CHIANTI-Related Sites

• The Iron Project

  The Iron Project seeks to provide new atomic data for all of the iron ions. Some of this data has already been included in CHIANTI.

• The UK RmaX Network

  This network has been formed to calculate electron and photon collisional properties with atoms and ions for transitions in the soft X-ray region. The UK RmaX Network extends the mission of the Iron Project into the X-ray region.

• The NIST spectroscopic database

  The National Institute of Standards and Technology (NIST) compiles energy levels, wavelengths and transition probabilities for many astrophysically relevant ions. For many of the ions in the CHIANTI database, energy level data has been taken from here.

• The Solar Software Library (SolarSoft)
  

  The CHIANTI database can be found within the SolarSoft system, a programming and data analysis environment for the solar physics community.

• A large list of Databases for Atomic and Plasma Physics
  

  compiled at the Weizmann Institute of Science.

• The Kelly Atomic Line Database

  A comprehensive line list compiled by Dr. R.L.Kelly.

• ATOMDB - APED (Astrophysical Plasma Emission Database)

  - An atomic database developed at the CfA, Harvard-Smithsonian (USA)

• Cloudy

  - Photoionization simulations for the discriminating astrophysicist since 1978

• PINTofALE

  - A Package for Interactive Analysis of Line Emission, developed at CfA, Harvard-Smithsonian (USA)

• XSPEC

  - An X-Ray Spectral Fitting Package developed at HEASARC/GSFC (USA).

• XSTAR

  - A package developed at HEASARC/GSFC (USA) for calculating the physical conditions and emission spectra of photoionized gases.