Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Apr-2024)

Result of query: info cati GPM2011]$

Details on Acronym:   [GPM2011]
  
[GPM2011] (Graur+Poznanski+Maoz+, 2011)= (SNSDF) = (hSDF)
Write:<<[GPM2011] SNSDF YYMM.NN>>
<<[GPM2011] hSDF YYMM.NN>>
N: 190+190
Object:SN + G  (SIMBAD class: Unknown = Object of Unknown Nature)
Note:Subaru telescope observations of the SDF to search for supernovae and their host galaxies.
Keck LRIS and DEIMOS spectroscopy.
See SNSDF and hSDF.
in source:NAME SDF
Ref:=2011MNRAS.417..916G
byGRAUR O. , POZNANSKI D., MAOZ D., YASUDA N., TOTANI T., FUKUGITA M., FILIPPENKO A.V., FOLEY R.J., SILVERMAN J.M., GAL-YAM A., HORESH A., JANNUZI B.T.
 Mon. Not. R. Astron. Soc., 417, 916-940 (2011)
  Supernovae in the Subaru Deep Field: the rate and delay-time distribution of type Ia supernovae out to redshift 2.
oThe SNSDF names in this reference are not the same than in 2007MNRAS.382.1169P. That's why the CDS team had to create an acronym [GPM2011].
oTable 2: <[GPM2011] SNSDF YYMM.NN> N=190. Table 3: <[GPM2011] hSDF YYMM.NN> N=190.
=E=Catalogue in electronic form as J/MNRAS/417/916
Originof the Acronym: S = Created by Simbad, the CDS Database

Details on Acronym:   hSDF
  
hSDF (host, SDF)
====>Equivalent to: [GPM2011]
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   SNSDF
  
SNSDF (SN, SDF)
***** Avoid the usage of SNSDF, prefer [GPM2011]
Originof the Acronym: A = Assigned by the author(s)