Search Publications

The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products
DOI: 10.1051/0004-6361/202243134 Bibcode: 2022A&A...666A.120G

Prusti, T.; Hatzidimitriou, D.; Gilmore, G. +165 more

Context. The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100 000 stars, including large representative samples of the stellar populations in the Galaxy, and a well-defined sample of 60 (plus 20 archive) open clusters. We provide internally consistent results …

2022 Astronomy and Astrophysics
Gaia 107
The eROSITA Final Equatorial-Depth Survey (eFEDS). Identification and characterization of the counterparts to point-like sources
DOI: 10.1051/0004-6361/202141631 Bibcode: 2022A&A...661A...3S

Finoguenov, A.; Georgakakis, A.; Salvato, M. +40 more

Context. In November 2019, eROSITA on board of the Spektrum-Roentgen-Gamma (SRG) observatory started to map the entire sky in X-rays. After the four-year survey program, it will reach a flux limit that is about 25 times deeper than ROSAT. During the SRG performance verification phase, eROSITA observed a contiguous 140 deg2 area of the s…

2022 Astronomy and Astrophysics
Gaia XMM-Newton 105
The MeerKAT Galaxy Cluster Legacy Survey. I. Survey Overview and Highlights
DOI: 10.1051/0004-6361/202141488 Bibcode: 2022A&A...657A..56K

Tasse, C.; Heywood, I.; Camilo, F. +148 more

MeerKAT's large number (64) of 13.5 m diameter antennas, spanning 8 km with a densely packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity over a wide range of angular scales. The MeerKAT Galaxy Cluster Legacy Survey (MGCLS) is a programme of long-track MeerKAT L-band (900−1670 MHz) observations of 115 galaxy…

2022 Astronomy and Astrophysics
Gaia XMM-Newton 104
PARSEC V2.0: Stellar tracks and isochrones of low- and intermediate-mass stars with rotation
DOI: 10.1051/0004-6361/202244166 Bibcode: 2022A&A...665A.126N

Chen, Y.; Bressan, A.; Girardi, L. +6 more

We present a new comprehensive collection of stellar evolutionary tracks and isochrones for rotating low- and intermediate-mass stars assembled with the updated version of PARSEC V2.0. This version includes our recent calibration of the extra mixing from overshooting and rotation, as well as several improvements regarding the nuclear reaction netw…

2022 Astronomy and Astrophysics
Gaia 102
Hunting for open clusters in Gaia EDR3: 628 new open clusters found with OCfinder
DOI: 10.1051/0004-6361/202142568 Bibcode: 2022A&A...661A.118C

Castro-Ginard, A.; Jordi, C.; Luri, X. +6 more

Context. The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia DR2, particularly for parallaxes and proper motions, offer the opportunity to increase the number of known open clusters in the Milky Way by detecting farther and fainter objects that have thus far gone unnoticed.
Aims: Our aim is to continue to…

2022 Astronomy and Astrophysics
Gaia 98
The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds
DOI: 10.1051/0004-6361/202142742 Bibcode: 2022A&A...663A..36B

Sana, Hugues; Vink, Jorick S.; Kaper, Lex +17 more

Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of massive stars, including the most massive stars known. The strong stellar winds of these very luminous stars impact their evolution and the surrounding environment. We currently lack detailed knowledge of the wind structure that is needed to quantify this i…

2022 Astronomy and Astrophysics
eHST 92
A tale of two DIGs: The relative role of H II regions and low-mass hot evolved stars in powering the diffuse ionised gas (DIG) in PHANGS-MUSE galaxies
DOI: 10.1051/0004-6361/202141859 Bibcode: 2022A&A...659A..26B

Boquien, M.; Chevance, M.; Kruijssen, J. M. Diederik +17 more

We use integral field spectroscopy from the PHANGS-MUSE survey, which resolves the ionised interstellar medium structure at ∼50 pc resolution in 19 nearby spiral galaxies, to study the origin of the diffuse ionised gas (DIG). We examine the physical conditions of the diffuse gas by first removing morphologically defined H II regions and then binni…

2022 Astronomy and Astrophysics
Gaia 91
Structural parameters of 389 local open clusters
DOI: 10.1051/0004-6361/202142186 Bibcode: 2022A&A...659A..59T

Miret-Roig, N.; Castro-Ginard, A.; Casamiquela, L. +4 more

Context. The distribution of member stars in the surroundings of an open cluster (OC) can shed light on the process of its formation, evolution, and dissolution. The analysis of structural parameters of OCs as a function of their age and position in the Galaxy constrains theoretical models of cluster evolution. The Gaia catalog is very appropriate…

2022 Astronomy and Astrophysics
Gaia 89
Gaia Early Data Release 3. The celestial reference frame (Gaia-CRF3)
DOI: 10.1051/0004-6361/202243483 Bibcode: 2022A&A...667A.148G

Prusti, T.; Mazeh, T.; Zucker, S. +448 more

Context. Gaia-CRF3 is the celestial reference frame for positions and proper motions in the third release of data from the Gaia mission, Gaia DR3 (and for the early third release, Gaia EDR3, which contains identical astrometric results). The reference frame is defined by the positions and proper motions at epoch 2016.0 for a specific set of extrag…

2022 Astronomy and Astrophysics
Gaia 87
GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
DOI: 10.1051/0004-6361/202141615 Bibcode: 2022A&A...658A..43G

Magnelli, B.; Daddi, E.; Elbaz, D. +35 more

Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally occurs in compact regions smaller than the stellar distribution. However, it remains to be understood how systematic these findings are. Studies often lack homogeneity i…

2022 Astronomy and Astrophysics
eHST 81