Improved (and revised) position of IGR J19140+0951 with INTEGRAL

Details Improved (and revised) position of IGR J19140+0951 with INTEGRAL Improved (and revised) position of IGR J19140+0951 with INTEGRAL

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..272....1c&link_type=abstract

The Astronomer's Telegram, #272

Astronomy and Astrophysics

Astronomy

5

X-Ray, Gamma Ray, Agn, Binaries, Transients

Scientific paper

We have analysed about 300 ks of JEM-X2 data and about 600ks of IBIS/ISGRI data in order to constrain with more accuracy the position of the transient IGR J19140+0951 (formerly known as IGR J19140+098). Based on 12 independent detections of the source in JEM-X2 and using JEM-X offline software (Lund et al., 2004) we have derived a weighted mean position. The new position (uncertainty at 90% : 1.7 arcmin) is 2.4 arcmin away from the first position derived with IBIS (IAUC #8088) obtained using early versions of the Offline Scientific Analysis Software.

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