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3 Hyper Suprime-Cam Hyper Subaru Prime-focus Camera 104 CCDs 3
4 HSC SupCam z = 1, 2, 7 HST 8Mpc 4
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9 Wide-field imaging with Hyper Suprime-Cam: Cosmology and Galaxy Evolution A Strategic Survey Proposal for the Subaru Telescope PI: Satoshi Miyazaki (NAOJ) Co-PI: Ikuru Iwata (NAOJ) The HSC collaboration team 1 : S. Abe (1), H. Aihara (2),(3), M. Akiyama (4), K. Aoki (5), N. Arimoto (5), N. A. Bahcall (6), S. J. Bickerton (3), J. Bosch (6),K.Bundy (3),C.W.Chen (7),M.Chiba (4),T.Chiba (8), N. E. Chisari (6), J. Coupon (7),M. Doi (2), M. Enoki (9) S. Foucaud (10), M. Fukugita (3),H.Furusawa (5), T. Futamase (4), R. Goto (2), T. Goto (11),J.E.Greene (6), J. E. Gunn (6), T. Hamana (5), T. Hashimoto (2), M. Hayashi (5), Y. Higuchi (2),(5), C. Hikage (12),J.C.Hill (6),P.T.P.Ho (7), B. C. Hsieh (7), K. Y. Huang (7), H. Ikeda (13), M. Imanishi (5), N. Inada (14), A. K. Inoue (15), W.-H. Ip (1), T. Ito (5), K. Iwasawa (16),M.Iye (5), H. Y. Jian (17), Y. Kakazu (18), H. Karoji (3), N. Kashikawa (5), N. Katayama (3), T. Kawaguchi (19),S. Kawanomoto (5),I.Kayo (20), T. Kitayama (20), G. R. Knapp (6), T. Kodama (5), K. Kohno (2), M. Koike (5), E. Kokubo (5),M. Kokubo (2), Y. Komiyama (5), A. Konno (2), Y. Koyama (5), C. N. Lackner (3), D. Lang (6), A. Leauthaud (3),M.J.Lehner (7),K.- Y. Lin (7),L.Lin (7),Y.-T.Lin (7), C. P. Loomis (6), R. H. Lupton (6),P.S.Lykawka (21), K. Maeda (3), R. Mandelbaum (22),Y. Matsuda (5), K. Matsuoka (13),(23), Y. Matsuoka (12),S.Mineo (2), T. Minezaki (2), H. Miyatake (6), R. Momose (2), A. More (3),S. More (3), T. J. Moriya (3), T. Morokuma (2), H. Murayama (3), K. Nagamine (24), T. Nagao (23), S. Nagataki (23), Y. Naito (2),K. Nakajima (2), F. Nakata (5), H. Nakaya (5), T. Namikawa (2), C.-C. Ngeow (1),T.Nishimichi (3), H. Nishioka (7),A.J.Nishizawa (3), K. Nomoto (3), M. Oguri (3),A.Oka (2), N. Okabe (7), S. Okamoto (25), S. Okamura (26),J.Okumura (23),S.Okumura (27),Y. Okura (5),Y.Ono (2) M. Onodera (28),K.Ota (23),M.Ouchi (2), S. Oyabu (12),P.A.Price (6),R.Quimby (3),C.E.Rusu (2),(5),S. Saito (29), T. Saito (3), Y. Saitou (30), M. Sato (12),T.Shibuya (5), K. Shimasaku (2), A. Shimono (3), S. Shinogi (2), M. Shirasaki (2), J. D. Silverman (3), D. N. Spergel (6),(3), M. A. Strauss (6), H. Sugai (3), N. Sugiyama (12),(3),D.Suto (2),Y.Suto (2), K. Tadaki (2), M. Takada (3), R. Takahashi (31), S. Takahashi (5), T. Takata (5), T. T. Takeuchi (12), N. Tamura (3), M. Tanaka (5), M. Tanaka (3), M. Tanaka (4), Y. Taniguchi (13), A. Taruya (2), T. Terai (5), Y. Terashima (13), N. Tominaga (32), J. Toshikawa (30), T. Totani (23), M. Tsai (1),E.L.Turner (6),Y.Ueda (23),K.Umetsu (7), Y. Urata (1),Y.Utsumi (5), B. Vulcani (3), K. Wada (33), S.-Y. Wang (7), W.-H. Wang (7), T. Yamada (4), Y. Yamada (5), K. Yamamoto (34), H. Yamanoi (5), C.-H. Yan (7), N. Yasuda (3), A. Yonehara (35), F. Yoshida (5), N. Yoshida (2), M. Yoshikawa (36),S.Yuma (2) (1) NCU, Taiwan (2) Tokyo (3) Kavli IPMU (4) Tohoku (5) NAOJ (6) Princeton (7) ASIAA (8) Nihon (9) Tokyo Keizai (10) NTNU, Taiwan (11) DARK, Copenhagen (12) Nagoya (13) Ehime (14) NNCT (15) Osaka Sangyo (16) Barcelona (17) NTU, Taiwan (18) Chicago (19) Tsukuba (20) Toho (21) Kinki (22) CMU (23) Kyoto (24) Las Vegas (25) KIAA, China (26) Hosei (27) JSGA (28) ETH (29) Berkeley (30) GUAS (31) Hirosaki (32) Konan (33) Kagoshima (34) Hiroshima (35) Kyoto Sangyo (36) JAXA 9
10 Layer Area # of Filters & Depth Comoving volume Key Science [deg 2 ] HSC fields [h 3 Gpc 3 ] Wide grizy (r 26) 4.4(z < 2) WL cosmology, z 1 gals, clusters Deep grizy+3nbs (r 27) 0.5(1<z<5) z < 2 gals, reionization, WL calib. Ultradeep grizy+3nbs (r 28) 0.07 (2 <z<7) z > 2 gals, reionization, SNeIa HSC-UD HSC-D HSC-Wide Figure 1: Left: The limiting magnitudes (in r) and solid angl 10
