Dictionary of Nomenclature of Celestial Objects
(Last update: 05-Dec-2018)

Result of query: info cati HTR$

Details on Acronym:   HTR
   HTR (HATNet TRansit candidate) (Not yet in Simbad) ***** Avoid the usage of HTR, prefer [BFV2016] Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   HTR
   HTR (Hyland+Thomas+Robinson) Write:<<HTR NN>> N: 24 Object:(IR)  (SIMBAD class: IR = Infra-Red source) Stat:is completely incorporated in Simbad Note:(Nos 1-8, 10-11, 13-24) are identical to MHR numbering, but 1981ApJ...250..116M is not considered as a continuation of 1978AJ.....83...20H, 'MH' being used in the literature as the usual acronym.
in source:Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula Ref:=1978AJ.....83...20H byHYLAND A.R. , THOMAS J.A., ROBINSON G. Astron. J., 83, 20-25 (1978) Infrared studies of 30 Doradus. I. The 2-µ sources of the inner region. oTable 1: <HTR NN> (Nos 1-24). Originof the Acronym: L (1981ApJ...250..116M)
Details on Acronym:   HTR
   HTR (HATNet TRansit candidate) ***** Avoid the usage of HTR, prefer [LBT2009] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* NGC 2516 HTR
   Cl* NGC 2516 HTR (Hawley+Tourtellot+Reid) Write:<<Cl* NGC 2516 HTR M NNN>>
<<Cl* NGC 2516 HTR M A>>
<<Cl* NGC 2516 HTR O NN>>
<<Cl* NGC 2516 HTR O A>> N: 146+9+43+4 Object:*inCl Rem:Table 1A, 1B:
Main field (M in the format)
Offset field (O in the format)
'NNN' are candidate members,
'A' are spectroscopically observed stars that are not
candidate members. Ref:=1999AJ....117.1341H byHAWLEY S.L. , TOURTELLOT J.G., REID I.N. Astron. J., 117, 1341-1359 (1999) Low-mass stars in open clusters. I. NGC 2516 and NGC 3680. oTable 1A: <Cl* NGC 2516 HTR M NNN> (Nos 1-146), <Cl* NGC 2516 HTR M A> (Nos A-I). Table 1B: <Cl* NGC 2516 HTR O NN> (Nos 1-43), <Cl* NGC 2516 HTR O A> (Nos A-D). Table 1C: <Cl* NGC 3680 HTR M NNN> (Nos 1-203), <Cl* NGC 3680 HTR M A> (Nos A-P). Table 1D: <Cl* NGC 3680 HTR O NNN> (Nos 1-149), <Cl* NGC 3680 HTR O A> (Nos A-H).
Details on Acronym:   Cl* NGC 3680 HTR
   Cl* NGC 3680 HTR (Hawley+Tourtellot+Reid) Write:<<Cl* NGC 3680 HTR M NNN>>
<<Cl* NGC 3680 HTR M A>>
<<Cl* NGC 3680 HTR O NNN>>
<<Cl* NGC 3680 HTR O A>> N: 203+16+149+8 Object:*inCl Rem:Table 1A, 1B:
Main field (M in the format)
Offset field (O in the format)
'NNN' are candidate members,
'A' are spectroscopically observed stars that are not
candidate members. Ref:=1999AJ....117.1341H byHAWLEY S.L. , TOURTELLOT J.G., REID I.N. Astron. J., 117, 1341-1359 (1999) Low-mass stars in open clusters. I. NGC 2516 and NGC 3680. oTable 1A: <Cl* NGC 2516 HTR M NNN> (Nos 1-146), <Cl* NGC 2516 HTR M A> (Nos A-I). Table 1B: <Cl* NGC 2516 HTR O NN> (Nos 1-43), <Cl* NGC 2516 HTR O A> (Nos A-D). Table 1C: <Cl* NGC 3680 HTR M NNN> (Nos 1-203), <Cl* NGC 3680 HTR M A> (Nos A-P). Table 1D: <Cl* NGC 3680 HTR O NNN> (Nos 1-149), <Cl* NGC 3680 HTR O A> (Nos A-H).

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