papers
Publications (13)
astro-ph.GA2014
The Subaru high-z quasar survey: discovery of faint z~6 quasars
Nobunari Kashikawa, Yoshifumi Ishizaki, Chris J. Willott +9
astro-ph.GA2016
The very wide-field $gzK$ galaxy survey -- II. The relationship between star-forming galaxies at $z \sim 2$ and their host haloes based upon HOD modelling
Shogo Ishikawa, Nobunari Kashikawa, Takashi Hamana +2
astro-ph.CO2011
Completing the Census of Ly-alpha Emitters at the Reionization Epoch
Nobunari Kashikawa, Kazuhiro Shimasaku, Yuichi Matsuda +16
astro-ph.GA2016
A Systematic Survey of Protoclusters at $z\sim3\mathrm{-}6$ in the CFHTLS Deep Fields
Jun Toshikawa, Nobunari Kashikawa, Roderik Overzier +8
astro-ph.GA2016
The very wide-field $gzK$ galaxy survey -- I. Details of the clustering properties of star-forming galaxies at $z \sim 2$
Shogo Ishikawa, Nobunari Kashikawa, Jun Toshikawa +1
astro-ph.GA2014
A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protocluster at $z=6.01$
Jun Toshikawa, Nobunari Kashikawa, Roderik Overzier +8
astro-ph.CO2012
A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?
Nobunari Kashikawa, Tohru Nagao, Jun Toshikawa +13
astro-ph.HE2017
The redshift selected sample of long gamma-ray burst host galaxies: the overall metallicity distribution at $z < 0.4$
Yuu Niino, Kentaro Aoki, Tetsuya Hashimoto +7
astro-ph.GA2017
The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
Shogo Ishikawa, Nobunari Kashikawa, Jun Toshikawa +5
astro-ph.CO2012
Discovery of a protocluster at z~6
Jun Toshikawa, Nobunari Kashikawa, Kazuaki Ota +10
astro-ph.CO2013
Extended Lyman-alpha emission from a high-z DLA at z=3.115
Nobunari Kashikawa, Toru Misawa, Yosuke Minowa +5
astro-ph.GA2017
A New Constraint on Reionization from Evolution of the Ly$α$ Luminosity Function at $z\sim6-7$ Probed by a Deep Census of $z=7.0$ Ly$α$ Emitter Candidates to 0.3 $L^*$
Kazuaki Ota, Masanori Iye, Nobunari Kashikawa +10
astro-ph.GA2016
Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
Yuichi Harikane, Masami Ouchi, Yoshiaki Ono +15