Difference: HipeWhatsNew9x (58 vs. 59)

Revision 592012-07-20 - DavideRizzo

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META TOPICPARENT name="HipeWhatsNew"

What's new in HIPE 9

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  HIFI
Changed:
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  • HIFI level 2.5 product introduced: for Spectral Scans it holds the deconvolved single sideband soluions; for Maps it holds the cubes; for all cases it holds a copy of the level 2 HTP.
  • Addition of an interactive pipeline between level 2 and 2.5, which allows the insertion of tasks like fitHifiFringe and fitBaseline into the pipeline between level 2 and 2.5.
  • Browse products for spectral scans and maps added
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>
  • HIFI level 2.5 product introduced. For Spectral Scans it holds the deconvolved single sideband solutions; for Maps it holds the cubes; for all cases it holds a copy of the level 2 HTP.
  • New interactive pipeline between level 2 and 2.5. This allows the insertion of tasks like fitHifiFringe and fitBaseline into the pipeline between level 2 and 2.5.
  • Browse products added. For spectral scans and maps.
  PACS
Changed:
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  • Photometer: Addressing additional specific cases in new interactive pipeline scripts
  • Spectrometer
    • Improved pipeline processing for better reliability of broadband features
    • Improved spectral flatfielding for wide spectral ranges (e.g. SED)
    • Correction for flux losses due to pointing jitter
  • Convolution kernels for photometer and spectrometer maps, aiding the interpretation of extended and point sources
  • Reduction in memory consumption (TBS) when pipeline processing
>
>
  • Photometer. Addressing additional specific cases in new interactive pipeline scripts.
  • Spectrometer pipeline processing. Improved pipeline processing for better reliability of broadband features.
  • Spectral flatfielding. Improved spectral flatfielding for wide spectral ranges (e.g. SED).
  • Flux losses. Correction for flux losses due to pointing jitter.
  • Convolution kernels. For photometer and spectrometer maps, aiding the interpretation of extended and point sources.
  SPIRE
Changed:
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  • common (both Photometer and Spectrometer)
    • improved processing speed using multi-threading
    • improved task for correction of "cooler burps"
    • PcalTask can now remove noise due to pointing (prevalent in really bright sources) and process Brigh mode Pcal flashes
  • Photometer
    • Pipeline Processing
      • improved error maps (possibly as an option)
      • improved baseline correction using "destriper“
    • Interactive processing
      • source timeline fitter task
      • improvements to bolometer finder tool
      • selection of turnaround data in map creation
  • Spectrometer
    • Pipeline Processing: smaller size for level 1 products
    • Improved calibration and data processing
      • updated point source calibration (improved Uranus model)
      • updated bright mode calibration (better PCAL module)
      • improved calibration for Low Resolution observations (hopefully improved calibration, but at minimum, updated advice)
      • more straightforward calling sequence for phase-correction task
      • corrected spectral averaging - more flexible usage
    • Interactive processing
      • drag and drop from SDS Explorer detector layout to variables tab
      • new and updated useful scripts for background subtraction and spectral noise
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>
  • Faster processing. Improved processing speed using multi-threading.
  • Cooler burps. Improved task for correction of cooler burps.
  • Photometer pipeline processing. Improved error maps and baseline correction.
  • Spectrometer calibration. Improved point source and bright mode calibration. Better calibration for low resolution observations.
  • Spectrometer scripts. New and updated useful scripts for background subtraction and spectral noise.
 

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