Dictionary of Nomenclature of Celestial Objects
(Last update: 02-Nov-2023)

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: Infrared = 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).