Processing Steps and Signal Analysis of ISOPHOT Polarisation Observations at 170 micron

Details Processing Steps and Signal Analysis of ISOPHOT Polarisation Observations at 170 micron Processing Steps and Signal Analysis of ISOPHOT Polarisation Observations at 170 micron

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.435...27l&link_type=abstract

WORKSHOP ON ISO POLARISATION OBSERVATIONS. Eds. R.J. Laureijs & R. Siebenmorgen. ESA-SP 435, p. 27

Astronomy and Astrophysics

Astronomy

Iso, Infrared Astronomy, Polarisation

Scientific paper

We present a detailed description of the structure and performance of the ISO astronomical observing template PHT51 which was used to measure the polarisation of astronomical targets in the far-infrared at 170 μm. We describe the data processing steps up to the mean signal per measurement. Special attention is given to the assessment of the instrumental stability and consistency. We have evaluated all background observations obtained with PHT51 in order to derive the instrumental polarisation. The results are compared with the previous assessment.

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