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Monthly Notices of the Royal Astronomical Society
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arXiv.org e-Print Archive
Preprint . 2003
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Monthly Notices of the Royal Astronomical Society
Article . 2003 . Peer-reviewed
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https://dx.doi.org/10.48550/ar...
Article . 2003
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Monthly Notices of the Royal Astronomical Society
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The host galaxies of active galactic nuclei

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Dec 2003Embargo end date: 01 Jan 2003 English Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 346, pages 1,055-1,077 (issn: 0035-8711, eissn: 1365-2966, Copyright policy )
Authors: Željko Ivezić; S. E. Ridgway; Gordon T. Richards; Stephane Charlot; Stephane Charlot; Timothy M. Heckman; Jarle Brinchmann; +8 Authors

doi: 10.1111/j.1365-2966.2003.07154.x , 10.48550/arxiv.astro-ph/0304239

arXiv: http://arxiv.org/abs/astro-ph/0304239

The host galaxies of active galactic nuclei

Abstract

submitted to MNRAS, 44 pages, version with full resolution figures available at http://www.mpa-garching.mpg.de/~gamk/agnpaper/agnpaper.ps

We examine the properties of the host galaxies of 22,623 narrow-line AGN with 0.02

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Keywords

galaxies : Seyfert, galaxies : active, Astrophysics (astro-ph), galaxies : structure, FOS: Physical sciences, galaxies : starburst, Astrophysics, 530, 520, galaxies : stellar content

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
3K
Top 0.01%
Top 0.1%
Top 0.1%
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