Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Sep-2023)

Result of query: info cati SwF3 JHHMMSS.ss+DDMMSS$


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 byKAUR 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. oTables 1-2: <SwF3 JHHMMSS.s+DDMMSS> N=217. Ref:=2021ApJ...908..177K byKAUR 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. oTables 1-2: <SwF3 JHHMMSS.s+DDMMSS> N=24+84. Table 1: <SwF3 JHHMMSS.ss+DDMMSS> (No. J174511.10-225455). Ref:=2021AJ....161..154K byKERBY 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. oTables 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/> Originof the Acronym: A = Assigned by the author(s)

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