Fe <scp>II</scp> emission in active galactic nuclei-Reference-Cited by-同舟云学术

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Fe II emission in active galactic nuclei

Published:2022-01 Issue:1-2 Volume:343 Page:
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron Nachr

Author:

Gaskell Martin¹^ORCID,Thakur Neha¹²,Tian Betsy¹³,Saravanan Anjana¹⁴

Affiliation:

1. Department of Astronomy and Astrophysics University of California Santa Cruz Santa Cruz California USA

2. Data Science Department University of California Berkeley Berkeley California USA

3. Physics Department Massachusetts Institute of Technology Cambridge Massachusetts USA

4. Department of Mechanical Engineering University of California Berkeley Berkeley California USA

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.20210112

Reference133 articles.

1. A Survey of the Seyfert Galaxies Based on Large-Scale Image-Tube Plates

2. DEPENDENCE OF THE OPTICAL/ULTRAVIOLET VARIABILITY ON THE EMISSION-LINE PROPERTIES AND EDDINGTON RATIO IN ACTIVE GALACTIC NUCLEI

3. Time development of the emission lines and continuum of NGC 4151

4. Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines

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3. Near-infrared emission line diagnostics for AGN from the local Universe to z ∼ 3;Astronomy & Astrophysics;2023-11

4. Influence of the optical Fe II quasi-continuum on measuring the spectral parameters of active galactic nuclei;Astronomy & Astrophysics;2023-11

5. Wavelength-resolved reverberation mapping of intermediate-redshift quasars HE 0413-4031 and HE 0435-4312: Dissecting Mg II, optical Fe II, and UV Fe II emission regions;Astronomy & Astrophysics;2023-10

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