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Welcome!

  • PypeIt Code of Conduct
  • Installation
  • What’s New in PypeIt
  • Troubleshooting and Known Issues

Quickstart & Tutorials

  • Cookbook
  • Tutorials
  • Quick-Look Reductions
  • Example Data
  • Reduction Tips

Core Processing

  • Setup
  • User-level Parameters
  • Execution
  • Outputs
  • QA
  • Step-by-step Processing

Processing Details

  • Calibrations
  • Combining Science Exposures
  • Object Finding
  • Sky Subtraction
  • Extraction
  • A-B image differencing

Further Processing

  • Fluxing
  • Coadd 1D Spectra
  • Telluric Correction
  • Collating 1D Spectra
  • Coadd 2D Spectra
  • Coadd 3D Spectra

Reference

  • User-level Parameters
  • Input File Format
  • PypeIt Reduction File
  • PypeIt Conventions
  • Spectrographs
  • Detector Specifications
  • Detector Mosaics
  • Frame Types
  • Command-line Scripts
  • Bitmasks

Project Information

  • PypeIt Governance Structure
  • PypeIt Advisory Council (PAC) Charter
  • PypeIt Team

For Developers

  • Development Guidelines
    • Installing and working with your fork
    • Persistent and development branches
    • Development Principles and Communication
    • Testing
    • Workflow
    • Pull Request Acceptance Requirements
    • Tagging Protocol
      • DOI
      • Additional Developer Links
        • MetaData
        • Developing New PypeIt Scripts
        • New Spectrograph
        • PypeIt Development Reports
        • How to manually update the PypeIt conda-forge feedstock (what to do if the bots are broken)
        • Creating archival sensitivity functions
        • Flux Calibration
  • Adding a New Spectrograph
  • API
PypeIt
  • Development Procedures and Guidelines
  • PypeIt Development Reports
  • View page source

PypeIt Development Reports

The following is a list of reports generated for instrument-specific development of PypeIt.

  • Automated typing of DEIMOS frames
  • Automated typing of Keck/MOSFIRE frames
  • Automated typing of NIRES frames
  • Slitmask ID assignment and missing slits
  • Automated sorting of DEIMOS frames by instrument configuration
  • Automated sorting of Keck/MOSFIRE frames by instrument configuration
  • Automated sorting of Keck/NIRES frames by instrument configuration
  • RA, Dec and object name assignment to 1D extracted spectra
  • DEIMOS Wavelength Calibration
  • Object position on the slit from slitmask design

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