Abstract:
We report the results of photometric observations of the blazars Mrk 421 and 3C 454.3 designed to search for
intraday variability (IDV) and short-term variability (STV). Optical photometric observations were spread over
18 nights for Mrk 421 and 7 nights for 3C 454.3 during our observing run in 2009–2010 at the 1.04 m telescope
at Aryabhatta Research Institute of Observational Sciences, India. Genuine IDV is found for the source 3C 454.3 but not for Mrk 421. Genuine STV is found for both sources. Mrk 421 was revealed by the Monitor of All-sky X-ray Image (MAXI) X-ray detector on the International Space Station to be in an exceptionally high flux state in 2010 January–February.We performed a correlation between the X-ray and optical bands to search for time delays and found a weak correlation with higher frequencies leading the lower frequencies by about 10 days. The blazer 3C 454.3 was found to be in a high flux state in 2009 November–December. We performed correlations in optical observations made at three telescopes, along with X-ray data from the MAXI camera and public release γ -ray data from the Fermi space telescope. We found strong correlations between the γ -ray and optical bands at a time lag of about four days, but the X-ray flux is not correlated with either.We briefly discuss the possible reasons for the time delays between these bands within the framework of existing models for X-ray and γ -ray emission mechanisms.
