Related pages: Burst Analyser | Light curve | Spectrum | Download obs data | SPER analysis
| RA (J2000): | 10 56 36.11 |
|---|---|
| Dec (J2000): | +14 26 30.3 |
| 90% Error radius: | 2.6" |
| Number of overlaps included in position: | 1 |
| Exposure time in final position: | 2254 s |
| Total number of overlaps considered: | 18 |
| Total overlap time: | 8786 s |
| Number of overlaps where no X-ray source was found: | 17 |
| Number of low-X-ray-count fits rejected: | 0 |
| Number of spurious fits rejected: | 0 |
| Number of bad astrometric corrections: | 0 |
| Number of outliers removed: | 0 |
For details of how these positions are produced, and why some positions are rejected, see the online documentation.
The following paragraphs should be used to announce this position in a GCN circular:
Using 2254 s of XRT Photon Counting mode data and 1 UVOT
images, we find an astrometrically corrected X-ray position (using the XRT-UVOT
alignment and matching to the USNO-B1 catalogue): RA, Dec = 164.1505, 14.4417 which
is equivalent to:
RA (J2000): 10 56 36.11
Dec (J2000): +14 26 30.3
with an uncertainty of 2.6 arcsec (90% confidence).
This position may be improved as more data are received. The latest position can be viewed at http://www.swift.ac.uk/xrt_positions. Position enhancement is described by Goad et al. (2007, A&A, 476, 1401) and Evans et al. (2009, arXiv:0812.3662).
The image below shows the UVOT field with the final, astrometrically corrected XRT refined position. The image is 50" to a side, and contains 890 s of data in the WHITE filter.
The final position (magenta) is the weighted mean of 1 positions (green). A further 0 positions were rejected, either because they had too few photons to be secure (red) or because they are more than 3 sigma away from the mean position, more than 40" from the early mean, or had a problematic astrometric correction (yellow). The image is 50" to a side.