Free Access

Fig. 1.

image

Light curves of blazar 3C 454.3. From the top, the first panel shows the γ-ray photon flux for photon energies above 100 MeV obtained from the Fermi LAT data in 10-day bins; the second panel shows the optical continuum at source-frame 3000 Å, obtained independently using two analysis methods (spectral decomposition, blue circles; simplified power-law fit, red/grey crosses); the third panel shows the corresponding values of the spectral index α such that fλ ∝ λα; the fourth panel shows estimates of the spectrally integrated Mg II line flux, either separated from the Fe II continuum (decomposition method) or not (simplified method); the fifth panel shows the source-frame FWHM width of Mg II line obtained in the decomposition method and corrected for instrumental broadening; the sixth panel shows the rms of continuum subtracted spectra calculated over the continuum fitting spectral windows, with the limiting value of 7 × 10−17 erg s−1 cm−2 Å−1 indicated with the dashed line. Results reported in León-Tavares et al. (2013; Steward) and Isler et al. (2013; SMARTS) are indicated in the second and fourth panels. Periods of interest for spectral stacking are marked with vertical stripes or lines.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.