Swift UVOT Observations of the X-ray transient in NGC 2770

Details Swift UVOT Observations of the X-ray transient in NGC 2770 Swift UVOT Observations of the X-ray transient in NGC 2770

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1356....1k&link_type=abstract

The Astronomer's Telegram, #1356

Astronomy and Astrophysics

Astronomy

2

Optical, X-Ray, Transients

Scientific paper

Swift performed an observation of the X-ray transient in NGC 2770 on 2008 Jan 11 02:45UT. No X-ray source was detected in the 1.1ks observation. However, the optical transient (e.g., GCN #7163) was clearly detected in the U, V, and B bands of the UVOT. The source was marginally seen in the UVW1 image. The very rough B and V magnitude is 18.8 and 18.4, respectively. The Swift observations indicate that the optical transient becomes brighter in the past 24 hours.

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