Search Publications

The effect of protons on the performance of swept-charge devices
DOI: 10.1016/j.nima.2009.01.051 Bibcode: 2009NIMPA.604..177S

Smith, David R.; Gow, Jason

The e2v technologies CCD54, or swept-charge device (SCD) has been extensively radiation tested for use in the Chandrayaan-1 X-ray Spectrometer (C1XS) instrument, to be launched as a part of the Indian Space Research Organisation (ISRO) Chandrayaan-1 payload in 2008. The principle use of the SCD is in X-ray fluorescence (XRF) applications, the devi…

2009 Nuclear Instruments and Methods in Physics Research A
Chandrayaan-1 SMART-1 7
X-Ray Studies of HESS J1837-069 with Suzaku and ASCA: a VHE Gamma-Ray Source Originated from the Pulsar Wind Nebula
DOI: 10.1093/pasj/61.sp1.S183 Bibcode: 2009PASJ...61S.183A

Dotani, Tadayasu; Ebisawa, Ken; Bamba, Aya +1 more

We present ASCA and Suzaku studies of the TeV source HESS J1837-069, which has not been identified in other wavelengths. We confirm the presence of two X-ray sources in the Suzaku XIS image, AX J1838.0-0655 and AX J1837.3-0652, near both ends of the elongated TeV emission region. The XIS spectra of the two sources were reproduced by an absorbed po…

2009 Publications of the Astronomical Society of Japan
Suzaku 7
Suzaku Spectroscopy of Vela Shrapnel B
DOI: 10.1088/0004-637X/696/2/1548 Bibcode: 2009ApJ...696.1548Y

Yamaguchi, H.; Katsuda, S.

We present the X-ray observation of Vela shrapnel B with the X-ray Imaging Spectrometer on board the Suzaku satellite. The shrapnel is one of several ejecta fragmentlike features protruding beyond the primary blast wave shock front of the Vela supernova remnant. The spectrum of shrapnel B is well represented by a single-temperature thin-thermal pl…

2009 The Astrophysical Journal
Suzaku 7
Advances in Plasmaspheric Wave Research with CLUSTER and IMAGE Observations
DOI: 10.1007/s11214-009-9508-7 Bibcode: 2009SSRv..145..137M

Carpenter, Donald L.; Darrouzet, Fabien; Grimald, Sandrine +8 more

This paper highlights significant advances in plasmaspheric wave research with Cluster and Image observations. This leap forward was made possible thanks to the new observational capabilities of these space missions. On one hand, the multipoint view of the four Cluster satellites, a unique capability, has enabled the estimation of wave characteris…

2009 Space Science Reviews
Cluster 7
Vector Magnetic Fields and Electric Currents From the Imaging Vector Magnetograph
DOI: 10.1088/0004-637X/692/2/1543 Bibcode: 2009ApJ...692.1543L

van Ballegooijen, A. A.; Li, Jing; Mickey, Don

First, we describe a general procedure to produce high-quality vector magnetograms using the Imaging Vector Magnetograph (IVM) at Mees Solar Observatory. Two IVM effects are newly discussed and taken into account: (1) the central wavelength of the Fabry-Pérot is found to drift with time as a result of undiagnosed thermal or mechanical instabilitie…

2009 The Astrophysical Journal
SOHO 7
Astrometric and photometric observations of solar system bodies with Pulkovo Observatory's automatic mirror astrograph ZA-320M
DOI: 10.1134/S0038094609030058 Bibcode: 2009SoSyR..43..229D

Gorshanov, D. L.; Kouprianov, V. V.; Devyatkin, A. V. +3 more

A brief description of the process of astrometric and photometric observations and their processing by an automatic complex, based on Pulkovo Observatory’s ZA-320M telescope, is presented. The basic results of astrometric and photometric observations of Solar System bodies obtained during 1997-2007 are given. They include, in particular, the resul…

2009 Solar System Research
Hipparcos 7
Mapping the Spatial Distribution of Dust Extinction in NGC 959 Using Broadband Visible and Mid-Infrared Filters
DOI: 10.1088/0004-6256/138/6/1634 Bibcode: 2009AJ....138.1634T

Jansen, R. A.; Windhorst, R. A.; Tamura, K.

We present a method to estimate and map the two-dimensional distribution of dust extinction in the late-type spiral galaxy NGC 959 from the theoretical and observed flux ratio of optical V and mid-IR (MIR) 3.6 µm images. Our method is applicable to both young and old stellar populations for a range of metallicities, and is not restricted to …

2009 The Astronomical Journal
eHST 7
Adapting Marchal's test of escape to real triple stars
DOI: 10.1051/0004-6361/200809392 Bibcode: 2009A&A...504..277L

Li, P. J.; Fu, Y. N.; Sun, Y. S.

Context: For a general N-body system, Marchal constructed an analytical test of escape, which uses only a one-dimensional projected motion state of the system at any given instant. This test is well adapted to identifying real, disintegrating small stellar systems, of which the full motion states are generally unavailable. However, to our knowledg…

2009 Astronomy and Astrophysics
Hipparcos 7
Cross-Calibration of SMART-1 XSM with GOES and RHESSI
DOI: 10.1007/s11207-009-9461-3 Bibcode: 2009SoPh..260..479V

Väänänen, Mikko; Alha, Lauri; Huovelin, Juhani

A number of X-ray instruments have been active in observing the solar coronal X-ray radiation this decade. We have compared XSM observations with simultaneous GOES and RHESSI observations. We present flux calibrations for all instruments and compare XSM and GOES total emission measures (TEM) and temperatures (T).

2009 Solar Physics
SMART-1 7
The X-ray properties of the energetic pulsar PSR J1838-0655
DOI: 10.1111/j.1365-2966.2009.15468.x Bibcode: 2009MNRAS.400..168L

Lin, Lupin Chun-Che; Takata, Jumpei; Hwang, Chorng-Yuan +1 more

We present and interpret several new X-ray features of the X-ray pulsar PSR J1838-0655. The X-ray data are obtained from the archival data of Chandra, RXTE and Suzaku. We combine all these X-ray data and fit the spectra with different models. We find that the joint spectra are difficult to fit with a single power law; a broken power-law model with…

2009 Monthly Notices of the Royal Astronomical Society
Suzaku 7