Properties of flat-spectrum radio-loud narrow-line Seyfert 1 galaxies

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Volume 575 (March 2015)

A&A, 575 (2015) A13

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201424972e]

Table 9

Shortest variability at optical-to-γ ray frequencies.

Name	γ rays	X-rays	uvw2	uvm2	uvw1	u	b	v

J0134 − 4258		−0.071 ± 0.025
		(3.8)
J0324 + 3410	0.10 ± 0.03 ^a	−0.079 ± 0.012	0.09 ± 0.03	0.10 ± 0.04	<0.43	7 ± 3	<0.7	<0.28
	(3.8)	(4.4)	(10.7)	(7.6)	(4.1)	(6.1)	(4.0)	(3.6)
J0849 + 5108	12 ± 8 ^b	< 18			< 0.27
	(4.7)	(3.5)			(3.6)
J0948 + 0022	< 0.8 ^b	< 0.21	0.12 ± 0.07	0.09 ± 0.05	0.08 ± 0.03	0.07 ± 0.03	0.06 ± 0.03	0.05 ± 0.03
	(5.4)	(5.2)	(6.3)	(6.1)	(7.3)	(7.9)	(7.8)	(5.7)
J0953 + 2836					< 18
					(3.1)
J1031 + 4234						< 0.15
						(3.0)
J1038 + 4227							< 12
							(3.4)
J1047 + 4725			< 0.83
			(3.4)
J1102 + 2239						< 0.24
						(3.1)
J1238 + 3942			< 0.58
			(3.4)
J1505 + 0326	1.3 ± 0.5 ^b							< 0.04
	(6.6)							(3.8)
J1629 + 4007		−0.12 ± 0.02	< 0.49			< 0.17	< 0.23	< 0.09
		(3.5)	(3.7)			(4.1)	(3.2)	(3.6)
J2007−4434	6 ± 2 ^b	<0.19	<0.12			<0.30		<0.14
	(12)	(3.3)	(3.0)			(3.1)		(3.1)

Notes. For each source, it is indicated the τ [days] and, in the second row between parentheses, the significance of the flux change [σ].

Reference.

^(a)

Paliya et al. (2014);

^(b)

Foschini (2011a).

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