Planck Sunyaev-Zel'dovich cluster mass calibration using Hyper Suprime-Cam weak lensing

Elinor Medezinski; Nicholas Battaglia; Keiichi Umetsu; Masamune Oguri; Hironao Miyatake; Atsushi J. Nishizawa; Cristóbal Sifón; David N. Spergel; I. Non Chiu; Yen Ting Lin; Neta Bahcall; Yutaka Komiyama

doi:10.1093/pasj/psx128

Planck Sunyaev-Zel'dovich cluster mass calibration using Hyper Suprime-Cam weak lensing

Elinor Medezinski, Nicholas Battaglia, Keiichi Umetsu, Masamune Oguri, Hironao Miyatake, Atsushi J. Nishizawa, Cristóbal Sifón, David N. Spergel, I. Non Chiu, Yen Ting Lin, Neta Bahcall, Yutaka Komiyama

Department of Physics

Research output: Contribution to journal › Article › peer-review

46 Citations (Scopus)

Abstract

Using ∼140 deg² Subaru Hyper Suprime-Cam (HSC) survey data, we stack the weak lensing (WL) signal around five Planck clusters found within the footprint. This yields a 15σ detection of the mean Planck cluster mass density profile. The five Planck clusters span a relatively wide mass range, M_WL,500c = (2-30) × 10¹⁴M with a mean mass of M_WL,500c = (4.15±0.61) × 10¹⁴M. The ratio of the stacked Planck Sunyaev-Zel'dovich (SZ) mass to the stacked WL mass is (M_SZ)/(M_WL) = 1 - b = 0.80±0.14. This mass bias is consistent with previous WL mass calibrations of Planck clusters within the errors. We discuss the implications of our findings for the calibration of SZ cluster counts and the much discussed tension between Planck SZ cluster counts and Planck ΣCDM cosmology.

Original language	English
Article number	S28
Journal	Publications of the Astronomical Society of Japan
Volume	70
Issue number	Special Issue 1
DOIs	https://doi.org/10.1093/pasj/psx128
Publication status	Published - 2018 Jan 1

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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Medezinski, E., Battaglia, N., Umetsu, K., Oguri, M., Miyatake, H., Nishizawa, A. J., Sifón, C., Spergel, D. N., Chiu, I. N., Lin, Y. T., Bahcall, N., & Komiyama, Y. (2018). Planck Sunyaev-Zel'dovich cluster mass calibration using Hyper Suprime-Cam weak lensing. Publications of the Astronomical Society of Japan, 70(Special Issue 1), Article S28. https://doi.org/10.1093/pasj/psx128

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title = "Planck Sunyaev-Zel'dovich cluster mass calibration using Hyper Suprime-Cam weak lensing",

abstract = "Using ∼140 deg2 Subaru Hyper Suprime-Cam (HSC) survey data, we stack the weak lensing (WL) signal around five Planck clusters found within the footprint. This yields a 15σ detection of the mean Planck cluster mass density profile. The five Planck clusters span a relatively wide mass range, MWL,500c = (2-30) × 1014M with a mean mass of MWL,500c = (4.15±0.61) × 1014M. The ratio of the stacked Planck Sunyaev-Zel'dovich (SZ) mass to the stacked WL mass is (MSZ)/(MWL) = 1 - b = 0.80±0.14. This mass bias is consistent with previous WL mass calibrations of Planck clusters within the errors. We discuss the implications of our findings for the calibration of SZ cluster counts and the much discussed tension between Planck SZ cluster counts and Planck ΣCDM cosmology.",

author = "Elinor Medezinski and Nicholas Battaglia and Keiichi Umetsu and Masamune Oguri and Hironao Miyatake and Nishizawa, {Atsushi J.} and Crist{\'o}bal Sif{\'o}n and Spergel, {David N.} and Chiu, {I. Non} and Lin, {Yen Ting} and Neta Bahcall and Yutaka Komiyama",

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T1 - Planck Sunyaev-Zel'dovich cluster mass calibration using Hyper Suprime-Cam weak lensing

AU - Medezinski, Elinor

AU - Battaglia, Nicholas

AU - Umetsu, Keiichi

AU - Oguri, Masamune

AU - Miyatake, Hironao

AU - Nishizawa, Atsushi J.

AU - Sifón, Cristóbal

AU - Spergel, David N.

AU - Chiu, I. Non

AU - Lin, Yen Ting

AU - Bahcall, Neta

AU - Komiyama, Yutaka

PY - 2018/1/1

Y1 - 2018/1/1

N2 - Using ∼140 deg2 Subaru Hyper Suprime-Cam (HSC) survey data, we stack the weak lensing (WL) signal around five Planck clusters found within the footprint. This yields a 15σ detection of the mean Planck cluster mass density profile. The five Planck clusters span a relatively wide mass range, MWL,500c = (2-30) × 1014M with a mean mass of MWL,500c = (4.15±0.61) × 1014M. The ratio of the stacked Planck Sunyaev-Zel'dovich (SZ) mass to the stacked WL mass is (MSZ)/(MWL) = 1 - b = 0.80±0.14. This mass bias is consistent with previous WL mass calibrations of Planck clusters within the errors. We discuss the implications of our findings for the calibration of SZ cluster counts and the much discussed tension between Planck SZ cluster counts and Planck ΣCDM cosmology.

AB - Using ∼140 deg2 Subaru Hyper Suprime-Cam (HSC) survey data, we stack the weak lensing (WL) signal around five Planck clusters found within the footprint. This yields a 15σ detection of the mean Planck cluster mass density profile. The five Planck clusters span a relatively wide mass range, MWL,500c = (2-30) × 1014M with a mean mass of MWL,500c = (4.15±0.61) × 1014M. The ratio of the stacked Planck Sunyaev-Zel'dovich (SZ) mass to the stacked WL mass is (MSZ)/(MWL) = 1 - b = 0.80±0.14. This mass bias is consistent with previous WL mass calibrations of Planck clusters within the errors. We discuss the implications of our findings for the calibration of SZ cluster counts and the much discussed tension between Planck SZ cluster counts and Planck ΣCDM cosmology.

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Planck Sunyaev-Zel'dovich cluster mass calibration using Hyper Suprime-Cam weak lensing

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