A Comparison of Mid-infrared Spectral Decomposition and Full Infrared Spectral Energy Distribution Modeling to Quantify AGN in Dusty Galaxies: The Necessity of Data between 6 and 14 Microns

2019 ◽  
Vol 3 (12) ◽  
pp. 199
Author(s):  
Owen K. Henry ◽  
Alexandra Pope ◽  
Jed McKinney ◽  
Allison Kirkpatrick
Keyword(s):  
Energy Distribution ◽  
Spectral Decomposition ◽  
Spectral Energy Distribution ◽  
Spectral Energy ◽  
Mid Infrared ◽  
Distribution Modeling ◽  
Dusty Galaxies ◽  
Infrared Spectral

scholarly journals Mid‐Infrared Spectral Energy Distribution of NGC 1068 with 0.̋1 Spatial Resolution

2001 ◽  
Vol 557 (2) ◽  
pp. 637-645 ◽  
Author(s):  
Daigo Tomono ◽  
Yoshiyuki Doi ◽  
Tomonori Usuda ◽  
Tetsuo Nishimura
Keyword(s):  
Energy Distribution ◽  
Spatial Resolution ◽  
Spectral Energy Distribution ◽  
Spectral Energy ◽  
Mid Infrared ◽  
Infrared Spectral ◽  
Ngc 1068

scholarly journals THE ULTRAVIOLET-TO-MID-INFRARED SPECTRAL ENERGY DISTRIBUTION OF WEAK EMISSION LINE QUASARS

2011 ◽  
Vol 743 (2) ◽  
pp. 163 ◽  
Author(s):  
Ryan A. Lane ◽  
Ohad Shemmer ◽  
Aleksandar M. Diamond-Stanic ◽  
Xiaohui Fan ◽  
Scott F. Anderson ◽  
...  
Keyword(s):  
Energy Distribution ◽  
Emission Line ◽  
Spectral Energy Distribution ◽  
Spectral Energy ◽  
Mid Infrared ◽  
Infrared Spectral

scholarly journals NuSTAROBSERVATIONS AND BROADBAND SPECTRAL ENERGY DISTRIBUTION MODELING OF THE MILLISECOND PULSAR BINARY PSR J1023+0038

2014 ◽  
Vol 797 (2) ◽  
pp. 111 ◽  
Author(s):  
K. L. Li ◽  
A. K. H. Kong ◽  
J. Takata ◽  
K. S. Cheng ◽  
P. H. T. Tam ◽  
...  
Keyword(s):  
Energy Distribution ◽  
Spectral Energy Distribution ◽  
Spectral Energy ◽  
Millisecond Pulsar ◽  
Distribution Modeling

scholarly journals Model for Infrared Properties of Extremely Young Galaxies

2004 ◽  
Vol 217 ◽  
pp. 214-215
Author(s):  
T. T. Takeuchi ◽  
H. Hirashita ◽  
T. T. Ishii ◽  
L. K. Hunt ◽  
A. Ferrara
Keyword(s):  
Energy Distribution ◽  
Size Distribution ◽  
Galaxy Evolution ◽  
Early Stage ◽  
Spectral Energy Distribution ◽  
Spectral Energy ◽  
Dust Size Distribution ◽  
Infrared Spectral

We constructed a model of the infrared spectral energy distribution for very young galaxies by taking into account the dust size distribution in the early stage of galaxy evolution.

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