Y. Kato
Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2–3
Kato, Y.; Matsuda, Y.; Smail, I.; Swinbank, A.M.; Hatsukade, B.; Umehata, H.; Tanaka, I.; Saito, T.; Iono, D.; Tamura, Y.; Kohno, K.; Erb, D.K.; Lehmer, B.D.; Geach, J.E.; Steidel, C.C.; Alexander, D.M.; Yamada, T.; Hayashino, T.
Authors
Y. Matsuda
Ian Smail ian.smail@durham.ac.uk
Emeritus Professor
Professor Mark Swinbank a.m.swinbank@durham.ac.uk
Professor
B. Hatsukade
H. Umehata
I. Tanaka
T. Saito
D. Iono
Y. Tamura
K. Kohno
D.K. Erb
B.D. Lehmer
J.E. Geach
C.C. Steidel
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
T. Yamada
T. Hayashino
Abstract
We present a Herschel/SPIRE survey of three protoclusters at z = 2 − 3 (2QZCluster, HS1700, SSA22). Based on the SPIRE colours (S350/S250 and S500/S350) of 250 μm sources, we selected high redshift dusty star-forming galaxies potentially associated with the protoclusters. In the 2QZCluster field, we found a 4σ overdensity of six SPIRE sources around 4.5′ (∼ 2.2 Mpc) from a density peak of Hα emitters at z = 2.2. In the HS1700 field, we found a 5σ overdensity of eight SPIRE sources around 2.1′ (∼ 1.0 Mpc) from a density peak of LBGs at z = 2.3. We did not find any significant overdensities in SSA22 field, but we found three 500 μm sources are concentrated 3′ (∼1.4 Mpc) east to the LAEs overdensity. If all the SPIRE sources in these three overdensities are associated with protoclusters, the inferred star-formation rate densities are 103 − 104 times higher than the average value at the same redshifts. This suggests that dusty star-formation activity could be very strongly enhanced in z ∼ 2 − 3 protoclusters. Further observations are needed to confirm the redshifts of the SPIRE sources and to investigate what processes enhance the dusty star-formation activity in z ∼ 2 − 3 protoclusters.
Citation
Kato, Y., Matsuda, Y., Smail, I., Swinbank, A., Hatsukade, B., Umehata, H., …Hayashino, T. (2016). Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2–3. Monthly Notices of the Royal Astronomical Society, 460(4), 3861-3872. https://doi.org/10.1093/mnras/stw1237
Journal Article Type | Article |
---|---|
Acceptance Date | May 19, 2016 |
Online Publication Date | May 23, 2016 |
Publication Date | Aug 21, 2016 |
Deposit Date | May 31, 2016 |
Publicly Available Date | Jun 15, 2016 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 460 |
Issue | 4 |
Pages | 3861-3872 |
DOI | https://doi.org/10.1093/mnras/stw1237 |
Public URL | https://durham-repository.worktribe.com/output/1380147 |
Related Public URLs | http://adsabs.harvard.edu/abs/2016MNRAS.tmp..901K |
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Copyright Statement
Advance online version This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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