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

Result of query: info cati SwF3 JHHMMSS.s+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)