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[vsnet-obs 186] VS observations (outbursts of DNe)


Visual and CCD magnitude estimates by VSOLJ members

object         YYMMDD(UT)   mag  code
ANDRX          950222.419   111  Ths.VSOLJ
ANDFN          950222.410  <133  Ths.VSOLJ
ANDLS          950222.412  <134  Ths.VSOLJ
ANDPQ          950222.422  <138  Ths.VSOLJ
ARISV          950222.436  <137  Ths.VSOLJ
AURSS          950222.453   112  Ths.VSOLJ  outburst
AURKR          950222.456  <140  Ths.VSOLJ
GEMU           950222.503   143  Ths.VSOLJ
GEMKT          950222.524   137  Arm.VSOLJ  very bright (*1)
GEMMV          950222.531  <161  Arm.VSOLJ
HYACT          950222.547   136  Arm.VSOLJ  outburst (*2)
LMIRU          950222.487  <162  Arm.VSOLJ
LMIRZ          950222.490   176  Arm.VSOLJ
LMISS          950222.495  <168  Arm.VSOLJ
LMISX          950222.499  <164  Arm.VSOLJ
ORIV1159       950222.462   139  Arm.VSOLJ
PERTZ          950222.425   125  Ths.VSOLJ  outburst
PERUV          950222.428  <137  Ths.VSOLJ
PERUW          950222.426  <136  Ths.VSOLJ
PERFO          950222.433   138  Ths.VSOLJ  outburst
PERFY          950222.431   117  Ths.VSOLJ
PERGK          950222.429   130  Ths.VSOLJ
PERPU          950222.478  <176  Arm.VSOLJ
PERPV          950222.473  <172  Arm.VSOLJ
PERPY          950222.481   167  Arm.VSOLJ
TAUT           950222.444   107  Ths.VSOLJ
TRIWY          950222.469  <171  Arm.VSOLJ
UMABC          950222.520  <173  Arm.VSOLJ
UMAEL          950222.503  <172  Arm.VSOLJ
HEMUV          950222.527  <173  Arm.VSOLJ
NSV00895       950222.422  <138  Ths.VSOLJ
PG0911-066     950222.510  <173  Arm.VSOLJ
PG0943+521     950222.465   156  Arm.VSOLJ
SN1995D        950222.444   127  Ths.VSOLJ

Observer's code:
  Arm: M. Iida (Nagano, Japan) 16-cm refl. + ST-6 unfiltered
  Ths: S.Takahashi(Dynic Astronomical Observatory.Shiga.Japan) 
       instruments: 60L,15B

(*1) Iida suggest an identification problem in Downes & Shara chart.
     Needs confirmatory observation.
(*2) Probably the first ever detected outburst since discovery.
     Since some authors suggest the non-CV spectrum of the quiescence,
     spectroscopic verification and accurate astrometry would be
     emergently needed during the current outburst.