Searching for similarities in the accretion flow of Seyfert 1 galaxies and cataclysmic variables based on the flare profiles of IRAS 13224–3809, 1H 0707–495, Mrk 766, and MV Lyr

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Volume 692 (December 2024)

A&A, 692 (2024) A94

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Table 2.

T_r and T_d parameters and corresponding PDS characteristic frequencies f_r and f_d for individual objects. t_ext is the time extension of the averaged flare.

Object	t_ext	T_r	T_d	log(f_r/Hz)	log(f_d/Hz)
	(ks)	(s)	(s)
IRAS 13224–3809	4	473.6 ± 21.6	794.5 ± 52.2	−3.47	−3.70
1H 0707–495	4	911.8 ± 44.8	950.2 ± 55.2	−3.76	−3.78
Mrk 766	4	691.5 ± 66.1	844.4 ± 64.4	−3.64	−3.72
MV Lyr	4	1232.2 ± 54.8	925.8 ± 37.1	−3.89	−3.76

IRAS 13224–3809	8	1838.1 ± 212.4 ^(a)	1495.0 ± 74.0	−4.06	−3.97
		898.2 ± 43.1 ^(b)		−3.75
		1368.8 ± 69.4 ^(c)	1361.6 ± 86.23 ^(c)	−3.93	−3.93
		731.7 ± 129.2 ^(d)		−3.66
1H 0707–495	8	1330.3 ± 31.7	826.0 ± 25.7	−3.92	−3.72
Mrk 766	8	1208.9 ± 58.4	1123.9 ± 43.4	−3.88	−3.85
MV Lyr	8	1026.3 ± 42.0 ^(a)	1027.4 ± 16.4	−3.81	−3.81
		1418.6 ± 48.4 ^(b)		−3.95

Notes.

^(a)

Fits on the whole time extension and without any alternation.

^(b)

Fits on altered time interval.

^(c)

Fits of the low-flux version of the flare.

^(d)

Fits of the side lobe of the high-flux version of the flare.

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