Search Publications

In-flight calibration of the ISGRI camera
DOI: 10.1051/0004-6361:20031391 Bibcode: 2003A&A...411L.167T

Goldoni, P.; Malaguti, G.; David, P. +12 more

ISGRI, the IBIS low energy camera (15 keV-1 MeV) on board INTEGRAL, is the first large CdTe gamma-ray imager in orbit. We present here an overview of the ISGRI in-flight calibrations performed during the first months after launch. We discuss the stability of the camera as well as the CdTe pixels response under cosmic radiation. The energy calibrat…

2003 Astronomy and Astrophysics
INTEGRAL 35
The central engines of radio-loud quasars
DOI: 10.1051/0004-6361:20031218 Bibcode: 2003A&A...409..887W

Ho, L. C.; Staubert, R.; Wang, J. -M.

We have assembled a sample of 37 radio-loud quasars that have been imaged with the Hubble Space Telescope in order to investigate their black hole masses, accretion rates, and the structure of their accretion disks. The black hole masses were estimated from the luminosities of the host galaxies, and the accretion powers were extrapolated from the …

2003 Astronomy and Astrophysics
eHST 35
The nature of the prompt X-ray and radio emission from SN 2002ap
DOI: 10.1051/0004-6361:20021576 Bibcode: 2003A&A...397.1011S

Ray, A.; Bhatnagar, S.; Chandra, P. +1 more

We report on the combined X-ray and radio observations of the type Ic SN 2002ap, using XMM-Newton TOO observation of M 74 and the Giant Metrewave Radio Telescope (GMRT). We account for the presence of a nearby source in the pre-supernova Chandra field of view in our measurements of the X-ray flux (0.3 - 10 KeV) 5.2 days after the explosion. The X-…

2003 Astronomy and Astrophysics
XMM-Newton 34
XMM-Newton light curves of the low-mass X-ray binary EXO 0748-676: Dips, eclipses, and bursts
DOI: 10.1051/0004-6361:20031484 Bibcode: 2003A&A...412..799H

Wijnands, R.; van den Berg, M.; Homan, J.

We present an analysis of XMM-Newton light curves of the dipping, bursting, and eclipsing low-mass X-ray binary EXO 0748-676, focusing on the variability on time scales of seconds to hours. The observed variability can be roughly divided in three types: dips, eclipses and bursts. We find that the appearance of the latter two, depends strongly on t…

2003 Astronomy and Astrophysics
XMM-Newton 34
Explanatory supplement of the ISOGAL-DENIS Point Source Catalogue
DOI: 10.1051/0004-6361:20030416 Bibcode: 2003A&A...403..955S

Alard, C.; Blommaert, J. A. D. L.; Ganesh, S. +10 more

We present version 1.0 of the ISOGAL-DENIS Point Source Catalogue (PSC), containing more than 100 000 point sources detected at 7 and/or 15 mu m in the ISOGAL survey of the inner Galaxy with the ISOCAM instrument on board the Infrared Space Observatory (ISO). These sources are cross-identified, wherever possible, with near-infrared (0.8-2.2 mu m) …

2003 Astronomy and Astrophysics
ISO 34
XMM-Newton observation of the ULIRG NGC 6240. The physical nature of the complex Fe K line emission
DOI: 10.1051/0004-6361:20031217 Bibcode: 2003A&A...411...63B

Costantini, E.; Hasinger, G.; Boller, Th. +5 more

We report on an XMM-Newton observation of the ultraluminous infrared galaxy NGC 6240. The 0.3-10 keV spectrum can be successfully modelled with: (i) three collisionally ionized plasma components with temperatures of about 0.7, 1.4, and 5.5 keV; (ii) a highly absorbed direct power-law component; and (iii) a neutral Fe Kalpha and Kbeta line. We dete…

2003 Astronomy and Astrophysics
XMM-Newton 34
A simple analytical expression for the power spectrum of cascading Alfvén waves in the solar wind
DOI: 10.1051/0004-6361:20030914 Bibcode: 2003A&A...407..713V

Laitinen, T.; Fichtner, H.; Vainio, R.

Alfvén wave transport in the solar wind, including non-linear spectral energy transfer, is studied. We present numerical solutions of wave transport using a diffusive flux function previously introduced for spectral energy transfer, and compare it with the analytical solution obtained for a convective flux function. The two models of cascading pro…

2003 Astronomy and Astrophysics
SOHO 34
Plasma properties above coronal active regions inferred from SOHO/UVCS and radio spectrograph observations
DOI: 10.1051/0004-6361:20021844 Bibcode: 2003A&A...400..347M

Raymond, J. C.; Wu, R.; Kohl, J. +3 more

Information on coronal plasma was inferred from the joint analysis of type {II} radio bursts and SOHO UltraViolet Coronagraph Spectrometer (UVCS) observations. The data sample comprises 37 metric type {II} radio bursts observed by ground-based radio spectrographs in 1999, during the rising phase of the solar cycle. The coronal electron densities n…

2003 Astronomy and Astrophysics
SOHO 34
Hipparcos red stars in the HpVT2 and VIC systems
DOI: 10.1051/0004-6361:20021589 Bibcode: 2003A&A...397..997P

Makarov, V. V.; Berdnikov, L. N.; Lebzelter, T. +6 more

For Hipparcos M, S, and C spectral type stars, we provide calibrated instantaneous (epoch) Cousins V - I color indices using newly derived HpVT2 photometry. Three new sets of ground-based Cousins VI data have been obtained for more than 170 carbon and red M giants. These datasets in combination with the published sources of V…

2003 Astronomy and Astrophysics
Hipparcos 33
Near-IR spectra of ISOGAL sources in the inner Galactic Bulge
DOI: 10.1051/0004-6361:20030459 Bibcode: 2003A&A...405..531S

Omont, A.; Schultheis, M.; Ojha, D. K. +2 more

We present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15;mu m detected during the ISOGAL survey. Making use of the DENIS interstellar extinction map from Schultheis et al. (1999) we derive luminosities and find that the Mbol vs. 12CO and M_bol vs. H2O diagrams are powerful to…

2003 Astronomy and Astrophysics
ISO 33