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12 z(lyα) NB NB g r i z y NB NB es of the HSC-Wide, Deep and Ultradeep (UD) laye 12
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18 Galaxy evolution at z<2 Relationship between galaxies and dark haloes Physics of growth, quenching, and mass assembly Galaxy evolution in clusters of galaxies Galaxy evolution at z>2 Relationship between galaxies and dark haloes Nature of LAEs and LABs Quasars and AGNs (SMBHs, dark haloes, environments, host gals) Cosmic reionization Epoch and topology Sources 18
19 z>2 z<2 Behroozi+13 19
20 gure 10: Left: Expected measurements of the Lyα LFs at z = 5.7 (blue), 6.6 (green), and 7.3 (red) with the tradeep and Deep layer data. The existing Suprime-Cam measurements at z = 7.3 go very deep, although over very small area. The open circles are the current best measurements given by Suprime-Cam observations. The crease in the LF with increasing redshift is interpreted as due to the onset of reionization. Right: Expected F ω(θ) ofz =6.6LAEs from the Deep layer in the case of full ionization, assuming that they are hosted by halo = M halos (red dots). The solid curves indicate the ACFs of LAEs with M halo = M x HI =0, 0.3, 0.5, 0.8 taken from McQuinn et al. (2007) simulations of inhomogeneous reionization. The black uares are the best estimates of the z =6.6 LAE ACF available to date (Ouchi et al. 2010). Our accurate ACF asurements over a range of a factor of 30 in θ will allow us to detect the difference in the ACF shape between the l and partial ionization cases and to constrain x HI with an uncertainty of
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23 Log in to hscsurvey.pbworks.com This wiki is a private wiki for HSC SSP survey. Researchers in Japan/Taiwan/Princeton are eligible for membership. When you request access, please use an institutional for verification, and write your name and affiliation in the Message box. /username Password Remember me Log in Forgot your password? Not a member? Request access To get in touch Contact the workspace owner 23
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26 z<2 HSC-Wide HSC-Deep z 0.65 (kpc) Vol (Gpc 3 ) logm lim N gal Vol (Gpc 3 ) logm lim N gal M k M k M k M k M k M k k k k k z>2 26
LAE で探る z~5 での AGN 環境と 周辺銀河へのフィードバック Based on Kikuta et al. in prep. 初代星 初代銀河研究会, Oct 25th Satoshi KIKUTA (SOKENDAI/NAOJ, M2) Collaborators: Masatoshi
LAE で探る z~5 での AGN 環境と 周辺銀河へのフィードバック Based on Kikuta et al. in prep., Oct 25th Satoshi KIKUTA (SOKENDAI/NAOJ, M2) Collaborators: Masatoshi Imanishi, Kazuhiro Shimasaku, Fumiaki Nakata, Yoshiki Matsuoka
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μ μ DMR-BZT700 DMR-BZT600 μ TM VQT3C03-2B ! ! l l l [HDD] [BD-RE] [BD-R] [DVD-V] [BD-V] [RAM] [CD] [SD] [-R] [USB] [-RW] [RAM AVCREC ] [-R AVCREC ] [RAM VR ][-R VR ] [-RW VR ] [-R V ] [-RW V ] [DVD-V]
Z7000操作編_本文.indb
2 8 17 37Z700042Z7000 46Z7000 28 42 52 61 72 87 2 3 12 13 6 7 3 4 11 21 34 61 8 17 4 11 4 53 12 12 10 75 18 12 42 42 13 30 42 42 42 42 10 62 66 44 55 14 25 9 62 65 23 72 23 19 24 42 8 26 8 9 9 4 11 18
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VQT3B82-1 DMP-BDT110 μ μ μ 2 VQT3B82 ÇÕÇ¹Ç Ç +- VQT3B82 3 4 VQT3B82 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 ij SD 1 2 3 4 5 6 7 8 Í VQT3B82 5 BD DVD CD SD USB 6 VQT3B82 2 ALL 1 2 4 VQT3B82 7
6 4 4 9RERE6RE 5 5 6 7 8 9 4 5 6 4 4 5 6 8 4 46 5 7 54 58 60 6 69 7 8 0 9 9 79 0 4 0 0 4 4 60 6 9 4 6 46 5 4 4 5 4 4 7 44 44 6 44 8 44 46 44 44 4 44 0 4 4 5 4 8 6 0 4 0 4 4 5 45 4 5 50 4 58 60 57 54
C FGIH C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C
TUDSR5SET TUDSR5 C 7 8 9 ch DIGITAL CS TUNER C C C C S-A C FGIH C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C C