Broadband study of blazar 1ES 1959+650 during flaring state in 2016

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Volume 611 (March 2018)

A&A, 611 (2018) A44

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Table 3

Goodness of fit for flux distributions in various energy bands.

Waveband	Gaussian	Lognormal	F_calculated	F_95%
	(d.o.f. (ν_g))	(d.o.f. (ν_l))
OVRO (15 GHz)	10.82 (6)	6.16 (6)	1.77	4.28
UVOT (Optical)	3.35 (6)	1.80 (6)	1.86	4.28
UVOT (UV)	5.56 (3)	2.67 (3)	2.08	9.28
Swift XRT (0.3–8 keV)	2.52 (5)	2.18 (5)	1.16	5.05
MAXI (0.2–20 keV)	6.82 (5)	4.25 (5)	1.60	5.05
Swift BAT (15–50 keV)	3.58 (5)	1.43 (5)	1.60	5.05
Fermi LAT (0.1–3 GeV)	1.08 (5)	2.20 (5)	2.05	5.05
Fermi LAT (3–300 GeV)	1.69 (4)	0.96 (4)	1.76	6.39

Notes. D.o.f. is the number of bins minus number of model parameters, which is three for both the models; F_calculated is the ratio of two variances with the larger variance as the numerator; F_95% is the F-statistic value at the 95% confidence level for the ν_g and ν_l degrees of freedom.

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