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Norwegian Astronomical Society - Variable Star Section
OBSERVATIONS OF 2027+52 NOVA CYGNI 1992 - REPORT NO. 052 (1992 December 5)
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YYYY MM DD.DDD OBSERVATION MAG CL INSTRUM. OBSERVER
1992 11 04.931 K-4;v=L;M+3 9.6 1 C203,80x Dahle, H.
1992 11 14.718 K-4;L+1;M+5 9.5 1 C203,80x Dahle, H.
1992 11 28.756 K-6;L-3;M+5 9.7 1 C023,123x Granslo, B.H.
1992 11 29.738 K-6;L-3;M+6 9.6 1 C203,123x Granslo, B.H.
1992 11 29.740 K-6;L-4;M+3 9.8 1 C203,80x Dahle, H.
1992 12 02.009 K-6;L-3;M+6 9.6 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 in mm): C = Schmidt-Cassegrain. Comparison
stars (sequence: The Astronomer): K = 9.01,L = 9.52, M = 10.07. Observers:
H. Dahle, Vestbrynet 12, N-1176 Oslo; B. H. Granslo, N. Griegsvei 22 A,
N-1472 Fjellhamar.
Bjorn H. Granslo
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