Details on Acronym: SwF3 | |
| SwF3 | (SwF3) |
| Write: | <<SwF3 JHHMMSS.s+DDMMSS>> <<SwF3 JHHMMSS.ss+DDMMSS>> |
| N: | 217+105+187 |
| Object: | (X) (SIMBAD class: X = X-ray Source) |
| Note: | Swift XRT observations of N=217+105+187 X-ray sources within the 95% confidence regions of Fermi unassociated sources. Use of 3FGL data. |
| Ref: | =2019ApJ...887...18K |
| by | KAUR A. , FALCONE A.D., STROH M.D., KENNEA J.A., FERRARA E.C. |
| Astrophys. J., 887, 18-18 (2019) | |
| Classification of new X-ray counterparts for Fermi unassociated γ-ray sources using the Swift X-Ray Telescope. | |
| o | Tables 1-2: <SwF3 JHHMMSS.s+DDMMSS> N=217. |
| Ref: | =2021ApJ...908..177K |
| by | KAUR A. , FALCONE A.D., STROH M.C. |
| Astrophys. J., 908, 177-177 (2021) | |
| Classifying blazar candidates from the 3FGL unassociated catalog into BL Lacertae objects and flat spectrum radio quasars Using Swift and WISE data. | |
| o | Tables 1-2: <SwF3 JHHMMSS.s+DDMMSS> N=24+84. Table 1: <SwF3 JHHMMSS.ss+DDMMSS> (No. J174511.10-225455). |
| Ref: | =2021AJ....161..154K |
| by | KERBY S. , KAUR A., FALCONE A.D., STROH M.C., FERRARA E.C., KENNEA J.A., COLOSIMO J. |
| Astron. J., 161, 154-154 (2021) | |
| X-ray spectra and multiwavelength machine learning classification for likely counterparts to Fermi 3FGL unassociated sources. | |
| o | Tables 3-4: <SwF3 JHHMMSS.s+DDMMSS> N=177, <SwF3 JHHMMSS.ss+DDMMSS> N=10. |
| =E= | Catalogue in electronic form as <J/ApJ/887/18/> |
| =E= | Catalogue in electronic form as <J/AJ/161/154/> |
| Origin | of the Acronym: A = Assigned by the author(s) |