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[vsnet-obs 7428] NAS.VSS obs. 1997 Sep 18 UT (Report 1997h-029)



Norwegian Astronomical Society - Variable Star Section

Visual observations by observers of NAS.VSS (Report 1997h-029):

Object       YYMMDD(UT)   Mag   Obs. Instrum.   Notes
ANDRX        970918.04  <13.1   GRL  C203;123x
ARITT        970918.04   10.9   GRL  C203;123x  Seq. RASNZ
AURRW        970918.03   10.8   GRL  C203;123x
AURSS        970918.01  <13.0   GRL  C203;123x
CAMZ         970918.00  <12.8   GRL  C203;123x
CASV723      970918.042  11.6   GRL  C203;123x  Seq. Skiff (V-mag)
CYGCH        970918.00    9.0   GRL  C203;123x  Seq. AAVSO (V-mag)
CYGSS        970918.00    9.3   GRL  C203;123x  Outburst, fading
DRAAG        970918.01    9.5   GRL  C203;123x
GEMU         970918.04  <12.4   GRL  C203;123x
PEGAG        970918.00    8.9   GRL  C203;123x
PEGII        970918.04    7.6   GRL  C203;123x  Seq. NAS.VSS
PEGRU        970918.00   12.6   GRL  C203;123x
SGEFG        970918.03    9.7   GRL  C203;123x  Brightening, seq. H/T
SGEHM        970918.03   11.3   GRL  C203;123x
SGER         970918.04    9.4   GRL  C203;123x  Seq. AFOEV
SGEV         970918.03   10.6   GRL  C203;123x
TAUBP        970918.03   12.1   GRL  C203;123x  Seq. AFOEV
TAUCQ        970918.01    9.1   GRL  C203;123x  Bright, seq. Skiff
TAURR        970918.01   12.3   GRL  C203;123x  Fading
TAURV        970918.03    9.8   GRL  C203;123x  Seq. H/T
TAURY        970918.03   11.1   GRL  C203;123x  Condsiderably fainter
TAUT         970918.03    9.9   GRL  C203;123x
VULPU        970918.03   11.5   GRL  C203;123x  Seq. BAA.VSS
VULWW        970918.03   10.8   GRL  C203;123x

Observer:
GRL = Bjorn H. Granslo (Fjellhamar, Norway). Instrument: 20.3-cm
  SCT (C203). Strong Moonlight, nearly clear sky. I attempted to
  observe the possible asteroidal occultation on 1997 Sep 18
  involving 27 Euterpe (V-mag. 11.0) and PPM 94351 (V-mag. 9.9).
  The star was monitored continously from 00h15m to 00h35m UT but
  no occultation was seen. At the beginning of the watch the
  minor planet was visible a couple of arcseconds West of the star
  and at the end it was seen a few arcseconds to the East (ie.
  27 Euterpe showed a prograde motion). During a time interval of
  12 minutes centered on 00h23m UT I was not able to separate the
  two objects. I was unfortunately completely clouded out during
  the total lunar eclipse on 1997 Sep 16 UT.