English
Related papers

Related papers: Systematic effects induced by half-wave plate diff…

200 papers

A half-wave plate (HWP) is often used as a modulator to suppress systematic error in the measurements of cosmic microwave background (CMB) polarization. A HWP can also be used to measure circular polarization (CP) through its optical…

Cosmology and Nongalactic Astrophysics · Physics 2023-06-29 T. Fujino , S. Takakura , Y. Chinone , M. Hasegawa , M. Hazumi , N. Katayama , A. T. Lee , T. Matsumura , Y. Minami , H. Nishino

We evaluate the effect of half-wave plate (HWP) imperfections inducing intensity leakage to the measurement of Cosmic Microwave Background (CMB) $B$-mode polarization signal with future satellite missions focusing on the tensor-to-scalar…

Cosmology and Nongalactic Astrophysics · Physics 2023-08-03 Guillaume Patanchon , Hiroaki Imada , Hirokazu Ishino , Tomotake Matsumura

The most accessible method to measure polarization features of the CMB radiation is by means of a Stokes Polarimeter based on the rotation of an Half Wave Plate. The current observational cosmology is starting to be limited by the presence…

Instrumentation and Methods for Astrophysics · Physics 2019-07-24 G. D'Alessandro , L. Mele , F. Columbro , L. Pagano , F. Piacentini , P. de Bernardis , S. Masi

We present an evaluation of systematic effects associated with a continuously-rotating, ambient-temperature half-wave plate (HWP) based on two seasons of data from the Atacama B-Mode Search (ABS) experiment located in the Atacama Desert of…

Instrumentation and Methods for Astrophysics · Physics 2016-10-12 T. Essinger-Hileman , A. Kusaka , J. W. Appel , S. K. Choi , K. Crowley , S. P. Ho , N. Jarosik , L. A. Page , L. P. Parker , S. Raghunathan , S. M. Simon , S. T. Staggs , K. Visnjic

The polarization of the Cosmic Microwave Background (CMB) radiation carries essential information on early stages of the Universe such as the cosmic inflation, forming cosmological structures through gravitational lensing, and the epoch of…

Cosmology and Nongalactic Astrophysics · Physics 2024-02-22 E. Carretti , C. Baccigalupi

We describe the development of an ambient-temperature continuously-rotating half-wave plate (HWP) for study of the Cosmic Microwave Background (CMB) polarization by the POLARBEAR-2 (PB2) experiment. Rapid polarization modulation suppresses…

We address in this work the instrumental systematic errors that can potentially affect the forthcoming and future Cosmic Microwave Background experiments aimed at observing its polarized emission. In particular, we focus on the systematics…

Cosmology and Nongalactic Astrophysics · Physics 2021-06-14 Giuseppe Puglisi , Reijo Keskitalo , Ted Kisner , Julian D. Borrill

LiteBIRD is a space-borne experiment dedicated to detecting large-scale $B$-mode anisotropies in the linear polarization of the Cosmic Microwave Background (CMB) predicted by the theory of inflation. It is planned to be launched in the late…

Instrumentation and Methods for Astrophysics · Physics 2022-09-27 Mayu Tominaga , Masahiro Tsujimoto , Graeme Smecher , Hirokazu Ishino

We discuss a systematic effect associated with measuring polarization with a continuously rotating half-wave plate. The effect was identified with the data from the E and B Experiment (EBEX), which was a balloon-borne instrument designed to…

CMB B-mode experiments are required to control systematic effects with an unprecedented level of accuracy. Polarization modulation by a half wave plate (HWP) is a powerful technique able to mitigate a large number of the instrumental…

Instrumentation and Methods for Astrophysics · Physics 2018-01-10 Alessandro Buzzelli , Paolo de Bernardis , Silvia Masi , Nicola Vittorio , Giancarlo de Gasperis

The quasi-optical modulation of linear polarization at millimeter and sub-millimeter wavelengths can be achieved by using rotating half wave plates (HWPs) in front of polarization sensitive detectors. Large operational bandwidths are…

Instrumentation and Methods for Astrophysics · Physics 2016-10-04 Giampaolo Pisano , Bruno Maffei , Peter A. R. Ade , Paolo de Bernardis , Peter De Maagt , Brian Ellison , Manju Henry , Ming Wah Ng , Brian Schortt , Carole Tucker

We present a study of unbiased reconstruction of cosmic microwave background (CMB) polarization maps from data collected by modern ground-based observatories. Atmospheric emission is a major source of correlated noise in such experiments,…

Instrumentation and Methods for Astrophysics · Physics 2025-12-08 Simon Biquard , Josquin Errard , Radek Stompor

The quest for primordial $B$-mode polarization signatures in the Cosmic Microwave Background (CMB) is a major goal of contemporary cosmology. Detecting these signatures would confirm primordial gravitational waves and allow precise…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-28 Yusuke Takase

