Search Publications

Discovery of two promising isolated neutron star candidates in the SRG/eROSITA All-Sky Survey
DOI: 10.1051/0004-6361/202346375 Bibcode: 2023A&A...674A.155K

Haberl, F.; Buckley, D. A. H.; Pires, A. M. +2 more

We report the discovery of the isolated neutron star (INS) candidates eRASSU J065715.3+260428 and eRASSU J131716.9−402647 from the Spectrum Roentgen Gamma (SRG) eROSITA All-Sky Survey. Selected for their soft X-ray emission and absence of catalogued counterparts, both objects were recently targeted with the La…

2023 Astronomy and Astrophysics
Gaia 7
A multi-technique approach to identifying and/or constraining radial-velocity substellar companions
DOI: 10.1051/0004-6361/202346612 Bibcode: 2023A&A...678A.107P

Kiefer, F.; Lagrange, A. -M.; Rubini, P. +3 more

Context. Although more than one thousand substellar companions have already been detected with the radial velocity (RV) method, many new companions remain to be detected in the public RV archives.
Aims: We wish to use the archival data obtained with the ESO/HARPS spectrograph to search for substellar companions.
Methods: We used the astr…

2023 Astronomy and Astrophysics
Gaia Hipparcos 7
Identifying Lyα emitter candidates with Random Forest: Learning from galaxies in the CANDELS survey
DOI: 10.1051/0004-6361/202347026 Bibcode: 2023A&A...677A.138N

Castellano, M.; Pentericci, L.; Fynbo, J. P. U. +8 more

The physical processes that make a galaxy a Lyman alpha emitter have been extensively studied over the past 25 yr. However, the correlations between physical and morphological properties of galaxies and the strength of the Lyα emission line are still highly debated. Here, we investigate the correlations between the rest-frame Lyα equivalent width …

2023 Astronomy and Astrophysics
eHST 7
A sub-Neptune planet around TOI-1695 discovered and characterized with SPIRou and TESS
DOI: 10.1051/0004-6361/202245129 Bibcode: 2023A&A...670A.136K

Carmona, A.; Donati, J. -F.; Winn, J. N. +39 more

TOI-1695 is a V-mag = 13 M-dwarf star from the northern hemisphere at 45 pc from the Sun, around which a 3.134-day periodic transit signal from a super-Earth candidate was identified in TESS photometry. With a transit depth of 1.3 mmag, the radius of candidate TOI-1695.01 was estimated by the TESS pipeline to be 1.82 R with an equilibr…

2023 Astronomy and Astrophysics
Gaia 7
Milky Way globular clusters on cosmological timescales. II. Interaction with the Galactic centre
DOI: 10.1051/0004-6361/202245753 Bibcode: 2023A&A...674A..70I

Berczik, Peter; Ishchenko, Maryna; Sobolenko, Margaryta +2 more


Aims: We estimate the dynamical evolution of the interaction of globular clusters' with the Galactic centre that dynamically changed in the past.
Methods: We simulated the orbits of 147 globular clusters over a 10 Gyr lookback time using the parallel N-body code `φ-GPU'. For each globular cluster, we generated 1000 sets of initial data w…

2023 Astronomy and Astrophysics
Gaia 7
Unbound stars hold the key to young star cluster history
DOI: 10.1051/0004-6361/202245242 Bibcode: 2023A&A...670A.128A

Pfalzner, Susanne; Arunima, Arunima; Govind, Amith

Aims.Gaia delivers the positions and velocities of stars at an unprecedented precision. Therefore, for star clusters, there exists much higher confidence in whether a specific star is a member of a particular cluster or not. However, membership determination is still especially challenging for young star clusters. At ages 2−10 Myr, the gas is expe…

2023 Astronomy and Astrophysics
Gaia 7
TOI-1801 b: A temperate mini-Neptune around a young M0.5 dwarf
DOI: 10.1051/0004-6361/202347346 Bibcode: 2023A&A...680A..76M

Nagel, E.; Amado, P. J.; Caballero, J. A. +79 more

We report the discovery, mass, and radius determination of TOI-1801 b, a temperate mini-Neptune around a young M dwarf. TOI-1801 b was observed in TESS sectors 22 and 49, and the alert that this was a TESS planet candidate with a period of 21.3 days went out in April 2020. However, ground-based follow-up observations, including seeing-limited phot…

2023 Astronomy and Astrophysics
AKARI Gaia 7
Gaia Focused Product Release: Asteroid orbital solution. Properties and assessment
DOI: 10.1051/0004-6361/202347270 Bibcode: 2023A&A...680A..37G

Prusti, T.; Mazeh, T.; Zucker, S. +403 more

Context. We report the exploitation of a sample of Solar System observations based on data from the third Gaia Data Release (Gaia DR3) of nearly 157 000 asteroids. It extends the epoch astrometric solution over the time coverage planned for the Gaia DR4, which is not expected before the end of 2025. This data set covers more than one full orbital …

2023 Astronomy and Astrophysics
Gaia 7
Quiet-time suprathermal ions in the inner heliosphere during the rising phase of solar cycle 25
DOI: 10.1051/0004-6361/202345978 Bibcode: 2023A&A...673L..12M

Wimmer-Schweingruber, R. F.; Allen, R. C.; Ho, G. C. +3 more

Context. The Solar Orbiter spacecraft made its first close perihelion passes in 2022, reaching 0.32 au on 26 March and 0.29 au on 12 October. Transient activity was relatively low, making it possible to perform measurements of the quiet-time suprathermal ion pool over multi-day periods.
Aims: The inner heliosphere suprathermal ion pool is a s…

2023 Astronomy and Astrophysics
SolarOrbiter 7
Identifying preflare spectral features using explainable artificial intelligence
DOI: 10.1051/0004-6361/202244835 Bibcode: 2023A&A...671A..73P

Kleint, Lucia; Panos, Brandon; Zbinden, Jonas

The prediction of solar flares is of practical and scientific interest; however, many machine learning methods used for this prediction task do not provide the physical explanations behind a model's performance. We made use of two recently developed explainable artificial intelligence techniques called gradient-weighted class activation mapping (G…

2023 Astronomy and Astrophysics
IRIS 7