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POINT_SOURCE_POL

Dual-beam spectropolarimetry data can be reduced using the POINT_SOURCE_POL recipe. This recipe reduces data using the steps in Sections [*], [*], and [*]. The data can be taken in any order between waveplate positions, but corresponding object-sky pairs for a given waveplate position must be observed together. Spectrum extraction is done such that separate E and O beam spectra are created for each waveplate position. After a cycle of eight observations has done, corresponding to one object-sky pair at each of the 0-, 45-, 22.5-, and 67.5-degree waveplate angles, the pipeline calculates the I, Q, and U Stokes parameters, from which the percentage polarization, polarization intensity, and polarization angle spectra are calculated.



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ORAC-DR -- spectroscopy data reduction
Starlink User Note 236
Paul Hirst
Brad Cavanagh
Joint Astronomy Centre, Hilo, Hawaii
October 2005
E-mail:ussc@star.rl.ac.uk

Copyright © 2005 Particle Physics and Astronomy Research Council