Search Publications

LQAC-6: Sixth Release of the Large Quasar Astrometric Catalogue. A compilation of 2 073 099 objects with 1 739 187 Gaia DR3 counterparts
DOI: 10.1051/0004-6361/202348505 Bibcode: 2024A&A...683A.112S

Barache, C.; Souchay, J.; Secrest, N. +1 more

Context. In addition to being objects of intense interest for cosmology and studies of the evolution of the universe, quasars are used to define quasi-inertial positions on the celestial sphere. Since its first publication in 2009, the purpose of the Large Quasar Astrometric Catalogue (LQAC) has been to provide the largest catalogue of bona fide q…

2024 Astronomy and Astrophysics
Gaia 1
New ephemerides and detection of transit-timing variations in the K2-138 system using high-precision CHEOPS photometry
DOI: 10.1051/0004-6361/202348013 Bibcode: 2024A&A...688A.192V

Deleuil, M.; Hoyer, S.; Sulis, S. +5 more

Context. Multi-planet systems are a perfect laboratory for constraining planetary formation models. A few of these systems present planets that come very close to mean motion resonance, potentially leading to significant transit-timing variations (TTVs) due to their gravitational interactions. Of these systems, K2-138 represents an excellent labor…

2024 Astronomy and Astrophysics
CHEOPS Gaia 1
First detection of the [CII] 158 µm line in the intermediate-velocity cloud Draco
DOI: 10.1051/0004-6361/202348349 Bibcode: 2024A&A...686A.109S

Ossenkopf-Okada, Volker; Simon, Robert; Klein, Bernd +7 more

High-latitude intermediate-velocity clouds (IVCs) are part of the Milky Way's H I halo and originate from either a galactic fountain process or extragalactic gas infall. They are partly molecular and can most of the time be identified in CO. Some of these regions also exhibit high-velocity cloud gas, which is mostly atomic, and gas at local veloci…

2024 Astronomy and Astrophysics
Herschel 1
Phase-resolved XMM-Newton observations of the massive post-RLOF system HD 149404
DOI: 10.1051/0004-6361/202348721 Bibcode: 2024A&A...686A.152R

Rauw, G.; Rosu, S.; Mossoux, E. +1 more

Context. We investigated the X-ray emission of HD 149404, a 9.81-day period O-star binary in a post-Roche lobe overflow evolutionary stage. X-ray emission of O-star binaries consists of the intrinsic emission of the individual O stars and a putative additional component arising from the wind-wind interaction.
Aims: Phase-locked variations in …

2024 Astronomy and Astrophysics
Gaia XMM-Newton 1
Spatial distributions of extreme-ultraviolet brightenings in the quiet Sun
DOI: 10.1051/0004-6361/202346886 Bibcode: 2024A&A...692A.236N

Barczynski, K.; Peter, H.; Müller, D. +16 more

Context. The identification of large numbers of localised transient extreme ultraviolet (EUV) brightenings, on very small spatial scales, in the quiet Sun corona has been one of the key early results from Solar Orbiter. However, there are still a great deal of unknowns about these events. Aims. In this work, we aim to better understand EUV brighte…

2024 Astronomy and Astrophysics
SolarOrbiter 1
The variation in the response of solar full-disc magnetographs
DOI: 10.1051/0004-6361/202450102 Bibcode: 2024A&A...688A..48Y

Solanki, S. K.; Yeo, K. L.; Krivova, N. A.

Context. The utility of full solar disc magnetograms as a long-term record of the photospheric magnetic field requires an understanding of how stable these observations are with time and the systematic differences between the various instruments.
Aims: We compared magnetograms from the KPVT/SPM, SoHO/MDI, SOLIS/VSM, and SDO/HMI with the aim o…

2024 Astronomy and Astrophysics
SOHO 1
KMT-2021-BLG-2609Lb and KMT-2022-BLG-0303Lb: Microlensing planets identified through signals produced by major-image perturbations
DOI: 10.1051/0004-6361/202450873 Bibcode: 2024A&A...689A.209H

Han, Cheongho; Lee, Chung-Uk; Zang, Weicheng +18 more

Aims. We investigate microlensing data collected by the Korea Microlensing Telescope Network (KMTNet) survey during the 2021 and 2022 seasons to identify planetary lensing events displaying a consistent anomalous pattern. Our investigation reveals that the light curves of two lensing events, KMT-2021-BLG-2609 and KMT-2022-BLG-0303, exhibit a simil…

2024 Astronomy and Astrophysics
eHST 1
A photometric and spectroscopic study of eight semi-detached eclipsing binaries
DOI: 10.1051/0004-6361/202449699 Bibcode: 2024A&A...692A.168L

Wang, Liang; Li, Kai; Yi, Tuan +3 more

Context. Semi-detached eclipsing binaries offer an exceptional opportunity to validate the evolutionary models of interacting binaries. This entails determining the absolute parameters and evaluating the evolutionary status of the binary components through simultaneous analysis of both light and radial velocity curves. The Transiting Exoplanet Sur…

2024 Astronomy and Astrophysics
Gaia 1
The unexpected role of heliospheric boundaries in facilitating interstellar dust penetration at 1-5 AU
DOI: 10.1051/0004-6361/202450257 Bibcode: 2024A&A...687L...4G

Izmodenov, V. V.; Godenko, E. A.


Aims: Interstellar dust (ISD) particles penetrate the heliosphere because of the relative motion of the local interstellar cloud and the Sun. The penetrated particles pass through the heliospheric interface, that is, the region in which solar wind and interstellar plasma interact. As a result, the ISD flow is modified after the passage throug…

2024 Astronomy and Astrophysics
Ulysses 1
DULAG: A DUal and Lensed AGN candidate catalog with the Gaia multipeak method
DOI: 10.1051/0004-6361/202452291 Bibcode: 2024A&A...692A.154W

Liao, S.; Mannucci, F.; Qi, Z. +2 more

Context. A series of studies have demonstrated that the Gaia multipeak (GMP) method is a very efficient technique for selecting active galactic nucleus (AGN) pair candidates. The number of candidates is determined by the size of the input AGN catalog, and is usually limited to spectroscopically confirmed objects. Aims. The objective of this work i…

2024 Astronomy and Astrophysics
Gaia 1