We present the environmental dependence of colour, stellar mass, and star
formation (SF) activity in H-alpha-selected galaxies along the huge cosmic web
at z=0.4 hosting twin clusters in DEEP2-3 field, discovered by Subaru Strategic
Programme of Hyper Suprime-Cam (HSC SSP). By combining photo-z selected
galaxies and H-alpha emitters selected with broad-band and narrow-band data of
the recent internal data release of HSC SSP (DR1), we confirm that galaxies in
higher-density environments or galaxies in the cluster central regions show
redder colours. We find that there still remains a colour-density and
colour-radius correlation even if we restrict the sample to H-alpha-selected
galaxies. We also find an increase of star formation rates (SFR), and possible
decline in specific SFRs, amongst H-alpha emitters towards the highest-density
environment, primarily driven by the excess of red/massive H-alpha emitters in
high-density environment. Finally, we find a hint that pairs of H-alpha
emitters located in higher-density environment show redder colours than those
in underdense regions, implying that galaxy-galaxy interaction in different
environments have different impacts on the properties of SF galaxies.
Description
[1704.05979] The nature of H$\alpha$-selected galaxies along the huge cosmic web at z=0.4 revealed by Subaru Hyper Suprime-Cam survey
%0 Generic
%1 koyama2017nature
%A Koyama, Yusei
%A Hayashi, Masao
%A Tanaka, Masayuki
%A Kodama, Tadayuki
%A Shimakawa, Rhythm
%A Yamamoto, Moegi
%A Nakata, Fumiaki
%A Tanaka, Ichi
%A Suzuki, Tomoko
%A Tadaki, Ken-ichi
%A Nishizawa, Atsushi J.
%A Yabe, Kiyoto
%A Toba, Yoshiki
%A Lin, Lihwai
%A Jian, Hung-Yu
%A Komiyama, Yutaka
%D 2017
%K HSC Ha SSP emission filament overdensity
%T The nature of H$\alpha$-selected galaxies along the huge cosmic web at
z=0.4 revealed by Subaru Hyper Suprime-Cam survey
%U http://arxiv.org/abs/1704.05979
%X We present the environmental dependence of colour, stellar mass, and star
formation (SF) activity in H-alpha-selected galaxies along the huge cosmic web
at z=0.4 hosting twin clusters in DEEP2-3 field, discovered by Subaru Strategic
Programme of Hyper Suprime-Cam (HSC SSP). By combining photo-z selected
galaxies and H-alpha emitters selected with broad-band and narrow-band data of
the recent internal data release of HSC SSP (DR1), we confirm that galaxies in
higher-density environments or galaxies in the cluster central regions show
redder colours. We find that there still remains a colour-density and
colour-radius correlation even if we restrict the sample to H-alpha-selected
galaxies. We also find an increase of star formation rates (SFR), and possible
decline in specific SFRs, amongst H-alpha emitters towards the highest-density
environment, primarily driven by the excess of red/massive H-alpha emitters in
high-density environment. Finally, we find a hint that pairs of H-alpha
emitters located in higher-density environment show redder colours than those
in underdense regions, implying that galaxy-galaxy interaction in different
environments have different impacts on the properties of SF galaxies.
@misc{koyama2017nature,
abstract = {We present the environmental dependence of colour, stellar mass, and star
formation (SF) activity in H-alpha-selected galaxies along the huge cosmic web
at z=0.4 hosting twin clusters in DEEP2-3 field, discovered by Subaru Strategic
Programme of Hyper Suprime-Cam (HSC SSP). By combining photo-z selected
galaxies and H-alpha emitters selected with broad-band and narrow-band data of
the recent internal data release of HSC SSP (DR1), we confirm that galaxies in
higher-density environments or galaxies in the cluster central regions show
redder colours. We find that there still remains a colour-density and
colour-radius correlation even if we restrict the sample to H-alpha-selected
galaxies. We also find an increase of star formation rates (SFR), and possible
decline in specific SFRs, amongst H-alpha emitters towards the highest-density
environment, primarily driven by the excess of red/massive H-alpha emitters in
high-density environment. Finally, we find a hint that pairs of H-alpha
emitters located in higher-density environment show redder colours than those
in underdense regions, implying that galaxy-galaxy interaction in different
environments have different impacts on the properties of SF galaxies.},
added-at = {2017-04-21T10:30:17.000+0200},
author = {Koyama, Yusei and Hayashi, Masao and Tanaka, Masayuki and Kodama, Tadayuki and Shimakawa, Rhythm and Yamamoto, Moegi and Nakata, Fumiaki and Tanaka, Ichi and Suzuki, Tomoko and Tadaki, Ken-ichi and Nishizawa, Atsushi J. and Yabe, Kiyoto and Toba, Yoshiki and Lin, Lihwai and Jian, Hung-Yu and Komiyama, Yutaka},
biburl = {https://www.bibsonomy.org/bibtex/25c493d791d6c812ecc30fb6d97a79d34/miki},
description = {[1704.05979] The nature of H$\alpha$-selected galaxies along the huge cosmic web at z=0.4 revealed by Subaru Hyper Suprime-Cam survey},
interhash = {93467470a0b22cba1f8adfd79cc84468},
intrahash = {5c493d791d6c812ecc30fb6d97a79d34},
keywords = {HSC Ha SSP emission filament overdensity},
note = {cite arxiv:1704.05979Comment: 15 pages, 13 figures, submitted to PASJ for publication in the HSC-SSP special issue},
timestamp = {2017-04-21T10:30:17.000+0200},
title = {The nature of H$\alpha$-selected galaxies along the huge cosmic web at
z=0.4 revealed by Subaru Hyper Suprime-Cam survey},
url = {http://arxiv.org/abs/1704.05979},
year = 2017
}