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J/PAZh/25/893         Optical outbursts of the blazar 3C 345    (Belokon+, 1999)

Spectral slope of the emission in "fast" and "slow" optical outbursts of the blazar 3C 345. Belokon E.T., Babadzhanyants M.K. <Pis'ma Astron. Zh. 25, 893 (1999)> =1999PAZh...25..893B =1999AstL...25..781B
ADC_Keywords: QSOs ; Photometry, UBV ; Photometry, photographic Abstract: We present photographic UBV photometry of the blazar 3C 345 that were made during 79 nights in 1971-1974 and 1983-1984 as a part of the Petersburg Quasar Monitoring Program (PQMP) carried out at the Astronomical Institute of the St.-Petersburg University. These data were previously published by piecemeal (references are presented in Section 4). Now after partial revision these data are united in Table 1 that presents nightly averaged UBV magnitudes together with its rms errors (see Section 4 of the paper for the details). These data were used for the comparison of the spectral indices of the emission in the "fast" (time scales of nearly 10-20 days) and "slow" (time scales of nearly 1 yeas) outbursts in 3C 345. Object: ---------------------------------------------------------------------- RA (2000) DE Designation ---------------------------------------------------------------------- 16 42 58.9 +39 48 37 3C 345 = B2 1641+39 = DA 420 = 1ES 1641+399 ---------------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 59 79 Photographic UBV photometry 3C 345
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 8 A8 "DD/MM/YY" Date Observation date 11- 20 F10.2 d JD [2441073/2445439] Julian date 23- 27 F5.2 mag Umag ? U magnitude (1) 30- 33 F4.2 mag e_Umag ? Standard error in Umag (2) 36- 40 F5.2 mag Bmag ? B magnitude (1) 43- 46 F4.2 mag e_Bmag ? Standard error in Umag (2) 49- 53 F5.2 mag Vmag ? V magnitude (1) 56- 59 F4.2 mag e_Vmag ? Standard error in Umag (2)
Note (1): The magnitude estimates in U, B, V bands. If there were several magnitude estimates during a night, then their mean is given; Note (2): rms errors calculated from the typical errors for the single estimation (0.07mag for B and V; 0.10mag for U) and then the number of the estimates were averaged.

(End) Veta Avedisova [INASAN] 05-May-2000
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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