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ATEL # 2159; Peter M. Woods (Dynetics), Stefanie Wachter (IPAC/Caltech), Ersin Gogus (Sabanci Univ.) & Chryssa Kouveliotou (NASA/MSFC) report on behalf of a larger collaboration:
on 14 Aug 2009; 19:05 UT
Password Certification: Peter Woods (Peter.Woods@dynetics.com)
Subjects: X-ray, Neutron Stars, Pulsars, Soft Gamma-ray Repeaters, Transients
The recently discovered Soft Gamma Repeater SGR 0418+5729 (GCN #9499, ATEL #2077) was observed with the Chandra HRC-I on 2009 July 12 for an exposure of 24 ks. The brightest X-ray source in the image was clearly identified as the SGR through detection of the 9 sec pulsations. Two additional, uncatalogued X-ray sources were discovered within 3 arcminutes of the telescope boresight, but well separated from the position of the SGR.
No IR or optical counterparts were found in the 2MASS and DSS archives. However, a deep IR frame obtained with the WIRC on the Palomar Hale telescope revealed unambiguous IR counterparts for the two fainter X-ray sources in our Chandra image. The WIRC image was registered to the 2MASS catalog to within 0.1" (1 sigma) and thus allowed the X-ray frame to be aligned with the 2MASS astrometric calibration. A systematic offset in right ascension (0.33") and no offset in declination were found between the X-ray and IR positions of these two sources.
The registered locations of the three X-ray sources are as follows:
The absolute positional uncertainty on the SGR position is 0.35" (95% confidence). We find our position to be consistent with the original Swift XRT location (ATEL #2121), but significantly offset from the refined XRT position (ATEL #2127).
We thank Harvey Tananbaum and the Chandra team for carrying out this ToO observation. We gratefully acknowledge Chris and Dawn Gelino for contributing their WIRC image for registration of the X-ray data.