Fe ii and Mg ii in Luminous, Intermediate‐Redshift, Narrow‐Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey

Karen M. Leighly; John R. Moore

Journal ArticleOPEN ACCESS

Fe ii and Mg ii in Luminous, Intermediate‐Redshift, Narrow‐Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey

Leighly K
Moore J

The Astrophysical Journal (2006) 644(2) 748-758

DOI: 10.1086/503621

11Citations

7Readers

Abstract

We present results from analysis of spectra from a sample of ~900 quasars from the Sloan Digital Sky Survey. These objects were selected for their intermediate redshift (1.2

References Powered by Scopus

View more at Scopus

Cited by Powered by Scopus

View more at Scopus

Cite

CITATION STYLE

APA

Leighly, K. M., & Moore, J. R. (2006). Fe ii and Mg ii in Luminous, Intermediate‐Redshift, Narrow‐Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey. The Astrophysical Journal, 644(2), 748–758. https://doi.org/10.1086/503621

Readers' Seniority

Professor / Associate Prof. 2

40%

Researcher 2

40%

PhD / Post grad / Masters / Doc 1

20%

Readers' Discipline

Physics and Astronomy 6

100%

Fe ii and Mg ii in Luminous, Intermediate‐Redshift, Narrow‐Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey

Abstract

References Powered by Scopus

The slope of the black hole mass versus velocity dispersion correlation

Atlas of quasar energy distributions

The emission-line properties of low-redshift quasi-stellar objects

Cited by Powered by Scopus

The intrinsically X-ray-weak quasar PHL 1811. II. Optical and UV spectra and analysis

Emergence of a broad absorption line outflow in the narrow-line seyfert 1 galaxy wpvs 007

What controls the Fe II strength in active galactic nuclei?

Register to see more suggestions

Cite

Readers' Seniority

Readers' Discipline