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

F. Poidevin; J.~A. Rubino-Martin; R. Genova-Santos; R. Rebolo; M. Aguiar; F. Gomez-Renasco; F. Guidi.; C. Gutierrez; 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

doi:10.48550/arXiv.1802.04594

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

F. Poidevin, J.~A. Rubino-Martin, R. Genova-Santos, R. Rebolo, M. Aguiar, F. Gomez-Renasco, F. Guidi., C. Gutierrez, 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. BarreiroB. 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

Department of Physics

Research output: Contribution to journal › Conference article › peer-review

Abstract

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.

Original language	English
Pages (from-to)	arXiv:1802.04594
Journal	arXiv e-prints
DOIs	https://doi.org/10.48550/arXiv.1802.04594
Publication status	Published - 1 Feb 2018

Keywords

Astrophysics - Cosmology and Nongalactic Astrophysics
Astrophysics - Instrumentation and Methods for Astrophysics

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10.48550/arXiv.1802.04594

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Poidevin, F., Rubino-Martin, J. A., Genova-Santos, R., Rebolo, R., Aguiar, M., Gomez-Renasco, F., Guidi., F., Gutierrez, C., Hoyland, R. J., Lopez-Caraballo, C., Oria Carreras, A., Pelaez-Santos, A. E., Perez-De-Taoro, M. R., Ruiz-Granados, B., Tramonte, D., Vega-Moreno, A., Viera-Curbelo, T., Vignaga, R., Martinez-Gonzalez, E., ... Scott, P. (2018). The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization. arXiv e-prints, arXiv:1802.04594. https://doi.org/10.48550/arXiv.1802.04594

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title = "The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization",

abstract = "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.",

keywords = "Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics",

author = "F. Poidevin and J.~A. Rubino-Martin and R. Genova-Santos and R. Rebolo and M. Aguiar and F. Gomez-Renasco and F. Guidi. and C. Gutierrez and R.~J. Hoyland and C. Lopez-Caraballo and {Oria Carreras}, A. and A.~E. Pelaez-Santos and M.~R. Perez-De-Taoro and B. Ruiz-Granados and D. Tramonte and A. Vega-Moreno and T. Viera-Curbelo and R. Vignaga and E. Martinez-Gonzalez and R.~B. Barreiro and B. Casaponsa and F.~J. Casas and J.~M. Diego and R. Fernandez-Cobos and D. Herranz and M. Lopez-Caniego and D. Ortiz and P. Vielva and E. Artal and B. Aja and J. Cagigas and J.~L. Cano and {De La Fuente}, L. and A. Mediavilla and J.~V. Teran and E. Villa and L. Piccirillo and C. Dickinson and K. Grainge and S. Harper and M. Mcculloch and S. Melhuish and G. Pisano and R.~A. Watson and A. Lasenby and M. Ashdown and Y. Perrott and N. Razavi-Ghods and D. Titterington and P. Scott",

year = "2018",

month = feb,

day = "1",

doi = "10.48550/arXiv.1802.04594",

language = "English",

pages = "arXiv:1802.04594",

journal = "arXiv e-prints",

}

Poidevin, F, Rubino-Martin, JA, Genova-Santos, R, Rebolo, R, Aguiar, M, Gomez-Renasco, F, Guidi., F, Gutierrez, C, Hoyland, RJ, Lopez-Caraballo, C, Oria Carreras, A, Pelaez-Santos, AE, Perez-De-Taoro, MR, Ruiz-Granados, B, Tramonte, D, Vega-Moreno, A, Viera-Curbelo, T, Vignaga, R, Martinez-Gonzalez, E, Barreiro, RB, Casaponsa, B, Casas, FJ, Diego, JM, Fernandez-Cobos, R, Herranz, D, Lopez-Caniego, M, Ortiz, D, Vielva, P, Artal, E, Aja, B, Cagigas, J, Cano, JL, De La Fuente, L, Mediavilla, A, Teran, JV, Villa, E, Piccirillo, L, Dickinson, C, Grainge, K, Harper, S, Mcculloch, M, Melhuish, S, Pisano, G, Watson, RA, Lasenby, A, Ashdown, M, Perrott, Y, Razavi-Ghods, N, Titterington, D & Scott, P 2018, 'The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization', arXiv e-prints, pp. arXiv:1802.04594. https://doi.org/10.48550/arXiv.1802.04594

TY - JOUR

T1 - The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization

AU - Poidevin, F.

AU - Rubino-Martin, J.~A.

AU - Genova-Santos, R.

AU - Rebolo, R.

AU - Aguiar, M.

AU - Gomez-Renasco, F.

AU - Guidi., F.

AU - Gutierrez, C.

AU - Hoyland, R.~J.

AU - Lopez-Caraballo, C.

AU - Oria Carreras, A.

AU - Pelaez-Santos, A.~E.

AU - Perez-De-Taoro, M.~R.

AU - Ruiz-Granados, B.

AU - Tramonte, D.

AU - Vega-Moreno, A.

AU - Viera-Curbelo, T.

AU - Vignaga, R.

AU - Martinez-Gonzalez, E.

AU - Barreiro, R.~B.

AU - Casaponsa, B.

AU - Casas, F.~J.

AU - Diego, J.~M.

AU - Fernandez-Cobos, R.

AU - Herranz, D.

AU - Lopez-Caniego, M.

AU - Ortiz, D.

AU - Vielva, P.

AU - Artal, E.

AU - Aja, B.

AU - Cagigas, J.

AU - Cano, J.~L.

AU - De La Fuente, L.

AU - Mediavilla, A.

AU - Teran, J.~V.

AU - Villa, E.

AU - Piccirillo, L.

AU - Dickinson, C.

AU - Grainge, K.

AU - Harper, S.

AU - Mcculloch, M.

AU - Melhuish, S.

AU - Pisano, G.

AU - Watson, R.~A.

AU - Lasenby, A.

AU - Ashdown, M.

AU - Perrott, Y.

AU - Razavi-Ghods, N.

AU - Titterington, D.

AU - Scott, P.

PY - 2018/2/1

Y1 - 2018/2/1

N2 - 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.

AB - 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.

KW - Astrophysics - Cosmology and Nongalactic Astrophysics

KW - Astrophysics - Instrumentation and Methods for Astrophysics

U2 - 10.48550/arXiv.1802.04594

DO - 10.48550/arXiv.1802.04594

M3 - Conference article

SP - arXiv:1802.04594

JO - arXiv e-prints

JF - arXiv e-prints

ER -

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

Abstract

Keywords

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