Lag between the optical and NIR variabilities of NGC 4151

Details Lag between the optical and NIR variabilities of NGC 4151 Lag between the optical and NIR variabilities of NGC 4151

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004an....325..256m&link_type=abstract

Astronomische Nachrichten, Vol.325, Issue 3, p.256-256

Astronomy and Astrophysics

Astronomy

Scientific paper

The most intense monitoring observations yet made were carried out on the Seyfert 1 galaxy NGC 4151 in the optical and near-infrared wave-bands. We obtained photometric data for NGC 4151 consisting of 44 nights in the V band and 49 nights in the K band between January and December 2001, using the multicolor imaging photometer (MIP) mounted on the MAGNUM telescope (Kobayashi et al. 1998a,b; Yoshii, Kobayashi & Minezaki 2003).

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