Search Publications

Structure and kinematics of a massive galaxy at z ∼ 7
DOI: 10.1051/0004-6361/202243399 Bibcode: 2023A&A...669A..46P

Bouwens, R. J.; Aravena, M.; Díaz-Santos, T. +9 more

Context. Observations of the rest-frame UV emission of high-redshift galaxies suggest that the early stages of galaxy formation involve disturbed structures. Imaging the cold interstellar medium (ISM) can provide a unique view of the kinematics associated with the assembly of galaxies.
Aims: In this paper, we analyze the spatial distribution …

2023 Astronomy and Astrophysics
Gaia eHST 31
Gaia Data Release 3. Validating the classification of variable young stellar object candidates
DOI: 10.1051/0004-6361/202244101 Bibcode: 2023A&A...674A..21M

Gavras, Panagiotis; Ábrahám, Péter; Kóspál, Ágnes +14 more

Context. The Gaia third Data Release (DR3) presents the first catalogue of full-sky variable young stellar object (YSO) candidates observed by the Gaia space telescope during the initial 34 months of science operations.
Aims: Numerous types of variable stars were classified using photometric data collected by Gaia. One of the new classes pres…

2023 Astronomy and Astrophysics
Gaia 30
JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies
DOI: 10.1051/0004-6361/202346673 Bibcode: 2023A&A...677A..34G

Papovich, Casey; Finkelstein, Steven L.; Buat, Véronique +38 more

In recent years, observations have uncovered a population of massive galaxies that are invisible or very faint in deep optical/near-infrared (near-IR) surveys but brighter at longer wavelengths. However, the nature of these optically dark or faint galaxies (OFGs; one of several names given to these objects) is highly uncertain. In this work, we in…

2023 Astronomy and Astrophysics
Gaia eHST JWST 30
Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
DOI: 10.1051/0004-6361/202245105 Bibcode: 2023A&A...672A.106L

Zhang, Zhi-Yu; Lelli, Federico; Bisbas, Thomas G. +6 more

We study the dynamics of cold molecular gas in two main-sequence galaxies at cosmic noon (zC-488879 at z ≃ 1.47 and zC-400569 at z ≃ 2.24) using new high-resolution ALMA observations of multiple 12CO transitions. For zC-400569 we also reanalyze high-quality Hα data from the SINS/zC-SINF survey. We find that (1) both galaxies have regula…

2023 Astronomy and Astrophysics
eHST 30
The phase spiral in Gaia DR3
DOI: 10.1051/0004-6361/202245518 Bibcode: 2023A&A...673A.115A

Katz, D.; Antoja, T.; Bernet, M. +3 more


Aims: We aim to study the phase spiral in the Milky Way (MW) disc with data from the third data release of Gaia (DR3) and use it as an inference tool to decipher the late-time evolution of the Galaxy.
Methods: We used an edge-detection algorithm to find the border of the phase spiral, allowing us to robustly quantify its shape at differe…

2023 Astronomy and Astrophysics
Gaia 30
The massive relic galaxy NGC 1277 is dark matter deficient. From dynamical models of integral-field stellar kinematics out to five effective radii
DOI: 10.1051/0004-6361/202346291 Bibcode: 2023A&A...675A.143C

Trujillo, Ignacio; Cappellari, Michele; Buitrago, Fernando +7 more

According to the Λ cold dark matter (ΛCDM) cosmology, present-day galaxies with stellar masses M > 1011 M should contain a sizable fraction of dark matter within their stellar body. Models indicate that in massive early-type galaxies (ETGs) with M ≈ 1.5 × 1011 M, dark matter …

2023 Astronomy and Astrophysics
eHST 30
Gaia Data Release 3. Reflectance spectra of Solar System small bodies
DOI: 10.1051/0004-6361/202243791 Bibcode: 2023A&A...674A..35G

Prusti, T.; Mazeh, T.; Zucker, S. +444 more

Context. The Gaia mission of the European Space Agency (ESA) has been routinely observing Solar System objects (SSOs) since the beginning of its operations in August 2014. The Gaia data release three (DR3) includes, for the first time, the mean reflectance spectra of a selected sample of 60 518 SSOs, primarily asteroids, observed between August 5,…

2023 Astronomy and Astrophysics
Gaia 30
Supermassive Black Hole Winds in X-rays: SUBWAYS. I. Ultra-fast outflows in quasars beyond the local Universe
DOI: 10.1051/0004-6361/202245036 Bibcode: 2023A&A...670A.182M

Maiolino, R.; Merloni, A.; Fiore, F. +49 more

We present a new X-ray spectroscopic study of 22 luminous (2 × 1045 ≲ Lbol/erg s−1 ≲ 2 × 1046) active galactic nuclei (AGNs) at intermediate redshifts (0.1 ≲ z ≲ 0.4), as part of the SUpermassive Black hole Winds in the x-rAYS (SUBWAYS) sample, mostly composed of quasars and type 1 AGNs. Here, 17 targets…

2023 Astronomy and Astrophysics
XMM-Newton 30
An updated measurement of the Hubble constant from near-infrared observations of Type Ia supernovae
DOI: 10.1051/0004-6361/202244893 Bibcode: 2023A&A...679A..95G

Leibundgut, B.; Galbany, L.; Dhawan, S. +12 more

We present a measurement of the Hubble constant (H0) using type Ia supernovae (SNe Ia) in the near-infrared (NIR) from the recently updated sample of SNe Ia in nearby galaxies with distances measured via Cepheid period-luminosity relations by the SH0ES project. We collected public near-infrared photometry of up to 19 calibrator SNe Ia a…

2023 Astronomy and Astrophysics
eHST 29
A state-of-the-art strong-lensing model of MACS J0416.1−2403 with the largest sample of spectroscopic multiple images
DOI: 10.1051/0004-6361/202244834 Bibcode: 2023A&A...674A..79B

Grillo, C.; Rosati, P.; Vanzella, E. +9 more

The combination of multi-band imaging from the Hubble Space Telescope with Multi-Unit Spectroscopic Explorer integral field spectroscopy, obtained at the Very Large Telescope, has recently driven remarkable progress in strong-lensing (SL) modeling of galaxy clusters. From a few tens of multiple images with photometric redshifts per cluster, a new …

2023 Astronomy and Astrophysics
eHST 29