stability_of_fit_a_spectrum.pro

This is an example of testing the stability of fitting an astronomical spectrum by iteratively removing the most contributing PAH species from a subsequent fit, built around the functionality provided by the AmesPAHdbIDLSuite and should help confirm that the it has been properly installed. The source code is annotated to guide users and developers in the inner workings of the suite.

Updated versions of the NASA Ames PAH IR Spectroscopic Database and more information can be found at: www.astrochemistry.org/pahdb.