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Our final relations have the form <MW1> = gamma(W1) - (2.381 +/- 0.097) log PF + (0.096 +/- 0.021)[Fe/H] and <MW2> = gamma(W2)-(2.269 +/- 0.127)log PF + (0.108 +/- 0.021)[Fe/H], where [Fe/H] values are on the scale of Carretta et al. (2009). We obtained two appreciably discrepant estimates for the zero points gamma(W1) and gamma(W2) of both relations: one based on a statistical-parallax ana"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1401.5523","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-01-22T00:02:30Z","cross_cats_sorted":[],"title_canon_sha256":"56fe166cfa5a1759bd79fa9369b3153919df09ac876e1f2f4fa3203d4ad8066b","abstract_canon_sha256":"245fe410a73709df9805a23ec1a19d0c57f71229be4fd308d532f2078b4a61f5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:56:58.165820Z","signature_b64":"2gXdZOloAxDhBkSrw/p+ZOTQCMPwt+IcTi+RgSfTOnd9IdnILcT1u5H9qJuRu8XTaPFtL4vvhu+aE7dEEBUuAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2235f7578ee400f90872c67f783a6fafbb0077034f2db50fb7ddeb2205e5142d","last_reissued_at":"2026-05-18T02:56:58.165304Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:56:58.165304Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Mid-infrared PL relations for Globular Cluster RR Lyrae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. 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