TT
Tadafumi Takata
astro-phastro-ph.GAastro-ph.COastro-ph.IMastro-ph.EPastro-ph.SRastro-ph.HE
On Valency
published · living versionsW_7nfkym4z·v1 · currentpublished
Photometric Redshifts for the Hyper Suprime-Cam Subaru Strategic Program Data Release 2
with Atsushi J. Nishizawa, Bau-Ching Hsieh, Masayuki Tanaka
1 version
Preprints & journals
59 papers in the corpus · 1995–2026Opposition effect of comet 28P/Neujmin observed with Subaru Hyper Suprime-Cam2608.11082v1 · Takafumi Ootsubo, Hideyo Kawakita, Tadafumi Takata et al.2026 · 0 citationsarXiv
Quasar Luminosity Function at z = 72305.11225v1 · Yoshiki Matsuoka, Masafusa Onoue, Kazushi Iwasawa et al.2023 · 66 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.02111.12766v1 · Yoshiki Matsuoka, Kazushi Iwasawa, Masafusa Onoue et al.2021 · 61 citationsarXiv
Third Data Release of the Hyper Suprime-Cam Subaru Strategic Program2108.13045v1 · Hiroaki Aihara, Yusra AlSayyad, Makoto Ando et al.2021 · 360 citationsarXiv
Photometric Redshifts for the Hyper Suprime-Cam Subaru Strategic Program Data Release 22003.01511v2 · Atsushi J. Nishizawa, Bau-Ching Hsieh, Masayuki Tanaka et al.2020 · 13 citationsarXivon Valency
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 z 7.01908.07910v1 · Yoshiki Matsuoka, Kazushi Iwasawa, Masafusa Onoue et al.2019 · 128 citationsApJ 883:183, 2019
Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program1905.12221v2 · Hiroaki Aihara, Yusra AlSayyad, Makoto Ando et al.2019 · 515 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IV. Discovery of 41 Quasars and Luminous Galaxies at 5.7 < z < 6.91803.01861v2 · Y. Matsuoka, K. Iwasawa, M. Onoue et al.2018 · 132 citationsApJS 237 (2018) 5
Deep Optical Imaging of the COSMOS Field with Hyper Suprime-Cam Using Data from the Subaru Strategic Program and the University of Hawaii1706.00566v1 · Masayuki Tanaka, Guenther Hasinger, John D. Silverman et al.2017 · 10 citationsarXiv
The Hyper Suprime-Cam Software Pipeline1705.06766v1 · James Bosch, Robert Armstrong, Steven Bickerton et al.2017 · 551 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 Quasars and Luminous Galaxies at 5.7 < z < 6.81704.05854v3 · Yoshiki Matsuoka, Masafusa Onoue, Nobunari Kashikawa et al.2017 · 140 citationsPASJ 70 (2018) 35
The Hyper Suprime-Cam SSP Survey: Overview and Survey Design1704.05858v3 · H. Aihara, N. Arimoto, R. Armstrong et al.2017 · 1,161 citationsPublications of the Astronomical Society of Japan, Volume 70, Issue SP1, S4 (2018)
First Data Release of the Hyper Suprime-Cam Subaru Strategic Program1702.08449v2 · Hiroaki Aihara, Robert Armstrong, Steven Bickerton et al.2017 · 647 citationsarXiv
Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at 5.7 < z < 6.91603.02281v3 · Yoshiki Matsuoka, Masafusa Onoue, Nobunari Kashikawa et al.2016 · 228 citationsApJ 828 (2016) 26
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 Data1511.07873v3 · Yuichi Harikane, Masami Ouchi, Yoshiaki Ono et al.2015 · 134 citationsarXiv
Hyper-luminous Dust Obscured Galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE1506.00320v1 · Yoshiki Toba, Tohru Nagao, Michael A. Strauss et al.2015 · 55 citationsarXiv
AzTEC/ASTE 1.1 mm survey of SSA22: Counterpart identification and photometric redshift survey of submillimeter galaxies1403.2725v1 · H. Umehata, Y. Tamura, K. Kohno et al.2014 · 60 citationsarXiv
