Search Publications

Ground calibration of the Chandrayaan-1 X-ray Solar Monitor (XSM)
DOI: 10.1016/j.nima.2009.06.049 Bibcode: 2009NIMPA.607..544A

Andersson, H.; Grande, M.; Alha, L. +9 more

The Chandrayaan-1 XSM ground calibrations are introduced. The aim of these calibrations was to characterize the performance of XSM, which enables a reliable spectral analysis with the solar X-ray data. The calibrations followed an improved procedure based on our experience from the SMART-1 XSM. The most important tasks in the calibrations were det…

2009 Nuclear Instruments and Methods in Physics Research A
Chandrayaan-1 SMART-1 17
In situ radiometric dating on Mars: Investigation of the feasibility of K-Ar dating using flight-type mass and X-ray spectrometers
DOI: 10.1016/j.pss.2009.02.012 Bibcode: 2009P&SS...57.1237T

Barber, S.; Talboys, D. L.; Bridges, J. C. +9 more

The absolute chronology of Mars is poorly known and, as a consequence, a key science aim is to perform accurate radiometric dating of martian geological materials. The scientific benefits of in situ radiometric dating are significant and arguably of most importance is the calibration of the martian cratering rate, similar to what has been achieved…

2009 Planetary and Space Science
MEx 17
CME-flare association during the 23rd solar cycle
DOI: 10.1016/j.asr.2009.01.028 Bibcode: 2009AdSpR..43.1032M

Beheary, M. M.; Youssef, M.; Mawad, R. +2 more

The relation between coronal mass ejections (CMEs) and solar flares are statistically studied. More than 10,000 CME events observed by SOHO/LASCO during the period 1996-2005 have been analyzed. The soft X-ray flux measurements provided by the Geostationary Operational Environmental Satellite (GOES), recorded more than 20,000 flares in the same tim…

2009 Advances in Space Research
SOHO 17
The spectroscopically confirmed huge cosmic structure at z = 0.55
DOI: 10.1051/0004-6361/200912929 Bibcode: 2009A&A...505L...9T

Finoguenov, A.; Tanaka, M.; Koyama, Y. +3 more

We report on the spectroscopic confirmation of a huge cosmic structure around the CL0016 cluster at z=0.55. We made wide-field imaging observations of the surrounding regions of the cluster and identified more than 30 concentrations of red galaxies near the cluster redshift. The follow-up spectroscopic observations of the most prominent part of th…

2009 Astronomy and Astrophysics
XMM-Newton 17
Sounding the subsurface of Athabasca Valles using MARSIS radar data: Exploring the volcanic and fluvial hypotheses for the origin of the rafted plate terrain
DOI: 10.1029/2008JE003299 Bibcode: 2009JGRE..114.8003B

Gurnett, Donald A.; Frigeri, Alessandro; Heggy, Essam +8 more

To test the volcanic and fluvial hypotheses for the origin of the rafted plate terrain observed in the vicinity of Athabasca Valles (5°N, 150°E, Central Elysium Planitia), we investigated the subsurface radar echo from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) 5-MHz band data over this area. The backscattered signal l…

2009 Journal of Geophysical Research (Planets)
MEx 17
New absolute magnitude calibrations for W Ursa Majoris type binaries
DOI: 10.1002/asna.200811041 Bibcode: 2009AN....330...68E

Demircan, O.; Eker, Z.; Bilir, S. +2 more

Parallaxes of W UMa stars in the Hipparcos catalogue have been analyzed. 31 W UMa stars, which have the most accurate parallaxes (σπ/π<0.15) which are neither associated with a photometric tertiary nor with evidence of a visual companion, were selected for re-calibrating the Period-Luminosity-Color (PLC) relation of W UMa stars. Usin…

2009 Astronomische Nachrichten
Hipparcos 17
Suzaku Observation Adjacent to the South End of the Radio Arc
DOI: 10.1093/pasj/61.3.593 Bibcode: 2009PASJ...61..593F

Koyama, Katsuji; Tsuru, Takeshi Go; Fukuoka, Ryosuke +1 more

Suzaku observed the Galactic center region near the Radio Arc at ∼20' southeast of Sagittarius A*. In an 18' × 18' field of view, we found four distinct X-ray sources: a bright star and a diffuse source associated with star clusters in the soft band (0.5-2.0keV), a small clump in a higher energy band (4-6keV), and a peculiar clump in th…

2009 Publications of the Astronomical Society of Japan
Suzaku 17
A dam around the Water Fountain Nebula?. The dust shell of IRAS16342-3814 spatially resolved with VISIR/VLT
DOI: 10.1051/0004-6361/200911984 Bibcode: 2009A&A...503..837V

Waters, L. B. F. M.; Peletier, R. F.; Verhoelst, T. +4 more

Context: Bipolar morphologies in planetary nebulae (PNe) are believed to be closely linked to binary central stars. Either by collimating a fast stellar wind or by driving a jet via accretion in the central system, dusty torii or stable disks may be crucial ingredients for the shaping of PNe.
Aims: We study the dust distribution in the very yo…

2009 Astronomy and Astrophysics
ISO 17
Impact of a Radius and Composition Variation on Stratification of the Solar Subsurface Layers
DOI: 10.1088/0004-637X/690/2/1272 Bibcode: 2009ApJ...690.1272L

Lefebvre, S.; Turck-Chièze, S.; Nghiem, P. A. P.

Several works have reported changes of the Sun's subsurface stratification inferred from f-mode or p-mode observations. Recently, a nonhomologous variation of the subsurface layers with depth and time has been deduced from f-modes. Progress on this important transition zone between the solar interior and the external part supposes a good understan…

2009 The Astrophysical Journal
SOHO 17
Different Types of Ultraluminous X-Ray Sources in NGC 4631
DOI: 10.1088/0004-637X/696/1/287 Bibcode: 2009ApJ...696..287S

Soria, Roberto; Ghosh, Kajal K.

We have re-examined the most luminous X-ray sources in the starburst galaxy NGC 4631, using XMM-Newton, Chandra, and ROSAT data. The most interesting source is a highly variable supersoft ultraluminous X-ray source (ULX). We suggest that its bolometric luminosity ~ a few 1039 erg s-1 in the high/supersoft state: this is an or…

2009 The Astrophysical Journal
XMM-Newton 17