A New Way to Reduce Spitzer 160 micron Data

Details A New Way to Reduce Spitzer 160 micron Data A New Way to Reduce Spitzer 160 micron Data

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.4701f&link_type=abstract

American Astronomical Society, AAS Meeting #211, #47.01; Bulletin of the American Astronomical Society, Vol. 39, p.803

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a new pipeline to reduce 160 micron data taken with the MIPS detector on-board Spitzer. Starting from raw data, our pipeline is able to correct short- and long-term transients that severely limit the quality of standard reductions. Transients occurring in the signal after a sudden change in the incident flux are fitted using a physical model and removed from the data. Flux calibration has been recomputed for our pipeline. A few examples from archival data featuring deep surveys and pointed observations are shown to compare the quality of our reduction with standard available pipelines.

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