Norwegian Astronomical Society - Variable Star Section OBSERVATIONS OF 2027+52 NOVA CYGNI 1992 - REPORT NO. 045 (1992 August 11) ========================================================================= YYYY MM DD.DDD OBSERVATION MAG CL INSTRUM. OBSERVER 1992 08 04.830 7-4;H-3;K+2 8.9 1 C203,80x Dahle, H. 1992 08 05.844 7-4;H-3;K+2 8.9 1 C203,80x Dahle, H. 1992 08 07.001 7-2;H-3;K+4;L+7 8.8 1 C203,123x Granslo, B.H. 1992 08 07.964 6-6;7-1;H-2;K+5;L+8 8.7 1 C203,123x Granslo, B.H. 1992 08 08.962 7-2;H-3;K+4;L+7 8.8 1 C203,123x Granslo, B.H. Time system is Universal Time. Magnitudes were calculated from Pogson's step method. CL = class: estimated accuracy of observation; 1 = good, 2 = fair, 3 = poor. Instrument (aperture inmm): C = Schmidt-Cassegrain. Comparison stars (sequence: The Astronomer): 6 = 8.0; 7 = 8.58, H = 8.74, K = 9.01, L = 9.52. H. Dahle observed from Khania, Crete, Greece. Observers: Haakon Dahle, Vestbrynet 12, N-1176 Oslo, Norway; Bjorn H. Granslo, Nordahl Griegsvei 22 A, N-1472 Fjellhamar, Norway. Bjorn H. Granslo
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