INTEGRAL observations of the GeV blazar PKS 1502+106 and the hard X-ray bright Seyfert galaxy Mkn 841

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Table 2

Parameters of the theoretical spectral energy distributions of PKS 1502+106.

date^a	R_diss^b	^c	B ^d	Γ^e	γ_b^f	γ_max^g	s₁^h	s₂ⁱ	log P_r^j	log P_B^k	log P_e^l	log P_p^m
(1)	(2)	(3)	4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)

Fermi LAT, 8 Aug. 2008 (light green)	300 (1000)	0.16	0.75	19	3000	6000	–1	2.6	46.8	44.8	44.9	47.2
Fermi LAT, 5–10 Aug. 2008 (orange)	195 (650)	0.1	2.2	19	500	5000	–1	2.4	47.1	45.4	45.0	47.2
15–22 Aug. 2008 (cyan)	210 (700)	0.05	2.2	19	250	4300	–1	2.3	46.3	45.5	44.8	47.1
historical (black)	120 (400)	0.015	7.3	10	800	2000	0.25	2.2	45.1	45.5	45.5	45.9

Notes.

^(a)

epoch/state (colors refer to the model curves in Fig. 3);

^(b)

dissipation radius in units of 10¹⁵ cm and (in parenthesis) in units of gravitational radii;

^(c)

power injected in the blob calculated in the comoving frame, in units of 10⁴⁵ erg s^-1;

^(d)

magnetic field, in gauss;

^(e)

bulk Lorentz factor at R_diss;

^(f)

break random Lorentz factors of the injected electrons;

^(g)

maximum random Lorentz factors of the injected electrons;

^(h)

slope of the injected electron distribution [Q(γ)] below γ_b;

⁽ⁱ⁾

slope of the injected electron distribution [Q(γ)] above γ_b;

^(j)

Logarithm of the jet power in the form of radiation, in erg s^-1;

^(k)

Logarithm of Poynting flux, in erg s^-1;

^(l)

Logarithm of bulk motion power of electrons, in erg s^-1;

^(m)

Logarithm of bulk motion power of protons, in erg s^-1.

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