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


Issue
A&A
Volume 575, March 2015
Article Number A13
Number of page(s) 33
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/201424972
Published online 11 February 2015

Online material

Table 4

Gamma-ray spectral characteristics.

Table 5

X-ray characteristics.

Table 6

Swift/UVOT observed average magnitudes (extracted from all the data integrated).

Table 7

Characteristics at radio frequencies (VLBI).

Table 8

Spectral indices (Sννα) at different frequencies.

Table 9

Shortest variability at optical-to-γ ray frequencies.

thumbnail Fig. 8

Spectral energy distributions of the sources in the present sample. Data are corrected for the Galactic absorption. Points refer to detections; arrows are upper limits; the continuous lines are the optical spectra.

Open with DEXTER

thumbnail Fig. 9

Spectral energy distributions of the sources in the present sample. Data are corrected for the Galactic absorption. Points refer to detections; arrows are upper limits; the continuous lines are the optical spectra.

Open with DEXTER

thumbnail Fig. 10

Spectral energy distributions of the sources in the present sample. Data are corrected for the Galactic absorption. Points refer to detections; arrows are upper limits; the continuous lines are the optical spectra.

Open with DEXTER

thumbnail Fig. 11

Spectral energy distributions of the sources in the present sample. Data are corrected for the Galactic absorption. Points refer to detections; arrows are upper limits; the continuous lines are the optical spectra.

Open with DEXTER

thumbnail Fig. 12

Spectral energy distributions of the sources in the present sample. Data are corrected for the Galactic absorption. Points refer to detections; arrows are upper limits; the continuous lines are the optical spectra.

Open with DEXTER

thumbnail Fig. 13

Spectral energy distributions of the sources in the present sample. Data are corrected for the Galactic absorption. Points refer to detections; arrows are upper limits; the continuous lines are the optical spectra.

Open with DEXTER


© ESO, 2015

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