A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data

P. A.R. Ade; M. Aguilar; Y. Akiba; K. Arnold; C. Baccigalupi; D. Barron; D. Beck; F. Bianchini; D. Boettger; J. Borrill; S. Chapman; Y. Chinone; K. Crowley; A. Cukierman; R. Dünner; M. Dobbs; A. Ducout; T. Elleflot; J. Errard; G. Fabbian; S. M. Feeney; C. Feng; T. Fujino; N. Galitzki; A. Gilbert; N. Goeckner-Wald; J. C. Groh; G. Hall; N. Halverson; T. Hamada; M. Hasegawa; M. Hazumi; C. A. Hill; L. Howe; Y. Inoue; G. Jaehnig; A. H. Jaffe; O. Jeong; D. Kaneko; N. Katayama; B. Keating; R. Keskitalo; T. Kisner; N. Krachmalnicoff; A. Kusaka; M. Le Jeune; A. T. Lee; E. M. Leitch; D. Leon; E. Linder; L. Lowry; F. Matsuda; T. Matsumura; Y. Minami; J. Montgomery; M. Navaroli; H. Nishino; H. Paar; J. Peloton; A. T.P. Pham; D. Poletti; G. Puglisi; C. L. Reichardt; P. L. Richards; C. Ross; Y. Segawa; B. D. Sherwin; M. Silva-Feaver; P. Siritanasak; N. Stebor; R. Stompor; A. Suzuki; O. Tajima; S. Takakura; S. Takatori; D. Tanabe; G. P. Teply; T. Tomaru; C. Tucker; N. Whitehorn; A. Zahn

doi:10.3847/1538-4357/aa8e9f

A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data

P. A.R. Ade, M. Aguilar, Y. Akiba, K. Arnold, C. Baccigalupi, D. Barron, D. Beck, F. Bianchini, D. Boettger, J. Borrill, S. Chapman, Y. Chinone, K. Crowley, A. Cukierman, R. Dünner, M. Dobbs, A. Ducout, T. Elleflot, J. Errard, G. FabbianS. M. Feeney, C. Feng, T. Fujino, N. Galitzki, A. Gilbert, N. Goeckner-Wald, J. C. Groh, G. Hall, N. Halverson, T. Hamada, M. Hasegawa, M. Hazumi, C. A. Hill, L. Howe, Y. Inoue, G. Jaehnig, A. H. Jaffe, O. Jeong, D. Kaneko, N. Katayama, B. Keating, R. Keskitalo, T. Kisner, N. Krachmalnicoff, A. Kusaka, M. Le Jeune, A. T. Lee, E. M. Leitch, D. Leon, E. Linder, L. Lowry, F. Matsuda, T. Matsumura, Y. Minami, J. Montgomery, M. Navaroli, H. Nishino, H. Paar, J. Peloton, A. T.P. Pham, D. Poletti, G. Puglisi, C. L. Reichardt, P. L. Richards, C. Ross, Y. Segawa, B. D. Sherwin, M. Silva-Feaver, P. Siritanasak, N. Stebor, R. Stompor, A. Suzuki, O. Tajima, S. Takakura, S. Takatori, D. Tanabe, G. P. Teply, T. Tomaru, C. Tucker, N. Whitehorn, A. Zahn

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

66 引文斯高帕斯（Scopus）

摘要

We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data from the first season (2012-2013), we have reduced twofold the band-power uncertainties. The band powers are reported over angular multipoles 500 ≤ ℓ ≤ 2100, where the dominant B-mode signal is expected to be due to the gravitational lensing of E-modes. We reject the null hypothesis of no B-mode polarization at a confidence of 3.1σ including both statistical and systematic uncertainties. We test the consistency of the measured B-modes with the Λ Cold Dark Matter (ΛCDM) framework by fitting for a single lensing amplitude parameter A _L = 0.60 +0.26_-0.24(stat)^+0.00_-0.04 (inst) ± 0.14(foreground) ± 0.04(multi), where A _L = 1 relative to the Planck 2015 best-fit model prediction. We obtain ±0.14(foreground) ±0.04(multi), where is the fiducial ΛCDM value.

