| | |
| | |
Stat |
Members: 3645 Articles: 2'504'928 Articles rated: 2609
26 April 2024 |
|
| | | |
|
Article overview
| |
|
Type 1 AGN at low z | Jonathan Stern
; Ari Laor
; | Date: |
22 Mar 2012 | Abstract: | We present the emission properties of a sample of 3,579 type 1 AGN, selected
based on the detection of broad H-alpha emission. The sample covers the range
of black hole mass 10^6<M_BH/M_Sun<10^9.5 and luminosity in Eddington units
10^-3 < L/L_Edd < 1. Our main results are: 1. The distribution of the H-alpha
FWHM values is independent of luminosity. 2. The observed mean optical-UV SED
is well matched by a fixed shape SED of luminous quasars, which scales linearly
with broad H-alpha luminosity, and a host galaxy contribution. 3. The host
galaxy r-band (fibre) luminosity function follows well the luminosity function
of inactive non-emission line galaxies (NEG), consistent with a fixed fraction
of ~3% of NEG hosting an AGN, regardless of the host luminosity. 4. The
optical-UV SED of the more luminous AGN shows a small dispersion, consistent
with dust reddening of a blue SED, as expected for thermal thin accretion disc
emission. 5. There is a rather tight relation of nuL_nu(2 keV) and broad
H-alpha luminosity, which provides a useful probe for unobscured (true) type 2
AGN. | Source: | arXiv, 1203.5005 | Services: | Forum | Review | PDF | Favorites |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)
|
| |
|
|
|
| News, job offers and information for researchers and scientists:
| |