Monitoring of the optical and 2.5-11.7 mu m spectrum and mid-IR imaging of the Seyfert 1 galaxy Mrk 279 with ISO
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...We examined two completely independent sets of data, one from theWise Observatory program in 1988 (Maoz et al. 1990) and one from an International AGN Watch project in 1996 (Santos-Lleó et al. 2001)....
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Cites result from "Monitoring of the optical and 2.5-1..."
...We include here only the results for Mrk 279 reported by Santos-Lleó et al. (2001)....
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"Monitoring of the optical and 2.5-1..." refers background in this paper
...Indeed, a faint extended nebulosity is apparent in the K-band (∼2.2µm) image of McLeod & Rieke (1995)....
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...In the K-band, McLeod & Rieke (1995) estimated that the AGN contributes 90% of the flux within the central 1....
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157 citations
"Monitoring of the optical and 2.5-1..." refers background or methods in this paper
...Assuming “normal” near-IR colors (K−L = 0.22±0.02mag; Clavel et al. 1989) for the stellar population, we derive a total host-galaxy flux of 18 mJy at 3.5µm; 2....
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...Using the B-and R-band nucleus–galaxy decomposition of Granato et al. (1993), and assuming normal optical-to-IR (V − K = 3.22 mag; Clavel et al. 1989) and K − L colors, we estimate a total galaxy flux of 20 mJy and 17 mJy respectively at 3.5µm....
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...We can estimate the distance to the central source of the innermost and hottest dust grains in Mrk 279, rin, by scaling directly from Fairall 9 (Clavel et al. 1989)....
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...…time delay corresponds closely to the lighttravel time to the dust sublimation radius rin; measured values of rin are 400 light days for Fairall 9 (Clavel et al. 1989), 50 light days for NGC 1566 (Baribaud et al. 1992), 80 light days for NGC 3783 (Glass 1992) and 32 light days for Mrk 744 (Nelson…...
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