[vsnet-mira-lb 74678] VZ Per recent (cont'd)

Taichi Kato tkato at kusastro.kyoto-u.ac.jp
Tue Jul 13 23:39:15 JST 2021


VZ Per recent (cont'd)

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

  YYYYMMDD(UT)   mag  observer
  20110906.8001 11.15V  (Kyoto Wide-field Survey)
  20110911.7735 11.34V  (Kyoto Wide-field Survey)
  20110923.7615 11.08V  (Kyoto Wide-field Survey)
  20111007.7134 10.92V  (Kyoto Wide-field Survey)
  20111008.6837 11.23V  (Kyoto Wide-field Survey)
  20111023.6766 11.06V  (Kyoto Wide-field Survey)
  20111025.6445 10.82V  (Kyoto Wide-field Survey)
  20111027.6495 10.75V  (Kyoto Wide-field Survey)
  20111031.6574 11.00V  (Kyoto Wide-field Survey)
  20111116.6177 11.17V  (Kyoto Wide-field Survey)
  20111124.5891 11.12V  (Kyoto Wide-field Survey)
  20120108.4885 11.15V  (Kyoto Wide-field Survey)
  20120112.962  10.99V  (Robert Wahlstrom)
  20120204.945  10.81V  (Robert Wahlstrom)
  20120215.924  10.82V  (Robert Wahlstrom)
  20120225.996  10.94V  (Robert Wahlstrom)
  20121027.972  10.71V  (Robert Wahlstrom)
  20121113.005  107V  (Robert Wahlstrom)
  20121202.941  10.88V  (Robert Wahlstrom)
  20130123.831  10.75V  (Robert Wahlstrom)
  20130225.874  10.95V  (Robert Wahlstrom)
  20130317.912  10.82V  (Robert Wahlstrom)
  20130323.886  10.79V  (Robert Wahlstrom)
  20130331.909  10.71V  (Robert Wahlstrom)
  20201018.5508 10.87V  (Minoru Sato)

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