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CANDELS: Elevated black hole growth in the progenitors of compact quiescent galaxies at z ? 2

Authors

Dale D. Kocevski

Guillermo Barro

S.M. Faber

Avishai Dekel

Rachel S. Somerville

Joshua A. Young

Christina C. Williams

Daniel H. McIntosh

Antonis Georgakakis

Guenther Hasinger

Kirpal Nandra

Francesca Civano

David M. Alexander

OMAR ALMAINI omar.almaini@nottingham.ac.uk
Professor of Astrophysics

Christopher J. Conselice

Jennifer L. Donley

Harry C. Ferguson

Mauro Giavalisco

Norman A. Grogin

Nimish Hathi

Matthew Hawkins

Anton M. Koekemoer

David C. Koo

Elizabeth J. McGrath

Bahram Mobasher

Pablo G.

Janine Pforr

Joel R. Primack

Paola Santini

Mauro Stefanon

Jonathan R. Trump

Arjen van der Wel

Stijn Wuyts

Haojing Yan



Abstract

We examine the fraction of massive (M* > 1010 M) compact star-forming galaxies (cSFGs) that host an active galactic nucleus (AGN) at z ~ 2. These cSFGs are likely the direct progenitors of the compact quiescent galaxies observed at this epoch, which are the first population of passive galaxies to appear in large numbers in the early Universe. We identify cSFGs that host an AGN using a combination of Hubble WFC3 imaging and Chandra X-ray observations in four fields: the Chandra Deep Fields, the Extended Groth Strip, and the UKIDSS Ultra Deep Survey field. We find that - 39.2+ % 3.6 3.9 (65/166) of cSFGs at 1.4 < z < 3.0 host an X-ray detected AGN. This fraction is 3.2 times higher than the incidence of AGN in extended star-forming galaxies with similar masses at these redshifts. This difference is significant at the 6.2s level. Our results are consistent with models in which cSFGs are formed through a dissipative contraction that triggers a compact starburst and concurrent growth of the central black hole. We also discuss our findings in the context of cosmological galaxy evolution simulations that require feedback energy to rapidly quench cSFGs. We show that the AGN fraction peaks precisely where energy injection is needed to reproduce the decline in the number density of cSFGs with redshift. Our results suggest that the first abundant population of massive quenched galaxies emerged directly following a phase of elevated supermassive black hole growth and further hints at a possible connection between AGN and the rapid quenching of star formation in these galaxies.

Citation

Kocevski, D. D., Barro, G., Faber, S., Dekel, A., Somerville, R. S., Young, J. A., …Yan, H. (2017). CANDELS: Elevated black hole growth in the progenitors of compact quiescent galaxies at z ∼ 2. Astrophysical Journal, 846(2), https://doi.org/10.3847/1538-4357/aa8566

Journal Article Type Article
Acceptance Date Aug 7, 2017
Online Publication Date Sep 7, 2017
Publication Date Sep 10, 2017
Deposit Date Oct 5, 2017
Publicly Available Date Oct 5, 2017
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 846
Issue 2
DOI https://doi.org/10.3847/1538-4357/aa8566
Public URL https://nottingham-repository.worktribe.com/output/882131
Publisher URL http://iopscience.iop.org/article/10.3847/1538-4357/aa8566/meta

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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf





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