Return to Home Page
Norwegian Astronomical Society - Variable Star Section
OBSERVATIONS OF 2027+52 NOVA CYGNI 1992 - REPORT NO. 051 (1992 November 22)
===========================================================================
YYYY MM DD.DDD OBSERVATION MAG CL INSTRUM. OBSERVER
1992 10 20.838 K-2;L+2 9.3 1 C203,80x Dahle, H.
1992 11 05.100 K-5;L-1;M+6 9.5 2 C203,123x Granslo, B.H.
1992 11 07.100 K-4;v=L;M+6 9.5 2 C203,123x Granslo, B.H.
1992 11 08.081 K-5;L-2;M+5 9.6 1 C203,123x Granslo, B.H.
1992 11 08.712 K-5;L-2;M+6 9.6 1 C203,123x Granslo, B.H.
1992 11 11.080 K-5;L-2;M+6 9.6 2 C203,123x Granslo, B.H.
1992 11 14.756 K-5;L-1;M+6 9.5 1 C203,123x Granslo, B.H.
1992 11 15.788 K-5;L-2;M+5 9.6 1 C203,123x Granslo, B.H.
1992 11 21.735 K-6;L-3;M+5 9.7 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
Return to the Daisaku
vsnet-adm@kusastro.kyoto-u.ac.jp
