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Description
Is there the ability to convert a Spectrum1D object's spectral axis from linear to log space (and reverse), with flux conservation? I have seen other issues (e.g. #255) discussing resampling/rebinning with or without flux conservation, but I haven't seen this particular case discussed. There are probably numerous implementations of this case out there (e.g. Michele Cappellari's ppxf package has a function called log_rebin - online docs here), would be great to have this integrated into specutils. Its a common step in a lot of analysis that involved radial velocities.