Optical variability of three extreme TeV blazars. Issue 2 (8th June 2020)

• Record Type: Journal Article
• Authors: Pandey, Ashwani; Gupta, Alok C; Damljanovic, G; Wiita, P J; Vince, O; Jovanovic, M D
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 496:Issue 2(2020)
• Page Start: 1430
• Page End: 1444
• Publication Date: 2020-06-08
• Subjects: galaxies: active -- BL Lacertae objects: general -- BL Lacertae objects: individual (1ES 0229+200, 1ES 0414+009, 1ES 2344+514); Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa1598
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present the results of optical photometric observations of three extreme TeV blazars, 1ES 0229+200, 1ES 0414+009, and 1ES 2344+514, taken with two telescopes (1.3 m Devasthal Fast Optical Telescope, and 1.04 m Sampuranand Telescope) in India and two (1.4 m Milanković telescope and 60 cm Nedeljković telescope) in Serbia during 2013–2019. We investigated their flux and spectral variability on diverse time-scales. We examined a total of 36 intraday R -band light curves of these blazars for flux variations using the power-enhanced F -test and the nested ANOVA test. No significant intraday variation was detected on 35 nights, and during the one positive detection the amplitude of variability was only 2.26 per cent. On yearly time-scales, all three blazars showed clear flux variations in all optical wavebands. The weighted mean optical spectral index (α BR ), calculated using B − R colour indices, for 1ES 0229+200 was 2.09 ± 0.01. We also estimated the weighted mean optical spectral indices of 0.67 ± 0.01 and 1.37 ± 0.01 for 1ES 0414+009, and 1ES 2344+514, respectively, by fitting a single power law ( F ν ∝ ν −α ) in their optical ( VRI ) spectral energy distributions. A bluer-when-brighter trend was only detected in the blazar 1ES 0414+009. We briefly discuss different possible physical mechanisms responsible for the observed flux and spectral changes in these blazars on diverse time-scales.