Restore the IDL SAVefile by 
> RESTORE, ‘/path to file/BATSE_Catalog.sav’

This will restore 10 IDL structure arrays containing the fluence and peak flux spectral information for each of the 5 spectral models: Band, Comptonized, Gaussian Log, Power Law, and Smoothly Broken Power Law.

Structure names: bandF, bandP, compF, compP, glogF, glogP, plF, plP, sbplF, sbplP

Each file is an array of structures and each structure is stored as:

bandF[i]=

{trig, dets, allTime, [tInt],
[eInt],
[amplitude],
[epeak],
[alpha],
[beta],
chisq, dof,
[pflux],
[eflux],
livetime, {eRange}, {obsRate}, {backRate}, {modelRate}, {obsCounts}, {sigmas}}

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[ ] - 2 element array
{ } - pointer

trig- the BATSE trigger number for each burst

dets- detectors used in the summed fitting. Detectors are represented by numbers 
          0-7 and are concatenated in order of brightest to weakest to form a single 
          string.  Example: detectors 3 & 7 become 37.

allTime- the total amount of time selected for spectral fitting, in seconds.

[tInt]- the convex hull of the lightcurve time selection in seconds relative to the 
          trigger time.

[eInt]- the convex hull of the energy spectrum selection, in keV

[amplitude]- the normalized amplitude and error

[epeak]- the derived Epeak and error, in keV

[alpha]- low energy power law index and error

[beta]- high energy power law index and error

chisq- the chi-square statistic for the model

dof- the degrees of freedom in the fitted model

[pflux]- photon flux and error in the 20-2000 keV range

[eflux]- energy flux and error in the 20-2000 keV range

livetime- the total livetime of the burst, in seconds

{eRange}- array of energy edges corresponding to the energy channels used 
		      in spectral fitting

{obsRate}- array of observed photon rates

{backRate}- array of background rates

{modelRates}- array of background-subtracted model rates

{obsCounts}- array of background-subtracted observed counts in the model

{sigmas}- array of standard errors for each energy channel fitted

----------------------------------------------------------------------------------------------------------------

Examples:
To extract the value of Epeak for the first entry in the catalog for the Band fluence fit:
> print, bandF[0].epeak

To extract the model rates array from the 5th entry in the catalog for the power law peak flux fit:
> print, *(plP[4]).modelRate