AGN and host galaxies in the COSMOS survey

Christopher D. Impey; Jonathan R. Trump; Jared M. Gabor

doi:10.1017/S1743921311022381

AGN and host galaxies in the COSMOS survey

Christopher D. Impey, Jonathan R. Trump, Jared M. Gabor

Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

The Cosmological Evolution Survey (COSMOS) is a unique tool for studying low level AGN activity and the co-evolution of galaxies and supermassive black holes. COSMOS involves the largest contiguous region of the sky ever imaged by HST; it includes very complete multiwavelength coverage, and the largest joint samples of galaxy and AGN redshifts in any deep survey. The result is a search for AGN with low black hole mass, low accretion rates, and levels of obscuration that can remove them from optical surveys. A complete census of intermediate mass black holes at redshifts of 1 to 3 is required to tell the story of the co-evolution of galaxies and their embedded, and episodically active, black holes.

Original language	English (US)
Title of host publication	Tracing the Ancestry of Galaxies
Subtitle of host publication	On the Land of our Ancestors
Editors	Claude Carignan, Claude Carignan, Francoise Combes, Ken Freeman
Pages	21-25
Number of pages	5
Edition	S277
DOIs	https://doi.org/10.1017/S1743921311022381
State	Published - Dec 2010

Publication series

Name	Proceedings of the International Astronomical Union
Number	S277
Volume	6
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1017/S1743921311022381

Cite this

AGN and host galaxies in the COSMOS survey. / Impey, Christopher D.; Trump, Jonathan R.; Gabor, Jared M.
Tracing the Ancestry of Galaxies: On the Land of our Ancestors. ed. / Claude Carignan; Claude Carignan; Francoise Combes; Ken Freeman. S277. ed. 2010. p. 21-25 (Proceedings of the International Astronomical Union; Vol. 6, No. S277).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

@inproceedings{5629cb37f1c841e7ab4eeee93b69213d,

title = "AGN and host galaxies in the COSMOS survey",

abstract = "The Cosmological Evolution Survey (COSMOS) is a unique tool for studying low level AGN activity and the co-evolution of galaxies and supermassive black holes. COSMOS involves the largest contiguous region of the sky ever imaged by HST; it includes very complete multiwavelength coverage, and the largest joint samples of galaxy and AGN redshifts in any deep survey. The result is a search for AGN with low black hole mass, low accretion rates, and levels of obscuration that can remove them from optical surveys. A complete census of intermediate mass black holes at redshifts of 1 to 3 is required to tell the story of the co-evolution of galaxies and their embedded, and episodically active, black holes.",

author = "Impey, {Christopher D.} and Trump, {Jonathan R.} and Gabor, {Jared M.}",

year = "2010",

month = dec,

doi = "10.1017/S1743921311022381",

language = "English (US)",

isbn = "9780521766029",

series = "Proceedings of the International Astronomical Union",

number = "S277",

pages = "21--25",

editor = "Claude Carignan and Claude Carignan and Francoise Combes and Ken Freeman",

booktitle = "Tracing the Ancestry of Galaxies",

edition = "S277",

}

TY - GEN

T1 - AGN and host galaxies in the COSMOS survey

AU - Impey, Christopher D.

AU - Trump, Jonathan R.

AU - Gabor, Jared M.

PY - 2010/12

Y1 - 2010/12

N2 - The Cosmological Evolution Survey (COSMOS) is a unique tool for studying low level AGN activity and the co-evolution of galaxies and supermassive black holes. COSMOS involves the largest contiguous region of the sky ever imaged by HST; it includes very complete multiwavelength coverage, and the largest joint samples of galaxy and AGN redshifts in any deep survey. The result is a search for AGN with low black hole mass, low accretion rates, and levels of obscuration that can remove them from optical surveys. A complete census of intermediate mass black holes at redshifts of 1 to 3 is required to tell the story of the co-evolution of galaxies and their embedded, and episodically active, black holes.

AB - The Cosmological Evolution Survey (COSMOS) is a unique tool for studying low level AGN activity and the co-evolution of galaxies and supermassive black holes. COSMOS involves the largest contiguous region of the sky ever imaged by HST; it includes very complete multiwavelength coverage, and the largest joint samples of galaxy and AGN redshifts in any deep survey. The result is a search for AGN with low black hole mass, low accretion rates, and levels of obscuration that can remove them from optical surveys. A complete census of intermediate mass black holes at redshifts of 1 to 3 is required to tell the story of the co-evolution of galaxies and their embedded, and episodically active, black holes.

UR - http://www.scopus.com/inward/record.url?scp=83655191649&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=83655191649&partnerID=8YFLogxK

U2 - 10.1017/S1743921311022381

DO - 10.1017/S1743921311022381

M3 - Conference contribution

AN - SCOPUS:83655191649

SN - 9780521766029

T3 - Proceedings of the International Astronomical Union

SP - 21

EP - 25

BT - Tracing the Ancestry of Galaxies

A2 - Carignan, Claude

A2 - Combes, Francoise

A2 - Freeman, Ken

ER -

AGN and host galaxies in the COSMOS survey

Abstract

Publication series

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this