[vsnet-mira-srb 81008] BS Per recent (cont'd)

[Taichi Kato]

BS Per recent (cont'd)

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

  YYYYMMDD(UT)   mag  observer
  20110828.8188 10.05V  (Kyoto Wide-field Survey)
  20110906.7982 10.07V  (Kyoto Wide-field Survey)
  20110909.7950 10.18V  (Kyoto Wide-field Survey)
  20110911.7752 10.01V  (Kyoto Wide-field Survey)
  20110914.7376 10.06V  (Kyoto Wide-field Survey)
  20110923.8006 10.04V  (Kyoto Wide-field Survey)
  20111007.7275 9.97V  (Kyoto Wide-field Survey)
  20111008.6845 10.12V  (Kyoto Wide-field Survey)
  20111023.6662 9.90V  (Kyoto Wide-field Survey)
  20111025.6462 9.85V  (Kyoto Wide-field Survey)
  20111026.6350 9.85V  (Kyoto Wide-field Survey)
  20111027.6507 9.92V  (Kyoto Wide-field Survey)
  20111031.6172 9.84V  (Kyoto Wide-field Survey)
  20111103.6335 9.76V  (Kyoto Wide-field Survey)
  20111108.6341 9.76V  (Kyoto Wide-field Survey)
  20111116.5969 9.71V  (Kyoto Wide-field Survey)
  20111124.5875 9.76V  (Kyoto Wide-field Survey)
  20111127.5636 9.68V  (Kyoto Wide-field Survey)
  20111213.5418 9.60V  (Kyoto Wide-field Survey)
  20111214.5246 9.61V  (Kyoto Wide-field Survey)
  20111225.4701 9.71V  (Kyoto Wide-field Survey)
  20120108.4874 9.90V  (Kyoto Wide-field Survey)
  20121017.215  10.06V  (Pierre Hallsten)
  20190222.4108 9.97V  (Minoru Sato)
  20190308.4230 9.89V  (Minoru Sato)

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