Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Oct-2021)

Result of query: info cati UCAC3$
 in source:Coma Cluster = ACO 1656
     byULMER M.P.
 Astron. J., 112, 2517-2532 (1996)

    Low surface brightness galaxies in the core of the Coma cluster.

oTables 1, 2: <[UBM96] NN> (Nos 1-18), <[UBM96] NNL> (Nos 1L to 18L)

Details on Acronym:   [UBS2020]
   [UBS2020] (Urquhart+Bahramian+Strader+, 2020) Write:<<[UBS2020] Ter5-VLANN>> N: 43 Object:(Rad)  (SIMBAD class: Radio = Radio-source) Note:Karl G. Jansky VLA deep 2-8GHz radio continuum observations of N=43 radio sources in the Galactic globular cluster Terzan 5, as part of the MAVERIC (Milky Way ATCA VLA Exploration of Radio Sources in Clusters) survey. in source:Cl Terzan 5 Ref:=2020ApJ...904..147U byURQUHART R. , BAHRAMIAN A., STRADER J., CHOMIUK L., RANSOM S.M., WANG Y., HEINKE C., TUDOR V., MILLER-JONES J.C.A., TETARENKO A.J., MACCARONE T.J., SIVAKOFF G.R., SHISHKOVSKY L., SWIHART S.J., TREMOU E. Astrophys. J., 904, 147-147 (2020) The MAVERIC survey: new compact binaries revealed by deep radio continuum observations of the galactic globular cluster Terzan 5. oTable 2: <[UBS2020] Ter5-VLANN> (Nos VLA1-VLA43). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   UBV
   UBV (UBV system)= (Blanco) = (USN) = (WPC) Write:<<UBV NNNNN>> N: 20705 Object:*  (SIMBAD class: Star) Stat:is completely incorporated in Simbad Ref:=1968PUSNO..21....0B byBLANCO V.M. , DEMERS S., DOUGLASS G.G., FITZGERALD M.P. Publ. U.S. Naval Obs. Second Serie, -1-None (1968) Photoelectric catalogue, magnitudes and colors of stars in the UBV and UCBV systems. oUBV o<UBV NNNNN> N=20705.
Details on Acronym:   [UBW2009]
   [UBW2009] (Urrutia+Becker+White+, 2009) Write:<<[UBW2009] NNN>> N: 122 Object:Poss. QSO  (SIMBAD class: QSO_Candidate = Possible Quasar) Stat:is completely incorporated in Simbad Note:N=122 potential red quasars obtained by combining the FIRST radio survey, the 2MASS Infrared Survey andthe Sloan Digital Sky Survey. Keck ESI spectroscopic follow-up.
See also F2MS. Ref:=2009ApJ...698.1095U byURRUTIA T. , BECKER R.H., WHITE R.L., GLIKMAN E., LACY M., HODGE J.

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