- A low redshift X|ray survey🔍
- A TWO|PARAMETER MODEL FOR THE INFRARED ...🔍
- The Role of AGN in Luminous Infrared Galaxies from the ...🔍
- Resolving the AGN and Host Emission in the Mid|infrared Using a ...🔍
- Properties of Estimators 🔍
- Roberto J. Assef🔍
- model independent decomposition of mid|infrared spectra🔍
- Spectral Energy Distributions of Far Infrared Selected X|ray AGN🔍
Mid|IR Properties of an Unbiased AGN Sample of the ...
(PDF) Optical and X-ray Properties of the Swift BAT-detected AGN ...
Mid-IR Properties of an Unbiased AGN Sample of the Local Universe. I ... unbiased view of local Compton thin active galactic nuclei sources (AGNs).
A low redshift X-ray survey: understanding the co-evolution of AGN ...
At these redshifts, X-ray surveys are the only way for compiling unbiased AGN samples. ... mid-IR SED of a nearby X-ray AGN sample will help ... i.e. the host ...
A TWO-PARAMETER MODEL FOR THE INFRARED ...
... AGN template is essentially devoid of PAH emission features. ... Figure 8 shows how the 5MUSES sample is biased toward AGN at higher infrared.
The Role of AGN in Luminous Infrared Galaxies from the ... - MDPI
Multiwavelength diagnosis combining radio and far-infrared, for instance, offers further insight into the nature of the compact sources by ...
Resolving the AGN and Host Emission in the Mid-infrared Using a ...
We conclude that the emission from the host galaxy can be reliably removed from the IRS spectra of AGNs. This allows for unbiased studies of the AGN ...
Properties of Estimators (Unbiased, Consistent) - Inference 1.3/4
When the purpose of a statistic is to estimate a population parameter, the statistic is called an estimator. A number of statistics are ...
Roberto J. Assef - Hot Dust Obscured Galaxies
Studying the most variable reliably AGN we identified in Assef et al. (2018a), we found a luminous transient in an AGN visible at both mid-IR and optical ...
model independent decomposition of mid-infrared spectra - Denebola
The mid-infrared spectra of active galactic nuclei (AGN) are often contaminated by the unresolved emission from the galaxies that hosts them.
Spectral Energy Distributions of Far Infrared Selected X-ray AGN
The strength of these individual features can vary depending on the geometry of the accretion disk and the amount of accreting material feeding the SMBH. In the ...