Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

CHChiaki HikageMOMasamune OguriTHTakashi HamanaSMSurhud MoreRMRachel Mandelbaum

Kavli Institute for the Physics and Mathematics of the Universe · The University of Tokyo · +20 more institutions

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Abstract

Abstract We measure cosmic weak lensing shear power spectra with the Subaru Hyper Suprime-Cam (HSC) survey first-year shear catalog covering 137 deg2 of the sky. Thanks to the high effective galaxy number density of ∼17 arcmin−2, even after conservative cuts such as a magnitude cut of i < 24.5 and photometric redshift cut of 0.3 ≤ z ≤ 1.5, we obtain a high-significance measurement of the cosmic shear power spectra in four tomographic redshift bins, achieving a total signal-to-noise ratio of 16 in the multipole range 300 ≤ ℓ ≤ 1900. We carefully account for various uncertainties in our analysis including the intrinsic alignment of galaxies, scatters and biases in photometric redshifts, residual…

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Authors

37
  • CH
    Chiaki HikageCorresponding

    Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo

  • MO
    Masamune Oguri

    Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo

  • TH
    Takashi Hamana

    National Astronomical Observatory of Japan

  • SM
    Surhud More

    Kavli Institute for the Physics and Mathematics of the Universe, Inter-University Centre for Astronomy and Astrophysics, The University of Tokyo

  • RM
    Rachel Mandelbaum

    Carnegie Mellon University

Topics & keywords

Keywords
  • Cosmic microwave background
  • COSMIC cancer database
  • Planck
  • Matter power spectrum
  • Galaxy
  • Redshift
  • Weak gravitational lensing
  • Cosmology
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