NIKA is a dual-band camera operating with 315 frequency multiplexed LEKIDs cooled at 100 mK. NIKA is designed to observe the sky in intensity and polarisation at 150 and 260 GHz from the IRAM 30-m telescope. It is a test-bench for the final NIKA2 camera. The incoming linear polarisation is modulated at four times the mechanical rotation frequency by a warm rotating multi-layer half- wave plate. Then, the signal is analyzed by a wire grid and finally absorbed by the lumped element kinetic inductance detectors (LEKIDs). The small time constant (<1 ms ) of the LEKIDs combined with the modulation of the HWP enables the quasi-simultaneous measurement of the three Stokes parameters I, Q, U, representing linear polarisation. In this paper, we present the results of recent observational campaigns demonstrating the good performance of NIKA in detecting polarisation at millimeter wavelength.

First Polarised Light with the NIKA Camera / Ritacco, A; Adam, R.; Adane, A.; Ade, P.; André, P.; Beelen, A.; Belier, B.; Benoît, A.; Bideaud, A.; Billot, N.; Bourrion, O.; Calvo, Martino; Catalano, A.; Coiffard, G.; Comis, B.; D'Addabbo, Antonio; Désert, F. X.; Doyle, S.; Goupy, J.; Kramer, C.; Leclercq, S.; Macías Pérez, J. F.; Martino, J.; Mauskopf, Philip; Maury, A.; Mayet, F.; Monfardini, A.; Pajot, F.; Pascale, Enzo; Perotto, L.; Pisano, Giampaolo; Ponthieu, N.; Rebolo Iglesias, M.; Revéret, V.; Rodriguez, L.; Savini, Giorgio; Schuster, K.; Sievers, A.; Thum, C.; Triqueneaux, S.; Tucker, C.; Zylka, R.. - In: JOURNAL OF LOW TEMPERATURE PHYSICS. - ISSN 0022-2291. - 184:3-4(2016), pp. 724-732. [10.1007/s10909-015-1340-8]

First Polarised Light with the NIKA Camera

CALVO, MARTINO;D'ADDABBO, ANTONIO;MAUSKOPF, PHILIP;PASCALE, ENZO;PISANO, Giampaolo;SAVINI, Giorgio;
2016

Abstract

NIKA is a dual-band camera operating with 315 frequency multiplexed LEKIDs cooled at 100 mK. NIKA is designed to observe the sky in intensity and polarisation at 150 and 260 GHz from the IRAM 30-m telescope. It is a test-bench for the final NIKA2 camera. The incoming linear polarisation is modulated at four times the mechanical rotation frequency by a warm rotating multi-layer half- wave plate. Then, the signal is analyzed by a wire grid and finally absorbed by the lumped element kinetic inductance detectors (LEKIDs). The small time constant (<1 ms ) of the LEKIDs combined with the modulation of the HWP enables the quasi-simultaneous measurement of the three Stokes parameters I, Q, U, representing linear polarisation. In this paper, we present the results of recent observational campaigns demonstrating the good performance of NIKA in detecting polarisation at millimeter wavelength.
2016
KIDs; Millimeter astronomy; NIKA; Polarisation; Atomic and Molecular Physics, and Optics; Materials Science (all); Condensed Matter Physics
01 Pubblicazione su rivista::01a Articolo in rivista
First Polarised Light with the NIKA Camera / Ritacco, A; Adam, R.; Adane, A.; Ade, P.; André, P.; Beelen, A.; Belier, B.; Benoît, A.; Bideaud, A.; Billot, N.; Bourrion, O.; Calvo, Martino; Catalano, A.; Coiffard, G.; Comis, B.; D'Addabbo, Antonio; Désert, F. X.; Doyle, S.; Goupy, J.; Kramer, C.; Leclercq, S.; Macías Pérez, J. F.; Martino, J.; Mauskopf, Philip; Maury, A.; Mayet, F.; Monfardini, A.; Pajot, F.; Pascale, Enzo; Perotto, L.; Pisano, Giampaolo; Ponthieu, N.; Rebolo Iglesias, M.; Revéret, V.; Rodriguez, L.; Savini, Giorgio; Schuster, K.; Sievers, A.; Thum, C.; Triqueneaux, S.; Tucker, C.; Zylka, R.. - In: JOURNAL OF LOW TEMPERATURE PHYSICS. - ISSN 0022-2291. - 184:3-4(2016), pp. 724-732. [10.1007/s10909-015-1340-8]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/958841
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