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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 3 CONTRIBUTI IN ATTI DI CONVEGNO (Proceedings)
  4. 3.01 Contributi in Atti di convegno
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/28446
Title: The STRIP instrument of the Large Scale Polarization Explorer: microwave eyes to map the Galactic polarized foregrounds
Authors: Franceschet, Cristian
Realini, Sabrina
MENNELLA, ANIELLO
Addamo, Giuseppe
Baú, Alessandro
BATTAGLIA, PAOLA MARIA 
Bersanelli, Marco
Caccianiga, Barbara
Caprioli, Silvia
Cavaliere, Francesco
Cleary, Kieran A.
CUTTAIA, FRANCESCO 
Del Torto, Francesco
Fafone, Viviana
Farooqui, Zunnoorain
Génova Santos, Ricardo T.
Gaier, Todd C.
Gervasi, Massimo
Ghigna, Tommaso
INCARDONA, FEDERICO
IOVENITTI, SIMONE
Jones, Mike
Kangaslahti, Pekka
Mainini, Roberto
Maino, Davide
MARIS, Michele 
Mena, Patricio
Molina, Rocío.
MORGANTE, GIANLUCA 
Passerini, Andrea
Perez-de-Taoro, Maria del Rosario
Peverini, Oscar A.
Pezzotta, Federico
Pincella, Claudio
Reyes, Nicolás.
Rocchi, Alessio
Rubiño-Martín, José A.
SANDRI, MAURA 
SARTOR, Stefano 
Soria, Mary
Tapia, Valeria
TERENZI, LUCA 
Tomasi, Maurizio
Tommasi, Elisabetta
Viganó, Daniele M.
VILLA, FABRIZIO 
Virone, Giuseppe
VOLPE, ANGELA
Watkins, Bob
ZACCHEI, Andrea 
Zannoni, Mario
Issue Date: 2018
Volume: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
Editors: Zmuidzinas, Jonas; Gao, Jian-Rong
Series: PROCEEDINGS OF SPIE 
Number: 10708
First Page: 107081G
Abstract: In this paper we discuss the latest developments of the STRIP instrument of the "Large Scale Polarization Explorer" (LSPE) experiment. LSPE is a novel project that combines ground-based (STRIP) and balloon-borne (SWIPE) polarization measurements of the microwave sky on large angular scales to attempt a detection of the "B-modes" of the Cosmic Microwave Background polarization. STRIP will observe approximately 25% of the Northern sky from the "Observatorio del Teide" in Tenerife, using an array of forty-nine coherent polarimeters at 43 GHz, coupled to a 1.5 m fully rotating crossed-Dragone telescope. A second frequency channel with six-elements at 95 GHz will be exploited as an atmospheric monitor. At present, most of the hardware of the STRIP instrument has been developed and tested at sub-system level. System-level characterization, starting in July 2018, will lead STRIP to be shipped and installed at the observation site within the end of the year. The on-site verification and calibration of the whole instrument will prepare STRIP for a 2-years campaign for the observation of the CMB polarization.
Conference Name: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
Conference Place: Austin, Texas, United States
Conference Date: 10-15 June, 2018
URI: http://hdl.handle.net/20.500.12386/28446
URL: http://arxiv.org/abs/1812.03687v1
https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10708/2313558/The-STRIP-instrument-of-the-Large-Scale-Polarization-Explorer/10.1117/12.2313558.short?SSO=1
ISSN: 0277-786X
ISBN: 9781510619692
9781510619708
DOI: 10.1117/12.2313558
Bibcode ADS: 2018SPIE10708E..1GF
Fulltext: open
Appears in Collections:3.01 Contributi in Atti di convegno

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