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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Additional excerpts
...…Denney et al. 2009b; (17) Bentz et al. 2006a; (18) Zhang et al. 2019; (19) Denney et al. 2006; (20) Bentz et al. 2016; (21) Bentz et al. 2014; (22) Santos-Lleó et al. 2001; (23) Peterson et al. 1991; (24) Peterson et al. 2013; (25) Peterson et al. 1992; (26) Peterson et al. 1994; (27) Korista et…...
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Cites background from "Monitoring of the optical and 2.5-1..."
...Santos-Lleo et al. (2001) have carried out a monitoring of the optical and NIR spectrum and MIR imaging of the Sy 1 galaxy Mrk 279....
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References
1,139 citations
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"Monitoring of the optical and 2.5-1..." refers methods in this paper
...Reverberation-mapping techniques (Blandford & McKee 1982) have been used extensively to map the BLR in several AGN, on scales of light days to light months, notably by the International AGN Watch1 consortium (Alloin et al. 1994)....
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818 citations
"Monitoring of the optical and 2.5-1..." refers methods in this paper
...We used both the interpolation method of Gaskell & Sparke (1986) and the discretecorrelation function (DCF) method of Edelson & Krolik (1988), in both cases employing the specific implementation described by White & Peterson (1994)....
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648 citations
"Monitoring of the optical and 2.5-1..." refers background in this paper
...The presence of a universal inflection point near 1.2µm in the spectral energy distribution of radio-quiet AGN’s strongly suggests that the bulk of the near IR flux arises from dust thermal emission (e.g., Barvainis 1987; Sanders et al. 1989)....
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644 citations
"Monitoring of the optical and 2.5-1..." refers background in this paper
...The presence of a universal inflection point near 1.2µm in the spectral energy distribution of radio-quiet AGN’s strongly suggests that the bulk of the near IR flux arises from dust thermal emission (e.g., Barvainis 1987; Sanders et al. 1989)....
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