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Swift Galactic Plane Survey: Sourcelist v3.0

ATel #5200; M. T. Reynolds, J. M. Miller, D. Maitra, K. Gultekin (University of Michigan); N. Gehrels (NASA/GSFC); J. A. Kennea, M. H. Siegel, J. Gelbord (PSU); P. Kuin (MSSL/UCL)
on 8 Jul 2013; 16:58 UT
Credential Certification: Mark Reynolds (markrey@umich.edu)

Subjects: Ultra-Violet, X-ray, Black Hole, Cataclysmic Variable, Neutron Star, Variables, Young Stellar Object, Pre-Main-Sequence Star

Referred to by ATel #: 16195

The Swift Galactic Plane Survey team report the detection of 248 point-like X-ray sources (0.3 - 10 keV) in observations covering the final 40% of our survey area (see also Atel #3951, #4318). The listed sources are those we consider to be robust detections at the current time. A comprehensive analysis with final source properties will be presented in Reynolds et al. (2013) in prep.

Sources are divided into those detected at a significance of greater than 3 sigma (189 in total - top) and 2-3 sigma (59 in total - bottom).

Please see the link at the bottom of the telegram for the full source list.
 
NAME                     |       RA      |      DEC       | Error |   Sig   |  Rate	  |       UV          |        Simbad            | Dist  
                         |    [ deg ]    |    [ deg ]     | [ " ] |         | [ ct/s ]    |    [ mag ] 	      |                          | [ " ] 
===================================================================================================================================================== 
SWIFT J163643.0-462727	 | 249.17920	 | -46.45741	  | 3.8	  |   10.1  |  4.43e-02	  |       --          |            --            | --	 
SWIFT J164635.3-450701	 | 251.64713	 | -45.11695	  | 2.1	  |   11.0  |  9.20e-02	  |       --          |     IGR J16465-4507      |  3.6	 
SWIFT J164807.0-451209	 | 252.02912	 | -45.20255	  | 4.2	  |   11.7  |  5.24e-02	  |       --          |     IGR J16479-4514      |  5.1		 
SWIFT J164913.3-435525	 | 252.30523	 | -43.92361	  | 1.4	  |   45.9  |  2.12e-01	  |       16.02       |   1RXS J164913.6-435527  |  2.9	 
SWIFT J164926.9-434909	 | 252.36229	 | -43.81922	  | 2.2	  |   41.8  |  2.12e-01	  |       --          |     IGR J16493-4348      |  0.2		 
SWIFT J165111.8-440235	 | 252.79931	 | -44.04312	  | 3.1	  |    6.8  |  3.40e-02	  |       --          |   1RXS J165111.8-440231  |  4.3	 
SWIFT J170004.7-415801	 | 255.01946	 | -41.96692	  | 3.2	  |    8.8  |  3.97e-02	  |       --          |     AX J1700.1-4157      | 18.3	 
SWIFT J170049.1-413920	 | 255.20460	 | -41.65554	  | 0.9	  |  177.0  |  2.48e+00*  |       --          |      OAO 1657-415        |  2.9	 
....... 
....... 
....... 
SWIFT J185844.5+032609	 | 284.68524	 | 3.43576	  | 7.2	  |    2.4  |  1.17e-02	  |       --	      |       XTE J1858+034      | 16.8	 
SWIFT J190429.9+060825	 | 286.12478	 | 6.14029	  | 4.3	  |    2.5  |  1.09e-02	  |       18.5,18.71  |            --            | --	 
 
 
Position error 
================== 
All position error are prelimiary 1 sigma uncertainties. 
 
Significance 
================== 
In the low count limit, source significance is calculated using the Gehrels error 
(Gehrels N., 1986, ApJ, 303, 336). 
 
 
X-ray Count rate 
================== 
* Source displays evidence of pile-up, which is not corrected for at this time. 
 
UV magnitudes 
================== 
X: Counterpart is saturated, photometry unreliable 
a: 2 measurements of the counterpart, i.e., counterpart detected in 2 seperate images 
b: 2 counterparts at approx similar separation from the X-ray source 
 
Simbad 
================== 
Candidate counterparts to the X-ray sources, as listed in the Simbad database, are indicated (w/ 
distance) if they lie within 30" of the XRT position.  
 
 
Queries: Please contact Mark Reynolds (markrey @ umich.edu) 
 
---------------------------------------------------------------------------------------------------  
The Swift Galactic Plane Survey is tiling 240 square degrees of the Galactic plane, from -60 < l < 
60 and -1 < b < -1. Each exposure is approximately 500 seconds in duration, and includes 
simultaneous XRT (0.3-10 keV) and UVOT/UVM2 images (2000-2500 Angstroms).  All values 
reported herein should be considered as preliminary, a comprehensive analysis will be presented in 
Reynolds et al. (2013) in prep.  

Swift Galactic Plane Survey: Sourcelist v3.0 (in full)