The HERSCHEL/PACS Spectrometer Pipeline

Details The HERSCHEL/PACS Spectrometer Pipeline The HERSCHEL/PACS Spectrometer Pipeline

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..411..478s&link_type=abstract

Astronomical Data Analysis Software and Systems XVIII ASP Conference Series, Vol. 411, proceedings of the conference held 2-5 No

Astronomy and Astrophysics

Astronomy

2

Scientific paper

ESA's Herschel Space Observatory, to be launched in 2009, is the first space observatory covering the full far-infrared and sub-millimeter wavelength range (60 - 670 micron). The Photodetector Array Camera & Spectrometer (PACS) is one of the three science instruments. It employs two Ge:Ga photoconductor arrays and two bolometer arrays to perform integral field spectroscopy and imaging photometry in the 60 - 210 micron wavelength band. The interactive PACS Spectrometer and Photometer \citep{wieprecht09} Data Reduction Pipeline is integrated in the Herschel Data Processing System.
The DP is implemented using Java technology and written in a common effort by the HERSCHEL Science Center (HSC) and the three instrument teams. We overview the concept and status of the PACS Spectrometer Data Reduction Pipeline. Additionally, we address the instrument mode-dependent data processing and the definition of the products of the different processing levels. Finally, we show first results by applying the pipeline on flight model instrument level test data.

Affiliated with

Also associated with

No associations

Rating

The HERSCHEL/PACS Spectrometer Pipeline does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The HERSCHEL/PACS Spectrometer Pipeline, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The HERSCHEL/PACS Spectrometer Pipeline will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-834637