原文	???core.languages.en_GB???
文章編號	121
期刊	Astrophysical Journal
卷	848
發行號	2
DOIs	https://doi.org/10.3847/1538-4357/aa8e9f
出版狀態	已出版 - 20 10月 2017

存取文件

10.3847/1538-4357/aa8e9f

引用此

Ade, P. A. R., Aguilar, M., Akiba, Y., Arnold, K., Baccigalupi, C., Barron, D., Beck, D., Bianchini, F., Boettger, D., Borrill, J., Chapman, S., Chinone, Y., Crowley, K., Cukierman, A., Dünner, R., Dobbs, M., Ducout, A., Elleflot, T., Errard, J., ... Zahn, A. (2017). A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data. Astrophysical Journal, 848(2), [121]. https://doi.org/10.3847/1538-4357/aa8e9f

@article{9b81f2df2c4b486f8ccb7db3020f569f,

title = "A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data",

abstract = "We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data from the first season (2012-2013), we have reduced twofold the band-power uncertainties. The band powers are reported over angular multipoles 500 ≤ ℓ ≤ 2100, where the dominant B-mode signal is expected to be due to the gravitational lensing of E-modes. We reject the null hypothesis of no B-mode polarization at a confidence of 3.1σ including both statistical and systematic uncertainties. We test the consistency of the measured B-modes with the Λ Cold Dark Matter (ΛCDM) framework by fitting for a single lensing amplitude parameter A L = 0.60 +0.26-0.24(stat)+0.00-0.04 (inst) ± 0.14(foreground) ± 0.04(multi), where A L = 1 relative to the Planck 2015 best-fit model prediction. We obtain ±0.14(foreground) ±0.04(multi), where is the fiducial ΛCDM value.",

keywords = "cosmic background radiation, cosmology: observations, large-scale structure of universe",

author = "Ade, {P. A.R.} and M. Aguilar and Y. Akiba and K. Arnold and C. Baccigalupi and D. Barron and D. Beck and F. Bianchini and D. Boettger and J. Borrill and S. Chapman and Y. Chinone and K. Crowley and A. Cukierman and R. D{\"u}nner and M. Dobbs and A. Ducout and T. Elleflot and J. Errard and G. Fabbian and Feeney, {S. M.} and C. Feng and T. Fujino and N. Galitzki and A. Gilbert and N. Goeckner-Wald and Groh, {J. C.} and G. Hall and N. Halverson and T. Hamada and M. Hasegawa and M. Hazumi and Hill, {C. A.} and L. Howe and Y. Inoue and G. Jaehnig and Jaffe, {A. H.} and O. Jeong and D. Kaneko and N. Katayama and B. Keating and R. Keskitalo and T. Kisner and N. Krachmalnicoff and A. Kusaka and Jeune, {M. Le} and Lee, {A. T.} and Leitch, {E. M.} and D. Leon and E. Linder and L. Lowry and F. Matsuda and T. Matsumura and Y. Minami and J. Montgomery and M. Navaroli and H. Nishino and H. Paar and J. Peloton and Pham, {A. T.P.} and D. Poletti and G. Puglisi and Reichardt, {C. L.} and Richards, {P. L.} and C. Ross and Y. Segawa and Sherwin, {B. D.} and M. Silva-Feaver and P. Siritanasak and N. Stebor and R. Stompor and A. Suzuki and O. Tajima and S. Takakura and S. Takatori and D. Tanabe and Teply, {G. P.} and T. Tomaru and C. Tucker and N. Whitehorn and A. Zahn",

year = "2017",

month = oct,

day = "20",

doi = "10.3847/1538-4357/aa8e9f",

language = "???core.languages.en_GB???",

volume = "848",

journal = "Astrophysical Journal",

issn = "0004-637X",

number = "2",

}

Ade, PAR, Aguilar, M, Akiba, Y, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Bianchini, F, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Crowley, K, Cukierman, A, Dünner, R, Dobbs, M, Ducout, A, Elleflot, T, Errard, J, Fabbian, G, Feeney, SM, Feng, C, Fujino, T, Galitzki, N, Gilbert, A, Goeckner-Wald, N, Groh, JC, Hall, G, Halverson, N, Hamada, T, Hasegawa, M, Hazumi, M, Hill, CA, Howe, L, Inoue, Y, Jaehnig, G, Jaffe, AH, Jeong, O, Kaneko, D, Katayama, N, Keating, B, Keskitalo, R, Kisner, T, Krachmalnicoff, N, Kusaka, A, Jeune, ML, Lee, AT, Leitch, EM, Leon, D, Linder, E, Lowry, L, Matsuda, F, Matsumura, T, Minami, Y, Montgomery, J, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Pham, ATP, Poletti, D, Puglisi, G, Reichardt, CL, Richards, PL, Ross, C, Segawa, Y, Sherwin, BD, Silva-Feaver, M, Siritanasak, P, Stebor, N, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Takatori, S, Tanabe, D, Teply, GP, Tomaru, T, Tucker, C, Whitehorn, N & Zahn, A 2017, 'A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data', Astrophysical Journal, 卷 848, 編號 2, 121. https://doi.org/10.3847/1538-4357/aa8e9f

TY - JOUR

T1 - A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data

AU - Ade, P. A.R.

