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J/AZh/81/925        R light curves of 5 blazars              (Bychkova+, 2004)

The Rapid Variability of Blazars at Optical Wavelengths. Bychkova V. S., Kardashev N.S., Vlasyuk V.V., Spiridonova O.I. <Astron. Zh. 81, 925 (2004)> =2004AZh....81..925B =2004ARep...48..840B
ADC_Keywords: Active gal. nuclei ; Photometry, CCD Abstract: We monitored five active galactic nuclei in the R optical band with a CCD mounted on the 1-m Zeiss-1000 telescope of the Special Astrophysical Observatory from April 2001 to August 2003. Three sources displayed intraday variability on several nights. Stronger variability was detected on time scales from two days to a week. The two-year light curves are presented for four of the observed objects. Objects: -------------------------------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------------------------------- 02 38 38.9 +16 36 59 [HB89] 0235+16 = [HB93] 0235+164 09 58 47.2 +65 33 55 [HB89] 0954+658 = [HB93] 0954+658 09 21 36.2 +62 15 52 TXS 0917+624 = [HB93] 0917+624 13 10 28.6 +32 20 44 [HB89] 1308+326 = [HB93] 1308+326 18 19 26.5 +38 45 02 MG3 J181925+3844 = MITG J181925+3844 -------------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 71 151 Results of the optical monitoring
See also: J/A+AS/106/361 : CCD Photometry of BL Lac objects (Xie+ 1994) VII/158 : Revised and Updated Catalog of QSO (Hewitt+ 1993) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Object name 18- 27 A10 "DD/MM/YYYY" Date1 Observation date: Begin 28 A1 --- --- [-] 29- 38 A10 "DD/MM/YYYY" Date2 Observation date: End 41- 47 I7 d HJD Heliocentric Julian date 49- 51 I3 --- Nobs Number of observations per night 54- 58 F5.2 mag Rmax Maximum R magnitude on each night 61- 65 F5.2 mag Rmin Minimum R magnitude on each night 68- 71 F4.2 mag e_Rmin rms error R magnitude

(End) Veta Avedisova[INASAN] 29-Sep-2005
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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