Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010a%26a...514a..70a&link_type=abstract
Astronomy and Astrophysics, Volume 514, id.A70
Astronomy and Astrophysics
Astrophysics
9
Ism: Supernova Remnants, Polarization, Cosmology: Cosmic Background Radiation
Scientific paper
Context. CMB experiments aiming at a precise measurement of the CMB polarization, such as the Planck satellite, need a strong polarized absolute calibrator on the sky to accurately set the detectors polarization angle and the cross-polarization leakage. As the most intense polarized source in the microwave sky at angular scales of few arcminutes, the Crab nebula will be used for this purpose. Aims: Our goal was to measure the Crab nebula polarization characteristics at 90 GHz with unprecedented precision. Methods: The observations were carried out with the IRAM 30 m telescope employing the correlation polarimeter XPOL and using two orthogonally polarized receivers. Results: We processed the Stokes I, Q, and U maps from our observations in order to compute the polarization angle and linear polarization fraction. The first is almost constant in the region of maximum emission in polarization with a mean value of αSky = 152.1±0.3° in equatorial coordinates, and the second is found to reach a maximum of Π = 30% for the most polarized pixels. We find that a CMB experiment having a 5 arcmin circular beam will see a mean polarization angle of αSky = 149.9±0.2° and a mean polarization fraction of Π = 8.8±0.2%.
Aumont J.
Conversi Luca
Falgarone Edith
Macías-Pérez Juan Francisco
Piacentini Fabrizio
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