Search Publications

Characterising the interior of five inner Saturnian moons using Cassini ISS data
DOI: 10.1051/0004-6361/202244757 Bibcode: 2023A&A...670L..25L

Lainey, V.; Rambaux, N.; Zhang, Q. +2 more

Context. The Cassini-Huygens space mission provided a huge amount of data for the Saturnian system. While the mission ended in September 2017, there is still much information to be retrieved from the data.
Aims: Here, from their orbital motion, we infer the interior of the five inner Saturnian moons, Atlas, Prometheus, Pandora, Janus, and Epi…

2023 Astronomy and Astrophysics
Cassini 2
L 363-38 b: A planet newly discovered with ESPRESSO orbiting a nearby M dwarf star
DOI: 10.1051/0004-6361/202244347 Bibcode: 2023A&A...670A..42S

Sartori, Lia F.; Lendl, Monika; Cugno, Gabriele +7 more

Context. Planets around stars in the solar neighbourhood will be prime targets for characterisation with upcoming large space- and ground-based facilities. Since large-scale exoplanet searches will not be feasible with such telescopes, it is crucial to use currently available data and instruments to find possible target planets before next-generat…

2023 Astronomy and Astrophysics
Gaia 2
VISIONS: the VISTA Star Formation Atlas. II. The data processing pipeline
DOI: 10.1051/0004-6361/202245772 Bibcode: 2023A&A...673A..59M

Meingast, Stefan; Rottensteiner, Alena; Bouy, Hervé +3 more

The VISIONS public survey provides large-scale, multi-epoch imaging of five nearby star-forming regions at sub-arcsecond resolution in the near-infrared. All data collected within the program and provided by the European Southern Observatory (ESO) science archive are processed with a custom end-to-end pipeline infrastructure to provide science-rea…

2023 Astronomy and Astrophysics
Gaia 2
Investigating the vertical distribution of the disk as a function of radial action
DOI: 10.1051/0004-6361/202142977 Bibcode: 2023A&A...669A.107J

Zhao, Gang; Chen, Yuqin; Du, Cuihua +1 more


Aims: As heating processes can broaden the distributions of radial actions and the vertical distributions of the Galactic disks, we investigate the vertical distribution of the Galactic disks as a function of radial action based on Apache Point Observatory Galactic Evolution Experiment (APOGEE) and Gaia data in order to deepen our understandi…

2023 Astronomy and Astrophysics
Gaia 2
New members of the Lupus I cloud based on Gaia astrometry. Physical and accretion properties from X-shooter spectra
DOI: 10.1051/0004-6361/202245261 Bibcode: 2023A&A...671A..46M

Bayo, A.; Alcalá, J. M.; Montalto, M. +13 more

We characterize twelve young stellar objects (YSOs) located in the Lupus I region, spatially overlapping with the Upper Centaurus Lupus (UCL) sub-stellar association. The aim of this study is to understand whether the Lupus I cloud has more members than what has been claimed so far in the literature and gain a deeper insight into the global proper…

2023 Astronomy and Astrophysics
Gaia 2
A multifrequency characterization of the extragalactic hard X-ray sky. Presenting the second release of the Turin-SyCAT
DOI: 10.1051/0004-6361/202243848 Bibcode: 2023A&A...670A.171K

Masetti, N.; Chavushyan, V.; Bottacini, E. +5 more

Context. Nowadays, we know that the origin of the cosmic X-ray background (CXB) is mainly due to the integrated emission of active galactic nuclei. Therefore, in order to obtain a precise estimate of the contribution of different source classes to the CXB, it is crucial to achieve full characterization of the hard-X ray sky.
Aims: We present …

2023 Astronomy and Astrophysics
INTEGRAL 2
Analysis of minimum ionising particles and soft protons using XMM-Newton EPIC pn-CCD as a particle detector
DOI: 10.1051/0004-6361/202244421 Bibcode: 2023A&A...670A..78B

Freyberg, M. J.; Kirsch, M. G. F.; Bender, V. +1 more

Context. Spacecrafts with imaging telescopes often carry a charge-coupled device (CCD) in their focal plane to detect electromagnetic radiation. Charged particles such as electrons, protons, and heavy ions can reach the CCD and deposit their energy in the detector material. To counteract this undesirable effect, algorithms are usually implemented …

2023 Astronomy and Astrophysics
Gaia XMM-Newton 2
The kinematics of the magnetized protostellar core IRAS15398-3359
DOI: 10.1051/0004-6361/202244861 Bibcode: 2023A&A...672A..72T

Caselli, Paola; Redaelli, Elena; Tabatabaei, Farideh S. +1 more

Context. Observations of protostellar envelopes are essential in order to understand better the process of gravitational collapse toward star and planet formation. From a theoretical perspective, magnetic fields are considered an important factor during the early stages of star formation, especially during the main accretion phase.
Aims: Our …

2023 Astronomy and Astrophysics
Herschel 2
The equilibrium shape of (65) Cybele: primordial or relic of a large impact?
DOI: 10.1051/0004-6361/202243859 Bibcode: 2023A&A...670A..52M

Jorda, L.; Carry, B.; Molina, D. +24 more

Context. Cybele asteroids constitute an appealing reservoir of primitive material genetically linked to the outer Solar System, and the physical properties (size and shape) of the largest members can be readily accessed by large (8m class) telescopes.
Aims: We took advantage of the bright apparition of the most iconic member of the Cybele pop…

2023 Astronomy and Astrophysics
AKARI 2
Stellar angular momentum of disk galaxies at z ≈ 0.7 in the MAGIC survey. I. Impact of the environment
DOI: 10.1051/0004-6361/202346700 Bibcode: 2023A&A...677A.143M

Ciesla, L.; Krajnović, D.; Lemaux, B. C. +6 more


Aims: At intermediate redshift, galaxy groups and clusters are thought to impact galaxy properties such as their angular momentum. We investigate whether the environment has an impact on the galaxies' stellar angular momentum and identify underlying driving physical mechanisms.
Methods: We derived robust estimates of the stellar angular …

2023 Astronomy and Astrophysics
eHST 2