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

Journal Article · · The Astrophysical Journal (Online)
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  1. Cardiff Univ., (UK). School of Physics
  2. Univ. de Chile, Santiago (Chile). Dept. de Fisica
  3. SOKENDAI, Kanagawa (Japan); High Energy Accelerator Research Organization (KEK), Tsukuba (Japan)
  4. Univ. of California, San Diego, CA (United States). Dept. of Physics
  5. The International School for Advanced Studies SISSA, Triste (Italy); The National Inst. for Nuclear Physics INFN, Triste (Italy)
  6. Univ. of California, Berkeley, CA (United States). Space Sciences Lab.
  7. Univ. Paris Diderot, Sorbonne Paris Cite (France). AstroParticule et Cosmologie
  8. Univ. of Melbourne (Australia). School of Physics
  9. Pontificia Univ. Catolica de Chile, Santiago (Chile). Centro de Astro-Ingenieria
  10. Univ. of California, Berkeley, CA (United States). Space Sciences Lab.; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Computational Cosmology Center
  11. Dalhousie Univ., Halifax, NS (Canada). Dept. of Physics and Atmospheric Science
  12. Univ. of California, Berkeley, CA (United States). Dept. of Physics; Univ. of Tokyo (Japan). Kavli IPMU
  13. Univ. of California, Berkeley, CA (United States). Dept. of Physics
  14. McGill Univ., Montreal, QC (Canada). Dept of Physics
  15. Univ. of Tokyo (Japan). Kavli IPMU
  16. Univ. Paris-Sud, Orsay (France). Inst. d'Astrophysique Spatiale
  17. Flatiron Inst., New York, NY (United States). Center for Computational Astrophysics; Imperial College, London (United Kingdom). Blackett Lab., Dept. of Physics
  18. Univ. of California, Irvine, CA (United States). Dept. of Physics and Astronomy
  19. Yokohama National Univ. (Japan)
  20. Harvard Univ., Cambridge, MA (United States). Harvard-Smithsonian Center for Astrophysics
  21. Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences; Univ. of Colorado, Boulder, CO (United States). Dept. of Physics; Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences
  22. High Energy Accelerator Research Organization (KEK), Tsukuba (Japan); Tohoku Univ., Sendai (Japan). Astronomical Inst., Graduate School of Science
  23. SOKENDAI (Japan); High Energy Accelerator Research Organization (KEK), Tsukuba (Japan)
  24. High Energy Accelerator Research Organization (KEK), Tsukuba (Japan); SOKENDAI (Japan); Univ. of Tokyo (Japan). Kavli IMPU; Japan Aerospace Exploration Agency, Tsukuba (Japan). Inst. of Space and Astronautical Science
  25. Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Dept.
  26. High Energy Accelerator Research Organization (KEK), Tsukuba (Japan); Academia Sinica, Taipei (Taiwan). Inst. of Physics
  27. Univ. of Colorado, Boulder, CO (United States) Center for Astrophysics and Space Astronomy; Univ. of Colorado, Boulder, CO (United States). Dept. of Physics
  28. Imperial College, London (United Kingdom). Blackett Lab., Dept. of Physics
  29. The International School for Advanced Studies SISSA, Triste (Italy)
  30. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Division; Univ. of Tokyo (Japan). Dept. of Physics
  31. Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Division; Univ. of California, Berkeley, CA (United States). Radio Astronomy Lab.
  32. Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics. et al.

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.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Organization:
USDOE Office of Science (SC)
Contributing Organization:
The POLARBEAR Collaboration
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1524240
Alternate ID(s):
OSTI ID: 1525246
Journal Information:
The Astrophysical Journal (Online), Vol. 848, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 62 works
Citation information provided by
Web of Science

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Radical Compression of Cosmic Microwave Background Data text January 1998

Cited By (21)

Cross-correlation of CMB Polarization Lensing with High- z Submillimeter Herschel -ATLAS Galaxies journal November 2019
Year two instrument status of the SPT-3G cosmic microwave background receiver
  • Carter, Faustin W.; Cecil, Thomas W.; Chang, Clarence L.
  • Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX https://doi.org/10.1117/12.2312426
conference August 2018
CMB lensing reconstruction biases in cross-correlation with large-scale structure probes journal October 2019
Optimal filtering for CMB lensing reconstruction journal December 2019
Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam journal September 2019
A unified pseudo- C ℓ framework journal January 2019
The POLARBEAR Fourier transform spectrometer calibrator and spectroscopic characterization of the POLARBEAR instrument journal November 2019
Forecasting the Contribution of Polarized Extragalactic Radio Sources in CMB Observations journal May 2018
Status of Neutrino Properties and Future Prospects—Cosmological and Astrophysical Constraints journal February 2018
Iterative map-making with two-level preconditioning for polarized cosmic microwave background data sets: A worked example for ground-based experiments journal October 2018
Wiener filtering and pure $\mathcal {E}/\mathcal {B}$ decomposition of CMB maps with anisotropic correlated noise journal September 2019
Constraints on Primordial Gravitational Waves Using P l a n c k , WMAP, and New BICEP2/ K e c k Observations through the 2015 Season journal November 2018
The Simons Observatory: science goals and forecasts journal February 2019
Measurements of Tropospheric Ice Clouds with a Ground-based CMB Polarization Experiment, POLARBEAR journal January 2019
Lensing reconstruction in post-Born cosmic microwave background weak lensing journal August 2018
Impact of a primordial magnetic field on cosmic microwave background B modes with weak lensing journal May 2018
The Simons Observatory: Science goals and forecasts text January 2019
The Simons Observatory: Science goals and forecasts text January 2018
Measurements of tropospheric ice clouds with a ground-based CMB polarization experiment, POLARBEAR text January 2018
The POLARBEAR Fourier Transform Spectrometer Calibrator and Spectroscopic Characterization of the POLARBEAR Instrument text January 2019
High-Precision Scanning Water Vapor Radiometers for Cosmic Microwave Background Site Characterization and Comparison preprint January 2018

Figures / Tables (16)