[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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