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In a previous comment (arXiv:0806.1341v1) we criticized purely technicalaspects of arXiv:0712.1645 but pointed out that many other inconsistencies werereadily apparent. In view of the imminent posting of another version ofarXiv:0712.1645, still containing these issues, we would like to offer withthis additional note a critical guide to the methodology followed by the TEXONOcollaboration, in their effort to extract dark matter limits from a spectralregion completely dominated by electronic noise. We find that systematics havebeen neglected through a combination of erroneous assumptions and failure toexplore all of their possible sources.

Additional Comments on "New Limits on Spin-Independent Couplings of Low-Mass WIMP Dark Matter with a Germanium Detector at a Threshold of 200 eV"