Search Publications

Planck intermediate results. XLI. A map of lensing-induced B-modes
DOI: 10.1051/0004-6361/201527932 Bibcode: 2016A&A...596A.102P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +178 more

The secondary cosmic microwave background (CMB) B-modes stem from the post-decoupling distortion of the polarization E-modes due to the gravitational lensing effect of large-scale structures. These lensing-induced B-modes constitute both a valuable probe of the dark matter distribution and an important contaminant for the extraction of the primary…

2016 Astronomy and Astrophysics
Planck 31
NuSTAR reveals the extreme properties of the super-Eddington accreting supermassive black hole in PG 1247+267
DOI: 10.1051/0004-6361/201628325 Bibcode: 2016A&A...590A..77L

Harrison, F. A.; Stern, D.; Zhang, W. W. +26 more

PG1247+267 is one of the most luminous known quasars at z ~ 2 and is a strongly super-Eddington accreting supermassive black hole (SMBH) candidate. We obtained NuSTAR data of this intriguing source in December 2014 with the aim of studying its high-energy emission, leveraging the broad band covered by the new NuSTAR and the archival XMM-Newton dat…

2016 Astronomy and Astrophysics
XMM-Newton eHST 31
Gaia Data Release 1. On-orbit performance of the Gaia CCDs at L2
DOI: 10.1051/0004-6361/201628990 Bibcode: 2016A&A...595A...6C

Prusti, T.; Mora, A.; Brown, A. G. A. +19 more

The European Space Agency's Gaia satellite was launched into orbit around L2 in December 2013 with a payload containing 106 large-format scientific CCDs. The primary goal of the mission is to repeatedly obtain high-precision astrometric and photometric measurements of one thousand million stars over the course of five years. The scientific value o…

2016 Astronomy and Astrophysics
Gaia 31
Probing deep photospheric layers of the quiet Sun with high magnetic sensitivity
DOI: 10.1051/0004-6361/201628489 Bibcode: 2016A&A...596A...6L

Franz, M.; Schmidt, W.; Solanki, S. K. +31 more

Context. Investigations of the magnetism of the quiet Sun are hindered by extremely weak polarization signals in Fraunhofer spectral lines. Photon noise, straylight, and the systematically different sensitivity of the Zeeman effect to longitudinal and transversal magnetic fields result in controversial results in terms of the strength and angular …

2016 Astronomy and Astrophysics
Hinode 31
Multiwavelength study of the flaring activity of Sagittarius A in 2014 February-April
DOI: 10.1051/0004-6361/201527554 Bibcode: 2016A&A...589A.116M

Grosso, N.; Porquet, D.; Eckart, A. +8 more

Context. The supermassive black hole named Sgr A* is located at the dynamical center of the Milky Way. This closest supermassive black hole is known to have a luminosity several orders of magnitude lower than the Eddington luminosity. Flares coming from the Sgr A* environment can be observed in infrared, X-ray, and submillimeter wavelengths, but t…

2016 Astronomy and Astrophysics
XMM-Newton eHST 31
Observations and analysis of a curved jet in the coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201527784 Bibcode: 2016A&A...588L...3L

Jorda, L.; Lamy, P. L.; Lara, L. M. +48 more


Aims: We analyze the physical properties and dynamical origin of a curved jet of comet 67P/Churyumov-Gerasimenko that was observed repeatedly in several nucleus rotations starting on May 30 and persisting until early August, 2015.
Methods: We simulated the motion of dust grains ejected from the nucleus surface under the influence of the …

2016 Astronomy and Astrophysics
Rosetta 30
Multi-band morpho-Spectral Component Analysis Deblending Tool (MuSCADeT): Deblending colourful objects
DOI: 10.1051/0004-6361/201527923 Bibcode: 2016A&A...589A...2J

Starck, J. -L.; Courbin, F.; Joseph, R.

We introduce a new algorithm for colour separation and deblending of multi-band astronomical images called MuSCADeT which is based on Morpho-spectral Component Analysis of multi-band images. The MuSCADeT algorithm takes advantage of the sparsity of astronomical objects in morphological dictionaries such as wavelets and their differences in spectra…

2016 Astronomy and Astrophysics
eHST 30
Hot prominence detected in the core of a coronal mass ejection: Analysis of SOHO/UVCS Lα and SOHO/LASCO visible-light observations
DOI: 10.1051/0004-6361/201527421 Bibcode: 2016A&A...589A.128H

Heinzel, P.; Anzer, U.; Jejčič, S. +2 more

Context. The paper deals with the physics of erupting prominences in the core of coronal mass ejections (CME).
Aims: We determine the physical parameters of an erupting prominence embedded in the core of a CME using SOHO/UVCS hydrogen Lα and Lβ lines and SOHO/LASCO visible light observations. In particular we analyze the CME event observed on…

2016 Astronomy and Astrophysics
SOHO 30
Firedec: a two-channel finite-resolution image deconvolution algorithm
DOI: 10.1051/0004-6361/201424003 Bibcode: 2016A&A...589A..81C

Jablonka, P.; Meylan, G.; Courbin, F. +2 more

We present a two-channel deconvolution method that decomposes images into a parametric point-source channel and a pixelized extended-source channel. Based on the central idea of the deconvolution algorithm proposed by Magain et al. (1998, ApJ, 494, 472), the method aims at improving the resolution of the data rather than at completely removing the…

2016 Astronomy and Astrophysics
eHST 30
The rotation-metallicity relation for the Galactic disk as measured in the Gaia DR1 TGAS and APOGEE data
DOI: 10.1051/0004-6361/201629787 Bibcode: 2016A&A...596A..98A

Cropper, Mark; Kawata, Daisuke; Allende Prieto, Carlos


Aims: Previous studies have found that the Galactic rotation velocity-metallicity (V-[Fe/H]) relations for the thin and thick disk populations show negative and positive slopes, respectively. The first Gaia data release includes the Tycho-Gaia Astrometric Solution (TGAS) information, which we use to analyze the V-[Fe/H] relation for a strictl…

2016 Astronomy and Astrophysics
Gaia 30