Dictionary of Nomenclature of Celestial Objects

CM Dra:[MHE2007] NN, SL JHHMM.m+DDMM
Note:Subaru weak-lensing survey: catalog of N=101 candidate halos. Among them, N=41 are identified as galaxy clusters and have measured redshifts.
Ref:=2007ApJ...669..714M
byMIYAZAKI S. , HAMANA T., ELLIS R.S., KASHIKAWA N., MASSEY R.J., TAYLOR J., REFREGIER A.
 Astrophys. J., 669, 714-728 (2007)
  A Subaru weak-lensing survey. I. Cluster candidates and spectroscopic verification.
oTable 2, col(1): <[MHE2007] DEEPNN NN>, <[MHE2007] SXDS NN>, <[MHE2007] XMM-LSS NN>, <[MHE2007] Lynx NN>, <[MHE2007] COSMOS NN>, <[MHE2007] Lockman Hole NN>, <[MHE2007] GD 140 NN>, <[MHE2007] PG 1159-035 NN>, <[MHE2007] UK 13 NN>, <[MHE2007] GTO 2°(2) NN>, <[MHE2007] CM Dra NN> N=101 = Table 2, col(2): <[MHE2007] SL JHHMM.m+DDMM> N=41.
Ref:=2009PASJ...61..833H
byHAMANA T. , MIYAZAKI S., KASHIKAWA N., ELLIS R.S., MASSEY R.J., REFREGIER A., TAYLOR J.E.
 PASJ, 61, 833-872 (2009)
  Subaru Weak-Lensing Survey II: Multi-object spectroscopy and cluster masses.
oTable 1: <[MHE2007] SL JHHMM.m+DDMM> N=12 added. Table 2: <[MHE2007] SL JHHMM.m+DDMMA> N=6.
=E=Catalogue in electronic form as J/ApJ/669/714

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