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SILVERRUSH. II. First catalogs and properties of ∼2000 Lyα emitters and blobs at z ∼ 6–7 identified over the 14–21 deg2 sky*

Authors :
Kimihiko Nakajima
Hisanori Furusawa
Yoshiaki Taniguchi
Haruka Kusakabe
Rieko Momose
Masami Ouchi
Ryo Higuchi
Takatoshi Shibuya
Masakazu A. R. Kobayashi
Yoshiaki Ono
Tohru Nagao
Yutaka Komiyama
Yuichi Harikane
Chien-Hsiu Lee
Akira Konno
Masaru Kajisawa
Tomotsugu Goto
Masayuki Tanaka
Nobunari Kashikawa
Shiang-Yu Wang
Suraphong Yuma
Kazuhiro Shimasaku
Source :
Publications of the Astronomical Society of Japan.
Publication Year :
2017
Publisher :
Oxford University Press (OUP), 2017.

Abstract

We present an unprecedentedly large catalog consisting of 2,230 > L* Lya emitters (LAEs) at z=5.7 and 6.6 on the 13.8 and 21.2 deg2 sky, respectively, that are identified by the SILVERRUSH program with the first narrowband imaging data of the Hyper Suprime-Cam (HSC) survey. We confirm that the LAE catalog is reliable on the basis of 96 LAEs whose spectroscopic redshifts are already determined by this program and the previous studies. This catalogue is also available on-line. Based on this catalogue, we derive the rest-frame Lya equivalent-width distributions of LAEs at z~5.7-6.6 that are reasonably explained by the exponential profiles with the scale lengths of ~120-170A, showing no significant evolution from z~5.7 to z~6.6. We find that 275 LAEs with a large equivalent width (LEW) of >240A are candidates of young-metal poor galaxies and AGNs. We also find that the fraction of LEW LAEs to all ones is 4% and 21% at z~5.7 and z~6.6, respectively. Our LAE catalog includes 11 Lya blobs (LABs) that are LAEs with spatially extended Lya emission whose profile is clearly distinguished from those of stellar objects at the >~ 3sigma level. The number density of the LABs at z=6-7 is ~ 10^-7-10^-6 Mpc^-3, being ~ 10-100 times lower than those claimed for LABs at z~ 2-3, suggestive of disappearing LABs at z>~6, albeit with the different selection methods and criteria for the low and high-z LABs.<br />19 pages, 11 figures. Accepted for publication in PASJ special issue

Details

ISSN :
2053051X and 00046264
Database :
OpenAIRE
Journal :
Publications of the Astronomical Society of Japan
Accession number :
edsair.doi.dedup.....47b67ffd1b04cba897259ab00c88d280
Full Text :
https://doi.org/10.1093/pasj/psx122