Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam

T. Namikawa; Y. Chinone; H. Miyatake; M. Oguri; R. Takahashi; A. Kusaka; N. Katayama; S. Adachi; M. Aguilar; H. Aihara; A. Ali; R. Armstrong; K. Arnold; C. Baccigalupi; D. Barron; D. Beck; S. Beckman; F. Bianchini; D. Boettger; J. Borrill; K. Cheung; L. Corbett; K. T. Crowley; H. El Bouhargani; T. Elleflot; J. Errard; G. Fabbian; C. Feng; N. Galitzki; N. Goeckner-Wald; J. Groh; T. Hamada; M. Hasegawa; M. Hazumi; C. A. Hill; L. Howe; O. Jeong; D. Kaneko; B. Keating; A. T. Lee; D. Leon; E. Linder; L. N. Lowry; A. Mangu; F. Matsuda; Y. Minami; S. Miyazaki; H. Murayama; M. Navaroli; H. Nishino; A. J. Nishizawa; A. T.P. Pham; D. Poletti; G. Puglisi; C. L. Reichardt; B. D. Sherwin; M. Silva-Feaver; P. Siritanasak; J. S. Speagle; R. Stompor; A. Suzuki; P. J. Tait; O. Tajima; M. Takada; S. Takakura; S. Takatori; D. Tanabe; M. Tanaka; G. P. Teply; C. Tsai; C. Vergés; B. Westbrook; Y. Zhou

doi:10.3847/1538-4357/ab3424

Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam

T. Namikawa, Y. Chinone, H. Miyatake, M. Oguri, R. Takahashi, A. Kusaka, N. Katayama, S. Adachi, M. Aguilar, H. Aihara, A. Ali, R. Armstrong, K. Arnold, C. Baccigalupi, D. Barron, D. Beck, S. Beckman, F. Bianchini, D. Boettger, J. BorrillK. Cheung, L. Corbett, K. T. Crowley, H. El Bouhargani, T. Elleflot, J. Errard, G. Fabbian, C. Feng, N. Galitzki, N. Goeckner-Wald, J. Groh, T. Hamada, M. Hasegawa, M. Hazumi, C. A. Hill, L. Howe, O. Jeong, D. Kaneko, B. Keating, A. T. Lee, D. Leon, E. Linder, L. N. Lowry, A. Mangu, F. Matsuda, Y. Minami, S. Miyazaki, H. Murayama, M. Navaroli, H. Nishino, A. J. Nishizawa, A. T.P. Pham, D. Poletti, G. Puglisi, C. L. Reichardt, B. D. Sherwin, M. Silva-Feaver, P. Siritanasak, J. S. Speagle, R. Stompor, A. Suzuki, P. J. Tait, O. Tajima, M. Takada, S. Takakura, S. Takatori, D. Tanabe, M. Tanaka, G. P. Teply, C. Tsai, C. Vergés, B. Westbrook, Y. Zhou

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

17 Citations (Scopus)

Abstract

We present the first measurement of cross-correlation between the lensing potential, reconstructed from cosmic microwave background (CMB) polarization data, and the cosmic shear field from galaxy shapes. This measurement is made using data from the Polarbear CMB experiment and the Subaru Hyper Suprime-Cam (HSC) survey. By analyzing an 11 deg² overlapping region, we reject the null hypothesis at 3.5σ and constrain the amplitude of the cross-spectrum to , where is the amplitude normalized with respect to the Planck 2018 prediction, based on the flat Λ cold dark matter cosmology. The first measurement of this cross-spectrum without relying on CMB temperature measurements is possible owing to the deep Polarbear map with a noise level of ∼6 μK arcmin, as well as the deep HSC data with a high galaxy number density of . We present a detailed study of the systematics budget to show that residual systematics in our results are negligibly small, which demonstrates the future potential of this cross-correlation technique.

