Refined position for Ginga 1843+009 with the Swift/XRT

Details Refined position for Ginga 1843+009 with the Swift/XRT Refined position for Ginga 1843+009 with the Swift/XRT

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.1973....1k&link_type=abstract

The Astronomer's Telegram, #1973

Astronomy and Astrophysics

Astronomy

1

X-Ray, Binaries, Pulsars, Transients

Scientific paper

The hard X-ray transient pulsar and high-mass X-ray binary system Ginga 1843+009 was recently reported to be in outburst (Krimm et al, ATel #1959). Observations of this source were performed with the X-Ray Telescope (XRT) on Swift covering 2169 total seconds beginning at 2009-03-15 12:31:14 UT. The source was strongly detected in the XRT and the position was determined to be RA(J2000) : 18h 45m 36s.9 (281.40372 deg) Dec (J2000): +00d 51' 48".2 (+0.86338 deg) with an estimated uncertainty of 1.5'' radius (90% confidence).

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