Search Publications

The Planck SZ Cluster Catalog: expected X-ray properties
DOI: 10.1051/0004-6361/201015431 Bibcode: 2012A&A...544A..40C

Bartlett, J. G.; Chamballu, A.; Melin, J. -B.

Surveys based on the Sunyaev-Zel'dovich (SZ) effect provide a fresh view of the galaxy cluster population, one that is complementary to X-ray surveys. To better understand the relation between these two kinds of survey, we construct an empirical cluster model using scaling relations constrained by current X-ray and SZ data. We apply our model to p…

2012 Astronomy and Astrophysics
XMM-Newton 8
Spectro-polarimetry of the bright side of Saturn's moon Iapetus
DOI: 10.1051/0004-6361/201117870 Bibcode: 2012A&A...537A..23E

Tozzi, G. P.; Boehnhardt, H.; Ejeta, C. +1 more

Context. Measurements of the polarized reflected sunlight from atmosphereless solar system bodies, over a range of phase angles, provide information about the surface structure and composition.
Aims: With this work, we provide analysis of the polarimetric observations of the bright side of Iapetus at five different phase angles, and over the …

2012 Astronomy and Astrophysics
Cassini 8
Recent Developments of NEMO: Detection of EUV Wave Characteristics
DOI: 10.1007/s11207-011-9894-3 Bibcode: 2012SoPh..276..479P

Podladchikova, O.; Van der Linden, R. A. M.; Vuets, A. +1 more

Recent developments in space instrumentation for solar observations and increased telemetry have necessitated the creation of advanced pattern recognition tools for different classes of solar events. The Extreme Ultraviolet Imaging Telescope (EIT) onboard the SOHO spacecraft has uncovered a new class of eruptive events on the solar disk, which are…

2012 Solar Physics
SOHO 8
Radio Pulsating Structures with Coronal Loop Contraction
DOI: 10.1007/s11207-012-0003-z Bibcode: 2012SoPh..280..491K

Pohjolainen, S.; Kallunki, J.

We present a multi-wavelength study of a solar eruption event on 20 July 2004, comprising observations in Hα, EUV, soft X-rays, and in radio waves with a wide frequency range. The analyzed data show both oscillatory patterns and shock wave signatures during the impulsive phase of the flare. At the same time, large-scale EUV loops located above the…

2012 Solar Physics
SOHO 8
Implementation of Martian virtual reality environment using very high-resolution stereo topographic data
DOI: 10.1016/j.cageo.2011.09.018 Bibcode: 2012CG.....44..184K

Kim, Jung-Rack; Lin, Shih-Yuan; Hong, Jeong-Woo +2 more

Topography over terrestrial or other planetary surfaces is an important base data for virtual reality construction. In particular, with inaccessible topography such as the Martian surface, virtual reality provides great value not only for public interaction but also for scientific research. For the latter application, since field surveys are essen…

2012 Computers and Geosciences
MEx 8
Super-resolution in map-making based on a physical instrument model and regularized inversion. Application to SPIRE/Herschel
DOI: 10.1051/0004-6361/201116817 Bibcode: 2012A&A...539A..38O

Abergel, A.; Rodet, T.; Orieux, F. +3 more

We investigate super-resolution methods for image reconstruction from data provided by a family of scanning instruments like the Herschel observatory. To do this, we constructed a model of the instrument that faithfully reflects the physical reality, accurately taking the acquisition process into account to explain the data in a reliable manner. T…

2012 Astronomy and Astrophysics
Herschel 8
In-flight calibration of the spin axis offset of a fluxgate magnetometer with an electron drift instrument
DOI: 10.1088/0957-0233/23/10/105003 Bibcode: 2012MeScT..23j5003L

Russell, C. T.; Torkar, K.; Leinweber, H. K.

We show that the spin axis offset of a fluxgate magnetometer can be calibrated with an electron drift instrument (EDI) and that the required input time interval is relatively short. For missions such as Cluster or the upcoming Magnetospheric Multiscale (MMS) mission the spin axis offset of a fluxgate magnetometer could be determined on an orbital …

2012 Measurement Science and Technology
Cluster 8
A wide-field near-infrared H2 2.122 µm line survey of the Braid Nebula star formation region in Cygnus OB7
DOI: 10.1051/0004-6361/201219124 Bibcode: 2012A&A...542A.111K

Smith, M. D.; Davis, C. J.; Beck, T. L. +8 more

Context. Outflows and jets are the first signposts of ongoing star formation processes in any molecular cloud, yet their study in optical bands provides limited results due to the large extinction present. Near-infrared unbiased wide-field observations in the H2 1-0 S(1) line at 2.122 µm alleviates the problem, enabling us to dete…

2012 Astronomy and Astrophysics
AKARI 8
A new Herschel view of the young star T54: not a transitional disk?
DOI: 10.1051/0004-6361/201220461 Bibcode: 2012A&A...548A.111M

Prusti, T.; Pilbratt, G. L.; Huélamo, N. +10 more

Context. Observations of transitional disks give us an understanding of the formation of planets and planetary systems such as our own. But care must be taken in identifying such sources: the higher spatial resolution of the Herschel Space Observatory provides a new view of the origin of the far-infrared and submillimeter excesses observed.
A…

2012 Astronomy and Astrophysics
Herschel 8
The Arp 220 Merger on kpc Scales
DOI: 10.1088/0004-637X/754/1/58 Bibcode: 2012ApJ...754...58K

Scharwächter, J.; König, S.; Eckart, A. +2 more

For the first time, we study the eastern nucleus in greater detail and search for the more extended emission in the molecular gas in different CO line transitions of the famous ultraluminous infrared galaxy (ULIRG) Arp 220. Furthermore, we present a model of the merger in Arp 220 on large scales with the help of the CO data and an optical and near…

2012 The Astrophysical Journal
eHST 8