An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.
Naval Research Laboratory (USA) -
Universita' degli Studi di Firenze (Italy) -
University of Cambridge (UK)
Rutherford Appleton Laboratory (UK)
CHIANTI and Other Codes
CHIANTI data are included (directly or indirectly) in many other spectral codes, such as:
XSTAR - A
package developed at HEASARC/GSFC (USA) for calculating the physical conditions and
emission spectra of photoionized gases.
APED (Astrophysical Plasma Emission Database)
- An atomic database developed at the CfA, Harvard-Smithsonian (USA)
XSPEC - An X-Ray Spectral Fitting Package developed at HEASARC/GSFC (USA).
CHIANTI data have recently been used via APED.
However, we will soon provide FITS files
that can directly be used within XSPEC.
PINTofALE - A Package for Interactive Analysis of Line
Emission, developed at CfA, Harvard-Smithsonian (USA)
Arcetri Spectral Code
- Initially developed by Massimo Landini and Brunella Monsignori-Fossi
in the 70s and continuously updated, this spectral code consists of tables of emissivity for line and continuum
as a function of density and temperature in the 1-2000 Å. The emissivities are mostly calculated with CHIANTI data.