The behavior of subluminous X-ray transients near the Galactic center as observed using the X-ray telescope aboard Swift

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Table 2:

*Chandra* positions (J2000) and errors of the transients that were found in archival data.
	Coordinates^a
Name	RA	Dec	Err.	Obs ID	Date
	(h m s)	$(^{\circ}~'~'')$	('')
AX J1745.6-2901	17:45:35.65	-29:01:34.0	0.6	6639	2006-04-11
CXOGC J174535.5-290124	17:45:35.56	-29:01:23.9	0.6	6644	2006-08-22
CXOGC J174540.0-290005	17:45:40.06	-29:00:05.5	0.6	6646	2006-10-29
Swift J174553.7-290347	17:45:53.94	-29:03:46.9	0.6	6363	2006-07-17
Swift J174622.1-290634	17:46:22.25	-29:06:32.5	1.3	6642	2006-07-04

^a The quoted position uncertainties ( $1 \sigma$ ) were calculated by taking the square root of the quadric sum of the statistical error (from the wavdetect routine) and the uncertainty in absolute astrometry (0.6''; Aldcroft et al. 2000).

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