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A coherent polarimeter array for the Large Scale Polarization Explorer balloon experiment
- Source :
- SPIE Conference Astronomical Telescopes + instrumentation, Amsterdam, 1-6 July 2012, info:cnr-pdr/source/autori:M. Bersanelli, A. Mennella, G. Morgante, M. Zannoni, G. Addamo, A. Baschirotto, P. Battaglia, A. Bau, B. Cappellini, F. Cavaliere, F. Cuttaia, F. Del Torto, S. Donzelli, Z. Farooqui, M. Frailis, C. Franceschet, E. Franceschi, T. Gaier, S. Galeotta, M. Gervasi, A. Gregorio, P. Kangaslahti, N. Krachmalnico, C. Lawrence, G. Maggio, R. Mainini, D. Maino, N. Mandolesi, B. Paroli, A. Passerini, O. A. Peverini, S. Poli, S. Ricciardi, M. Rossetti, M. Sandri, M. Seiert, L. Stringhetti, A. Tartari, R. Tascone, D. Tavagnacco, L. Terenzi, M. Tomasi, E. Tommasi, F. Villa, G. Virone, A. Zacchei/congresso_nome:SPIE Conference Astronomical Telescopes + instrumentation/congresso_luogo:Amsterdam/congresso_data:1-6 July 2012/anno:2012/pagina_da:/pagina_a:/intervallo_pagine
- Publication Year :
- 2012
-
Abstract
- We discuss the design and expected performance of STRIP (STRatospheric Italian Polarimeter), an array of coherent receivers designed to fly on board the LSPE (Large Scale Polarization Explorer) balloon experiment. The STRIP focal plane array comprises 49 elements in Q band and 7 elements in W-band using cryogenic HEMT low noise amplifiers and high performance waveguide components. In operation, the array will be cooled to 20 K and placed in the focal plane of a $\sim 0.6$ meter telescope providing an angular resolution of $\sim1.5$ degrees. The LSPE experiment aims at large scale, high sensitivity measurements of CMB polarization, with multi-frequency deep measurements to optimize component separation. The STRIP Q-band channel is crucial to accurately measure and remove the synchrotron polarized component, while the W-band channel, together with a bolometric channel at the same frequency, provides a crucial cross-check for systematic effects.<br />In press on the Proceedings of the SPIE Conference Astronomical Telescopes + instrumentation 2012, Amsterdam, paper 8446-279
- Subjects :
- Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Cosmic microwave background
Radiometers
FOS: Physical sciences
law.invention
Telescope
FIS/05 - ASTRONOMIA E ASTROFISICA
Optics
Q band
CMB physic
Settore FIS/05 - Astronomia e Astrofisica
law
CMB physics
STRIP instrument
Instrumentation and Methods for Astrophysics (astro-ph.IM)
astrophysics: instrumentation and methods for astrophysics
astrophysics: cosmology and extragalactic astrophysics
Physics
business.industry
Amplifier
Bolometer
Cosmology, CMB, Polarization, Millimetric, Stratospheric Balloon
Astrophysics::Instrumentation and Methods for Astrophysics
Polarimeter
Polarization (waves)
LSPE
Cardinal point
business
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Cosmology and Nongalactic Astrophysics
Subjects
Details
- Database :
- OpenAIRE
- Journal :
- SPIE Conference Astronomical Telescopes + instrumentation, Amsterdam, 1-6 July 2012, info:cnr-pdr/source/autori:M. Bersanelli, A. Mennella, G. Morgante, M. Zannoni, G. Addamo, A. Baschirotto, P. Battaglia, A. Bau, B. Cappellini, F. Cavaliere, F. Cuttaia, F. Del Torto, S. Donzelli, Z. Farooqui, M. Frailis, C. Franceschet, E. Franceschi, T. Gaier, S. Galeotta, M. Gervasi, A. Gregorio, P. Kangaslahti, N. Krachmalnico, C. Lawrence, G. Maggio, R. Mainini, D. Maino, N. Mandolesi, B. Paroli, A. Passerini, O. A. Peverini, S. Poli, S. Ricciardi, M. Rossetti, M. Sandri, M. Seiert, L. Stringhetti, A. Tartari, R. Tascone, D. Tavagnacco, L. Terenzi, M. Tomasi, E. Tommasi, F. Villa, G. Virone, A. Zacchei/congresso_nome:SPIE Conference Astronomical Telescopes + instrumentation/congresso_luogo:Amsterdam/congresso_data:1-6 July 2012/anno:2012/pagina_da:/pagina_a:/intervallo_pagine
- Accession number :
- edsair.doi.dedup.....64f68684ff22a1c907228450a339d4ec