output
20132026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

52 papers

astro-ph.SR2026

Discovery of sulfur oxides in the ejecta of a B[e] supergiant

C. Bordiu, J. Ricardo Rizzo, D. Navarro-Almaida +12

B[e] supergiants represent a rare class of luminous, evolved massive stars surrounded by dusty circumstellar disks. Since their intense UV fields were long thought to sterilize the…

astro-ph.EP2026

ExoDNN: Boosting exoplanet detection with artificial intelligence. Application to Gaia Data Release 3

A. Abreu, J. Lillo-Box, A. M. Perez-Garcia +3

We combine Gaia Data Release 3 and artificial intelligence to enhance the current statistics of substellar companions, particularly within regions of the orbital period vs. mass pa…

astro-ph.GA2025★ 1 cited

GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster ZwCl 0024.0+1652 at z~0.4. III. The mass-SFR relation and the quenching of cluster galaxies

Simon B. De Daniloff, Ángel Bongiovanni, Miguel Sánchez-Portal +21

Galaxy clusters are among the largest and densest structures in the Universe. Their high density generally increases the suppression of star formation, known as quenching, altering…

astro-ph.GA2025★ 1 cited

MeerKAT discovery of 164 compact radio rings toward the Galactic Plane

C. Bordiu, F. Bufano, G. Umana +14

We report the discovery of 164 compact (radius < 1 arcmin) radio rings using MeerKAT 1.3 GHz data from the SARAO MeerKAT Galactic Plane Survey (l=2-60deg, 252-358deg, |b|<1.5deg) a…

astro-ph.SR2025★ 1 cited

Millimetre continuum from LBV stars and their environs. NIKA2 observations and Virtual Observatory data

J. R. Rizzo, C. Bordiu, A. Ritacco

Multi-wavelength studies of their circumstellar environments around LBVs are essential to quantify their feedback at Galactic scales. Dominant emission mechanisms at millimetre wav…

astro-ph.SR2024

Substellar candidates at the earliest stages: the SUCANES database

A. M. Pérez-García, N. Huélamo, A. García-López +11

Brown dwarfs are the bridge between low-mass stars and giant planets. One way of shedding light on their dominant formation mechanism is to study them at the earliest stages of the…

astro-ph.GA2024★ 5 cited

MeerKAT reveals a ghostly thermal radio ring towards the Galactic Centre

C. Bordiu, M. D. Filipovic, G. Umana +26

We present the serendipitous discovery of a new radio-continuum ring-like object nicknamed Kyklos (J1802-3353), with MeerKAT UHF and L-band observations. The radio ring, which rese…

astro-ph.SR2023★ 23 cited

The CARMENES search for exoplanets around M dwarfs. Telluric absorption corrected high S/N optical and near-infrared template spectra of 382 M dwarf stars

E. Nagel, S. Czesla, A. Kaminski +22

Light from celestial objects interacts with the molecules of the Earth's atmosphere, resulting in the production of telluric absorption lines in ground-based spectral data. Correct…

astro-ph.SR2023★ 3 cited

The rich molecular environment of the luminous blue variable star AFGL 2298

J. R. Rizzo, C. Bordiu, C. Buemi +6

We investigated the molecular environment of AFGL 2298, an obscured Galactic Luminous blue variable (LBV) star which hosts a highly structured circumstellar environment with hints…

astro-ph.GA2023★ 5 cited

Main Sequence to Starburst Transitioning Galaxies: Gamma-ray Burst Hosts at

Jakub Nadolny, Michał Jerzy Michałowski, J. Ricardo Rizzo +8

Star-forming galaxies populate a main sequence (MS), a well-defined relation between stellar mass (M*) and star-formation rate (SFR). Starburst (SB) galaxies lie significantly abov…

astro-ph.EP2023★ 96 cited

The CARMENES search for exoplanets around M dwarfs. Guaranteed time observations Data Release 1 (2016-2020)

I. Ribas, A. Reiners, M. Zechmeister +102

The CARMENES instrument was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of n…

astro-ph.GA2022★ 9 cited

First detection of silicon-bearing molecules in Car

C. Bordiu, J. R. Rizzo, F. Bufano +11

We present ALMA band 6 observations of the luminous blue variable Eta Car, obtained within the ALMAGAL program. We report SiO J=5-4, SiS J=12-11 and SiN N=5-4 emission in the equat…

astro-ph.GA2022★ 7 cited

The interstellar medium in the environment of the supernova-less long-duration GRB 111005A

