A 5.5–35 μm Spectral Analysis of Active Galactic Nuclei
2009 ◽
Vol 5
(S267)
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pp. 137-137
Keyword(s):
Raw Data
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The spectroscopic properties of a sample of nine Seyfert 1, six NLS1, 26 Seyfert 2, and three starburst galaxies have been studied at mid-infrared wavelengths in order to determine if the frequency of detection of the brightest emission lines and the continuum shape are correlated with the degree of activity. The raw data were obtained from the Spitzer Infrared Spectrograph (IRS) archive and reduced with the pipeline (version 17.2). The spectra of the galaxies were grouped by type of activity. We conclude through this study that in general the continuum shape of the active galactic nuclei (AGN) is flat between 5 μm and 12 μm, and strong variations are found at longer wavelengths in this sample.
2014 ◽
Vol 790
(1)
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pp. 15
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Keyword(s):
2013 ◽
Vol 9
(S304)
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pp. 225-226
2019 ◽
Vol 15
(S359)
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pp. 415-417
Keyword(s):
2019 ◽
Vol 15
(S356)
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pp. 247-251
Keyword(s):
2017 ◽
Vol 468
(1)
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pp. 196-206
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Keyword(s):
2021 ◽
Vol 507
(4)
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pp. 5205-5213
Keyword(s):
2019 ◽
Vol 15
(S352)
◽
pp. 121-122
2010 ◽
Vol 713
(1)
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pp. 503-519
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