Open a FITS file with columns containing variable-length arrays.
ABOUT THE DATA: To illustrate such a case we use a Redistribution Matrix File (RMF) conform with the HEASARC OGIP specifications OGIP definition https://heasarc.gsfc.nasa.gov/docs/heasarc/ofwg/docs/spectra/ogip_92_007/ogip_92_007.html RMF defintion https://heasarc.gsfc.nasa.gov/docs/heasarc/caldb/docs/memos/cal_gen_92_002/cal_gen_92_002.html#tth_sEc3.1
Variable-length arrays are used to return the non-null row elements of a sparse matrix containing the probability of detecting a photon of a given energy at a given detector channel.
The test data file, rmf.fits, is taken from the test data of the sherpa X-ray analysis tools https://cxc.harvard.edu/sherpa/ the original file is available under the repository https://github.com/sherpa/sherpa-test-data
Definition in file FITS_tutorial8.C.