GUPPI#
The Green Bank Ultimate Pulsar Processing Instrument (GUPPI) was previously the main pulsar backend for the GBT. It is retired as of January 2021 and has been replaced by VEGAS Pulsar Modes (VPM).
Transitioning from GUPPI to VPM#
Experienced pulsar observers will recognize that GUPPI and VPM observing are very similar, especially the parameters used in scheduling blocks. The following table summarizes the similarities and some differences between GUPPI and VPM.
Astrid: Most "guppi." parameters can be replaced with "vegas.". The exceptions are guppi.datadisk,
which has no VPM equivalent.
File names: VPM output file names include a new element, the number of seconds after midnight UTC.
vegas_<MJD>_<secUTC>_<sourceName>_<scanNumber>_<fileNumber>.fits
vegas_<MJD>_<secUTC>_<sourceName>_cal_<scanNumber>_<fileNumber>.fits
The table below can be used a cheat-sheet for navigating between some common GUPPI and VPM tasks.
GUPPI Tool or Procedure |
VEGAS Tool or Procedure |
Notes |
|---|---|---|
|
VEGAS Data Monitor |
Data monitor updates continuously; No need to pause a scheduling block to check ADC levels. |
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Must be run from the appropriate VEGAS HPC (e.g. |
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Can be run from any computer. |
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Web interface is preferred; Must be run from the appropriate VEGAS HPC (e.g. |
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Used to find mode-dependent timing offsets. |
Firefox is recommended (Google Chrome does not always update properly) |
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Firefox is recommended (Google Chrome does not always update properly) |
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Output directory for incoherent dedispersion modes. |
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Output directory for coherent dedispersion modes. |
Note
The asterisk denotes a shortcut for /lustre/gbtdata.