Detection and Possible Flare of GM SGR at 29-34 GHz

Details Detection and Possible Flare of GM SGR at 29-34 GHz Detection and Possible Flare of GM SGR at 29-34 GHz

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999atel...45....1m&link_type=abstract

The Astronomer's Telegram, #45

Astronomy and Astrophysics

Astronomy

2

Radio, X-Ray, Binaries, Transients

Scientific paper

GM Sgr (SAX J1819.3-2525 = XTE J1819-254) was observed with the OVRO 40m telescope, for 10 1-minute integrations, between Sept 16.15566-16.16340 UT, following reports of the bright X-ray outburst (ATEL #43, IAUC #7253). The observations were made using a dual-beam, Dicke-switching receiver. The source was detected in four bands averaged over the full 10 minutes, with flux densities 98 +/- 21, 76 +/- 13, 86 +/- 17, 78 +/- 22 at 27, 29, 31, and 33 GHz.

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