The Galaxy Luminosity Functions down to M_R=-10 in the Coma Cluster1205.5366v1 · Hitomi Yamanoi, Yutaka Komiyama, Masafumi Yagi et al.2012 · 24 citationsarXiv
The Mass-Dependent Clustering History of K-selected Galaxies at z < 4 in the SXDS/UDS Field1101.1566v1 · Junko Furusawa, Kazuhiro Sekiguchi, Tadafumi Takata et al.2011 · 21 citationsarXiv
Submillimeter Array Identification of the Millimeter-Selected Galaxy SSA22-AzTEC1: A Protoquasar in a Protocluster?1010.1267v1 · Y. Tamura, D. Iono, D. J. Wilner et al.2010 · 46 citationsarXiv
Detection of an ultra-bright submillimeter galaxy in the Subaru/XMM-Newton Deep Field using AzTEC/ASTE1009.1455v2 · S. Ikarashi, K. Kohno, J. E. Aguirre et al.2010 · 52 citationsarXiv
Suzaku Observations of the Merging Cluster Abell 85: Temperature Map and Impact Direction1006.4328v1 · Nobuhiro Tanaka, Akihiro Furuzawa, Shigeru J. Miyoshi et al.2010 · 12 citationsPublications of the Astronomical Society of Japan, 2010, Vol. 62 pp. 743-754
"Dark" GRB 080325 in a Dusty Massive Galaxy at z ~ 21003.3717v2 · T. Hashimoto, K. Ohta, K. Aoki et al.2010 · 34 citationsarXiv
Early Science Result from the Japanese Virtual Observatory: AGN and Galaxy Clustering at z = 0.3 to 3.00907.5380v3 · Yuji Shirasaki, Masahiro Tanaka, Masatoshi Ohishi et al.2009 · 14 citationsarXiv
Spatial correlation between submillimetre and Lyman-alpha galaxies in the SSA 22 protocluster.19424150 · Tamura, Yoichi, Kohno, Kotaro, Nakanishi, Kouichiro et al.2009 · 113 citationsNature. 2009;459(7243):61-3
The SCUBA HAlf Degree Extragalactic Survey (SHADES) - VII. Optical/IR photometry and stellar masses of sub-millimeter galaxies0802.0497v1 · Simon Dye, S. A. Eales, I. Aretxaga et al.2008 · 95 citationsarXiv
Asphericity in supernova explosions from late-time spectroscopy.18239091 · Maeda, Keiichi, Kawabata, Koji, Mazzali, Paolo A et al.2008 · 248 citationsScience (New York, N.Y.). 2008;319(5867):1220-3
The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs0801.4017v1 · H. Furusawa, G. Kosugi, M. Akiyama et al.2008 · 316 citationsarXiv
The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- V. Submillimetre properties of near-infrared--selected galaxies in the Subaru/XMM--Newton deep field0708.0845v1 · T. Takagi, A. M. J. Mortier, K. Shimasaku et al.2007 · 23 citationsarXiv
The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN0707.3161v3 · Masami Ouchi, Kazuhiro Shimasaku, Masayuki Akiyama et al.2007 · 581 citationsarXiv
Radio imaging of the Subaru/XMM-Newton Deep Field - I. The 100-microJy catalogue, optical identifications, and the nature of the faint radio source populationastro-ph/0609529v1 · Chris Simpson, Alejo Martinez-Sansigre, Steve Rawlings et al.2006 · 194 citationsMon.Not.Roy.Astron.Soc.372:741-757,2006
Restframe Optical Spectroscopic Classifications for Submillimeter Galaxiesastro-ph/0607580v1 · Tadafumi Takata, Kazuhiro Sekiguchi, Ian Smail et al.2006 · 80 citationsAstrophys.J.651:713-727,2006
Low- and Medium-Dispersion Spectropolarimetry of Nova V475 Sct (Nova Scuti 2003): Discovery of an Asymmetric High-Velocity Wind in a Moderately Fast Novaastro-ph/0604341v1 · Koji S. Kawabata, Youichi Ohyama, Noboru Ebizuka et al.2006 · 10 citationsAstron.J.132:433-442,2006
