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#data is taken from the HEASARC data base (http://heasarc.gsfc.nasa.gov/)
#File name : xn0620.o751B2
#Source : 0620-00
#Outburst : 1975
#Reference : Lloyd et al. 1977, MNRAS, 179, 675
#Observatry:
#Band : V
#Time of zero phase: 2446082.7481(8)
#Time of peak in X-rays 2442638.4
#Conversion: 1.
#Data dimen: 90
#
#
#translated to LF by G.V.Lipunova
#LF = log flux
#flux = erg/cm^2/sec
#1=TJD 2=V 3=err 4=B-V 6=V,LF 7=V-errors,LF
#1(JD-2440000) 2,3,4=(mag)
# 1 2 3 4 6 7
2660.653 11.59 0.2 0.21 -10.12661 0.08
2676.627 11.86 0.07 0.26 -10.23461 0.028
2679.621 11.96 0.07 0.18 -10.27461 0.028
2690.676 11.90 0.07 0.3 -10.25061 0.028
2691.634 11.86 0.07 0.15 -10.23461 0.028
2717.539 12.57 0.07 0.04 -10.51861 0.028
2718.497 12.44 0.07 0.25 -10.46661 0.028
2718.538 12.41 0.07 0.26 -10.45461 0.028
2728.501 12.50 0.07 0.41 -10.49061 0.028
2728.569 12.57 0.07 0.36 -10.51861 0.028
2743.577 12.89 0.07 0.21 -10.64661 0.028
2753.552 12.97 0.07 0.24 -10.67861 0.028
2755.590 12.97 0.07 0.28 -10.67861 0.028
2771.513 13.62 0.07 0.24 -10.93861 0.028
2842.402 13.45 0.07 0.26 -10.87061 0.028
#From the paper:
# 1)The data is reduced to UBV system with m=0.07 errors.
# 2)For values brigter B=11.8 the electronographs were overexposed
# => systematical errors; "To agree with the photoelectric values
# reported in the literature they should be about 0.1 mag brighter."
Lipunova Galina
2002-01-14