CLOVER Experiment: the receiver block

G. Pisano; P.A.R. Ade; C. Calderon; A.D. Challinor; P. De Bernardis; L. Dunlop; W.K. Gear; Y. Giraud-Héraud; D.J. Goldie; K.J.B. Grainge; K.G. Isaak; B. Johnson; M.E. Jones; A.N. Lasenby; B. Maffei; P.D. Mauskopf; S.J. Melhuish; A. Orlando; L. Piccirillo; A.C. Taylor; S. Withington; G. Yassin

HAL : in2p3-00025437, version 1

DOI : 10.1051/eas:2005038

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Dome C Astronomy and Astrophysics Meeting, Toulouse : France (2004)

CLOVER Experiment: the receiver block

G. Pisano, P.A.R. Ade, C. Calderon, A.D. Challinor, P. De Bernardis, L. Dunlop, W.K. Gear, Y. Giraud-Héraud¹, D.J. Goldie, K.J.B. Grainge, K.G. Isaak, B. Johnson, M.E. Jones, A.N. Lasenby, B. Maffei, P.D. Mauskopf, S.J. Melhuish, A. Orlando, L. Piccirillo, A.C. Taylor, S. Withington, G. Yassin

(2005)

The C$_{\it l}$OVER instrument (described elsewhere in this volume) is being built to measure the B-mode polarisation of the Cosmic Microwave Background. Each of the 256 pixels is made up a pseudo-correlation receiver that can be realised using either waveguide or microstrip technology. In this work we present a design study for a possible waveguide-based solution. Each of the individual components has been optimised using electromagnetic finite-element modelling software (HFSS).

1 :	APC - AstroParticule et Cosmologie

équipe(s) de recherche : APC - Cosmologie et Gravitation

Thème(s)

Physique/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique


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