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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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