Pith. sign in

REVIEW

Optical monitoring in southern blazars. Analysis of variability and spectral colour behaviours

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2411.16347 v1 pith:GAOQ6OGN submitted 2024-11-25 astro-ph.HE astro-ph.GA

classification astro-ph.HEastro-ph.GA
keywords blazarsopticalwereanalysiscolourdatafoundmonitoring
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We present the results of the optical monitoring of 18 southern blazars in the V and R Johnson-Cousins bands. Our main objective is to study the variations in the optical flux and theis relationship with the colour and spectral variabilities. The optical observations were acquired with the 2.15 m "Jorge Sahade" telescope, CASLEO, Argentina.The whole campaign comprised from 2014 April to 2019 September. In addition, X-ray data were taken from the Chandra X-ray Observatory and the Swift/XRT databases, and gamma-ray data were taken from the Fermi-Large Area Telescope 3FGL catalogue. From the total of 18 blazars, we found variability in each one of the time-scales considired for 6 blazars (PKS 0208-512, PKS 1116-46, PKS 1440-389, PKS 1510-089, PKS 2005-489, and PKS 2155-304). In particular, from the colour-magnitude and the multiwavelength analysis, we found that PKS 1510-089 (flat-spectrum radio quasar) is undergoing an activity phase. For the case of PKS 2005-489 (BL Lac), this blazar is in a quiescent state, in which it has been for more than a decade, and it is compatible with its bluer-when-brighter moderate tendency, possibly due to the presence of shocks within the jet.

Discussion (0). Continue with ORCID to comment.

Pith tools