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The PolarKID project: polarization measurements with KIDs for the next generation of CMB telescopes

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arxiv 2407.10201 v1 pith:YJTEKAMN submitted 2024-07-14 astro-ph.IM

Sofia Savorgnano , Julien Bounmy , Olivier Bourrion , Martino Calvo , Andrea Catalano , Olivier Choulet , Gregory Garde , Anne Gerardin
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Mile Kusulja Juan Francisco Macias Perez Alessandro Monfardini Damien Tourres Francis Vezzu
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keywords kidspolarizationpolarkidprojectsourcesadvantagesb-modesblack
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The goal of the PolarKID project is testing a new method for the measurement of polarized sources, in order to identify all the possible instrumental systematic effects that could impact the detection of CMB B-modes of polarization. It employs the KISS (KIDs Interferometer Spectrum Survey) instrument coupled to a sky simulator and to sources such as point-like black bodies (simulating planets), a dipole (extended source) and a polarizer. We use filled-arrays Lumped Element Kinetic Inductance Detectors (LEKIDs) since they have multiple advantages when observing both in a photometry and in a polarimetry configuration

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