Multi-wavelength INTEGRAL NEtwork (MINE) observations of the microquasar GRS 1915+105
| dc.creator | Fuchs, Yael | |
| dc.creator | Rodriguez, J. | |
| dc.creator | Shaw, S. E. | |
| dc.creator | Kretschmar, P. | |
| dc.creator | Ribo, M. | |
| dc.creator | Chaty, S. | |
| dc.creator | Mirabel, I. F. | |
| dc.creator | Dhawan, V. | |
| dc.creator | Pooley, G. G. | |
| dc.creator | Brown, I. | |
| dc.creator | Spencer, R. | |
| dc.creator | Hannikainen, D. C. | |
| dc.date | 2004-04-01 | |
| dc.date.accessioned | 2026-07-07T02:12:48Z | |
| dc.date.available | 2026-07-07T02:12:48Z | |
| dc.description | We present the international collaboration MINE (Multi-lambda Integral NEtwork) aimed at conducting multi-wavelength observations of X-ray binaries and microquasars simultaneously with the INTEGRAL gamma-ray satellite. We will focus on the 2003 March-April campaign of observations of the peculiar microquasar GRS 1915+105 gathering radio, IR and X-ray data. The source was observed 3 times in the plateau state, before and after a major radio and X-ray flare. It showed strong steady optically thick radio emission corresponding to powerful compact jets resolved in the radio images, bright near-infrared emission, a strong QPO at 2.5 Hz in the X-rays and a power law dominated spectrum without cutoff in the 3-300 keV range. We compare the different observations, their multi-wavelength light curves, including JEM-X, ISGRI and SPI, and the parameters deduced from fitting the spectra obtained with these instruments on board INTEGRAL. | |
| dc.description | 4 pages, 9 fig., Proc. of the 5th INTEGRAL Workshop (Feb. 16-20 2004), to be published by ESA | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0404030 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0404030 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7583 | |
| dc.subject | Astrophysics | |
| dc.title | Multi-wavelength INTEGRAL NEtwork (MINE) observations of the microquasar GRS 1915+105 | |
| dc.type | text |