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The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization

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arxiv 1802.04594 v1 pith:CUM6AUAX submitted 2018-02-13 astro-ph.CO astro-ph.IM

F. Poidevin , J.A. Rubino-Martin , R. Genova-Santos , R. Rebolo , M. Aguiar , F. Gomez-Renasco , F. Guidi. , C. Gutierrez
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R. J. Hoyland C. Lopez-Caraballo A. Oria Carreras A. E. Pelaez-Santos M. R. Perez-De-Taoro B. Ruiz-Granados D. Tramonte A. Vega-Moreno T. Viera-Curbelo R. Vignaga E. Martinez-Gonzalez R. B. Barreiro B. Casaponsa F. J. Casas J. M. Diego R. Fernandez-Cobos D. Herranz M. Lopez-Caniego D. Ortiz P. Vielva E. Artal B. Aja J. Cagigas J. L. Cano L. De La Fuente A. Mediavilla J. V. Teran E. Villa L. Piccirillo C. Dickinson K. Grainge S. Harper M. Mcculloch S. Melhuish G. Pisano R. A. Watson A. Lasenby M. Ashdown Y. Perrott N. Razavi-Ghods D. Titterington P. Scott
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QUIJOTE (Q-U-I JOint TEnerife) is an experiment designed to achieve CMB B-mode polarization detection and sensitive enough to detect a primordial gravitational-wave component if the B-mode amplitude is larger than r = 0.05. It consists in two telescopes and three instruments observing in the frequency range 10-42 GHz installed at the Teide Observatory in the Canary Islands, Spain. The observing strategy includes three raster scan deep integration fields for cosmology, a nominal wide survey covering the Northen Sky and specific raster scan deep integration observations in regions of specific interest. The main goals of the project are presented and the first scientific results obtained with the first instrument are reviewed.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. B-mode Power Spectrum of CMB via Polarized Compton Scattering

    astro-ph.CO 2019-09 conditional novelty 5.0 of 10

    Compton scattering off partially polarized electrons can generate B-mode polarization from scalar density perturbations, with an amplitude proportional to the square of the electron polarization asymmetry.

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