Hyper Suprime-Cam Year 3 results: Cosmology from galaxy clustering and weak lensing with HSC and SDSS using the minimal bias model

被引：26

作者：

Sugiyama, Sunao ^{[1
,2
]}

Miyatake, Hironao ^{[1
,3
,4
]}

More, Surhud ^{[1
,5
]}

Li, Xiangchong ^{[1
,6
]}

Shirasaki, Masato ^{[7
,8
]}

Takada, Masahiro ^{[1
]}

Kobayashi, Yosuke ^{[1
,9
]}

Takahashi, Ryuichi ^{[10
]}

Nishimichi, Takahiro ^{[1
,11
,12
]}

Nishizawa, Atsushi J. ^{[13
,14
]}

Rau, Markus M. ^{[6
,15
]}

Zhang, Tianqing ^{[6
]}

Dalal, Roohi ^{[16
]}

Mandelbaum, Rachel ^{[6
]}

Strauss, Michael A. ^{[16
]}

Hamana, Takashi ^{[17
]}

Oguri, Masamune ^{[1
,2
,18
,19
]}

Osato, Ken ^{[20
,21
]}

Kannawadi, Arun ^{[16
]}

Hsieh, Bau-Ching ^{[22
]}

Luo, Wentao ^{[23
,24
]}

Armstrong, Robert ^{[25
]}

Bosch, James ^{[16
]}

Komiyama, Yutaka ^{[26
]}

Lupton, Robert H. ^{[16
]}

Lust, Nate B. ^{[16
]}

Miyazaki, Satoshi ^{[27
]}

Murayama, Hitoshi ^{[1
,28
,29
]}

Okura, Yuki ^{[17
]}

Price, Paul A. ^{[16
]}

Tait, Philip J. ^{[27
]}

Tanaka, Masayuki ^{[17
]}

Wang, Shiang-Yu ^{[22
]}

机构：

[1] Univ Tokyo, Univ Tokyo Inst Adv Study UTIAS, Kavli Inst Phys & Math Universe WPI, Chiba 2778583, Japan

[2] Univ Tokyo, Dept Phys, Bunkyo, Tokyo 1130031, Japan

[3] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi 4648602, Japan

[4] Nagoya Univ, Inst Adv Res, Nagoya, Aichi 4648601, Japan

[5] Interuniv Ctr Astron & Astrophys, Post Bag 4, Pune 411007, Maharashtra, India

[6] Carnegie Mellon Univ, Dept Phys, McWilliams Ctr Cosmol, Pittsburgh, PA 15213 USA

[7] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

[8] Inst Stat Math, Tachikawa, Tokyo 1908562, Japan

[9] Univ Arizona, Steward Observ, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA

[10] Hirosaki Univ, Fac Sci & Technol, 3 Bunkyo Cho, Hirosaki, Aomori 0368561, Japan

[11] Kyoto Univ, Yukawa Inst Theoret Phys, Ctr Gravitat Phys & Quantum Informat, Kyoto 6068502, Japan

[12] Kyoto Sangyo Univ, Fac Sci, Dept Astrophys & Atmospher Sci, Kita Ku, Kyoto 6038555, Japan

[13] Gifu Shotoku Gakuen Univ, Gifu 5016194, Japan

[14] Nagoya Univ, Kobayashi Maskawa Inst, Inst Adv Res, Nagoya, Aichi 4648602, Japan

[15] Argonne Natl Lab, Div High Energy Phys, Lemont, IL 60439 USA

[16] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[17] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

[18] Chiba Univ, Ctr Frontier Sci, 1-33 Yayoi Cho,Inage Ku, Chiba 2638522, Japan

[19] Univ Tokyo, Res Ctr Early Universe, Bunkyo, Tokyo 1130031, Japan

[20] Chiba Univ, Ctr Frontier Sci, Chiba 2638522, Japan

[21] Chiba Univ, Grad Sch Sci, Dept Phys, Chiba 2638522, Japan

[22] Acad Sinica, Inst Astron & Astrophys, 1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan

[23] Univ Sci & Technol China, Sch Phys Sci, Hefei 230026, Anhui, Peoples R China

[24] Univ Sci & Technol China, Sch Astron & Space Sci, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China

[25] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA

[26] Hosei Univ, Fac Sci & Engn, Dept Adv Sci, 3-7-2 Kajino Cho, Koganei, Tokyo 1848584, Japan

[27] Natl Astron Observ Japan, Subaru Telescope, 650 N Aohoku Pl, Hilo, HI 96720 USA

[28] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA

[29] Lawrence Berkeley Natl Lab, Theory Grp, Berkeley, CA 94720 USA

来源：

PHYSICAL REVIEW D | 2023年 / 108卷 / 12期

基金：

日本科学技术振兴机构; 美国国家科学基金会; 美国国家航空航天局; 日本学术振兴会;

关键词：

DIGITAL SKY SURVEY; LARGE-SCALE STRUCTURE; DATA RELEASE; INTRINSIC ALIGNMENTS; SYSTEMATIC-ERRORS; SHEAR CALIBRATION; POWER SPECTRA; CONSTRAINTS; SIMULATIONS; COVARIANCE;

D O I：

10.1103/PhysRevD.108.123521

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present cosmological parameter constraints from a blind joint analysis of three two-point correlation functions measured from the Year 3 Hyper Suprime-Cam (HSC-Y3) imaging data, covering about 416 deg(2), and the SDSS DR11 spectroscopic galaxies spanning the redshift range [0.15, 0.70]. We subdivide the SDSS galaxies into three luminosity-cut, and therefore nearly volume-limited samples separated in redshift, each of which acts as a large-scale structure tracer characterized by the measurement of the projected correlation function, w(p)(R). We also use the measurements of the galaxy-galaxy weak-lensing signal Delta Sigma(R) for each of these SDSS samples which act as lenses for a secure sample of source galaxies selected from the HSC-Y3 shape catalog based on their photometric redshifts. We combine these measurements with the cosmic shear correlation functions, xi(+/-)(theta) measured for our HSC source sample. We model these observables with the minimal bias model of the galaxy clustering observables in the context of a flat Lambda CDM cosmology. We use conservative scale cuts, R > 12 and 8h(-1) Mpc for Delta Sigma and w(p), respectively, where the minimal bias model is valid, in addition to conservative prior on the residual bias in the mean redshift of the HSC photometric source galaxies. We present various validation tests of our model as well as analysis methods. Our baseline analysis yields S-8 = 0.775(-0.038)(+0.043) (68% C.I.) for the.CDM model, after marginalizing over uncertainties in other parameters. Our value of S-8 is consistent with that from the Planck 2018 data, but the credible interval of our result is still relatively large. We show that various internal consistency tests based on different splits of the data are passed. Our results are statistically consistent with those of a companion paper, which extends this analysis to smaller scales with an emulator-based halo model, using Delta Sigma(R) and w(p)(R) down to R > 3 and 2h(-1) Mpc, respectively.

引用

页数：31

共 42 条

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