Hyper Suprime-Cam Year 3 results: Measurements of clustering of SDSS-BOSS galaxies, galaxy-galaxy lensing, and cosmic shear

被引:13
|
作者
More, Surhud [1 ,2 ]
Sugiyama, Sunao [2 ,3 ]
Miyatake, Hironao [2 ,4 ,5 ]
Rau, Markus Michael [6 ,7 ]
Shirasaki, Masato [8 ,9 ]
Li, Xiangchong [2 ,7 ]
Nishizawa, Atsushi J. [10 ,11 ]
Osato, Ken [12 ,13 ]
Zhang, Tianqing [7 ]
Takada, Masahiro [2 ]
Hamana, Takashi [14 ]
Takahashi, Ryuichi [15 ]
Dalal, Roohi [16 ]
Mandelbaum, Rachel
Strauss, Michael A. [16 ]
Kobayashi, Yosuke [2 ,17 ]
Nishimichi, Takahiro [2 ,18 ,19 ]
Oguri, Masamune [12 ,13 ]
Luo, Wentao [20 ,21 ]
Kannawadi, Arun [16 ]
Hsieh, Bau-Ching [22 ]
Armstrong, Robert [23 ]
Bosch, James [16 ]
Komiyama, Yutaka [24 ]
Lupton, Robert H. [16 ]
Lust, Nate B. [16 ]
MacArthur, Lauren A. [16 ]
Miyazaki, Satoshi [25 ]
Murayama, Hitoshi [2 ,26 ,27 ]
Okura, Yuki [14 ]
Price, Paul A. [16 ]
Tait, Philip J. [25 ]
Tanaka, Masayuki [14 ]
Wang, Shiang-Yu [22 ]
机构
[1] Interuniv Ctr Astron & Astrophys, Post Bag 4, Pune 411007, Maharashtra, India
[2] Univ Tokyo, Univ Tokyo Inst Adv Study UTIAS, Kavli Inst Phys & Math Univ WPI, Chiba 2778583, Japan
[3] Univ Tokyo, Dept Phys, Bunkyo, Tokyo 1130031, Japan
[4] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi 4648602, Japan
[5] Nagoya Univ, Inst Adv Res, Nagoya, Aichi 4648601, Japan
[6] Argonne Natl Lab, Div High Energy Phys, Lemont, IL 60439 USA
[7] Carnegie Mellon Univ, Dept Phys, McWilliams Ctr Cosmol, Pittsburgh, PA 15213 USA
[8] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
[9] Inst Stat Math, Tachikawa, Tokyo 1908562, Japan
[10] Gifu Shotoku Gakuen Univ, Gifu 5016194, Japan
[11] Nagoya Univ, Kobayashi Maskawa Inst, Inst Adv Res, Nagoya, Aichi 4648602, Japan
[12] Chiba Univ, Ctr Frontier Sci, Chiba 2638522, Japan
[13] Chiba Univ, Grad Sch Sci, Dept Phys, Chiba 2638522, Japan
[14] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
[15] Hirosaki Univ, Fac Sci & Technol, 3 Bunkyo Cho, Hirosaki, Aomori 0368561, Japan
[16] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[17] Univ Arizona, Steward Observ, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA
[18] Kyoto Univ, Yukawa Inst Theoret Phys, Ctr Gravitat Phys & Quantum Informat, Kyoto 6068502, Japan
[19] Kyoto Sangyo Univ, Dept Astrophys & Atmospher Sci, Fac Sci, Kita Ku, Kyoto 6038555, Japan
[20] Univ Sci & Technol China, Sch Phys Sci, Hefei 230026, Anhui, Peoples R China
[21] Univ Sci & Technol China, Sch Astron & Space Sci, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
[22] Acad Sinica, Inst Astron & Astrophys, 1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan
[23] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA
[24] Hosei Univ, Dept Adv Sci, Fac Sci & Engn, 3-7-2 Kajino Cho, Koganei, Tokyo 1848584, Japan
[25] Natl Astron Observ Japan, Subaru Telescope, 650 N Aohoku Pl, Hilo, HI 96720 USA
[26] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA
[27] Lawrence Berkeley Natl Lab, Theory Grp, Berkeley, CA 94720 USA
基金
日本科学技术振兴机构; 美国国家航空航天局; 美国国家科学基金会; 日本学术振兴会; 国家重点研发计划;
关键词
OSCILLATION SPECTROSCOPIC SURVEY; DIGITAL SKY SURVEY; BARYON ACOUSTIC-OSCILLATIONS; COSMOLOGICAL CONSTRAINTS; DATA RELEASE; 1ST DATA; COMBINATION; CALIBRATION; CATALOG; SIGNAL;
D O I
10.1103/PhysRevD.108.123520
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We utilize the Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey (SDSS-BOSS) galaxies and its overlap with approximately 416 sq degrees of deep grizy-band imaging from the Subaru Hyper Suprime-Cam Survey (HSC). We perform measurements of three two-point correlations which form the basis of the cosmological inference presented in our companion papers, Miyatake et al. and Sugiyama et al. We use three approximately volume limited subsamples of spectroscopic galaxies by their i-band magnitude from the SDSS-BOSS: LOWZ (0.1 < z < 0.35), CMASS1 (0.43 < z < 0.55) and CMASS2 (0.55 < z < 0.7), respectively. We present high signal-to-noise ratio measurements of the projected correlation functions of these galaxies, which is expected to be proportional to the projected matter correlation function on large scales with a proportionality constant dependent on the bias of galaxies. In order to help break the degeneracy between the amplitude of the matter correlation and the bias of these spectroscopic galaxies, we use the distortions of the shapes of fainter galaxies in HSC due to weak gravitational lensing, to measure the galaxy-galaxy lensing signal, which probes the projected galaxy-matter cross-correlation function of the SDSS-BOSS galaxies. We also measure the cosmic shear correlation functions from HSC galaxies which is related to the projected matter correlation function. We demonstrate the robustness of our measurements by subjecting each of them to a variety of systematic tests. Our use of a single sample of HSC source galaxies is crucial to calibrate any residual systematic biases in the inferred redshifts of our galaxies. We also describe the construction of a suite of mocks: (i) spectroscopic galaxy catalogs which obey the clustering and abundance of each of the three SDSS-BOSS subsamples, and (ii) galaxy shape catalogs which obey the footprint of the HSC survey and have been appropriately sheared by the large-scale structure expected in a Lambda Cold Dark Matter model. We use these mock catalogs to compute the covariance of each of our observables.
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页数:32
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