An optical spectrum of the afterglow of a gamma-ray burst at a redshift of z = 6.295.16525466 · Kawai, N, Kosugi, G, Aoki, K et al.2006 · 267 citationsNature. 2006;440(7081):184-6
XMM-Newton 13H Deep field - I. X-ray sourcesastro-ph/0507408v1 · N. S. Loaring, T. Dwelly, M. J. Page et al.2005 · 28 citationsMon.Not.Roy.Astron.Soc.362:1371-1395,2005
The Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift 6astro-ph/0412648v1 · M. Ouchi, K. Shimasaku, M. Akiyama et al.2004 · 227 citationsAstrophys.J.620:L1-L4,2005
Nature of a Strongly-Lensed Submillimeter Galaxy SMM J14011+0252astro-ph/0411048v1 · K. Motohara, T. Takata, F. Iwamuro et al.2004 · 11 citationsarXiv
Dusty ERO Search behind Two Massive Clustersastro-ph/0308064v1 · Tadafumi Takata, Nobunari Kashikawa, Kouichiro Nakanishi et al.2003 · 23 citationsarXiv
Superwind-driven Intense H Emission in NGC 6240 II: Detailed Comparison of Kinematical and Morphological Structures of the Warm and Cold Molecular Gasastro-ph/0307517v1 · Youichi Ohyama, NAOJ, Michitoshi Yoshida et al.2003 · 21 citationsarXiv
On The Spectrum and Spectropolarimetry of Type Ic Hypernova SN 2003dh/GRB 030329astro-ph/0306155v2 · K. S. Kawabata, J. Deng, L. Wang et al.2003 · 114 citationsAstrophys.J. 593 (2003) L19-L22
On the Origin of Lyman- Blobs at High Redshift: Kinematic Evidence for a Hyperwind Galaxy at z = 3.1astro-ph/0305028v1 · Y. Ohyama, Y. Taniguchi, K. S. Kawabata et al.2003 · 60 citationsAstrophys.J. 591 (2003) L9-L12
A Vigorous Starburst in the SCUBA Galaxy N2 850.4astro-ph/0303128v1 · Ian Smail, S.C. Chapman, R.J. Ivison et al.2003 · 65 citationsMon.Not.Roy.Astron.Soc. 342 (2003) 1185
A medium deep Chandra and Subaru survey of the 13hr XMM/ROSAT deep survey areaastro-ph/0302553v1 · I. M. McHardy, K. F. Gunn, A. M. Newsam et al.2003 · 22 citationsMon.Not.Roy.Astron.Soc. 342 (2003) 802
X-ray and optical properties of X-ray sources in the 13hr XMM-Newton/Chandra deep surveyastro-ph/0212035v1 · M.J. Page (MSSL), I.M. McHardy (Southampton), K.F. Gunn (Southampton) et al.2002 · 24 citationsarXiv
Radio observations of the XMM-Newton/Chandra 13hr deep survey fieldastro-ph/0212036v1 · K. F. Gunn, I. M. McHardy, N. Seymour et al.2002 · 5 citationsarXiv
Evolution of Elliptical Galaxies at z >~ 1 Revealed from a Large, Multicolor Sample of Extremely Red Objectsastro-ph/0210509v1 · M. Miyazaki, K. Shimasaku, T. Kodama et al.2002 · 41 citationsarXiv
Decomposition of the Superwind in M82astro-ph/0209442v1 · Youichi Ohyama, Yoshiaki Taniguchi, Masanori Iye et al.2002 · 77 citationsarXiv
Subaru Deep Survey III. Evolution of Rest-Frame Luminosity Functions Based on the Photometric Redshifts for A K'-band Selected Galaxy Sampleastro-ph/0209445v2 · Nobunari Kashikawa, Tadafumi Takata, Youichi Ohyama et al.2002 · 60 citationsAstron.J. 125 (2003) 53
A New High-Redshift Lyman alpha Emitter: Possible Superwind Galaxy at z = 5.69astro-ph/0207303v2 · M. Ajiki, Y. Taniguchi, T. Murayama et al.2002 · 68 citationsAstrophys.J. 576 (2002) L25-L28
Optical Spectropolarimetry of SN 2002ap: High Velocity Asymmetric Explosionastro-ph/0205414v3 · K.S. Kawabata, D.J. Jeffery, M. Iye et al.2002 · 91 citationsAstrophys.J. 580 (2002) L39-L42
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