Search Publications

The XMM-Newton slew survey in the 2-10 keV band
DOI: 10.1051/0004-6361/201118642 Bibcode: 2012A&A...548A..99W

Read, A. M.; Warwick, R. S.; Saxton, R. D.

Context. The on-going XMM-Newton Slew Survey (XSS) provides coverage of a significant fraction of the sky in a broad X-ray bandpass. Although shallow by contemporary standards, in the "classical" 2-10 keV band of X-ray astronomy, the XSS provides significantly better sensitivity than any currently available all-sky survey.
Aims: We investigat…

2012 Astronomy and Astrophysics
XMM-Newton 37
Topographic, spectral and thermal inertia analysis of interior layered deposits in Iani Chaos, Mars
DOI: 10.1016/j.icarus.2012.06.036 Bibcode: 2012Icar..221...20S

Teanby, N. A.; Grindrod, P. M.; Sefton-Nash, E. +2 more

We present an analysis of Interior Layered Deposits (ILDs) in Iani Chaos using visible, infrared, hyperspectral and topographic datasets acquired by instruments aboard NASA’s Mars Global Surveyor, Mars Odyssey, Mars Reconnaissance Orbiter and ESA’s Mars Express spacecraft. We focus on four main regions where ILDs outcrop in Iani Chaos. Deposits sp…

2012 Icarus
MEx 37
Detection and characterization of a 500 µm dust emissivity excess in the Galactic plane using Herschel/Hi-GAL observations
DOI: 10.1051/0004-6361/201117956 Bibcode: 2012A&A...537A.113P

Bernard, J. -P.; Marshall, D. J.; Paladini, R. +7 more

Context. Past and recent observations have revealed unexpected variations in the far-infrared - millimeter (FIR-mm) dust emissivity in the interstellar medium. In the Herschel spectral range, those are often referred to as a 500 µm emission excess. Several dust emission models have been developed to interpret astrophysical data in the FIR-mm…

2012 Astronomy and Astrophysics
Herschel 37
The environmental dependence of the structure of outer galactic discs in STAGES spiral galaxies
DOI: 10.1111/j.1365-2966.2011.19727.x Bibcode: 2012MNRAS.419..669M

Bell, Eric F.; Wolf, Christian; Aragón-Salamanca, Alfonso +7 more

We present an analysis of V-band radial surface brightness profiles for spiral galaxies from the field and cluster environments using Hubble Space Telescope/Advanced Camera for Surveys imaging and data from the Space Telescope A901/2 Galaxy Evolution Survey (STAGES). We use a large sample of ∼330 face-on to intermediately inclined spiral galaxies …

2012 Monthly Notices of the Royal Astronomical Society
eHST 37
Energetic charged particle weathering of Saturn's inner satellites
DOI: 10.1016/j.pss.2011.02.012 Bibcode: 2012P&SS...61...60P

Krupp, N.; Roussos, E.; Hendrix, A. R. +9 more

We characterize the relative importance of energetic electrons and protons to the weathering of five of the inner satellites of Saturn. To do this, we present data from the Magnetospheric Imaging Instrument on the Cassini spacecraft, some of which is averaged over the whole mission to date. We also compute averaged proton and electron energy spect…

2012 Planetary and Space Science
Cassini 37
Profile of strong magnetic field By component in magnetotail current sheets
DOI: 10.1029/2011JA017402 Bibcode: 2012JGRA..117.6216R

Petrukovich, A. A.; Zhang, T. L.; Lucek, E. +8 more

The strong magnetic field By component (in GSM coordinates) has been increasingly noticed to play an important role in the dynamics of tail current sheet (CS). The distribution profile of strong By components in the tail CS (i.e., those with guide field), however, is not well known. In the present work, by using the simultane…

2012 Journal of Geophysical Research (Space Physics)
Cluster 37
Water vapor in Titan's stratosphere from Cassini CIRS far-infrared spectra
DOI: 10.1016/j.icarus.2012.06.014 Bibcode: 2012Icar..220..855C

Lellouch, E.; Irwin, P. G. J.; Teanby, N. A. +12 more

Here we report the measurement of water vapor in Titan's stratosphere using the Cassini Composite Infrared Spectrometer (CIRS, Flasar, F.M. et al. [2004]. Space Sci. Rev. 115, 169-297). CIRS senses water emissions in the far infrared spectral region near 50 µm, which we have modeled using two independent radiative transfer codes (NEMESIS (Ir…

2012 Icarus
Cassini 37
Bar pattern speed evolution over the last 7 Gyr
DOI: 10.1051/0004-6361/201118396 Bibcode: 2012A&A...540A.103P

Aguerri, J. A. L.; Pérez, I.; Méndez-Abreu, J.

Context. The tumbling pattern of a bar is the main parameter characterising its dynamics. From numerical simulations, its evolution since bar formation is tightly linked to the dark halo in which the bar is formed through dynamical friction and angular momentum exchange. Observational measurements of the bar pattern speed with redshift can restric…

2012 Astronomy and Astrophysics
eHST 37
Pulsation spectrum of δ Scuti stars: the binary HD 50870 as seen with CoRoT and HARPS
DOI: 10.1051/0004-6361/201118682 Bibcode: 2012A&A...542A..24M

Auvergne, M.; Amado, P. J.; Baudin, F. +14 more


Aims: We present the results obtained with the CoRoT satellite for HD 50870, a δ Sct star which was observed for 114.4 d. The aim of these observations was to evaluate the results obtained for HD 50844, the first δ Sct star monitored with CoRoT, on a longer time baseline.
Methods: The 307,570 CoRoT datapoints were analysed with different…

2012 Astronomy and Astrophysics
CoRoT 37
Interacting dark matter contribution to the galactic 511 keV gamma ray emission: constraining the morphology with INTEGRAL/SPI observations
DOI: 10.1088/1475-7516/2012/04/022 Bibcode: 2012JCAP...04..022V

Martin, Pierrick; Vincent, Aaron C.; Cline, James M.

We compare the full-sky morphology of the 511 keV gamma ray excess measured by the INTEGRAL/SPI experiment to predictions of models based on dark matter (DM) scatterings that produce low-energy positrons: either MeV-scale DM that annihilates directly into e+e- pairs, or heavy DM that inelastically scatters into an excited sta…

2012 Journal of Cosmology and Astroparticle Physics
INTEGRAL 37