p3d to run in windows online over linux online

We have hosted the application p3d to run in windows online over linux online in order to run this application in our online workstations with Wine or directly.

Quick description about p3d to run in windows online over linux online:

p3d is a general data-reduction tool for use with fiber-fed integral-field spectrographs (IFSs); although, the spectrum viewer works with spectrum data cubes of any origin. The tool is built about the proprietary software IDL (Harris/EXELIS; see http: //www.harrisgeospatial.com), but can be used without any license. Most slowly running loops are implemented in parallelized C (OpenMP).

Features:

• p3d works on all platforms supported by IDL.
• p3d can be used with full functionality without an IDL license.
• Optimal extraction, including correction for so-called cross-talk.
• Flux calibration can be done both interactively and non interactively.
• Can correct data for differential atmospheric refraction.
• Single images are cleaned of cosmic-ray hits - using IFS-specific approaches that work paricularly well with oversampled data.
• Time-consuming tasks are implemented in (automatically) compiled C, using OpenMP.
• Information on all operations are (optionally) saved to log files.
• p3d currently supports thirteen IFUs - more can be added on request.
• Calar Alto 3.5m / PMAS (LARR+PPAK, old and new CCD).
• McDonald Observatory 2.7m / VIRUS-P (fiber bundles 1,2, and VP2.7).
• McDonald Observatory 2.7m / VIRUS-W.
• AAT 3.9m / AAOMEGA/SAMI (basic support, could be improved upon request)
• AAT 3.9m / AAOMEGA/SPIRAL (blue and red arms).
• ESO VLT/UT3 / VIMOS (all HR and MR-modes, old and new configurations).
• ESO VLT/UT2 / FLAMES (the ARGUS IFU, and the two mini-IFUs).
• BTA 6m / MPFS (the new CCD).
• WHT 4m / INTEGRAL/SB1-3 (both the old and the new CCDs).
• Gemini North and South 8m / GMOS-N and GMOS-S (one-slit modes).
• ERA2 / An AIP integral-field spectrograph for life sciences.
• Allows use of either a master-bias image or prescan and overscan bias regions.
• The spectrum viewer can be used with all output of the "CALIFA" data-reduction pipeline.
• The spectrum viewer accepts reduced data cubes of the MUSE pipeline (all sizes, RAM permitting; no args. required).
• All IDL source files have the prefix p3d_, i.e. no interference with other IDL programs.
• Output data cubes (ver. >=2.2) can be viewed with the ESO / CASA viewer.
• Tutorials for: data-reduction, visualization, and p3d setup.
• Contains tool to generate simulated data.

Audience: Science/Research.
User interface: Console/Terminal, Other toolkit, Motif/LessTif.
Programming Language: Unix Shell, C, IDL.

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