Optical counterpart to IGR J17098-3628

Details Optical counterpart to IGR J17098-3628 Optical counterpart to IGR J17098-3628

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..494....1s&link_type=abstract

The Astronomer's Telegram, #494

Astronomy and Astrophysics

Astronomy

4

Radio, Infra-Red, Optical, X-Ray, Black Holes, Neutron Stars, Transients

Scientific paper

Following the recent report of a possible radio counterpart to the X-ray transient IGR J17098-3628 (ATEL #490), we re-investigated our Magellan I-band exposures obtained on 2005 April 9 UT (see ATEL #478). The frames show a point source located at R.A.(J2000)=17:09:45.93, DEC(J2000)= -36:27:58.2 in the 2MASS reference frame (0.2" uncertainty). This optical position is consistent within 2 sigma with that derived from the radio observations (ATEL #490).

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