AmesPAHdbPythonSuite
  • 1 Installation
  • 2 Usage
  • 3 API
    • 3.1 Main Interface
    • 3.2 Accessing the molecular PAH data
    • 3.3 Working with Molecular PAH Properties
    • 3.4 Working with fundamental vibrational transitions
    • 3.5 Working with Molecular Geometric Data
    • 3.6 Working with Raw Laboratory Spectra
    • 3.7 Working Outside the AmesPAHdbIDLSuite Object Classes
    • 3.8 Creating PAH Spectra
      • 3.8.1 Emission models
      • 3.8.2 Line profiles
    • 3.9 Spectroscopic Database Fitting
      • 3.9.1 Dealing with astronomical observations
      • 3.9.2 Database fitting
      • 3.9.3 Monte Carlo
  • 4 Release History
    • 4.1 v0.5.0 (2022-03-28)
    • 4.2 v0.1.0 (2019-08-20)
  • 5 FAQ
  • src
    • Submodules
    • amespahdb class
      • AmesPAHdb
    • data class
      • Data
    • xmlparser class
      • XMLparser
    • transitions class
      • Transitions
      • Tstar
      • charge
      • energy
      • frequencies
      • frequency
      • intensities
      • nc
      • star_model
    • spectrum class
      • Spectrum
    • coadd class
      • Coadded
    • species class
      • Species
      • formatformula()
    • geometry class
      • Geometry
    • laboratory class
      • Laboratory
    • fitted class
      • Fitted
    • mcfitted class
      • MCFitted
    • observation class
      • Observation
    • Module contents
AmesPAHdbPythonSuite
  • Overview: module code

All modules for which code is available

  • amespahdbpythonsuite.amespahdb
  • amespahdbpythonsuite.coadded
  • amespahdbpythonsuite.data
  • amespahdbpythonsuite.fitted
  • amespahdbpythonsuite.geometry
  • amespahdbpythonsuite.laboratory
  • amespahdbpythonsuite.mcfitted
  • amespahdbpythonsuite.observation
  • amespahdbpythonsuite.species
  • amespahdbpythonsuite.spectrum
  • amespahdbpythonsuite.transitions
  • amespahdbpythonsuite.xmlparser

© Copyright 2019/2021 Dr. Christiaan Boersma, Dr. Matthew J. Shannon, and Dr. Alexandros Maragkoudakis.

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