Search Publications

"TNOs are Cool": A survey of the trans-Neptunian region. X. Analysis of classical Kuiper belt objects from Herschel and Spitzer observations
DOI: 10.1051/0004-6361/201322416 Bibcode: 2014A&A...564A..35V

Fornasier, S.; Pál, A.; Lellouch, E. +14 more

Context. The Kuiper belt is formed of planetesimals which failed to grow to planets and its dynamical structure has been affected by Neptune. The classical Kuiper belt contains objects both from a low-inclination, presumably primordial, distribution and from a high-inclination dynamically excited population.
Aims: Based on a sample of classic…

2014 Astronomy and Astrophysics
Herschel 74
Planck 2013 results. XXXI. Consistency of the Planck data
DOI: 10.1051/0004-6361/201423743 Bibcode: 2014A&A...571A..31P

Miville-Deschênes, M. -A.; Bernard, J. -P.; Planck Collaboration +181 more

The Planck design and scanning strategy provide many levels of redundancy that can be exploited to provide tests of internal consistency. One of the most important is the comparison of the 70 GHz (amplifier) and 100 GHz (bolometer) channels. Based on different instrument technologies, with feeds located differently in the focal plane, analysed ind…

2014 Astronomy and Astrophysics
Planck 73
X-ray monitoring of classical novae in the central region of M 31 III. Autumn and winter 2009/10, 2010/11, and 2011/12
DOI: 10.1051/0004-6361/201322426 Bibcode: 2014A&A...563A...2H

Della Valle, M.; Pietsch, W.; Haberl, F. +7 more

Context. Classical novae (CNe) represent the major class of supersoft X-ray sources (SSSs) in the central region of our neighbouring galaxy M 31.
Aims: We performed a dedicated monitoring of the M 31 central region, which aimed to detect SSS counterparts of CNe, with XMM-Newton and Chandra between Nov. and Mar. of the years 2009/10, 2010/11, …

2014 Astronomy and Astrophysics
XMM-Newton 72
Planck 2013 results. V. LFI calibration
DOI: 10.1051/0004-6361/201321527 Bibcode: 2014A&A...571A...5P

Bernard, J. -P.; Planck Collaboration; Aghanim, N. +217 more

We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the orbital dipole plus the solar dipole, caused respectively by the motion of the Planck spacecraft with respect to the Sun and by motion of the solar system with respect to the cos…

2014 Astronomy and Astrophysics
Planck 72
Open questions on prominences from coordinated observations by IRIS, Hinode, SDO/AIA, THEMIS, and the Meudon/MSDP
DOI: 10.1051/0004-6361/201423922 Bibcode: 2014A&A...569A..85S

Golub, L.; Schmieder, B.; Tian, H. +5 more

Context. A large prominence was observed by multiple instruments on the ground and in space during an international campaign on September 24, 2013, for three hours (12:12 UT -15:12 UT). Instruments used in the campaign included the newly launched (June 2013) Interface Region Imaging Spectrograph (IRIS), THEMIS (Tenerife), the Hinode Solar Optical …

2014 Astronomy and Astrophysics
Hinode IRIS 72
ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z = 4.75
DOI: 10.1051/0004-6361/201322892 Bibcode: 2014A&A...562A..67G

Daddi, E.; Elbaz, D.; Maiolino, R. +19 more

We report ALMA Cycle 0 observations at 1.3 mm of LESS J033229.4-275619 (XID403), an ultraluminous infrared galaxy at z = 4.75 in the Chandra Deep Field South hosting a Compton-thick QSO. The source is not resolved in our data at a resolution of ~0.75 arcsec, placing an upper-limit of 2.5 kpc to the half-light radius of the continuum emission from …

2014 Astronomy and Astrophysics
Herschel eHST 71
VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster at z ~ 3.3
DOI: 10.1051/0004-6361/201423828 Bibcode: 2014A&A...572A..41L

Maccagni, D.; Cimatti, A.; Ilbert, O. +46 more

Using new spectroscopic observations obtained as part of the VIMOS Ultra-Deep Survey (VUDS), we performed a systematic search for overdense environments in the early universe (z> 2) and report here on the discovery of Cl J0227-0421, a massive protocluster at z = 3.29. This protocluster is characterized by both the large overdensity of spectrosc…

2014 Astronomy and Astrophysics
XMM-Newton 70
The rise and fall of the Type Ib supernova iPTF13bvn. Not a massive Wolf-Rayet star
DOI: 10.1051/0004-6361/201423884 Bibcode: 2014A&A...565A.114F

Cenko, S. B.; Sollerman, J.; Gal-Yam, A. +9 more

Context. We investigate iPTF13bvn, a core-collapse (CC) supernova (SN) in the nearby spiral galaxy NGC 5806. This object was discovered by the intermediate Palomar Transient Factory (iPTF) very close to the estimated explosion date and was classified as a stripped-envelope CC SN, likely of Type Ib. Furthermore, a possible progenitor detection in p…

2014 Astronomy and Astrophysics
eHST 70
Relating jet structure to photometric variability: the Herbig Ae star HD 163296
DOI: 10.1051/0004-6361/201323092 Bibcode: 2014A&A...563A..87E

Mendigutía, I.; Kaper, L.; Podio, L. +21 more

Herbig Ae/Be stars are intermediate-mass pre-main sequence stars surrounded by circumstellar dust disks. Some are observed to produce jets, whose appearance as a sequence of shock fronts (knots) suggests a past episodic outflow variability. This "jet fossil record" can be used to reconstruct the outflow history. We present the first optical to nea…

2014 Astronomy and Astrophysics
eHST 70
Revisiting CoRoT RR Lyrae stars: detection of period doubling and temporal variation of additional frequencies
DOI: 10.1051/0004-6361/201424522 Bibcode: 2014A&A...570A.100S

Poretti, E.; Baglin, A.; Szabó, R. +7 more

Context. High-precision, space-based photometric missions like CoRoT and Kepler have revealed new and surprising phenomena in classical variable stars. Such discoveries were the period doubling in RR Lyrae stars and the frequent occurrence of additional periodicities some of which can be explained by radial overtone modes, but others are discordan…

2014 Astronomy and Astrophysics
CoRoT 69