Swift-XRT Survey of Fermi Unassociated Sources

These results are part of the Swift program to follow-up Fermi unassociated sources in an attempt to find X-ray counterparts to the unidentified gamma-ray sources. As new observations are performed, these pages will be updated in nearly real time. Please use these results as a guide and proceed with caution when using them in a publication since they are the result of an automated analysis.

When using these data and results in publications, please reference M.C. Stroh & A.D. Falcone 2013, ApJS, 207, 28; arXiv: 1305.4949 for a description of many of the analysis techniques used to reduce these data (note: a more detailed paper describing the complete data set and analysis is forthcoming). Please contact Abe Falcone and Michael Stroh at unassociated@swift.psu.edu if you have any questions about the program or the analysis, or to simply to let us know that you've made use of these data.

Caution: For completeness, sources are listed if the "detection" exceeds 3 sigma. The significances and images are shown so you can make more stringent significance cuts, if desired.

3FGL J1025.9-5930

Field

Detected Excesses

Swift-XRT detections in the field for 3FGL J1025.9-5930

No detected excesses found.

X-Ray and Gamma Ray Catalogs

More Catalogs

Swift-XRT image with known X-ray and gamma ray sources for 3FGL J1025.9-5930

No known X-ray or gamma ray sources found.

Known Radio, Optical and UV Sources

#	Source Name	R.A. (J2000)	Dec. (J2000)	Offset (')	Database Table
1	PMN J1025-5934	10 25 30.79	-59 34 40.08	4.90	PMN
2	MGPS J102625-592408	10 26 25.90	-59 24 07.92	7.76	MGPS2
3	MGPS J102448-593420	10 24 48.79	-59 34 21.00	9.02	MGPS2
4	PMN J1024-5932	10 24 39.91	-59 32 36.96	9.59	PMN
5	MGPS J102539-591946	10 25 39.60	-59 19 45.84	11.15	MGPS2