DUAL SUPERMASSIVE BLACK HOLE CANDIDATES IN THE AGN AND GALAXY EVOLUTION SURVEY

Dual supermassive black holes (SMBHs) with kiloparsec-scale separations in merger-remnant galaxies are informative tracers of galaxy evolution, but the avenue for identifying them in large numbers for such studies is not yet clear. Dual AGNs may produce double-peaked narrow AGN emission lines, while...

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Veröffentlicht in:The Astrophysical journal 2013-11, Vol.777 (1), p.1-10
Hauptverfasser: Comerford, Julia M, Schluns, Kyle, Greene, Jenny E, Cool, Richard J
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container_title The Astrophysical journal
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creator Comerford, Julia M
Schluns, Kyle
Greene, Jenny E
Cool, Richard J
description Dual supermassive black holes (SMBHs) with kiloparsec-scale separations in merger-remnant galaxies are informative tracers of galaxy evolution, but the avenue for identifying them in large numbers for such studies is not yet clear. Dual AGNs may produce double-peaked narrow AGN emission lines, while offset AGNs may produce single-peaked narrow AGN emission lines with line-of-sight velocity offsets relative to the host galaxy. We search for such dual and offset systems among 173 Type 2 AGNs at z < 0.37 in the AGN and Galaxy Evolution Survey (AGES), and we find two double-peaked AGNs and five offset AGN candidates. When we compare these results to a similar search of the DEEP2 Galaxy Redshift Survey and match the two samples in color, absolute magnitude, and minimum velocity offset, we find that the fraction of AGNs that are dual SMBH candidates increases from z = 0.25 to z = 0.7 by a factor of ~6 (from 2/70 to 16/91, or 2.9 super(+3.6) sub(-1.9)% to 18 super(+5) sub(-5)%).
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subjects Active galactic nuclei
ASTRONOMY
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BLACK HOLES
Black holes (astronomy)
COLOR
COMPARATIVE EVALUATIONS
Emission
GALACTIC EVOLUTION
GALAXIES
GALAXY NUCLEI
Line of sight
Offsets
RED SHIFT
Searching
VELOCITY
title DUAL SUPERMASSIVE BLACK HOLE CANDIDATES IN THE AGN AND GALAXY EVOLUTION SURVEY
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