The Simons Observatory (SO) will observe the temperature and polarization anisotropies of the cosmic microwave background (CMB) over a wide range of frequencies (27 to 270 GHz) and angular scales by using both small (0.5 m) and large (6 m)…

We simulate a variety of optical systematics for Taurus, a balloon-borne cosmic microwave background (CMB) polarisation experiment, to assess their impact on large-scale E-mode polarisation measurements and constraints of the optical depth…

The polarization of the cosmic microwave background (CMB) can be used to search for parity-violating processes like that predicted by a Chern-Simons coupling to a light pseudoscalar field. Such an interaction rotates $E$ modes into $B$…

LiteBIRD has been selected as JAXA's strategic large mission in the 2020s, to observe the cosmic microwave background (CMB) $B$-mode polarization over the full sky at large angular scales. The challenges of LiteBIRD are the wide…

Instrumentation and Methods for Astrophysics · Physics 2021-01-19 Y. Sekimoto , P. A. R. Ade , A. Adler , E. Allys , K. Arnold , D. Auguste , J. Aumont , R. Aurlien , J. Austermann , C. Baccigalupi , A. J. Banday , R. Banerji , R. B. Barreiro , S. Basak , J. Beall , D. Beck , S. Beckman , J. Bermejo , P. de Bernardis , M. Bersanelli , J. Bonis , J. Borrill , F. Boulanger , S. Bounissou , M. Brilenkov , M. Brown , M. Bucher , E. Calabrese , P. Campeti , A. Carones , F. J. Casas , A. Challinor , V. Chan , K. Cheung , Y. Chinone , J. F. Cliche , L. Colombo , F. Columbro , J. Cubas , A. Cukierman , D. Curtis , G. D'Alessandro , N. Dachlythra , M. De Petris , C. Dickinson , P. Diego-Palazuelos , M. Dobbs , T. Dotani , L. Duband , S. Duff , J. M. Duval , K. Ebisawa , T. Elleflot , H. K. Eriksen , J. Errard , T. Essinger-Hileman , F. Finelli , R. Flauger , C. Franceschet , U. Fuskeland , M. Galloway , K. Ganga , J. R. Gao , R. Genova-Santos , M. Gerbino , M. Gervasi , T. Ghigna , E. Gjerløw , M. L. Gradziel , J. Grain , F. Grupp , A. Gruppuso , J. E. Gudmundsson , T. de Haan , N. W. Halverson , P. Hargrave , T. Hasebe , M. Hasegawa , M. Hattori , M. Hazumi , S. Henrot-Versillé , D. Herman , D. Herranz , C. A. Hill , G. Hilton , Y. Hirota , E. Hivon , R. A. Hlozek , Y. Hoshino , E. de la Hoz , J. Hubmayr , K. Ichiki , T. iida , H. Imada , K. Ishimura , H. Ishino , G. Jaehnig , T. Kaga , S. Kashima , N. Katayama , A. Kato , T. Kawasaki , R. Keskitalo , T. Kisner , Y. Kobayashi , N. Kogiso , A. Kogut , K. Kohri , E. Komatsu , K. Komatsu , K. Konishi , N. Krachmalnicoff , I. Kreykenbohm , C. L. Kuo , A. Kushino , L. Lamagna , J. V. Lanen , M. Lattanzi , A. T. Lee , C. Leloup , F. Levrier , E. Linder , T. Louis , G. Luzzi , T. Maciaszek , B. Maffei , D. Maino , M. Maki , S. Mandelli , E. Martinez-Gonzalez , S. Masi , T. Matsumura , A. Mennella , M. Migliaccio , Y. Minanmi , K. Mitsuda , J. Montgomery , L. Montier , G. Morgante , B. Mot , Y. Murata , J. A. Murphy , M. Nagai , Y. Nagano , T. Nagasaki , R. Nagata , S. Nakamura , T. Namikawa , P. Natoli , S. Nerval , T. Nishibori , H. Nishino , C. O'Sullivan , H. Ogawa , H. Ogawa , S. Oguri , H. Ohsaki , I. S. Ohta , N. Okada , N. Okada , L. Pagano , A. Paiella , D. Paoletti , G. Patanchon , J. Peloton , F. Piacentini , G. Pisano , G. Polenta , D. Poletti , T. Prouvé , G. Puglisi , D. Rambaud , C. Raum , S. Realini , M. Reinecke , M. Remazeilles , A. Ritacco , G. Roudil , J. A. Rubino-Martin , M. Russell , H. Sakurai , Y. Sakurai , M. Sandri , M. Sasaki , G. Savini , D. Scott , J. Seibert , B. Sherwin , K. Shinozaki , M. Shiraishi , P. Shirron , G. Signorelli , G. Smecher , S. Stever , R. Stompor , H. Sugai , S. Sugiyama , A. Suzuki , J. Suzuki , T. L. Svalheim , E. Switzer , R. Takaku , H. Takakura , S. Takakura , Y. Takase , Y. Takeda , A. Tartari , E. Taylor , Y. Terao , H. Thommesen , K. L. Thompson , B. Thorne , T. Toda , M. Tomasi , M. Tominaga , N. Trappe , M. Tristram , M. Tsuji , M. Tsujimoto , C. Tucker , J. Ullom , G. Vermeulen , P. Vielva , F. Villa , M. Vissers , N. Vittorio , I. Wehus , J. Weller , B. Westbrook , J. Wilms , B. Winter , E. J. Wollack , N. Y. Yamasaki , T. Yoshida , J. Yumoto , M. Zannoni , A. Zonca

