Does the mid-infrared–hard X-ray luminosity relation for active galactic nuclei depend on Eddington ratio?
Overview & Synopsis
This academic paper investigates whether the mid-infrared to hard X-ray luminosity relation for active galactic nuclei shows any dependence on the Eddington ratio. It analyzes observational data to better understand the accretion physics and obscuration properties of supermassive black holes.
Indexed from repository: NASA Technical Reports Server
(
ntrs.nasa.gov)
Document Information
| Document Title | Does the mid-infrared–hard X-ray luminosity relation for active galactic nuclei depend on Eddington ratio? |
|---|---|
| Author / Organization | Yoshiki Toba, Yoshihiro Ueda, Kenta Matsuoka, Megumi Shidatsu, Tohru Nagao, Yuichi Terashima, Wei-Hao Wang, Yu-Yen Chang |
| Subject & Discipline | REPRINT |
| Categories | Aerospace & Aviation |
| Publication Year | 2026 |
| License / Rights | Public Domain / NASA STI Open Access |
| Resource Verification | Listed PDF (Verification Pending) |
| Original Host Website |
NASA Technical Reports Server
(ntrs.nasa.gov)
|
| File Format | application/pdf (Portable Document Format) |
| Language | EN |
| Catalog ID | DOC-381 |
| Original Source Link | Visit Source Page on ntrs.nasa.gov » |