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Improved Data Reduction for Far‐Infrared/Submillimeter Polarimetry

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC(2005)

Univ Chicago

Cited 11|Views22
Abstract
Fluctuations in atmospheric emission introduce noise and systematic errors into measurements of polarization at far‐infrared and submillimeter wavelengths. We describe a new analysis method that corrects for the bias and reduces the errors caused by the fluctuations. The method exploits repeated observations of a source and is especially effective on faint sources for which the polarized flux is on the same order as the atmospheric fluctuations.
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