GroundBIRD is a ground-based experiment for the precise observation of the polarization of the cosmic microwave background (CMB). To achieve high sensitivity at large angular scale, we adopt three features in this experiment: fast rotation…

LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan's fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the…

Instrumentation and Methods for Astrophysics · Physics 2024-06-08 T. Ghigna , A. Adler , K. Aizawa , H. Akamatsu , R. Akizawa , E. Allys , A. Anand , J. Aumont , J. Austermann , S. Azzoni , C. Baccigalupi , M. Ballardini , A. J. Banday , R. B. Barreiro , N. Bartolo , S. Basak , A. Basyrov , S. Beckman , M. Bersanelli , M. Bortolami , F. Bouchet , T. Brinckmann , P. Campeti , E. Carinos , A. Carones , F. J. Casas , K. Cheung , Y. Chinone , L. Clermont , F. Columbro , A. Coppolecchia , D. Curtis , P. de Bernardis , T. de Haan , E. de la Hoz , M. De Petris , S. Della Torre , G. Delle Monache , E. Di Giorgi , C. Dickinson , P. Diego-Palazuelos , J. J. Díaz García , M. Dobbs , T. Dotani , G. D'Alessandro , H. K. Eriksen , J. Errard , T. Essinger-Hileman , N. Farias , E. Ferreira , C. Franceschet , U. Fuskeland , G. Galloni , M. Galloway , K. Ganga , M. Gerbino , M. Gervasi , R. T. Génova-Santos , S. Giardiello , C. Gimeno-Amo , E. Gjerløw , R. González González , L. Grandsire , A. Gruppuso , N. W. Halverson , P. Hargrave , S. E. Harper , M. Hazumi , S. Henrot-Versillé , L. T. Hergt , D. Herranz , E. Hivon , R. A. Hlozek , T. D. Hoang , J. Hubmayr , K. Ichiki , K. Ikuma , H. Ishino , G. Jaehnig , B. Jost , K. Kohri , K. Konishi , L. Lamagna , M. Lattanzi , C. Leloup , F. Levrier , A. I. Lonappan , G. Luzzi , J. Macias-Perez , B. Maffei , E. Marchitelli , E. Martínez-González , S. Masi , S. Matarrese , T. Matsumura , S. Micheli , M. Migliaccio , M. Monelli , L. Montier , G. Morgante , L. Mousset , Y. Nagano , R. Nagata , P. Natoli , A. Novelli , F. Noviello , I. Obata , A. Occhiuzzi , K. Odagiri , R. Omae , L. Pagano , A. Paiella , D. Paoletti , G. Pascual-Cisneros , G. Patanchon , V. Pavlidou , F. Piacentini , M. Piat , G. Piccirilli , M. Pinchera , G. Pisano , L. Porcelli , N. Raffuzzi , C. Raum , M. Remazeilles , A. Ritacco , J. Rubino-Martin , M. Ruiz-Granda , Y. Sakurai , G. Savini , D. Scott , Y. Sekimoto , M. Shiraishi , G. Signorelli , S. L. Stever , R. M. Sullivan , A. Suzuki , R. Takaku , H. Takakura , S. Takakura , Y. Takase. A. Tartari , K. Tassis , K. L. Thompson , M. Tomasi , M. Tristram , C. Tucker , L. Vacher , B. van Tent , P. Vielva , K. Watanuki , I. K. Wehus , B. Westbrook , G. Weymann-Despres , B. Winter , E. J. Wollack , A. Zacchei , M. Zannoni , Y. Zhou , the LiteBIRD Collaboration

The LiteBIRD satellite is planned to be launched by JAXA in the late 2020s. Its main purpose is to observe the large-scale B-mode polarization in the Cosmic Microwave Background (CMB) anticipated from the Inflation theory. LiteBIRD will…

Instrumentation and Methods for Astrophysics · Physics 2021-01-22 Mayu Tominaga , Masahiro Tsujimoto , Samantha Lynn Stever , Tommaso Ghigna , Hirokazu Ishino , Ken Ebisawa