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The XMM-Newton/2dF survey - V. The radio properties of the X-ray population
DOI: 10.1111/j.1365-2966.2004.07991.x Bibcode: 2004MNRAS.352.1005G

Georgakakis, A.; Georgantopoulos, I.; Akylas, A. +3 more

In this paper, we cross-correlate the FIRST (Faint Images of the Radio Sky at Twenty centimeters) 1.4-GHz radio survey with a wide-field (1.6 deg2) shallow [fX(0.5 - 8keV) ~ 10-14erg s-1]XMM-Newton survey. We find 12 X-ray/radio matches representing 4 per cent of the X-ray-selected sample. Most of them a…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
VISPO project: visible image-spectrometer for planetary observations
DOI: 10.1016/j.newast.2004.04.007 Bibcode: 2004NewA....9..635M

Piccioni, G.; Capaccioni, F.; De Petris, M. +3 more

Satellite instrumentations designed for planetary studies are often open to other interesting applications from ground: not only one can efficiently carry out detailed calibrations before space data become available, but also the prototypes of the satellite instruments can be successfully employed in different fields ranging from astrophysics to c…

2004 New Astronomy
Rosetta 1
Simulation studies of high-latitude magnetospheric boundary dynamics
DOI: 10.1360/03yd0117 Bibcode: 2004ScChE..47..421P

Zhang, H.; Liu, Z. X.; Shi, Q. Q. +4 more

2004 Science in China E: Technological Sciences
Cluster 1
X-ray Archaeology of Galaxy Groups
Bibcode: 2004cgpc.sympE..39O

Ponman, T. J.; Osmond, J. P. F.

We have assembled a sample of 60 galaxy groups in order to study the hot intragroup medium and better understand the processes by which it formed. We have analysed ROSAT data for all 60 groups and have obtained XMM data for a small subset. Here we present an initial analysis of the XMM data for NGC 5171, and a comparison with the ROSAT data. This …

2004 Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution
XMM-Newton 1
A Search for Short-Timescale Microvariability in Active Galactic Nuclei in the Ultraviolet
DOI: 10.1086/383460 Bibcode: 2004ApJ...607...84D

Dolan, Joseph F.; Clark, L. Lee

We observed four active galactic nuclei (AGNs) (the type 1 Seyfert systems 3C 249.1, NGC 6814, and Mrk 205, and the BL Lac object 3C 371) using the High Speed Photometer on the Hubble Space Telescope (HST) to search for short-timescale microvariability in the UV. Continuous observations of ~3000 s duration were obtained for each system on several …

2004 The Astrophysical Journal
eHST 1
Probing diffusion parameters of suprathermal ions near heliospheric shocks
DOI: 10.1016/j.asr.2003.03.067 Bibcode: 2004AdSpR..34..157K

Klecker, B.; Hilchenbach, M.; Kallenbach, R. +1 more

The distribution functions of suprathermal ions in the energy range 35-2000 keV/amu associated with the interplanetary coronal mass ejection of 14-16 July 2000 are analyzed. The ion spectra agree with a theoretical model on momentum diffusion in two-dimensional magnetohydrodynamic turbulence.

2004 Advances in Space Research
SOHO 1
Measurements and Calibration of Tropospheric Delay at Goldstone from the Cassini Media Calibration System
Bibcode: 2004IPNPR.158A...1K

Tanner, A.; Keihm, S. J.; Rosenberger, H.

One and one-half years of near-continuous measurements of the troposphere-induced path delay at Goldstone have been analyzed in order to (1) characterize the troposphere-delay fluctuations in a statistical sense and (2) evaluate the path-delay calibration performance of the Media Calibration System (MCS) at DSS 25. Both the wet and dry components …

2004 Interplanetary Network Progress Report
Cassini 1
The Compton trail of gamma-ray bursts: A long-after glow
DOI: 10.1051/0004-6361:20041344 Bibcode: 2004A&A...420..501A

Parizot, E.; Allard, D.

As they travel through the gas of the host galaxy, some of the gamma-rays emitted in a Gamma-Ray Burst (GRB) may experience Compton scattering and reach an observer even if he is not located in the direction of the primary photon beam. Such a process will last until the GRB photons have left their host galaxy, and the ambient electron density beco…

2004 Astronomy and Astrophysics
INTEGRAL 1
Classical Cepheids and the Distances of HST Program Galaxies
DOI: 10.1023/B:ASYS.0000040167.18807.52 Bibcode: 2004Ap.....47..389A

Abrahamyan, H. V.

The distances of HST program galaxies are revised using the PL-relations we have obtained previously along with a different method from that employed by Freedman et al. On the average, the resulting distances to these galaxies have higher internal accuracies than those obtained before by others. In addition, we have used no corrections for metalli…

2004 Astrophysics
eHST 1
The Transition from Outburst to Low Level Activity in the Low-Mass X-Ray Binary SAX J1747.0-2853
Bibcode: 2004BaltA..13..163W

Ubertini, P.; Bazzano, A.; Heise, J. +6 more

SAX J1747.0-2853 is an X-ray transient which exhibited several outbursts between 1998 and 2001 and most probably in 1976. The outburst of 2000 was the longest and brightest. We have analyzed X-ray data sets that focus on times around the 2000 outburst and were obtained with l BeppoSAX, XMM-Newton and l RXTE.

2004 Baltic Astronomy
XMM-Newton 1