AU - Aguilar, M.

AU - Akiba, Y.

AU - Arnold, K.

AU - Baccigalupi, C.

AU - Barron, D.

AU - Beck, D.

AU - Bianchini, F.

AU - Boettger, D.

AU - Borrill, J.

AU - Chapman, S.

AU - Chinone, Y.

AU - Crowley, K.

AU - Cukierman, A.

AU - Dünner, R.

AU - Dobbs, M.

AU - Ducout, A.

AU - Elleflot, T.

AU - Errard, J.

AU - Fabbian, G.

AU - Feeney, S. M.

AU - Feng, C.

AU - Fujino, T.

AU - Galitzki, N.

AU - Gilbert, A.

AU - Goeckner-Wald, N.

AU - Groh, J. C.

AU - Hall, G.

AU - Halverson, N.

AU - Hamada, T.

AU - Hasegawa, M.

AU - Hazumi, M.

AU - Hill, C. A.

AU - Howe, L.

AU - Inoue, Y.

AU - Jaehnig, G.

AU - Jaffe, A. H.

AU - Jeong, O.

AU - Kaneko, D.

AU - Katayama, N.

AU - Keating, B.

AU - Keskitalo, R.

AU - Kisner, T.

AU - Krachmalnicoff, N.

AU - Kusaka, A.

AU - Jeune, M. Le

AU - Lee, A. T.

AU - Leitch, E. M.

AU - Leon, D.

AU - Linder, E.

AU - Lowry, L.

AU - Matsuda, F.

AU - Matsumura, T.

AU - Minami, Y.

AU - Montgomery, J.

AU - Navaroli, M.

AU - Nishino, H.

AU - Paar, H.

AU - Peloton, J.

AU - Pham, A. T.P.

AU - Poletti, D.

AU - Puglisi, G.

AU - Reichardt, C. L.

AU - Richards, P. L.

AU - Ross, C.

AU - Segawa, Y.

AU - Sherwin, B. D.

AU - Silva-Feaver, M.

AU - Siritanasak, P.

AU - Stebor, N.

AU - Stompor, R.

AU - Suzuki, A.

AU - Tajima, O.

AU - Takakura, S.

AU - Takatori, S.

AU - Tanabe, D.

AU - Teply, G. P.

AU - Tomaru, T.

AU - Tucker, C.

AU - Whitehorn, N.

AU - Zahn, A.

PY - 2017/10/20

Y1 - 2017/10/20

N2 - We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data from the first season (2012-2013), we have reduced twofold the band-power uncertainties. The band powers are reported over angular multipoles 500 ≤ ℓ ≤ 2100, where the dominant B-mode signal is expected to be due to the gravitational lensing of E-modes. We reject the null hypothesis of no B-mode polarization at a confidence of 3.1σ including both statistical and systematic uncertainties. We test the consistency of the measured B-modes with the Λ Cold Dark Matter (ΛCDM) framework by fitting for a single lensing amplitude parameter A L = 0.60 +0.26-0.24(stat)+0.00-0.04 (inst) ± 0.14(foreground) ± 0.04(multi), where A L = 1 relative to the Planck 2015 best-fit model prediction. We obtain ±0.14(foreground) ±0.04(multi), where is the fiducial ΛCDM value.

AB - We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data from the first season (2012-2013), we have reduced twofold the band-power uncertainties. The band powers are reported over angular multipoles 500 ≤ ℓ ≤ 2100, where the dominant B-mode signal is expected to be due to the gravitational lensing of E-modes. We reject the null hypothesis of no B-mode polarization at a confidence of 3.1σ including both statistical and systematic uncertainties. We test the consistency of the measured B-modes with the Λ Cold Dark Matter (ΛCDM) framework by fitting for a single lensing amplitude parameter A L = 0.60 +0.26-0.24(stat)+0.00-0.04 (inst) ± 0.14(foreground) ± 0.04(multi), where A L = 1 relative to the Planck 2015 best-fit model prediction. We obtain ±0.14(foreground) ±0.04(multi), where is the fiducial ΛCDM value.

KW - cosmic background radiation

KW - cosmology: observations

KW - large-scale structure of universe

UR - http://www.scopus.com/inward/record.url?scp=85032796298&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/aa8e9f

DO - 10.3847/1538-4357/aa8e9f

M3 - 期刊論文

AN - SCOPUS:85032796298

SN - 0004-637X

VL - 848

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 121

ER -

A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data

摘要

存取文件

指紋

引用此