[vsnet-recent-eb 6272] RY Sct recent (cont'd)

Taichi Kato tkato at kusastro.kyoto-u.ac.jp
Wed Aug 10 17:12:24 JST 2011


RY Sct recent (cont'd)

  For general info see:
  http://www.kusastro.kyoto-u.ac.jp/vsnet/gcvs/SCTRY.html
  http://www.kusastro.kyoto-u.ac.jp/vsnet/object/SCTRY.html

  YYYYMMDD(UT)   mag  observer
  20030509.3693 12.874:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.0951 9.095:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.0973 9.094:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.0995 9.097V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.1017 9.092:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.1039 9.093:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.1084 9.088:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.1106 9.093:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.1150 9.090:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.1172 9.091:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.1194 9.090V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030817.1328 9.099:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030917.1170 13.907V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20030919.1154 10.685V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20040405.3885 9.158:V (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20060305.3922 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20110409.8292 9.07V  (Kyoto Wide-field Survey)
  20110411.8234 9.34V  (Kyoto Wide-field Survey)
  20110420.7771 8.90V  (Kyoto Wide-field Survey)
  20110424.7959 8.94V  (Kyoto Wide-field Survey)
  20110505.7849 9.02V  (Kyoto Wide-field Survey)
  20110514.7489 9.33V  (Kyoto Wide-field Survey)
  20110518.7321 8.98V  (Kyoto Wide-field Survey)
  20110605.7027 9.30V  (Kyoto Wide-field Survey)
  20110628.6472 9.29V  (Kyoto Wide-field Survey)
  20110710.6584 9.11V  (Kyoto Wide-field Survey)
  20110803.5873 8.98V  (Kyoto Wide-field Survey)
  20110807.5702 9.17V  (Kyoto Wide-field Survey)

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