Hyper Suprime-Cam Year 3 results: Cosmology from cosmic shear two-point correlation functions Article Swipe
Xiangchong Li
,
Tianqing Zhang
,
Sunao Sugiyama
,
Roohi Dalal
,
Ryo Terasawa
,
Markus Michael Rau
,
Rachel Mandelbaum
,
Masahiro Takada
,
Surhud More
,
Michael A. Strauss
,
Hironao Miyatake
,
Masato Shirasaki
,
Takashi Hamana
,
Masamune Oguri
,
Wentao Luo
,
Atsushi J. Nishizawa
,
Ryuichi Takahashi
,
Andrina Nicola
,
Ken Osato
,
Arun Kannawadi
,
Tomomi Sunayama
,
R. Armstrong
,
James Bosch
,
Yutaka Komiyama
,
Robert H. Lupton
,
Nate B. Lust
,
Lauren A. MacArthur
,
Satoshi Miyazaki
,
Hitoshi Murayama
,
Takahiro Nishimichi
,
Yuki Okura
,
P. A. Price
,
Philip J. Tait
,
Masayuki Tanaka
,
Shiang‐Yu Wang
·
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.1103/physrevd.108.123518
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.1103/physrevd.108.123518
Here, we perform a blinded cosmology analysis with cosmic shear two-point correlation functions measured from more than 25 million galaxies in the Hyper Suprime-Cam three-year shear catalog in four tomographic redshift bins ranging from 0.3 to 1.5. After conservative masking and galaxy selection, the survey covers 416 deg2 of the northern sky with an effective galaxy number density of 15 arcmin–2 over the four redshift bins. The 2PCFs adopted for cosmology analysis are measured in the angular range; 7.1 <θ/arcmin < 56.6 for ξ+ and 31.2 < θ/arcmin < 248 for ξ–, with a total signal-to-noise ratio of 26.6. We apply a conservative, wide, flat prior on the photometric redshift errors on the last two tomographic bins, and the relative magnitudes of the cosmic shear amplitude across four redshift bins allow us to calibrate the photometric redshift errors. With this flat prior on redshift errors, we find Ωm = 0.256$^{+0.056}_{–0.044}$ and S8 ≡ σ8 $\\sqrt{Ω_{m}/0.3}$ = 0.769$^{+0.031}_{–0.034}$ (both 68% C.I.) for a flat Λ cold dark matter cosmology. We find, after unblinding, that our constraint on S8 is consistent with the Fourier space cosmic shear and the 3 × 2 pt analyses on the same HSC dataset. We carefully study the potential systematics from astrophysical and systematic model uncertainties in our fiducial analysis using synthetic data, and report no biases (including projection bias in the posterior space) greater than 0.5σ in the estimation of S8. Our analysis hints that the mean redshifts of the two highest tomographic bins are higher than initially estimated. In addition, a number of consistency tests are conducted to assess the robustness of our analysis. Comparing our result with Planck-2018 cosmic microwave background observations, we find a ~2σ tension for the Λ CDM model.
Related Topics
Concepts
Physics
Astrophysics
Redshift
Cosmology
Galaxy
Photometric redshift
Cosmic microwave background
Observational cosmology
COSMIC cancer database
Astronomy
Reionization
Dark matter
Redshift survey
Quantum mechanics
Anisotropy
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1103/physrevd.108.123518
- OA Status
- green
- Cited By
- 114
- References
- 177
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4389548443
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4389548443Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.1103/physrevd.108.123518Digital Object Identifier
- Title
-
Hyper Suprime-Cam Year 3 results: Cosmology from cosmic shear two-point correlation functionsWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2023Year of publication
- Publication date
-
2023-12-11Full publication date if available
- Authors
-
Xiangchong Li, Tianqing Zhang, Sunao Sugiyama, Roohi Dalal, Ryo Terasawa, Markus Michael Rau, Rachel Mandelbaum, Masahiro Takada, Surhud More, Michael A. Strauss, Hironao Miyatake, Masato Shirasaki, Takashi Hamana, Masamune Oguri, Wentao Luo, Atsushi J. Nishizawa, Ryuichi Takahashi, Andrina Nicola, Ken Osato, Arun Kannawadi, Tomomi Sunayama, R. Armstrong, James Bosch, Yutaka Komiyama, Robert H. Lupton, Nate B. Lust, Lauren A. MacArthur, Satoshi Miyazaki, Hitoshi Murayama, Takahiro Nishimichi, Yuki Okura, P. A. Price, Philip J. Tait, Masayuki Tanaka, Shiang‐Yu WangList of authors in order
- Landing page
-
https://doi.org/10.1103/physrevd.108.123518Publisher landing page
- Open access
-
YesWhether a free full text is available
- OA status
-
greenOpen access status per OpenAlex
- OA URL
-
https://www.osti.gov/biblio/2498392Direct OA link when available
- Concepts
-
Physics, Astrophysics, Redshift, Cosmology, Galaxy, Photometric redshift, Cosmic microwave background, Observational cosmology, COSMIC cancer database, Astronomy, Reionization, Dark matter, Redshift survey, Quantum mechanics, AnisotropyTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
114Total citation count in OpenAlex
- Citations by year (recent)
-
2025: 64, 2024: 44, 2023: 6Per-year citation counts (last 5 years)
- References (count)
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177Number of works referenced by this work
- Related works (count)
-
10Other works algorithmically related by OpenAlex
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| primary_location.is_accepted | True |
| primary_location.is_published | True |
| primary_location.raw_source_name | Physical Review D |
| primary_location.landing_page_url | https://doi.org/10.1103/physrevd.108.123518 |
| publication_date | 2023-12-11 |
| publication_year | 2023 |
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