Search Publications

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
JADES NIRSpec initial data release for the Hubble Ultra Deep Field: Redshifts and line fluxes of distant galaxies from the deepest JWST Cycle 1 NIRSpec multi-object spectroscopy
DOI: 10.1051/0004-6361/202347094 Bibcode: 2024A&A...690A.288B

Chevallard, Jacopo; Maseda, Michael V.; Parlanti, Eleonora +63 more

We describe the NIRSpec component of the JWST Deep Extragalactic Survey (JADES), and provide deep spectroscopy of 253 sources targeted with the NIRSpec micro-shutter assembly in the Hubble Ultra Deep Field and surrounding GOODS-South. The multi-object spectra presented here are the deepest so far obtained with JWST, amounting to up to 28 hours in …

2024 Astronomy and Astrophysics
Gaia eHST JWST 187
Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry
DOI: 10.1051/0004-6361/202449763 Bibcode: 2024A&A...686L...2G

Valtchanov, I.; Prusti, T.; Mazeh, T. +413 more

Context. Gravitational waves from black-hole (BH) merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected based on most stellar evolution models - and also higher than known stellar-origin black holes in our Galaxy. It has been proposed that those high-mass BHs are…

2024 Astronomy and Astrophysics
Gaia 86
A parsec-scale Galactic 3D dust map out to 1.25 kpc from the Sun
DOI: 10.1051/0004-6361/202347628 Bibcode: 2024A&A...685A..82E

Speagle, Joshua S.; Zucker, Catherine; Finkbeiner, Douglas +4 more

Context. High-resolution 3D maps of interstellar dust are critical for probing the underlying physics shaping the structure of the interstellar medium, and for foreground correction of astrophysical observations affected by dust.
Aims: We aim to construct a new 3D map of the spatial distribution of interstellar dust extinction out to a distan…

2024 Astronomy and Astrophysics
Gaia 82
Improving the open cluster census. III. Using cluster masses, radii, and dynamics to create a cleaned open cluster catalogue
DOI: 10.1051/0004-6361/202348662 Bibcode: 2024A&A...686A..42H

Reffert, Sabine; Hunt, Emily L.

Context. The census of open clusters has exploded in size thanks to data from the Gaia satellite. However, it is likely that many of these reported clusters are not gravitationally bound, making the open cluster census impractical for many scientific applications.
Aims: We aim to test different physically motivated methods for distinguishing …

2024 Astronomy and Astrophysics
Gaia 58
The more the merrier: SRG/eROSITA discovers two further galaxies showing X-ray quasi-periodic eruptions
DOI: 10.1051/0004-6361/202348881 Bibcode: 2024A&A...684A..64A

Gromadzki, M.; Salvato, M.; Liu, Z. +20 more

X-ray quasi-periodic eruptions (QPEs) are a novel addition to the group of extragalactic transients. With only a select number of known sources, and many more models published trying to explain them, we are so far limited in our understanding by small number statistics. In this work, we report the discovery of two further galaxies showing QPEs, he…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 48
The Pristine survey: XXIII. Data Release 1 and an all-sky metallicity catalogue based on Gaia DR3 BP/RP spectro-photometry
DOI: 10.1051/0004-6361/202347633 Bibcode: 2024A&A...692A.115M

Fouesneau, Morgan; Sestito, Federico; McConnachie, Alan W. +38 more

We used the spectro-photometric information of ∼219 million stars from Gaia's Data Release 3 (DR3) to calculate synthetic, narrowband, metallicity-sensitive CaHK magnitudes that mimic the observations of the Pristine survey, a survey of photometric metallicities of Milky Way stars that has been mapping more than 6500 deg2 of the norther…

2024 Astronomy and Astrophysics
Gaia 47
GA-NIFS: The core of an extremely massive protocluster at the epoch of reionisation probed with JWST/NIRSpec
DOI: 10.1051/0004-6361/202348824 Bibcode: 2024A&A...688A.146A

Pérez-González, Pablo G.; Charlot, Stéphane; Chevallard, Jacopo +24 more

Context. The SPT0311-58 system resides in a massive dark-matter halo at z ∼ 6.9. It hosts two dusty galaxies (E and W) with a combined star formation rate (SFR) of ∼3500 M yr−1, mostly obscured and identified by the rest-frame IR emission. The surrounding field exhibits an overdensity of submillimetre sources, making it a ca…

2024 Astronomy and Astrophysics
Gaia eHST JWST 44
1100 days in the life of the supernova 2018ibb. The best pair-instability supernova candidate, to date
DOI: 10.1051/0004-6361/202346855 Bibcode: 2024A&A...683A.223S

Filippenko, Alexei V.; Fransson, Claes; Gromadzki, Mariusz +63 more

Stars with zero-age main sequence masses between 140 and 260 M are thought to explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe can produce up to several tens of solar masses of radioactive nickel, resulting in luminous transients similar to some superluminous supernovae (SLSNe). Yet, no unambigu…

2024 Astronomy and Astrophysics
Gaia XMM-Newton eHST 36
Beyond Gaia DR3: Tracing the [α/M] - [M/H] bimodality from the inner to the outer Milky Way disc with Gaia-RVS and convolutional neural networks
DOI: 10.1051/0004-6361/202347122 Bibcode: 2024A&A...682A...9G

Guiglion, G.; Fabbro, S.; Valentini, M. +17 more

Context. In June 2022, Gaia DR3 provided the astronomy community with about one million spectra from the Radial Velocity Spectrometer (RVS) covering the CaII triplet region. In the next Gaia data releases, we anticipate the number of RVS spectra to successively increase from several 10 million spectra to eventually more than 200 million spectra. T…

2024 Astronomy and Astrophysics
Gaia 30