High time resolution monitoring at 2.2 microns of the Seyfert 1 galaxy NGC 4051

Details High time resolution monitoring at 2.2 microns of the Seyfert 1 galaxy NGC 4051 High time resolution monitoring at 2.2 microns of the Seyfert 1 galaxy NGC 4051

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...257..434h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 257, no. 2, p. 434-436.

Astronomy and Astrophysics

Astrophysics

11

Astronomical Photometry, Infrared Photometry, Seyfert Galaxies, Temporal Resolution, Active Galactic Nuclei, Near Infrared Radiation, Spectrophotometry, X Ray Sources

Scientific paper

We present here time-resolved differential photometric observations at 2.2 microns of NGC 4051. The measurements were taken at 20 min intervals over time scales of several hours, with a differential photometric accuracy of less than about 1 percent. The results of measurements performed on two nights are discussed in the context of the origin of the near-infrared continuum in AGN.

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