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A solar spectrum for PFS data analysis
DOI: 10.1016/j.pss.2004.12.008 Bibcode: 2005P&SS...53.1009F

Formisano, Vittorio; Fiorenza, Carlo

A measured calibrated solar radiance in the range 1.2- 5µm, with the spectral sampling of 1cm-1 does not exist. When studying the measured Planetary Fourier Spectrometer (PFS) spectra of the Earth's or Mars's atmosphere we discover that the most used solar spectrum contains several important errors. Here we present a "calibrated" …

2005 Planetary and Space Science
MEx 37
Theoretical Interpretation of the Luminosity and Spectral Properties of GRB 031203
DOI: 10.1086/498614 Bibcode: 2005ApJ...634L..29B

Ruffini, Remo; Bernardini, Maria Grazia; Fraschetti, Federico +3 more

The X-ray and gamma-ray observations of the source GRB 031203 by INTEGRAL are interpreted within our theoretical model. In addition to a complete spacetime parameterization of the GRB, we specifically assume that the afterglow emission originates from a thermal spectrum in the comoving frame of the expanding baryonic matter shell. By determining t…

2005 The Astrophysical Journal
INTEGRAL 37
X-Ray Timing, Spectroscopy, and Photometry of the Anomalous X-Ray Pulsar Candidate CXOU J010043.1-721134
DOI: 10.1086/432441 Bibcode: 2005ApJ...627L.137M

Ransom, S. M.; Gaensler, B. M.; Kaspi, V. M. +2 more

We present new X-ray timing and spectral results on the 8.0 s X-ray pulsar CXOU J010043.1-721134 from a series of observations using the Chandra X-Ray Observatory. We found a spin period in 2004 January of 8.020392+/-0.000009 s. A comparison of this to the 2001 Chandra observations implies a period derivative P˙=(1.88+/-0.08)×10-11 s s<…

2005 The Astrophysical Journal
XMM-Newton 37
On the Combination of Differential Emission Measure Analysis and Rotational Tomography for Three-dimensional Solar EUV Imaging
DOI: 10.1086/431295 Bibcode: 2005ApJ...628.1070F

Frazin, R. A.; Weber, M. A.; Kamalabadi, F.

Conventional differential emission measure (DEM) analysis allows one to determine the amount of plasma as a function of temperature along a given line of sight. A completely different technique called solar rotational tomography (SRT) exploits the view angles provided by solar rotation to determine the spatial distribution of emissivity in three d…

2005 The Astrophysical Journal
SOHO 37
X-ray observations of the edge-on star-forming galaxy NGC 891 and its supernova SN1986J
DOI: 10.1111/j.1365-2966.2005.09336.x Bibcode: 2005MNRAS.362..581T

Stevens, Ian R.; Raychaudhury, Somak; Temple, Rowan F.

We present XMM-Newton observations of NGC 891, a nearby edge-on spiral galaxy. We analyse the extent of the diffuse emission emitted from the disc of the galaxy, and find that it has a single-temperature profile with best-fitting temperature of 0.26 keV, though the fit of a dual-temperature plasma with temperatures of 0.08 and 0.30 keV is also acc…

2005 Monthly Notices of the Royal Astronomical Society
XMM-Newton 37
Solar energetic electrons related to the 28 October 2003 flare
DOI: 10.1029/2004JA010910 Bibcode: 2005JGRA..110.9S04K

Krucker, S.; Mann, G.; Kunow, H. +4 more

We investigate the solar origin of near-relativistic electrons and protons during the X17.2/4B flare as observed by the Comprehensive Suprathermal and Energetic Particle Analyser (COSTEP) and Three-Dimensional Plasma (3DP) analyzer experiments on board the SOHO and Wind spacecraft. These observations are combined with ground- and space-based spect…

2005 Journal of Geophysical Research (Space Physics)
SOHO 37
The First Precise Determination of an Optical-Far-Ultraviolet Extinction Curve Beyond the Local Group (z=0.83)
DOI: 10.1086/426579 Bibcode: 2005ApJ...619..749M

Kochanek, C. S.; Arribas, S.; Muñoz, J. A. +3 more

We present the optical-far-ultraviolet extinction curve of the dust in the lens galaxy of the gravitational lens system SBS 0909+532 (z=0.83). Extending our previous optical-UV estimate (from λ-10~2 to 5 µm-1) into the far ultraviolet (from λ-10~5 to 8 µm-1) is crucial f…

2005 The Astrophysical Journal
eHST 37
A Multi-Instrument Study of the Helix Nebula Knots with the Hubble Space Telescope
DOI: 10.1086/430803 Bibcode: 2005AJ....130..172O

O'Dell, C. R.; Henney, W. J.; Ferland, G. J.

We have conducted a combined observational and theoretical investigation of the ubiquitous knots in the Helix Nebula (NGC 7293). We have constructed a combined hydrodynamic + radiation model for the ionized portion of these knots and have accurately calculated a static model for their molecular regions. Imaging observations in optical emission lin…

2005 The Astronomical Journal
eHST 37
Independent Global Modes of Solar Magnetic Field Fluctuations
DOI: 10.1007/s11207-005-8187-0 Bibcode: 2005SoPh..226..359C

Lawrence, J. K.; Cadavid, A. C.; Ruzmaikin, A. +1 more

Observed solar, interplanetary and geomagnetic time series contain quasi periodicities on scales of 1-2.5 years. The further discovery of 1.3 year fluctuations in helioseismic observations suggests that a variety of signals may be related to the underlying dynamo in the Sun. We use independent component analysis to study the temporal and spatial v…

2005 Solar Physics
SOHO 37
Ion sound wave packets at the quasiperpendicular shock front
DOI: 10.1029/2005GL024660 Bibcode: 2005GeoRL..3224106B

Krasnoselskikh, V.; Dunlop, M.; Fazakerley, A. +6 more

Electric field measurements from a single spacecraft have been used to study ion-sound turbulence observed within the Earth's bow shock. The observed frequency of the ion-sound waves can be both lower and higher than the local electron cyclotron frequency depending upon the direction of wave propagation in the plasma rest frame. The ion-sound wave…

2005 Geophysical Research Letters
Cluster 37