Search Publications

Long XMM observation of the narrow-line Seyfert 1 galaxy IRAS 13224-3809: rapid variability, high spin and a soft lag
DOI: 10.1093/mnras/sts504 Bibcode: 2013MNRAS.429.2917F

Young, A. J.; Brandt, W. N.; Ponti, G. +21 more

The narrow-line Seyfert 1 galaxy IRAS 13224-3809 has been observed with XMM-Newton for 500 ks. The source is rapidly variable on time-scales down to a few 100 s. The spectrum shows strong broad Fe - K and L emission features which are interpreted as arising from reflection from the inner parts of an accretion disc around a rapidly spinning black h…

2013 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 117
The Herschel and JCMT Gould Belt Surveys: Constraining Dust Properties in the Perseus B1 Clump with PACS, SPIRE, and SCUBA-2
DOI: 10.1088/0004-637X/767/2/126 Bibcode: 2013ApJ...767..126S

Bernard, J. -P.; Hill, T.; André, Ph. +29 more

We present Herschel observations from the Herschel Gould Belt Survey and SCUBA-2 science verification observations from the JCMT Gould Belt Survey of the B1 clump in the Perseus molecular cloud. We determined the dust emissivity index using four different techniques to combine the Herschel PACS+SPIRE data at 160-500 µm with the SCUBA-2 data …

2013 The Astrophysical Journal
Herschel Planck 116
Planck constraints on holographic dark energy
DOI: 10.1088/1475-7516/2013/09/021 Bibcode: 2013JCAP...09..021L

Zhang, Xin; Li, Miao; Ma, Yin-Zhe +2 more

We perform a detailed investigation on the cosmological constraints on the holographic dark energy (HDE) model by using the Plank data. We find that HDE can provide a good fit to the Plank high-l (l gtrsim 40) temperature power spectrum, while the discrepancy at l simeq 20-40 found in the ΛCDM model remains unsolved in the HDE model. The Plank dat…

2013 Journal of Cosmology and Astroparticle Physics
Planck 116
Cryovolcanism on Titan: New results from Cassini RADAR and VIMS
DOI: 10.1002/jgre.20062 Bibcode: 2013JGRE..118..416L

Barnes, J. W.; Janssen, M. A.; Lunine, J. I. +13 more

The existence of cryovolcanic features on Titan has been the subject of some controversy. Here we use observations from the Cassini RADAR, including Synthetic Aperture Radar (SAR) imaging, radiometry, and topographic data as well as compositional data from the Visible and Infrared Mapping Spectrometer (VIMS) to reexamine several putative cryovolca…

2013 Journal of Geophysical Research (Planets)
Cassini 116
"TNOs are Cool": A survey of the trans-Neptunian region. IX. Thermal properties of Kuiper belt objects and Centaurs from combined Herschel and Spitzer observations
DOI: 10.1051/0004-6361/201322047 Bibcode: 2013A&A...557A..60L

Fornasier, S.; Groussin, O.; Lellouch, E. +14 more


Aims: The goal of this work is to characterize the ensemble thermal properties of the Centaurs / trans-Neptunian population.
Methods: Thermal flux measurements obtained with Herschel/PACS and Spitzer/MIPS provide size, albedo, and beaming factors for 85 objects (13 of which are presented here for the first time) by means of standard radi…

2013 Astronomy and Astrophysics
Herschel 115
Gas fraction and star formation efficiency at z < 1.0
DOI: 10.1051/0004-6361/201220392 Bibcode: 2013A&A...550A..41C

Braine, J.; Colina, L.; Walter, F. +3 more

After new observations of 39 galaxies at z ~ 0.6-1.0 obtained at the IRAM 30-m telescope, we present our full CO line survey covering the redshift range 0.2 < z < 1. Our aim is to determine the driving factors accounting for the steep decline in the star formation rate during this epoch. We study both the gas fraction, defined as Mgas

2013 Astronomy and Astrophysics
eHST 115
Global investigation of olivine on Mars: Insights into crust and mantle compositions
DOI: 10.1029/2012JE004149 Bibcode: 2013JGRE..118..234O

Bibring, J. -P.; Gondet, B.; Langevin, Y. +4 more

present the distribution of olivine on Mars, derived from spectral parameters based on the 1 µm olivine absorption band. The olivine can be defined with respect to two spectral end-members: type 1 corresponds to olivine with low iron content and/or small grain size and/or small abundance, and type 2, which corresponds to olivine with higher iron c…

2013 Journal of Geophysical Research (Planets)
MEx 115
X-ray follow-ups of XSS J12270-4859: a low-mass X-ray binary with gamma-ray Fermi-LAT association
DOI: 10.1051/0004-6361/201220393 Bibcode: 2013A&A...550A..89D

Mukai, K.; Belloni, T.; de Martino, D. +10 more

Context. XSS J1227.0-4859 is a peculiar, hard X-ray source recently positionally associated to the Fermi-LAT source 1FGL J1227.9-4852/2FGL J1227.7-4853. Multi-wavelength observations have added information on this source, indicating a low-luminosity low-mass X-ray binary (LMXB), but its nature is still unclear.
Aims: To progress in our unders…

2013 Astronomy and Astrophysics
INTEGRAL XMM-Newton 115
Flux calibration of the Herschel-SPIRE photometer
DOI: 10.1093/mnras/stt948 Bibcode: 2013MNRAS.433.3062B

Valtchanov, I.; Bock, J. J.; Spencer, L. D. +16 more

We describe the procedure used to flux calibrate the three-band submillimetre photometer in the Spectral and Photometric Imaging Receiver instrument on the Herschel Space Observatory. This includes the equations describing the calibration scheme, a justification for using Neptune as the primary calibration source, a description of the observations…

2013 Monthly Notices of the Royal Astronomical Society
Herschel 115
Galaxy Evolution in Overdense Environments at High Redshift: Passive Early-type Galaxies in a Cluster at z ~ 2
DOI: 10.1088/0004-637X/772/2/118 Bibcode: 2013ApJ...772..118S

Finoguenov, A.; Cimatti, A.; Daddi, E. +8 more

We present a study of galaxy populations in the central region of the IRAC-selected, X-ray-detected galaxy cluster Cl J1449+0856 at z = 2. Based on a sample of spectroscopic and photometric cluster members, we investigate stellar populations and the morphological structure of cluster galaxies over an area of ~0.7 Mpc2 around the cluster…

2013 The Astrophysical Journal
eHST 115