[vsnet-chat 1229] V592 Her: comparison between sequences

[Taichi Kato <tkato>]

V592 Her: comparison between sequences

 No.      (J2000.0)      GSC   USNO-V VSNET   VSOLJ
 ------------------------------------------------------
  1 163049.07 +211039.3 11.71  11.84  11.70
  2 163048.10 +212037.0 11.62  11.90          128 = c
  3 163048.04 +211204.6 13.86  13.81  13.75
  4 163048.62 +211318.9 14.21  13.84  14.06   142
  5 163056.73 +211202.8 14.50  14.41  14.38
  6 163048.57 +211919.2 14.69  14.46          144
  7 163102.99 +211917.1 14.90  14.80          149
  8 163053.36 +211553.4 14.95  14.89  14.91   152
  9 163050.92 +211826.9 15.36  15.29  15.40   150
 10 163049.46 +211745.7 15.27  15.41  15.23   154
 11 163102.55 +211316.4        16.46          160
 12 163105.15 +211707.0        16.92          169
 13 163056.76 +211504.0        17.39          172
 14 163048.38 +211536.9        17.86          174
 15 163057.11 +211742.3        17.80          173
 16 163053.84 +211604.7        17.89          181

  GSC: GSC V1.1 (also used in AAVSO?)
  USNO-V: USNO A1.0-based, V = r + 0.375(b-r) assumed
  VSNET: Ouda CCD(V), calibrated using GSC 11.7
  VSOLJ: old sequence used by VSOLJ members; photographically determined
         and visually checked.  Stars 8,9,10 were usually visible through
         15-20 cm telescopes; star 15 occasionally visible, which usually
         defined the deepest upper limits of this object, by good 25-30 cm
         telescopes.  Some observers reported upper limits 1 mag fainter
         than the star 15.

Regards,
Taichi Kato

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