Search Publications

Space test of the equivalence principle: first results of the MICROSCOPE mission
DOI: 10.1088/1361-6382/ab4707 Bibcode: 2019CQGra..36v5006T

Bergé, Joel; Chhun, Ratana; Métris, Gilles +31 more

The weak equivalence principle (WEP), stating that two bodies of different compositions and/or mass fall at the same rate in a gravitational field (universality of free fall), is at the very foundation of general relativity. The MICROSCOPE mission aims to test its validity to a precision of 10-15, two orders of magnitude better than cur…

2019 Classical and Quantum Gravity
MICROSCOPE 72
The Pristine survey - VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates
DOI: 10.1093/mnras/stz2643 Bibcode: 2019MNRAS.490.2241A

Sestito, Federico; Navarro, Julio F.; Martin, Nicolas +27 more

We present the results of a 3-yr long, medium-resolution spectroscopic campaign aimed at identifying very metal-poor stars from candidates selected with the CaHK, metallicity-sensitive Pristine survey. The catalogue consists of a total of 1007 stars, and includes 146 rediscoveries of metal-poor stars already presented in previous surveys, 707 new …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 72
A loud quasi-periodic oscillation after a star is disrupted by a massive black hole
DOI: 10.1126/science.aar7480 Bibcode: 2019Sci...363..531P

Steiner, James F.; Remillard, Ronald A.; Homan, Jeroen +9 more

The tidal forces close to massive black holes can rip apart stars that come too close to them. As the resulting stellar debris spirals toward the black hole, the debris heats up and emits x-rays. We report observations of a stable 131-second x-ray quasi-periodic oscillation from the tidal disruption event ASASSN-14li. Assuming the black hole mass …

2019 Science
XMM-Newton 72
Praesepe (NGC 2632) and its tidal tails
DOI: 10.1051/0004-6361/201935502 Bibcode: 2019A&A...627A...4R

Röser, Siegfried; Schilbach, Elena


Aims: Within a 400 pc sphere around the Sun, we search for Praesepe's tidal tails in the Gaia Data Release 2 (DR2) data set.
Methods: We used a modified convergent-point method to find stars with space velocities close to the space velocity of the Praesepe cluster.
Results: We find a clear indication for the existence of Praesepe's …

2019 Astronomy and Astrophysics
Gaia 72
Dark Energy Surveyed Year 1 results: calibration of cluster mis-centring in the redMaPPer catalogues
DOI: 10.1093/mnras/stz1361 Bibcode: 2019MNRAS.487.2578Z

Bechtol, K.; Smith, M.; Allam, S. +84 more

The centre determination of a galaxy cluster from an optical cluster finding algorithm can be offset from theoretical prescriptions or N-body definitions of its host halo centre. These offsets impact the recovered cluster statistics, affecting both richness measurements and the weak lensing shear profile around the clusters. This paper models the …

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 72
HELP: a catalogue of 170 million objects, selected at 0.36-4.5 µm, from 1270 deg2 of prime extragalactic fields
DOI: 10.1093/mnras/stz2509 Bibcode: 2019MNRAS.490..634S

Oliver, Seb; Vaccari, Mattia; Farrah, Duncan +15 more

We present an optical to near-infrared (NIR) selected astronomical catalogue covering 1270 deg2. This is the first attempt to systematically combine data from 23 of the premier extragalactic survey fields - the product of a vast investment of telescope time. The fields are those imaged by the Herschel Space Observatory that form the Her…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 72
Consistent Dust and Gas Models for Protoplanetary Disks. III. Models for Selected Objects from the FP7 DIANA Project
DOI: 10.1088/1538-3873/aaf4e5 Bibcode: 2019PASP..131f4301W

Waters, L. B. F. M.; Pinte, C.; Woitke, P. +17 more

The European FP7 project DIANA has performed a coherent analysis of a large set of observational data of protoplanetary disks by means of thermo-chemical disk models. The collected data include extinction-corrected stellar UV and X-ray input spectra (as seen by the disk), photometric fluxes, low and high resolution spectra, interferometric data, e…

2019 Publications of the Astronomical Society of the Pacific
ISO IUE eHST 72
Achievements of Hinode in the first eleven years
DOI: 10.1093/pasj/psz084 Bibcode: 2019PASJ...71R...1H

Solanki, Sami K.; Tiwari, Sanjiv K.; Reeves, Katharine K. +33 more

Hinode is Japan's third solar mission following Hinotori (1981-1982) and Yohkoh (1991-2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries three instruments: the Solar Optical Telescope, the X-Ray Telescope, and the EUV Imaging Spectrometer. These instruments were built under international collaboration with th…

2019 Publications of the Astronomical Society of Japan
Hinode 72
Saturn's Deep Atmospheric Flows Revealed by the Cassini Grand Finale Gravity Measurements
DOI: 10.1029/2018GL078087 Bibcode: 2019GeoRL..46..616G

Iess, L.; Guillot, T.; Miguel, Y. +4 more

How deep do Saturn's zonal winds penetrate below the cloud level has been a decades-long question, with important implications not only for the atmospheric dynamics but also for the interior density structure, composition, magnetic field, and core mass. The Cassini Grand Finale gravity experiment enables answering this question for the first time,…

2019 Geophysical Research Letters
Cassini 72
MAGPHYS+photo-z: Constraining the Physical Properties of Galaxies with Unknown Redshifts
DOI: 10.3847/1538-4357/ab345d Bibcode: 2019ApJ...882...61B

Daddi, E.; Salvato, M.; Vaccari, M. +8 more

We present an enhanced version of the multiwavelength spectral modeling code MAGPHYS that allows the estimation of galaxy photometric redshift and physical properties (e.g., stellar mass, star formation rate, dust attenuation) simultaneously, together with robust characterization of their uncertainties. The self-consistent modeling over ultraviole…

2019 The Astrophysical Journal
eHST 72