Search Publications

Repeating tidal disruptions in GSN 069: Long-term evolution and constraints on quasi-periodic eruptions' models
DOI: 10.1051/0004-6361/202244512 Bibcode: 2023A&A...670A..93M

Read, A. M.; Bianchi, S.; Miniutti, G. +4 more

Context. GSN 069 is the first galactic nucleus where quasi-periodic eruptions (QPEs) have been identified in December 2018. These are high-amplitude, soft X-ray bursts recurring every ∼9 h, lasting ∼1 h, and during which the X-ray count rate increases by up to two orders of magnitude with respect to an otherwise stable quiescent level. The X-ray s…

2023 Astronomy and Astrophysics
XMM-Newton eHST 71
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars
DOI: 10.1051/0004-6361/202245399 Bibcode: 2023A&A...673A.155Q

Valentini, M.; Anders, F.; Chiappini, C. +16 more

The Gaia mission has provided an invaluable wealth of astrometric data for more than a billion stars in our Galaxy. The synergy between Gaia astrometry, photometry, and spectroscopic surveys gives us comprehensive information about the Milky Way. Using the Bayesian isochrone-fitting code StarHorse, we derive distances and extinctions for more than…

2023 Astronomy and Astrophysics
Gaia 71
New high-precision strong lensing modeling of Abell 2744. Preparing for JWST observations
DOI: 10.1051/0004-6361/202244575 Bibcode: 2023A&A...670A..60B

Brammer, G.; Grillo, C.; Rosati, P. +8 more

We present a new strong lensing (SL) model of the Hubble Frontier Fields (HFF) galaxy cluster Abell 2744, at z = 0.3072, by exploiting archival Hubble Space Telescope (HST) multiband imaging and Multi Unit Spectroscopic Explorer (MUSE) follow-up spectroscopy. The lens model considers 90 spectroscopically confirmed multiple images (from 30 backgrou…

2023 Astronomy and Astrophysics
eHST 68
Gaia Data Release 3. The extragalactic content
DOI: 10.1051/0004-6361/202243232 Bibcode: 2023A&A...674A..41G

Prusti, T.; Mazeh, T.; Zucker, S. +445 more

The Gaia Galactic survey mission is designed and optimized to obtain astrometry, photometry, and spectroscopy of nearly two billion stars in our Galaxy. Yet as an all-sky multi-epoch survey, Gaia also observes several million extragalactic objects down to a magnitude of G ∼ 21 mag. Due to the nature of the Gaia onboard-selection algorithms, these …

2023 Astronomy and Astrophysics
Gaia 66
Closing in on the sources of cosmic reionization: First results from the GLASS-JWST program
DOI: 10.1051/0004-6361/202345866 Bibcode: 2023A&A...672A.155M

Vulcani, B.; Bradač, M.; Brammer, G. +29 more

The escape fraction of Lyman-continuum (LyC) photons (fesc) is a key parameter for determining the sources of cosmic reionization at z ≥ 6. At these redshifts, owing to the opacity of the intergalactic medium, the LyC emission cannot be measured directly. However, LyC leakers during the epoch of reionization could be identified using in…

2023 Astronomy and Astrophysics
eHST JWST 66
Deciphering the extreme X-ray variability of the nuclear transient eRASSt J045650.3−203750. A likely repeating partial tidal disruption event
DOI: 10.1051/0004-6361/202244805 Bibcode: 2023A&A...669A..75L

Gromadzki, M.; Liu, Z.; Buchner, J. +17 more

Context. During its all-sky survey, the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum-Roentgen-Gamma (SRG) observatory has uncovered a growing number of X-ray transients associated with the nuclei of quiescent galaxies. Benefitting from its large field of view and excellent sensitivity, the eROSITA window…

2023 Astronomy and Astrophysics
Gaia XMM-Newton 64
Gaia DR3 view of dynamical substructure in the stellar halo near the Sun
DOI: 10.1051/0004-6361/202244546 Bibcode: 2023A&A...670L...2D

Ruiz-Lara, Tomás; Helmi, Amina; Matsuno, Tadafumi +4 more

Context. Debris from past merger events is expected and also known, to some extent, to populate the stellar halo near the Sun.
Aims: We aim to identify and characterise such merger debris using Gaia DR3 data supplemented with metallicity and chemical abundance data from LAMOST LRS and APOGEE for halo stars within 2.5 kpc from the Sun.
Me…

2023 Astronomy and Astrophysics
Gaia 63
An empirical model of the Gaia DR3 selection function
DOI: 10.1051/0004-6361/202244784 Bibcode: 2023A&A...669A..55C

Hogg, David W.; Casey, Andrew R.; Rix, Hans-Walter +12 more

Interpreting and modelling astronomical catalogues requires an understanding of the catalogues' completeness or selection function: what properties determine an object's probability of being including in the catalogue? Here we set out to empirically quantify the completeness of the overall catalogue of Gaia's third data release (DR3). This task is…

2023 Astronomy and Astrophysics
Gaia 63
Gaia Data Release 3. The first Gaia catalogue of eclipsing-binary candidates
DOI: 10.1051/0004-6361/202245330 Bibcode: 2023A&A...674A..16M

Mazeh, T.; Audard, M.; Rimoldini, L. +11 more

Context. Gaia Data Release 3 (DR3) provides a number of new data products that complement the early DR3 made available two years ago. Among these is the first Gaia catalogue of eclipsing-binary candidates containing 2 184 477 sources with brightnesses from a few magnitudes to 20 mag in the Gaia G-band and covering the full sky.
Aims: We prese…

2023 Astronomy and Astrophysics
Gaia 62
Gaia Data Release 3. Apsis. III. Non-stellar content and source classification
DOI: 10.1051/0004-6361/202243423 Bibcode: 2023A&A...674A..31D

Hatzidimitriou, D.; Marshall, D. J.; Recio-Blanco, A. +78 more

Context. As part of the third Gaia Data Release, we present the contributions of the non-stellar and classification modules from the eighth coordination unit (CU8) of the Data Processing and Analysis Consortium, which is responsible for the determination of source astrophysical parameters using Gaia data. This is the third in a series of three pap…

2023 Astronomy and Astrophysics
Gaia 61