Spitzer 3.6 and 5.8 micron Monitoring of the Seyfert 1 NGC 4051

Details Spitzer 3.6 and 5.8 micron Monitoring of the Seyfert 1 NGC 4051 Spitzer 3.6 and 5.8 micron Monitoring of the Seyfert 1 NGC 4051

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21342006g&link_type=abstract

American Astronomical Society, AAS Meeting #213, #420.06; Bulletin of the American Astronomical Society, Vol. 41, p.236

Astronomy and Astrophysics

Astronomy

Scientific paper

We used the Spitzer Space Telescope Infrared Array Camera (IRAC) to monitor the Seyfert 1 active galactic nucleus NGC 4051. We took data at 3.6 and 5.8 microns every day for 10 days in June 2008. We also observed in the optical at B, V, and R bands starting a month before the IRAC observations with various ground based observatories, though we were unable to achieve daily coverage. We will present the IR and optical light curves and will search for correlated variability that may be evidence of dust reverberation. For the education and public outreach component of this program please see Sepulveda et al.

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