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A&A 422, 505-508 (2004)
DOI: 10.1051/0004-6361:20040306
Research Note
Near infrared intraday variability of Mrk 421
A. C. Gupta1, D. P. K. Banerjee2, N. M. Ashok2 and U. C. Joshi21 Harish-Chandra Research Institute, Chhatnag Road, Jhunsi, Allahabad 211 019, India
e-mail: agupta@mri.ernet.in
2 Astronomy and Astrophysics Division, Physical Research Laboratory, Navrangpura, Ahmedabad 380 009, India
e-mail: [orion;ashok;joshi]@prl.ernet.in
(Received 20 February 2004 / Accepted 2 April 2004 )
Abstract
We report results from our monitoring of the BL Lac object Mrk 421 in the near-IR
J
band. The observations, aimed at studying the intraday variability (IDV) of the object,
were carried out systematically over an extended (and near-continuous) period of eight
nights from the 1.2 m Mount Abu Infrared Telescope, India. There are limited studies
for Mrk 421 in the
J band for such an extended period. The observation epoch for this
study (25 February-5 March 2003) was chosen to significantly overlap other concurrent
studies of Mrk 421 in the X-ray/
-ray regions being conducted using the Rossi X-ray timing
explorer (RXTE) and the solar tower atmospheric Cherenkov effect experiment (STACEE).
Hence these results could be useful for a multi-wavelength analysis of the variability
behavior of Mrk 421. We find that Mrk 421 was quite active during the observed period and
showed significant IDV and short term variability. A maximum variation of 0.89 mag
is seen over the entirety of the observed period. Flaring activity, with typical brightness
variations of ~0.4, are also seen on several occasions. The extent of the variability
observed by us is compared with the results of other similar studies of Mrk 421 in the
J band.
Key words: BL Lacertae objects: individual: Mrk 421 -- BL Lacertae objects: general -- infrared: general
SIMBAD Objects
© ESO 2004
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