Probable radio counterpart to IGR J17098-3628

Details Probable radio counterpart to IGR J17098-3628 Probable radio counterpart to IGR J17098-3628

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..490....1r&link_type=abstract

The Astronomer's Telegram, #490

Astronomy and Astrophysics

Astronomy

6

Radio, X-Ray, Binaries, Black Holes, Neutron Stars, Transients

Scientific paper

Very Large Array (VLA) observations of IGR J17098-3628 (ATEL #444) were made on March 31st, April 5th, April 12th, and May 4th UT, all at 4.86 GHz. The first data set showed the only significant radio source within the 2 arcminute INTEGRAL error circle, located at (J2000)

17h 09m 45.934s +/- 0.011s -36d 27' 57.30" +/- 0.55" where the error bars are based on uncertainties in a Gaussian fit (and hence reflect only the noise in the image).

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