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We investigate the tolerance for systematic errors in lensing analysis applied to a patchwork map of Cosmic Microwave Background polarization. We focus on the properties of the individual polarization maps that comprise the patchwork and…

宇宙学与河外天体物理 · 物理学 2024-08-27 Ryo Nagata , Toshiya Namikawa

In this paper, we study the effects of instrumental systematics on the reconstruction of the deflection angle power spectrum from weak lensing of Cosmic Microwave Background (CMB) temperature and polarization observations. We consider seven…

宇宙学与河外天体物理 · 物理学 2009-06-30 Meng Su , Amit P. S. Yadav , Matias Zaldarriaga

Weak gravitational lensing of the cosmic microwave background (CMB) is an important cosmological tool that allows us to learn about the structure, composition and evolution of the Universe. Upcoming CMB experiments, such as the Simons…

宇宙学与河外天体物理 · 物理学 2021-06-30 Mark Mirmelstein , Giulio Fabbian , Antony Lewis , Julien Peloton

Gravitational lensing of the cosmic microwave background (CMB) polarization field has been recognized as a potentially valuable probe of the cosmological density field. We apply likelihood-based techniques to the problem of lensing of CMB…

天体物理学 · 物理学 2011-06-21 Christopher M. Hirata , Uros Seljak

We investigate the impact of instrumental systematic errors on the potential of cosmic microwave background polarization experiments targeting primordial B-modes. To do so, we introduce spin-weighted Muller matrix-valued fields describing…

天体物理学 · 物理学 2008-11-26 Daniel O'Dea , Anthony Challinor , Bradley R. Johnson

Cosmic microwave background (CMB) polarization observations will require superb control of systematic errors in order to achieve their full scientific potential, particularly in the case of attempts to detect the B modes that may provide a…

天体物理学 · 物理学 2008-11-26 Emory F. Bunn

CMB polarization provides a unique window into cosmological inflation; the amplitude of the B-mode polarization from last scattering is uniquely sensitive to the energetics of inflation. However, numerous systematic effects arising from…

天体物理学 · 物理学 2009-09-29 Meir Shimon , Brian Keating , Nicolas Ponthieu , Eric Hivon

We investigate the impact of instrumental systematic errors in interferometric measurements of the cosmic microwave background (CMB) temperature and polarization power spectra. We simulate interferometric CMB observations to generate mock…

宇宙学与河外天体物理 · 物理学 2013-06-06 Le Zhang , Ata Karakci , Paul M. Sutter , Emory F. Bunn , Andrei Korotkov , Peter Timbie , Gregory S. Tucker , Benjamin D. Wandelt

The detection of the primordial $B$-mode spectrum of the polarized cosmic microwave background (CMB) signal may provide a probe of inflation. However, observation of such a faint signal requires excellent control of systematic errors.…

宇宙学与河外天体物理 · 物理学 2015-06-15 Ata Karakci , Le Zhang , P. M. Sutter , Emory F. Bunn , Andrei Korotkov , Peter Timbie , Gregory S. Tucker , Benjamin D. Wandelt

The CMB's B-mode polarization provides a handle on several cosmological parameters most notably the tensor-to-scalar ratio, $r$, and is sensitive to parameters which govern the growth of large scale structure (LSS) and evolution of the…

天体物理学 · 物理学 2009-03-20 N. J. Miller , M. Shimon , B. G. Keating

Gravitational lensing by large-scale structure significantly impacts observations of the cosmic microwave background (CMB): it smooths the acoustic peaks in temperature and $E$-mode polarization power spectra, correlating previously…

宇宙学与河外天体物理 · 物理学 2017-12-20 Daniel Green , Joel Meyers , Alexander van Engelen

The effects of gravitational lensing of the cosmic microwave background (CMB) have been measured at high significance with existing data and will be measured even more precisely in future surveys. Reversing the effects of lensing on the…

宇宙学与河外天体物理 · 物理学 2022-04-20 Selim C. Hotinli , Joel Meyers , Cynthia Trendafilova , Daniel Green , Alexander van Engelen

Cosmic microwave background (CMB) lensing is an integrated effect whose kernel is greater than half the peak value in the range $1<z<5$. Measuring this effect offers a powerful tool to probe the large-scale structure of the Universe at high…

宇宙学与河外天体物理 · 物理学 2019-03-27 Toshiya Namikawa , Benjamin Bose , François R. Bouchet , Ryuichi Takahashi , Atsushi Taruya

One of the primary scientific targets of current and future CMB polarization experiments is the search for a stochastic background of gravity waves in the early universe. As instrumental sensitivity improves, the limiting factor will…

宇宙学与河外天体物理 · 物理学 2015-05-20 Kendrick M. Smith , Duncan Hanson , Marilena LoVerde , Christopher M. Hirata , Oliver Zahn

Gravitational lensing information from the two and higher point statistics of the CMB temperature and polarization fields are intrinsically correlated because they are lensed by the same realization of structure between last scattering and…

宇宙学与河外天体物理 · 物理学 2017-03-01 Pavel Motloch , Wayne Hu , Aurélien Benoit-Lévy

We investigate the impact of both slow and fast polarization modulation strategies on the science return of upcoming ground-based experiments aimed at measuring the B-mode polarization of the CMB. Using simulations of the Clover experiment,…

Searches for the imprint of primordial gravitational waves in degree-scale CMB $B$-mode polarisation data must account for significant contamination from gravitational lensing. Fortunately, the lensing effects can be partially removed by…

宇宙学与河外天体物理 · 物理学 2021-03-12 Antón Baleato Lizancos , Anthony Challinor , Julien Carron

Lensing of the CMB by modes that are larger than the size of the survey dilates intrinsic scales in the temperature and polarization fields and coherently shifts their observed power spectra with respect to the ensemble or all-sky mean. The…

宇宙学与河外天体物理 · 物理学 2014-07-09 Alessandro Manzotti , Wayne Hu , Aurélien Benoit-Lévy

The delensing procedure is an effective tool for removing lensing-induced $B$-mode polarization in the Cosmic Microwave Background to allow for deep searches of primordial $B$-modes. However, the delensing algorithm existing in the…

宇宙学与河外天体物理 · 物理学 2011-03-01 Wei-Hsiang Teng , Chao-Lin Kuo , Jiun-Huei Proty Wu
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