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Statistics of optical intraday variability in a complete sample of radio-selected BL Lac objects

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arxiv astro-ph/9506032 v1 pith:36PFUWTV submitted 1995-06-06 astro-ph

classification astro-ph
keywords objectsvariabilityableintradaytypicalwerebehaviourcomplete
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We present a study of the intraday variability behaviour of a complete sample of radio-selected BL Lac objects taken from the 1 Jy catalogue. In 28 out of 34 BL Lac objects (82\%) we detected intraday variability. 7 objects were observed during several campaigns. None of them changed its variability behaviour. The duty cycle in radio-loud BL Lac objects is very high, i.e. at least 0.8. The typical peak-to-peak amplitudes of the variability were 30\%. By means of structure function and autocorrelation analyses we investigated the typical time-scales of the variability and determined the activity of the BL Lac objects. In 21 of the variable BL Lac objects we were able to measure a typical time-scale, which lies in the range between 0.5 and 3 days. In general, the results can be explained by the standard model, where shocks are propagating down a relativistic jet. However, in the two most densely sampled observations we found variability characteristics, which cannot easily be explained by the standard model alone, demonstrating that at least in these objects alternative models should be taken into account. Nevertheless, all models, which are able to explain variability on time-scales of days must be able to consider the high duty cycle of these BL Lac objects.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 27 citations worldwide. Full citation record

  1. Comprehensive Analysis of Optical brightness and Color Variability of Blazars in the ZTF Survey DR22

    astro-ph.CO 2026-06 unverdicted novelty 5.0 of 10

    Analysis of ZTF data shows BL Lacs with BWB color trend at 14.7% vs 2.3% RWB, FSRQs with 8.8% BWB vs 14.1% RWB, and brighter states more likely to show BWB, with variability amplitude correlating differently by type.

  2. Multiband Optical Variability of the Blazar 3C 454.3 on Diverse Timescales

    astro-ph.HE 2024-12 conditional novelty 5.0 of 10

    Twenty years of optical light curves of blazar 3C 454.3 show a redder-when-brighter trend that flattens near I-band magnitude 14.5 and a two-peaked distribution of spectral indices.

  3. Multi-band optical variability of the blazar OP 313 in the outburst state during 2024-2025

    astro-ph.HE 2025-07 conditional novelty 4.0 of 10

    Multi-band optical monitoring of the blazar OP 313 during its 2024-2025 outburst reveals a bluer-when-brighter color trend on short-term timescales, a behavior more typical of BL Lac objects than FSRQs.

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