WINGSPAN: A WINdows Gamma-ray SPectral Analysis program

Details WINGSPAN: A WINdows Gamma-ray SPectral Analysis program WINGSPAN: A WINdows Gamma-ray SPectral Analysis program

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ascl.soft10007p&link_type=abstract

Astrophysics Source Code Library, record ascl:9910.007

Astronomy and Astrophysics

Astrophysics

Scientific paper

WINGSPAN is a program written to analyze spectral data from the Burst and Transient Source Experiment (BATSE) on NASA's Compton Gamma-Ray Observatory. Data files in the FITS (BFITS) format are suitable for input into the program. WINGSPAN can be used to view and manipulate event time histories or count spectra, and also has the capability to perform spectral deconvolution via a standard forward folding model fitting technique (Levenberg-Marquardt algorithm). Although WINGSPAN provides many functions for data manipulation, the program was designed to allow users to easily plug in their own external IDL routines. These external routines have access to all data read from the FITS files, as well as selection intervals created in the main part of WINGSPAN (background intervals and model, etc).

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