Search Publications

Analysis of Cassini magnetic field observations over the poles of Rhea
DOI: 10.1029/2012JA017747 Bibcode: 2012JGRA..117.7211S

Dougherty, Michele K.; Saur, Joachim; Kriegel, Hendrik +5 more

We analyze Cassini magnetic field observations from the only two polar flybys of Saturn's largest icy satellite Rhea (R2 on 02 March 2010 and R3 on 11 January 2011) which are scheduled between Saturn Orbit Insertion and the end of the mission in 2017. For the interpretation of these data, we apply estimations from simple analytical models as well …

2012 Journal of Geophysical Research (Space Physics)
Cassini 37
Initiation and Development of the White-light and Radio Coronal Mass Ejection on 2001 April 15
DOI: 10.1088/0004-637X/750/2/147 Bibcode: 2012ApJ...750..147D

Pick, M.; Démoulin, P.; Vourlidas, A. +1 more

The 2001 April 15 event was one of the largest of the last solar cycle. A former study established that this event was associated with a coronal mass ejection (CME) observed both at white light and radio frequencies. This radio CME is illuminated by synchrotron emission from relativistic electrons. In this paper, we investigate the relation of the…

2012 The Astrophysical Journal
SOHO 37
The Faint End of the Cluster-galaxy Luminosity Function at High Redshift
DOI: 10.1088/0004-637X/761/2/141 Bibcode: 2012ApJ...761..141M

Wright, Edward L.; Eisenhardt, Peter R. M.; Gonzalez, Anthony H. +7 more

We measure the faint-end slope of the galaxy luminosity function (LF) for cluster galaxies at 1 < z < 1.5 using Spitzer IRAC data. We investigate whether this slope, α, differs from that of the field LF at these redshifts, and with the cluster LF at low redshifts. The latter is of particular interest as low-luminosity galaxies are expected t…

2012 The Astrophysical Journal
eHST 37
A mid-IR study of the circumstellar environment of Herbig Be stars
DOI: 10.1051/0004-6361/201014916 Bibcode: 2012A&A...538A.101V

Waters, L. B. F. M.; Pantin, E.; van Boekel, R. +7 more

Context. The study of the formation of massive stars is complicated because of the short times scales, large distances, and obscuring natal clouds. There are observational and theoretical indications that the circumstellar environment of Herbig Be (HBe) stars is substantially different from that of their lower mass counterparts, the T Tauri and He…

2012 Astronomy and Astrophysics
ISO 37
A Significant Problem with Using the Amati Relation for Cosmological Purposes
DOI: 10.1088/0004-637X/747/1/39 Bibcode: 2012ApJ...747...39C

Collazzi, Andrew C.; Schaefer, Bradley E.; Goldstein, Adam +1 more

We consider the distribution of many samples of gamma-ray bursts when plotted in a diagram with their bolometric fluence (S bolo) versus the observed photon energy of peak spectral flux (E peak, obs). In this diagram, all bursts that obey the Amati relation (a luminosity relation where the total burst energy has a power-law r…

2012 The Astrophysical Journal
Suzaku 37
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