Aleksandra Leśniewska, M. J. Michałowski, P. Kamphuis +17

Long ( s) gamma ray bursts (GRBs) are associated with explosions of massive stars, although in three instances, supernovae (SNe) have not been detected, despite deep observatio…

astro-ph.SR2022

Identification and spectroscopic characterization of 128 new Herbig stars

Miguel Vioque, René D. Oudmaijer, Chumpon Wichittanakom +6

We present optical spectroscopy observations of 145 high-mass pre-main sequence candidates from the catalogue of Vioque et al. (2020). From these, we provide evidence for the Herbi…

astro-ph.EP2021★ 13 cited

Raman spectroscopy and planetary exploration: testing the ExoMars/RLS system at the Tabernas Desert (Spain)

Marco Veneranda, Guillermo Lopez-Reyes, Jose Antonio Manrique-Martinez +8

ExoFit trials are field campaigns financed by ESA to test the Rosalind Franklin rover and to enhance collaboration practices between ExoMars working groups. During the first trial,…

astro-ph.SR2021★ 16 cited

SiO, 29SiO, and 30SiO emission from 67 oxygen-rich stars. A survey of 61 maser lines from 7 to 1 mm

J. R. Rizzo, J. Cernicharo, C. Garcia-Miro

Circumstellar environments of oxygen-rich stars are among the strongest SiO maser emitters. Physical processes such as collisions, infrared pumping and overlaps favors the inversio…

astro-ph.GA2020★ 6 cited

A warm molecular ring in AG Car: composing the mass-loss puzzle

C. Bordiu, F. Bufano, L. Cerrigone +9

We present APEX observations of CO J=3-2 and ALMA observations of CO J=2-1, 13CO J=2-1 and continuum toward the galactic luminous blue variable AG Car. These new observations revea…

astro-ph.SR2020★ 77 cited

Catalogue of new Herbig Ae/Be and classical Be stars. A machine learning approach to Gaia DR2

M. Vioque, R. D. Oudmaijer, M. Schreiner +4

The intermediate-mass pre-main sequence Herbig Ae/Be stars are key to understanding the differences in formation mechanisms between low- and high-mass stars. The study of the gener…

astro-ph.SR2019

NIKA2 observations around LBV stars: emission from stars and circumstellar material

J. Ricardo Rizzo, A. Ritacco, C. Bordiu

Luminous Blue Variable (LBV) stars are evolved massive objects, previous to core-collapse supernova. LBVs are characterized by photometric and spectroscopic variability, produced b…

astro-ph.SR2019★ 12 cited

The peculiar chemistry of the inner ejecta of Eta Carina

C. Bordiu, J. R. Rizzo

We investigated continuum and molecular line emission of four species (CO, HCN, HCN, and HCO) at 0.8 mm in the inner arcsec around Eta Car, using ALMA archival observati…

astro-ph.SR2018★ 188 cited

Gaia DR2 study of Herbig Ae/Be stars

M. Vioque, R. D. Oudmaijer, D. Baines +2

We use Gaia Data Release 2 (DR2) to place 252 Herbig Ae/Be stars in the HR diagram and investigate their characteristics and properties. For all known Herbig Ae/Be stars with paral…

astro-ph.GA2018★ 8.6k cited

Gaia Data Release 2. Summary of the contents and survey properties

Gaia Collaboration, A. G. A. Brown, A. Vallenari +4

We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities, and information on astrophysical parameters and variability, for sources…

astro-ph.GA2018★ 14 cited

Herschel Planetary Nebula Survey (HerPlaNS): Hydrogen Recombination Laser Lines in Mz 3

Isabel Aleman, Katrina Exter, Toshiya Ueta +12

The bipolar nebula Menzel 3 (Mz 3) was observed as part of the \textit{Herschel} Planetary Nebula Survey (\textit{HerPlaNS}), which used the PACS and SPIRE instruments aboard the \…

astro-ph.GA2018★ 423 cited

Gaia Data Release 2: Mapping the Milky Way disc kinematics

Gaia Collaboration, D. Katz, T. Antoja +12

To illustrate the potential of GDR2, we provide a first look at the kinematics of the Milky Way disc, within a radius of several kiloparsecs around the Sun. We benefit for the firs…