X-ray localization and possible IR counterpart of XTE J1747-274/ IGR J17473-2721

Details X-ray localization and possible IR counterpart of XTE J1747-274/ IGR J17473-2721 X-ray localization and possible IR counterpart of XTE J1747-274/ IGR J17473-2721

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..521....1j&link_type=abstract

The Astronomer's Telegram, #521

Astronomy and Astrophysics

Astronomy

13

Infra-Red, X-Ray, Gamma Ray, Binaries, Transients

Scientific paper

On 2005 June 6 23:56UT, we observed a field centered on the source XTE J1747-274 (Markwardt et al., ATEL #498) using the HRC-I on Chandra for 1.1 ks. With a 30' x 30' field of view, we were able to cover an area twice the error circle of the RXTE detection. We found only 1 source in the entire Chandra FOV at a position of RA = 17 47 18.06 Dec. = -27 20 38.9 with an error radius of 0.8". This position is consistent with the source found in a Swift observation of the field (Kennea et al., ATEL #500).

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