Original language	English
Article number	62
Journal	Astrophysical Journal
Volume	882
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/ab3424
Publication status	Published - Sept 1 2019
Externally published	Yes

Keywords

cosmic background radiation
cosmology: observations
gravitational lensing: weak
polarization

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/1538-4357/ab3424

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Namikawa, T., Chinone, Y., Miyatake, H., Oguri, M., Takahashi, R., Kusaka, A., Katayama, N., Adachi, S., Aguilar, M., Aihara, H., Ali, A., Armstrong, R., Arnold, K., Baccigalupi, C., Barron, D., Beck, D., Beckman, S., Bianchini, F., Boettger, D., ... Zhou, Y. (2019). Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam. Astrophysical Journal, 882(1), [62]. https://doi.org/10.3847/1538-4357/ab3424

Namikawa, T, Chinone, Y, Miyatake, H, Oguri, M, Takahashi, R, Kusaka, A, Katayama, N, Adachi, S, Aguilar, M, Aihara, H, Ali, A, Armstrong, R, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Beckman, S, Bianchini, F, Boettger, D, Borrill, J, Cheung, K, Corbett, L, Crowley, KT, Bouhargani, HE, Elleflot, T, Errard, J, Fabbian, G, Feng, C, Galitzki, N, Goeckner-Wald, N, Groh, J, Hamada, T, Hasegawa, M, Hazumi, M, Hill, CA, Howe, L, Jeong, O, Kaneko, D, Keating, B, Lee, AT, Leon, D, Linder, E, Lowry, LN, Mangu, A, Matsuda, F, Minami, Y, Miyazaki, S, Murayama, H, Navaroli, M, Nishino, H, Nishizawa, AJ, Pham, ATP, Poletti, D, Puglisi, G, Reichardt, CL, Sherwin, BD, Silva-Feaver, M, Siritanasak, P, Speagle, JS, Stompor, R, Suzuki, A, Tait, PJ, Tajima, O, Takada, M, Takakura, S, Takatori, S, Tanabe, D, Tanaka, M, Teply, GP, Tsai, C, Vergés, C, Westbrook, B & Zhou, Y 2019, 'Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam', Astrophysical Journal, vol. 882, no. 1, 62. https://doi.org/10.3847/1538-4357/ab3424

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title = "Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam",

abstract = "We present the first measurement of cross-correlation between the lensing potential, reconstructed from cosmic microwave background (CMB) polarization data, and the cosmic shear field from galaxy shapes. This measurement is made using data from the Polarbear CMB experiment and the Subaru Hyper Suprime-Cam (HSC) survey. By analyzing an 11 deg2 overlapping region, we reject the null hypothesis at 3.5σ and constrain the amplitude of the cross-spectrum to , where is the amplitude normalized with respect to the Planck 2018 prediction, based on the flat Λ cold dark matter cosmology. The first measurement of this cross-spectrum without relying on CMB temperature measurements is possible owing to the deep Polarbear map with a noise level of ∼6 μK arcmin, as well as the deep HSC data with a high galaxy number density of . We present a detailed study of the systematics budget to show that residual systematics in our results are negligibly small, which demonstrates the future potential of this cross-correlation technique.",

keywords = "cosmic background radiation, cosmology: observations, gravitational lensing: weak, polarization",

author = "T. Namikawa and Y. Chinone and H. Miyatake and M. Oguri and R. Takahashi and A. Kusaka and N. Katayama and S. Adachi and M. Aguilar and H. Aihara and A. Ali and R. Armstrong and K. Arnold and C. Baccigalupi and D. Barron and D. Beck and S. Beckman and F. Bianchini and D. Boettger and J. Borrill and K. Cheung and L. Corbett and Crowley, {K. T.} and Bouhargani, {H. El} and T. Elleflot and J. Errard and G. Fabbian and C. Feng and N. Galitzki and N. Goeckner-Wald and J. Groh and T. Hamada and M. Hasegawa and M. Hazumi and Hill, {C. A.} and L. Howe and O. Jeong and D. Kaneko and B. Keating and Lee, {A. T.} and D. Leon and E. Linder and Lowry, {L. N.} and A. Mangu and F. Matsuda and Y. Minami and S. Miyazaki and H. Murayama and M. Navaroli and H. Nishino and Nishizawa, {A. J.} and Pham, {A. T.P.} and D. Poletti and G. Puglisi and Reichardt, {C. L.} and Sherwin, {B. D.} and M. Silva-Feaver and P. Siritanasak and Speagle, {J. S.} and R. Stompor and A. Suzuki and Tait, {P. J.} and O. Tajima and M. Takada and S. Takakura and S. Takatori and D. Tanabe and M. Tanaka and Teply, {G. P.} and C. Tsai and C. Verg{\'e}s and B. Westbrook and Y. Zhou",

year = "2019",

month = sep,

day = "1",

doi = "10.3847/1538-4357/ab3424",

language = "English",

volume = "882",

journal = "Astrophysical Journal",

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T1 - Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam

AU - Namikawa, T.

