Bibcode
                                    
                            Wijnands, R.; Rupen, M.; Steeghs, D.; Wang, Q. D.; Cackett, E.; Kuulkers, E.; Fender, R.; Cornelisse, R.; Maccarone, T.; Grindlay, J.; Miller-Jones, J.; van der Klis, M.; Homan, J.; in't Zand, J.; Markwardt, C. B.
    Bibliographical reference
                                    The Astronomer's Telegram, #638
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                        10
            
                        2005
            
  Citations
                                    8
                            Refereed citations
                                    4
                            Description
                                    On 20-21 October 2005, the remaining six Chandra/HRC-I observations  (as
mentioned in ATEL #637) were performed as part of the  XMM-Newton/
Chandra monitoring campaign of the 1.7 square degree region  around Sgr
A* (Wijnands et al. 2005, A&A submitted,  astro-ph/0508648). The
neutron star X-ray transient SAX J1747.0-2853  was in the field-of-view
of one of  these observations and we detected the source at a 2-10 keV
luminosity  (at a distance of 8 kpc) of ~8E35 erg/s (obtained using
PIMMS and  assuming an absorbed power-law model with a column density of
7E22  cm^-2 and a photon index of 2; uncorrected for vignetting 
effects).