Norwegian Astronomical Society - Variable Star Section Visual observations by observers of NAS.VSS (Report 1998h-020): Object YYMMDD(UT) Mag Obs. Instrum. Remarks ANDEG 981203.99 7.5 GRL L70;24x Seq. HIP CASWZ 981203.99 7.0 GRL L70;24x Seq. HIP CASV723 981102.26 12.5 MOK M316;130x Est. g 4 v 2 h CASV723 981106.28 12.5 MOK M316;130x Est. g 3 v 2 h CASV723 981119.23 12.4 MOK M316;130x Est. g 3 v 3 h CASrho 981203.99 4.9 GRL B10x50 Seq. HIP CEPmu 981203.98 4.4 GRL B10x50 Seq. HIP CETomicron 981125.90 5.1 HSY B7x50 Est. 54+3 CYGW 981203.98 6.6 GRL L70;24x Seq. HIP CYGRU 981203.98 8.9 GRL L70;24x Seq. Tycho CYGAF 981203.98 7.2 GRL L70;24x Seq. HIP CYGCH 981203.98 8.3 GRL L70;24x Seq. Tycho CYGV1339 981203.98 6.6 GRL L70;24x Seq. HIP CYGchi 981125.72 5.6 HSY B7x50 Est. 51(3)v(2)59 CYGP 981125.72 5.3 HSY B7x50 Est. 50(2)v(1)54 DRAR 981125.86 9.6 HSY L60;36x Est. 94-2 GEMR 981125.91 7.8 HSY L60;36x Est. 79+1 PERGK 981102.26 13.3 MOK M316;270x Est. u 5 v 0 x PERGK 981106.29 13.3 MOK M316;130x Est. w 5 v 0 x PERGK 981107.23 13.3 MOK M316;130x Est. w 5 v 0 x PERGK 981119.23 13.2 MOK M316;130x Est. w 4 v 1 x PERGK 981120.20 13.5 MOK M316;270x Est. x 2 v 3 y TRIR 981125.86 7.9 HSY L60;36x Est. 77(2)v(1)80 UMAR 981125.88 <10.5 HSY L60;72x Est. 105>V UMAS 981125.87 9.0 HSY L60;36x Est. 88-2 UMIR 981125.90 9.3 HSY L60;36x Est. 91-2 Observers: GRL = Bjorn H. Granslo (Fjellhamar, Norway). Instruments: 70-mm refractor (L70), 10x50 binoculars (B10x50. Comparison stars: V-mag. sequences from the Hipparcos and Tycho catalogues. Notes: ~80 % cloudy at first, then fog; Moon. Observed from a height near my home location. The observing conditions since last summer have been the worst in my over 20 years of regular variable star observing. Clear nights have been rare. HSY = Stein Hoydalsvik (Tromso, Norway). Instrument: 60mm f/15 refractor (L60), 7x50 binoculars (B7x50). AAVSO sequences unless otherwise noted. Observations are fractional or Pogson step estimates. MOK = Ornulf Midtskogen (Tranby, Norway). Instrument: 31.6-cm reflector (M316). Observations are step estimates and magnitudes are derived from private sequences.