The microquasar GRS 1915+105

See Fig.9 from Dhawan+, 2000, ApJ, v543, n1)
where Radio flux density variations are shown at three wavelengths, monitored by the VLA during the plateau state on 1997 May 15, 06 - 16 UTC. Inset is the VLBA at 2 cm, from observations during the gap in the VLA coverage from 10 to 12 UTC.

See Fig.4 from Dhawan+, 2000, ApJ, v543, n1)

See total ASM Rossi XTE data about GRS 1915+105 in 2-12 keV range.

The total light curves GRS 1915+105 with GBI at 2.25 and 8.3 GHz.
See GBI data, alpha 8.3-2.25 GHz

GRS 1915+105 monitoring with RATAN-600 in 17 July - 25 November 2000 at 3.9 GHz.
The ASM Rossi XTE data in 2-12 keV range during the same time.

The preliminary light curves at 3.9, 7.7 and 11.2 GHz (17 July - 25 November 2000)
See the light curves at 3.9 GHz and dwell-by-dwell ASM XTE data in July 2000

The RATAN spectra of GRS 1915+105:

The flare in 25 Jul 2000 , where spectral index = -0.36 (RATAN).

The flare in 05 and 06 August 2000 .

The high-frequency flare in 21 - 26 November 2000 .

See Light curves in September 2000 when there is the good correlation of the light curves at 3.9 GHz (RATAN) and 2.25+8.3 GHz (GBI).

The spectra of the flare in 22 - 25 March 2001 .

Light curves in May 2004 .

The RATAN light curves from 15 September 2005 to 15 April 2006 .

The RATAN spectra in 03-15 October 2005 .

S.Trushkin, 03/02/2006