Search Publications

Dust and power: Unravelling the merger-active galactic nucleus connection in the second half of cosmic history
DOI: 10.1051/0004-6361/202348188 Bibcode: 2024A&A...690A.326L

Wang, L.; Davé, R.; Yang, G. +8 more

Aims. Galaxy mergers represent a fundamental physical process under hierarchical structure formation, but their role in triggering active galactic nuclei (AGNs) is still unclear. We aim to investigate the merger-AGN connection using state-of-the-art observations and novel methods for detecting mergers and AGNs. Methods. We selected stellar mass-li…

2024 Astronomy and Astrophysics
Herschel 9
Broadband X-ray/UV/optical time-resolved spectroscopy of NGC 5548: The origin of the UV/optical variability in active galactic nuclei
DOI: 10.1051/0004-6361/202348686 Bibcode: 2024A&A...686A..69K

Papadakis, I. E.; Dovčiak, M.; Kammoun, E. +1 more

Context. Recently, nearby bright galaxies have been the subject of long monitoring surveys in the X-rays, UV, and optical. All of these campaigns revealed a strong correlation between the various UV and optical bands, with time lags that increase with wavelength. In a series of papers, we have demonstrated that a scenario in which an X-ray source …

2024 Astronomy and Astrophysics
eHST 9
Investigating episodic mass loss in evolved massive stars. I. Spectroscopy of dusty massive stars in ten southern galaxies
DOI: 10.1051/0004-6361/202348527 Bibcode: 2024A&A...686A..77B

Zapartas, E.; de Wit, S.; Bonanos, A. Z. +7 more

Context. Episodic mass-loss events such as giant eruptions in luminous blue variables or pre-supernova eruptions in red supergiants drastically alter the evolutionary path of a massive star, resulting in a rich and complex circumstellar environment and IR excess. However, the incidence of these events, and hence their importance in massive star ev…

2024 Astronomy and Astrophysics
Gaia eHST 9
A 500 pc volume-limited sample of hot subluminous stars. I. Space density, scale height, and population properties
DOI: 10.1051/0004-6361/202348319 Bibcode: 2024A&A...686A..25D

Geier, S.; Kepler, S. O.; Heber, U. +25 more

We present the first volume-limited sample of spectroscopically confirmed hot subluminous stars out to 500 pc, defined using the accurate parallax measurements from the Gaia space mission data release 3 (DR3). The sample comprises a total of 397 members, with 305 (~77%) identified as hot subdwarf stars, including 83 newly discovered systems. Of th…

2024 Astronomy and Astrophysics
Gaia 9
TESS and ESPRESSO discover a super-Earth and a mini-Neptune orbiting the K-dwarf TOI-238*
DOI: 10.1051/0004-6361/202348958 Bibcode: 2024A&A...685A..56S

Bouchy, F.; Rebolo, R.; Pallé, E. +53 more

The number of super-Earth and mini-Neptune planet discoveries has increased significantly in the last two decades thanks to transit and radial velocity (RV) surveys. When it is possible to apply both techniques, we can characterise the internal composition of exoplanets, which in turn provides unique insights on their architecture, formation and e…

2024 Astronomy and Astrophysics
Gaia 9
The VISTA Variables in the Vía Láctea extended (VVVX) ESO public survey: Completion of the observations and legacy
DOI: 10.1051/0004-6361/202450584 Bibcode: 2024A&A...689A.148S

Tamura, M.; Schultheis, M.; Minniti, D. +143 more

Context. The ESO public survey VISTA Variables in the Vía Láctea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from 2009–2015. Upon its conclusion, the complementary VVV extended (VVVX) survey has expanded both the temporal as well as spatial coverage of the original VVV area, widening it from 562 to 1700 sq. deg.…

2024 Astronomy and Astrophysics
JWST 9
Tracing the rise of supermassive black holes. A panchromatic search for faint, unobscured quasars at z ≳ 6 with COSMOS-Web and other surveys
DOI: 10.1051/0004-6361/202349025 Bibcode: 2024A&A...685A..25A

Casey, Caitlin M.; Koekemoer, Anton M.; Wilkins, Stephen M. +20 more

We report the identification of 64 new candidates of compact galaxies, potentially hosting faint quasars with bolometric luminosities of Lbol = 1043-1046 erg s−1, residing in the reionization epoch within the redshift range of 6 ≲ z ≲ 8. These candidates were selected by harnessing the rich multiband dat…

2024 Astronomy and Astrophysics
Gaia eHST JWST 9
PDRs4All: X. ALMA and JWST detection of neutral carbon in the externally irradiated disk d203-506: Undepleted gas-phase carbon
DOI: 10.1051/0004-6361/202450988 Bibcode: 2024A&A...689L...4G

Le Bourlot, J.; Le Petit, F.; Roueff, E. +26 more

The gas-phase abundance of carbon, xC = [C/H]gas = xC+ + xC0 + xCO + … , and its depletion factors are essential parameters for understanding the gas and solid compositions that are ultimately incorporated into (exo)planets. The majority of protoplanetary disks are born i…

2024 Astronomy and Astrophysics
JWST 9
Separation of dust emission from the cosmic infrared background in Herschel observations with wavelet phase harmonics
DOI: 10.1051/0004-6361/202346814 Bibcode: 2024A&A...681A...1A

Miville-Deschênes, Marc-Antoine; Béthermin, Matthieu; Lagache, Guilaine +7 more

The low-brightness dust emission at high Galactic latitudes is of interest with respect to studying the interplay among the physical processes involved in shaping the structure of the interstellar medium (ISM), as well as in statistical characterizations of the dust emission as a foreground to the cosmic microwave background (CMB). Progress in thi…

2024 Astronomy and Astrophysics
Herschel 9
TOI-4860 b, a short-period giant planet transiting an M3.5 dwarf
DOI: 10.1051/0004-6361/202346999 Bibcode: 2024A&A...683A.166A

Bouchy, F.; Moutou, C.; Carmona, A. +47 more

We report the discovery and characterisation of a giant transiting planet orbiting a nearby M3.5V dwarf (d = 80.4pc, G = 15.1 mag, K=11.2mag, R* = 0.358 ± 0.015 R, M* = 0.340 ± 0.009 M). Using the photometric time series from TESS sectors 10, 36, 46, and 63 and near-infrared spectrophotometry from ExTr…

2024 Astronomy and Astrophysics
Gaia 9