet Transient Astronomy Satellite (ULTRASAT) is scheduled to be launched to geostationary orbit in 2027. It will carry a telescope with an unprecedentedly large field of view (204 deg2) and near-ultraviolet (NUV; 230–290 nm) sensitivity (22.5 mag, 5σ, at 900 s). ULTRASAT will conduct the first wide-field survey of transient …

2024 The Astrophysical Journal
Gaia XMM-Newton 89
A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst
DOI: 10.1038/s41586-023-06979-5 Bibcode: 2024Natur.626..742Y

Kilpatrick, Charles D.; Lee, Chung-Uk; Im, Myungshin +24 more

Observationally, kilonovae are astrophysical transients powered by the radioactive decay of nuclei heavier than iron, thought to be synthesized in the merger of two compact objects1-4. Over the first few days, the kilonova evolution is dominated by a large number of radioactive isotopes contributing to the heating rate2,5. On…

2024 Nature
XMM-Newton eHST JWST 84
The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data
DOI: 10.3847/1538-4357/ad5f1f Bibcode: 2024ApJ...974..294S

Chakrabarty, Deepto; Bogdanov, Slavko; Salmi, Tuomo +14 more

We report an updated analysis of the radius, mass, and heated surface regions of the massive pulsar PSR J0740+6620 using Neutron Star Interior Composition Explorer (NICER) data from 2018 September 21 to 2022 April 21, a substantial increase in data set size compared to previous analyses. Using a tight mass prior from radio-timing measurements and …

2024 The Astrophysical Journal
XMM-Newton 71
SO2, silicate clouds, but no CH4 detected in a warm Neptune
DOI: 10.1038/s41586-023-06849-0 Bibcode: 2024Natur.625...51D

Henning, Thomas; Östlin, Göran; Güdel, Manuel +43 more

WASP-107b is a warm (approximately 740 K) transiting planet with a Neptune-like mass of roughly 30.5 M and Jupiter-like radius of about 0.94 RJ (refs. 1,2), whose extended atmosphere is eroding3. Previous observations showed evidence for water vapour and a thick, high-altitude condensate layer in the at…

2024 Nature
XMM-Newton eHST JWST 66
Deep Synoptic Array Science: First FRB and Host Galaxy Catalog
DOI: 10.3847/1538-4357/ad3736 Bibcode: 2024ApJ...967...29L

Hallinan, Gregg; Hodges, Mark; Lamb, James W. +19 more

Fast radio bursts (FRBs) are a powerful and mysterious new class of transients that are luminous enough to be detected at cosmological distances. By associating FRBs to host galaxies, we can measure intrinsic and environmental properties that test FRB origin models, in addition to using them as precise probes of distant cosmic gas. The Deep Synopt…

2024 The Astrophysical Journal
XMM-Newton 63
A Systematic Analysis of the X-Ray Emission in Optically Selected Tidal Disruption Events: Observational Evidence for the Unification of the Optically and X-Ray-selected Populations
DOI: 10.3847/1538-4357/ad2f9f Bibcode: 2024ApJ...966..160G

Cenko, S. Bradley; van Velzen, Sjoert; Gezari, Suvi +4 more

We present a systematic analysis of the X-ray emission of a sample of 17 optically selected, X-ray-detected tidal disruption events (TDEs) discovered between 2014 and 2021. The X-ray light curves show a diverse range of temporal behaviors, with most sources not following the expected power-law decline. The X-ray spectra are mostly extremely soft a…

2024 The Astrophysical Journal
XMM-Newton 54
X-ray eruptions every 22 days from the nucleus of a nearby galaxy
DOI: 10.1038/s41550-023-02178-4 Bibcode: 2024NatAs...8..347G

Gendreau, Keith; van Velzen, Sjoert; Gezari, Suvi +15 more

Galactic nuclei showing recurrent phases of activity and quiescence have recently been discovered. Some have recurrence times as short as a few hours to a day and are known as quasi-periodic X-ray eruption (QPE) sources. Others have recurrence times as long as hundreds to a thousand days and are called repeating nuclear transients. Here we present…

2024 Nature Astronomy
XMM-Newton 50