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Tailward flow of energetic neutral atoms observed at Venus
DOI: 10.1029/2008JE003096 Bibcode: 2008JGRE..113.0B15G

Kallio, E.; Barabash, S.; Gunell, H. +7 more

The Analyzer of Space Plasma and Energetic Atoms (ASPERA-4) experiment on Venus Express provides the first measurements of energetic neutral atoms (ENAs) from Venus. The results improve our knowledge on the interaction of the solar wind with a nonmagnetized planet and they present an observational constraint to existing plasma models. We character…

2008 Journal of Geophysical Research (Planets)
VenusExpress 18
A Lyman Break Galaxy Candidate at z ~ 9
DOI: 10.1086/589944 Bibcode: 2008ApJ...680L..97H

Teplitz, Harry I.; Siana, Brian; Malkan, Matthew A. +3 more

We report the discovery of a z ~ 9 Lyman break galaxy candidate, selected from the NICMOS Parallel Imaging Survey as a J-dropout with J110 - H160 = 1.7. Spitzer/IRAC photometry reveals that the galaxy has a blue H160 - 3.6 µm color and a spectral break between 3.6 and 4.5 µm. We interpret this break as …

2008 The Astrophysical Journal
eHST 18
Reconstruction of Cluster Masses Using Particle Based Lensing. I. Application to Weak Lensing
DOI: 10.1086/590544 Bibcode: 2008ApJ...687...39D

Goldberg, David M.; Deb, Sanghamitra; Ramdass, Vede J.

We present Particle Based Lensing (PBL), a new technique for gravitational lensing mass reconstructions of galaxy clusters. Traditionally, most methods have employed either a finite inversion or gridding to turn observational lensed galaxy ellipticities into an estimate of the surface mass density of a galaxy cluster. We approach the problem from …

2008 The Astrophysical Journal
eHST 18
New XMM-Newton Analysis of Three Bright X-Ray Sources in M31 Globular Clusters, Including a New Black Hole Candidate
DOI: 10.1086/592594 Bibcode: 2008ApJ...689.1215B

Stiele, H.; Pietsch, W.; Haberl, F. +6 more

We present a detailed analysis of three globular cluster X-ray sources in the XMM-Newton extended survey of M31. The X-ray counterpart to the M31 globular cluster Bo 45 (XBo 45) was observed with XMM-Newton on 2006 December 26. Its combined pn+MOS 0.3-10 keV light curve was seen to vary by ~10%, and its 0.3-7.0 keV emission spectrum was well descr…

2008 The Astrophysical Journal
XMM-Newton 18
Asiago eclipsing binaries program. II. V505 Persei
DOI: 10.1051/0004-6361:20078384 Bibcode: 2008A&A...480..465T

Munari, U.; Zwitter, T.; Sordo, R. +4 more

The orbit and fundamental physical parameters of the double-lined eclipsing binary V505 Per are derived by means of Echelle high-resolution and high S/N spectroscopy, and B, V photometry. In addition, effective temperatures, gravities, rotational velocities, and metallicities of both components are also obtained from atmospheric χ2 anal…

2008 Astronomy and Astrophysics
Hipparcos 18
Energetic electron signatures of Saturn's smaller moons: Evidence of an arc of material at Methone
DOI: 10.1016/j.icarus.2007.03.034 Bibcode: 2008Icar..193..455R

Krupp, N.; Woch, J.; Jones, G. H. +6 more

We present several energetic charged particle microsignatures of two Lagrange moons, Telesto and Helene, measured by the MIMI/LEMMS instrument. These small moons absorb charged particles but their effects are usually obscured by Tethys and Dione, the two larger saturnian satellites that occupy the same orbits. The scales and structures of these mi…

2008 Icarus
Cassini 18
Lorentz Force: A Possible Driving Force for Sunspot Rotation
DOI: 10.1007/s11207-008-9236-2 Bibcode: 2008SoPh..252...55S

Zhang, Hongqi; Liu, Yu; Li, Hui +5 more

Zhao and Kosovichev (Astrophys. J.591, 446, 2003) found two opposite sub-photospheric vortical flows in the depth range of 0 - 12 Mm around a fast rotating sunspot. So far there is no theoretical model explaining such flow motions. In this paper, we try to explain this phenomenon from the point of view of magnetic flux tubes interacting with large…

2008 Solar Physics
Hinode SOHO 18
The in-flight performance of the X-ray Solar Monitor (XSM) on-board SMART-1
DOI: 10.1016/j.nima.2008.08.138 Bibcode: 2008NIMPA.596..317A

Andersson, H.; Alha, L.; Huovelin, J. +4 more

The operation, performance, and in-flight calibrations of the X-ray Solar Monitor (XSM) on-board ESA's SMART-1 mission to the Moon are presented. The basic method of deriving the response and effective area of the XSM is described. The evolution of the energy resolution as a function of time is studied, and sample data of high quality broadband so…

2008 Nuclear Instruments and Methods in Physics Research A
SMART-1 18
Diverse young stellar populations in the intermediate-redshift radio galaxies 3C 213.1 and 3C 459: implications for the evolution of the host galaxies
DOI: 10.1111/j.1365-2966.2008.12865.x Bibcode: 2008MNRAS.385..136W

Morganti, R.; Inskip, K. J.; Holt, J. +4 more

We present European Southern Observatory Very Large Telescope (ESO VLT) and William Herschel Telescope (WHT) spectroscopic observations of two powerful radio galaxies at intermediate redshifts (3C 213.1 and 3C 459), obtained with the aim of establishing the nature and evolutionary status of the host galaxies. Spectral synthesis modelling has been …

2008 Monthly Notices of the Royal Astronomical Society
eHST 18
Observations of a comet tail disruption induced by the passage of a CME
DOI: 10.1029/2007JA012603 Bibcode: 2008JGRA..113.4101K

Webb, D. F.; Arge, C. N.; Tappin, S. J. +7 more

The Solar Mass Ejection Imager observed an extremely faint interplanetary coronal mass ejection (ICME) as it passed Comet C/2001 Q4 (NEAT) on 5 May 2004, apparently causing a disruption of its plasma tail. This is the first time that an ICME has been directly observed interacting with a comet. SMEI's nearly all-sky coverage and image cadence affor…

2008 Journal of Geophysical Research (Space Physics)
SOHO 18