AU - Chinone, Y.

AU - Miyatake, H.

AU - Oguri, M.

AU - Takahashi, R.

AU - Kusaka, A.

AU - Katayama, N.

AU - Adachi, S.

AU - Aguilar, M.

AU - Aihara, H.

AU - Ali, A.

AU - Armstrong, R.

AU - Arnold, K.

AU - Baccigalupi, C.

AU - Barron, D.

AU - Beck, D.

AU - Beckman, S.

AU - Bianchini, F.

AU - Boettger, D.

AU - Borrill, J.

AU - Cheung, K.

AU - Corbett, L.

AU - Crowley, K. T.

AU - Bouhargani, H. El

AU - Elleflot, T.

AU - Errard, J.

AU - Fabbian, G.

AU - Feng, C.

AU - Galitzki, N.

AU - Goeckner-Wald, N.

AU - Groh, J.

AU - Hamada, T.

AU - Hasegawa, M.

AU - Hazumi, M.

AU - Hill, C. A.

AU - Howe, L.

AU - Jeong, O.

AU - Kaneko, D.

AU - Keating, B.

AU - Lee, A. T.

AU - Leon, D.

AU - Linder, E.

AU - Lowry, L. N.

AU - Mangu, A.

AU - Matsuda, F.

AU - Minami, Y.

AU - Miyazaki, S.

AU - Murayama, H.

AU - Navaroli, M.

AU - Nishino, H.

AU - Nishizawa, A. J.

AU - Pham, A. T.P.

AU - Poletti, D.

AU - Puglisi, G.

AU - Reichardt, C. L.

AU - Sherwin, B. D.

AU - Silva-Feaver, M.

AU - Siritanasak, P.

AU - Speagle, J. S.

AU - Stompor, R.

AU - Suzuki, A.

AU - Tait, P. J.

AU - Tajima, O.

AU - Takada, M.

AU - Takakura, S.

AU - Takatori, S.

AU - Tanabe, D.

AU - Tanaka, M.

AU - Teply, G. P.

AU - Tsai, C.

AU - Vergés, C.

AU - Westbrook, B.

AU - Zhou, Y.

PY - 2019/9/1

Y1 - 2019/9/1

N2 - We present the first measurement of cross-correlation between the lensing potential, reconstructed from cosmic microwave background (CMB) polarization data, and the cosmic shear field from galaxy shapes. This measurement is made using data from the Polarbear CMB experiment and the Subaru Hyper Suprime-Cam (HSC) survey. By analyzing an 11 deg2 overlapping region, we reject the null hypothesis at 3.5σ and constrain the amplitude of the cross-spectrum to , where is the amplitude normalized with respect to the Planck 2018 prediction, based on the flat Λ cold dark matter cosmology. The first measurement of this cross-spectrum without relying on CMB temperature measurements is possible owing to the deep Polarbear map with a noise level of ∼6 μK arcmin, as well as the deep HSC data with a high galaxy number density of . We present a detailed study of the systematics budget to show that residual systematics in our results are negligibly small, which demonstrates the future potential of this cross-correlation technique.

AB - We present the first measurement of cross-correlation between the lensing potential, reconstructed from cosmic microwave background (CMB) polarization data, and the cosmic shear field from galaxy shapes. This measurement is made using data from the Polarbear CMB experiment and the Subaru Hyper Suprime-Cam (HSC) survey. By analyzing an 11 deg2 overlapping region, we reject the null hypothesis at 3.5σ and constrain the amplitude of the cross-spectrum to , where is the amplitude normalized with respect to the Planck 2018 prediction, based on the flat Λ cold dark matter cosmology. The first measurement of this cross-spectrum without relying on CMB temperature measurements is possible owing to the deep Polarbear map with a noise level of ∼6 μK arcmin, as well as the deep HSC data with a high galaxy number density of . We present a detailed study of the systematics budget to show that residual systematics in our results are negligibly small, which demonstrates the future potential of this cross-correlation technique.

KW - cosmic background radiation

KW - cosmology: observations

KW - gravitational lensing: weak

KW - polarization

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UR - http://www.scopus.com/inward/citedby.url?scp=85072341375&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/ab3424

DO - 10.3847/1538-4357/ab3424

M3 - Article

AN - SCOPUS:85072341375

SN - 0004-637X

VL - 882

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 62

ER -

Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam

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