To resample data and its errors linearly in log space, interpolation can be applied to both the data and its associated errors. The discussion highlights the importance of treating errors similarly to the original data during the resampling process. Concerns are raised about the legitimacy of interpolating experimental errors, particularly in the context of astronomical spectra. The conversation suggests that rebinning from linear to logarithmic scales while maintaining signal-to-noise ratios is a common practice, despite potential criticisms. An example of using the IRAF package for this purpose is also mentioned.