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[vsnet-obs 5513] N Cas 1995
- Date: Fri, 11 Apr 1997 16:57:03 +0400 (MSK DST)
- To: vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Vitaliy Goranskiy <goray@sai.msu.su>
- Subject: [vsnet-obs 5513] N Cas 1995
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
The photoelectric observations of N Cas 1995.
JD hel.24... V B U R Observatory-
Device-
Observer
50487.4038 10.609 10.743 9.962 - Cr-L-Me
50487.4100 10.588 10.754 9.949 - Cr-L-Me
50491.3319 11.090 11.174 10.416 - Cr-L-Me
50491.3382 11.101 11.167 10.435 - Cr-L-Me
50495.3424 10.819 10.930 10.180 - Cr-L-Me
50495.3483 10.835 10.922 10.178 - Cr-L-Me
50501.3888 10.479 10.711 9.920 - Cr-L-Me
50501.3940 10.485 10.754 9.889 - Cr-L-Me
50504.2198 10.592 10.758 9.924 - Cr-L-Me
50504.2257 10.589 10.768 9.932 - Cr-L-Me
50505.3412 11.271 11.374 10.635 - Cr-L-Me
50505.3495 11.261 11.375 10.652 - Cr-L-Me
50512.3469 10.955 11.133 10.339 - Mo-ShV-G,Ka,Sh
50512.3592 10.961 11.109 10.341 - Mo-ShV-G,Ka,Sh
50512.3665 10.949 11.088 10.320 - Mo-ShV-G,Ka,Sh
50517.3691 11.147 11.243 10.325 - Mo-ShV-G
50517.3840 11.146 11.231 10.189 - Mo-ShV-G
50518.2099 11.123 11.274 10.542 - Mo-ShV-Sh
50518.2172 11.101 11.249 10.486 - Mo-ShV-Sh
50518.2221 11.112 11.276 10.493 - Mo-ShV-Sh
50518.2339 11.100 11.269 10.521 - Mo-ShV-Sh
50518.3237 11.200 11.289 10.544 - Cr-L-Me
50518.3309 11.182 11.276 10.589 - Cr-L-Me
50519.2756 11.022 11.213 10.483 - Mo-ShV-G,Ka
50519.3167 11.221 11.300 10.593 - Cr-L-Me
50519.3239 11.208 11.298 10.556 - Cr-L-Me
50521.2114 11.159 11.355 10.388 - Mo-ShV-G
50521.2297 11.163 11.390 10.654 - Mo-ShV-G
50521.2395 11.325 11.398 10.653 - Cr-L-Me
50521.2457 11.312 11.396 10.630 - Cr-L-Me
50523.1668 11.223 11.305 - 9.433 Mo-Ko-G
50523.1731 11.210 11.316 - 9.343 Mo-Ko-G
50523.1800 11.231 11.328 - 9.340 Mo-Ko-G
Remark: Our observations of this Nova in the instrumental
(W-B) colour made in Tien-Shan Observatory with Kornilov's
WBVR photometer (AA-Ko) may well be reduced to the standard
(U-B) colour with the following formula:
U-B = 0.321+1.709*(W-B).
Designations.
Observatory: Cr - Crimean station of the Sternberg Institute,
60-cm reflector; Mo - Sternberg Institute, Moscow University,
70-cm reflector.
Device: Ko - 4-channel WBVR photometer by V.G.Kornilov,
L - UBV photometer by V.M.Lyuty; ShV - UBV photometer by
S.Yu.Shugarov and I.M.Volkov.
Observers: G - V.P.Goranskij (Sternberg Institute), Ka - E.A.Karitskaya
(Institute for Astronomy), Me - N.V.Metlova (Crimean station, SAI),
Sh - S.Yu.Shugarov (Sternberg Institute).
Vitaly Goranskij. Sternberg Institute, Moscow, Russia.