Downloads provided by UsageCountsThe QUIJOTE-CMB experiment: studying the polarisation of the galactic and cosmological microwave emissions
Copyright policy ) Rubino-Martin J. A.; Rebolo R.; Aguiar M.; Genova-Santos R.; Gomez-Renasco F.; Herreros J. M.; Hoyland R. J.; +40 Authors
Rubino-Martin J. A.; Rebolo R.; Aguiar M.; Genova-Santos R.; Gomez-Renasco F.; Herreros J. M.; Hoyland R. J.; Lopez-Caraballo C.; Pelaez Santos A. E.; De La Rosa V. S.; Vega-Moreno A.; Viera-Curbelo T.; Martinez-Gonzalez E.; Barreiro R. B.; Casas F. J.; Diego J. M.; Fernandez-Cobos R.; Herranz D.; Lopez-Caniego M.; Ortiz D.; Vielva P.; Artal E.; Aja B.; Cagigas J.; Cano J. L.; De La Fuente L.; Mediavilla A.; Teran J. V.; Villa E.; Piccirillo L.; Battye R.; Blackhurst E.; Brown M.; Davies R. D.; Davis R. J.; Dickinson C.; Harper S.; Maffei B.; McCulloch M.; Melhuish S.; Pisano G.; Watson R. A.; Hobson M.; Grainge K.; Lasenby A.; Saunders R.; Scott P.;
The QUIJOTE-CMB experiment: studying the polarisation of the galactic and cosmological microwave emissions
The QUIJOTE (Q-U-I JOint Tenerife) CMB Experiment will operate at the Teide Observatory with the aim of characterizing the polarisation of the CMB and other processes of Galactic and extragalactic emission in the frequency range of 10–40 GHz and at large and medium angular scales. The first of the two QUIJOTE telescopes and the first multi-frequency (10–30 GHz) instrument are already built and have been tested in the laboratory. QUIJOTE-CMB will be a valuable complement at low frequencies for the Planck mission, and will have the required sensitivity to detect a primordial gravitational-wave component if the tensor-to-scalar ratio is larger than r = 0.05.
Partial financial support is provided by the Spanish Ministry of Economy and Competitiveness (MINECO) under the projects AYA2010-21766-C03 (01, 02 and 03), and also by the Consolider-Ingenio project CSD2010-00064 (EPI: Exploring the Physics of Inflation).
Trabajo presentado a la conferencia: "Ground-based and Airborne Telescopes IV" (Poster session: Concepts for future telescopes) celebrada en Amsterdam (Holanda) el 1 de julio de 2012.-- et al.
Peer Reviewed
United Kingdom, United Kingdom, Italy
- University of Manchester United Kingdom
- University of Manchester United Kingdom
- University of La Laguna Spain
- University of Cantabria Spain
- Spanish National Research Council Spain
cosmic microwave background, Cosmological parameters, wmap, Early universe, polarisation, telescope, Early Universe, Cosmic microwave background, background power spectrum, anisotropy-probe, perseus molecular-complex, Cosmic microwave background; Cosmological parameters; Early universe; Instrumentation; Polarisation; Telescope, cosmological parameters, sky, Instrumentation, Telescope, Polarisation, instrumentation, cosmosomas experiment, early universe, ghz, small array, constraints, Telescopes
cosmic microwave background, Cosmological parameters, wmap, Early universe, polarisation, telescope, Early Universe, Cosmic microwave background, background power spectrum, anisotropy-probe, perseus molecular-complex, Cosmic microwave background; Cosmological parameters; Early universe; Instrumentation; Polarisation; Telescope, cosmological parameters, sky, Instrumentation, Telescope, Polarisation, instrumentation, cosmosomas experiment, early universe, ghz, small array, constraints, Telescopes
selected citations These citations are derived from selected sources.This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).44 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Top 10% influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Top 10% impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Top 10% views 108 downloads 180 - 108views180downloads
selected citations
Citations provided by BIP!
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Citations provided by BIP!popularityPopularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP!influenceInfluence provided by BIP!
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Influence provided by BIP!impulseImpulse provided by BIP!
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
Impulse provided by BIP!viewsViews provided by UsageCounts
Views provided by UsageCountsdownloadsDownloads provided by UsageCounts
Downloads provided by UsageCounts 44
Top 10%
Top 10%
Top 10%
108
180
Green
Beta
Fields of Science
Related to Research communities
STARS EU