Search Publications

STEPARSYN: A Bayesian code to infer stellar atmospheric parameters using spectral synthesis
DOI: 10.1051/0004-6361/202141763 Bibcode: 2022A&A...657A..66T

Montes, D.; González Hernández, J. I.; Tabernero, H. M. +1 more

Context. STEPARSYN is an automatic code written in Python 3.X designed to infer the stellar atmospheric parameters Teff, log g, and [Fe/H] of FGKM-type stars following the spectral synthesis method.
Aims: We present a description of the STEPARSYN code and test its performance against a sample of late-type stars that were observed w…

2022 Astronomy and Astrophysics
Gaia 45
Substructure in the stellar halo near the Sun. II. Characterisation of independent structures
DOI: 10.1051/0004-6361/202243061 Bibcode: 2022A&A...665A..58R

Koppelman, H. H.; Helmi, A.; Ruiz-Lara, T. +3 more

Context. In an accompanying paper, we present a data-driven method for clustering in `integrals of motion' space and apply it to a large sample of nearby halo stars with 6D phase-space information. The algorithm identified a large number of clusters, many of which could tentatively be merged into larger groups.
Aims: The goal here is to estab…

2022 Astronomy and Astrophysics
Gaia 44
Two temperate super-Earths transiting a nearby late-type M dwarf
DOI: 10.1051/0004-6361/202244041 Bibcode: 2022A&A...667A..59D

Tamura, M.; Kudo, T.; Bouchy, F. +82 more

Context. In the age of JWST, temperate terrestrial exoplanets transiting nearby late-type M dwarfs provide unique opportunities for characterising their atmospheres, as well as searching for biosignature gases. In this context, the benchmark TRAPPIST-1 planetary system has garnered the interest of a broad scientific community.
Aims: We report…

2022 Astronomy and Astrophysics
Gaia 43
First JWST observations of a gravitational lens. Mass model from new multiple images with near-infrared observations of SMACS J0723.3−7327
DOI: 10.1051/0004-6361/202244517 Bibcode: 2022A&A...666L...9C

Brammer, G.; Vanzella, E.; Mercurio, A. +4 more

We present our lens mass model of SMACS J0723.3−7327, the first strong gravitational lens observed by the James Webb Space Telescope (JWST). We use data from the Hubble Space Telescope and the Multi Unit Spectroscopic Explorer (MUSE) to build our `pre-JWST' lens model and then refine it with newly available JWST near-infrared imaging in our JWST m…

2022 Astronomy and Astrophysics
eHST JWST 43
Hot subdwarfs in close binaries observed from space. I. Orbital, atmospheric, and absolute parameters, and the nature of their companions
DOI: 10.1051/0004-6361/202244214 Bibcode: 2022A&A...666A.182S

Geier, S.; Pelisoli, I.; Schaffenroth, V. +2 more

Context. About a third of the hot subdwarfs of spectral type B (sdBs), which are mostly core-helium-burning objects on the extreme horizontal branch, are found in close binaries with cool, low-mass stellar, substellar, or white dwarf companions. They can show light variations due to different phenomena.
Aims: Many hot subdwarfs now have space…

2022 Astronomy and Astrophysics
Gaia 42
Planet populations inferred from debris discs. Insights from 178 debris systems in the ISPY, LEECH, and LIStEN planet-hunting surveys
DOI: 10.1051/0004-6361/202142720 Bibcode: 2022A&A...659A.135P

Gennaro, Mario; Launhardt, Ralf; Kennedy, Grant M. +11 more

We know little about the outermost exoplanets in planetary systems because our detection methods are insensitive to moderate-mass planets on wide orbits. However, debris discs can probe the outer-planet population because dynamical modelling of observed discs can reveal properties of perturbing planets. We use four sculpting and stirring arguments…

2022 Astronomy and Astrophysics
AKARI Gaia 42
Substructure in the stellar halo near the Sun. I. Data-driven clustering in integrals-of-motion space
DOI: 10.1051/0004-6361/202243060 Bibcode: 2022A&A...665A..57L

Koppelman, H. H.; Helmi, A.; Ruiz-Lara, T. +3 more

Context. Merger debris is expected to populate the stellar haloes of galaxies. In the case of the Milky Way, this debris should be apparent as clumps in a space defined by the orbital integrals of motion of the stars.
Aims: Our aim is to develop a data-driven and statistics-based method for finding these clumps in integrals-of-motion space fo…

2022 Astronomy and Astrophysics
Gaia 41
Low-power jet-interstellar medium interaction in NGC 7319 revealed by JWST/MIRI MRS
DOI: 10.1051/0004-6361/202244725 Bibcode: 2022A&A...665L..11P

Colina, L.; Hönig, S. F.; García-Burillo, S. +8 more

We present JWST/MIRI MRS spectroscopy of NGC 7319, the largest galaxy in the Stephan's Quintet, observed as part of the Early Release Observations (ERO). NGC 7319 hosts a type 2 active galactic nucleus (AGN) and a low-power radio jet (L1.4 GHz = 3.3 × 1022 W Hz−1) with two asymmetric radio hotspots at 430 pc (N2) a…

2022 Astronomy and Astrophysics
eHST JWST 41
The first ground-level enhancement of solar cycle 25 on 28 October 2021
DOI: 10.1051/0004-6361/202142855 Bibcode: 2022A&A...660L...5P

Usoskin, I.; Vainio, R.; Gieseler, J. +8 more


Aims: The first relativistic solar proton event of solar cycle 25 was detected on 28 October 2021 by neutron monitors (NMs) on the ground and particle detectors on board spacecraft in near-Earth space. This is the first ground-level enhancement (GLE) of the current cycle. A detailed reconstruction of the NM response together with the identifi…

2022 Astronomy and Astrophysics
SOHO 41
GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching
DOI: 10.1051/0004-6361/202142352 Bibcode: 2022A&A...659A.196G

Magnelli, B.; Daddi, E.; Elbaz, D. +38 more

Compact star formation appears to be generally common in dusty star-forming galaxies (SFGs). However, its role in the framework set by the scaling relations in galaxy evolution remains to be understood. In this work we follow up on the galaxy sample from the GOODS-ALMA 2.0 survey, an ALMA blind survey at 1.1 mm covering a continuous area of 72.42 …

2022 Astronomy and Astrophysics
eHST 41