Search Publications

Gaia Data Release 2. Catalogue validation
DOI: 10.1051/0004-6361/201833234 Bibcode: 2018A&A...616A..17A

Jordi, C.; Luri, X.; Cantat-Gaudin, T. +35 more

Context. The second Gaia data release (DR2) contains very precise astrometric and photometric properties for more than one billion sources, astrophysical parameters for dozens of millions, radial velocities for millions, variability information for half a million stars from selected variability classes, and orbits for thousands of solar system obj…

2018 Astronomy and Astrophysics
Gaia eHST 552
From thermal dissociation to condensation in the atmospheres of ultra hot Jupiters: WASP-121b in context
DOI: 10.1051/0004-6361/201833059 Bibcode: 2018A&A...617A.110P

Fortney, Jonathan J.; Désert, Jean-Michel; Showman, Adam P. +10 more

Context. A new class of exoplanets has emerged: the ultra hot Jupiters, the hottest close-in gas giants. The majority of them have weaker-than-expected spectral features in the 1.1-1.7 µm bandpass probed by HST/WFC3 but stronger spectral features at longer wavelengths probed by Spitzer. This led previous authors to puzzling conclusions about…

2018 Astronomy and Astrophysics
eHST 287
The nature of the TRAPPIST-1 exoplanets
DOI: 10.1051/0004-6361/201732233 Bibcode: 2018A&A...613A..68G

Triaud, Amaury H. M. J.; Burgasser, Adam J.; Gillon, Michaël +23 more

Context. The TRAPPIST-1 system hosts seven Earth-sized, temperate exoplanets orbiting an ultra-cool dwarf star. As such, it represents a remarkable setting to study the formation and evolution of terrestrial planets that formed in the same protoplanetary disk. While the sizes of the TRAPPIST-1 planets are all known to better than 5% precision, the…

2018 Astronomy and Astrophysics
eHST 272
Near infrared spectroscopy and star-formation histories of 3 ≤ z ≤ 4 quiescent galaxies
DOI: 10.1051/0004-6361/201833070 Bibcode: 2018A&A...618A..85S

Papovich, C.; Glazebrook, K.; Kacprzak, G. G. +8 more

We present Keck-MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 < z < 4, identified from their rest-frame UVJ colors and photometric redshifts in the ZFOURGE and 3DHST surveys. With median integration times of one hour in H and five in K, we obtain spectroscopic redshifts for half of the sample, using either Balm…

2018 Astronomy and Astrophysics
eHST 214
GOODS-ALMA: 1.1 mm galaxy survey. I. Source catalog and optically dark galaxies
DOI: 10.1051/0004-6361/201832928 Bibcode: 2018A&A...620A.152F

Magnelli, B.; Daddi, E.; Elbaz, D. +36 more


Aims: We present a 69 arcmin2 ALMA survey at 1.1 mm, GOODS-ALMA, matching the deepest HST-WFC3 H-band part of the GOODS-South field.
Methods: We tapered the 0″24 original image with a homogeneous and circular synthesized beam of 0″60 to reduce the number of independent beams - thus reducing the number of purely statistical spu…

2018 Astronomy and Astrophysics
Gaia Herschel eHST 210
Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0 < z < 4
DOI: 10.1051/0004-6361/201731506 Bibcode: 2018A&A...609A..30S

Elbaz, D.; Franco, M.; Ciesla, L. +3 more

We present a new, publicly available library of dust spectral energy distributions (SEDs). These SEDs are characterized by only three parameters: the dust mass (Mdust), the dust temperature (Tdust), and the mid-to-total infrared color (IR8 ≡ LIR/L8). The latter measures the relative contribution of polyc…

2018 Astronomy and Astrophysics
Herschel eHST 204
The evolution of the X-ray afterglow emission of GW 170817/ GRB 170817A in XMM-Newton observations
DOI: 10.1051/0004-6361/201832664 Bibcode: 2018A&A...613L...1D

Covino, S.; D'Avanzo, P.; Campana, S. +12 more

We report our observation of the short gamma-ray burst (GRB) GRB 170817A, associated to the binary neutron star merger gravitational wave (GW) event GW 170817, performed in the X-ray band with XMM-Newton 135 d after the event (on 29 December, 2017). We find evidence for a flattening of the X-ray light curve with respect to the previously observed …

2018 Astronomy and Astrophysics
XMM-Newton eHST 197
Starbursts in and out of the star-formation main sequence
DOI: 10.1051/0004-6361/201732370 Bibcode: 2018A&A...616A.110E

Daddi, E.; Elbaz, D.; Franco, M. +13 more


Aims: We use high-resolution continuum images obtained with the Atacama Large Millimeter Array (ALMA) to probe the surface density of star formation in z ~ 2 galaxies and study the different physical properties between galaxies within and above the star-formation main sequence of galaxies.
Methods: We use ALMA images at 870 µm with…

2018 Astronomy and Astrophysics
AKARI Herschel eHST 166
Hubble PanCET: an extended upper atmosphere of neutral hydrogen around the warm Neptune GJ 3470b
DOI: 10.1051/0004-6361/201833675 Bibcode: 2018A&A...620A.147B

Sanz-Forcada, J.; Ehrenreich, D.; Lecavelier des Etangs, A. +16 more

GJ 3470b is a warm Neptune transiting an M-dwarf star at the edge of the evaporation desert. It offers the possibility of investigating how low-mass, close-in exoplanets evolve under the irradiation from their host stars. We observed three transits of GJ 3470b in the Lyman-α line with the Hubble Space Telescope (HST) as part of the Panchromatic Co…

2018 Astronomy and Astrophysics
Gaia XMM-Newton eHST 165
Reanalysis of the Gaia Data Release 2 photometric sensitivity curves using HST/STIS spectrophotometry
DOI: 10.1051/0004-6361/201834051 Bibcode: 2018A&A...619A.180M

Weiler, M.; Maíz Apellániz, J.

Context. The second data release (DR2) from the European Space Agency mission Gaia took place on April 2018. DR2 included photometry for more than 1.3 × 109 sources in the three bands G, GBP, and GRP. Even though the Gaia DR2 photometry is very precise, there are currently three alternative definitions of the sensi…

2018 Astronomy and Astrophysics
Gaia eHST 148