Multi-wavelength picture of the misaligned BL Lac object 3C 371

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Table 3.

Results of the LTV analysis performed on the MWL emission of 3C 371.

Band	F_min	F_max	ΔF_max	A_mp	ΔA_mp
	[mJy]	[mJy]	[mJy]	[%]	[%]
γ rays ^(a)	0.53	14.49	13.96	238.5	72.4
1 keV ^(b)	0.28	0.95	1.20	125.4	48.8
w2 ^(c)	0.33	1.07	0.74	115.5	13.3
m2 ^(c)	0.38	1.25	0.87	116.2	11.7
w1 ^(c)	0.47	1.55	1.08	113.5	10.7
u^(c)	0.67	1.70	1.03	96.9	16.7
b^(c)	1.24	1.40	0.16	–	–
v^(c)	1.77	1.97	0.20	–	–
B^(c)^,^(d)	0.85	6.92	6.08	247.0	28.4
V^(c)^,^(d)	1.16	10.09	8.92	276.3	21.9
R^(c)^,^(d)	1.84	14.49	12.65	264.4	13.9
I^(c)^,^(d)	2.38	16.15	13.78	203.0	43.5
230 GHz ^(e)	1.06	1.93	0.87	60.3	5.7
24 GHz ^(e)	1.66	2.73	1.07	45.4	3.6
8.5 GHz ^(e)	1.57	2.82	1.25	57.0	1.8
4.8 GHz ^(e)	1.57	2.56	0.99	49.0	1.7

Notes.

^(a)

Flux of the γ-ray band in units of 10⁸ cm⁻² s⁻¹.

^(b)

Flux of the X-ray 1 keV light curve in units of μJy.

^(c)

Dereddened and host-galaxy-subtracted flux density values.

^(d)

Estimations from Paper I.

^(e)

Flux of the radio bands in units of Jy.

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