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The mean and standard deviation of the absolute magnitude residuals, -0.001 and 0.195 mag, respectively, estimated for 224 red clump stars in Laney et al. 2012 are (absolutely) smaller than the corresponding ones estimated by the procedure which adopts a mean $M_{K_s}=-1.613$ mag absolute magnitude for all red clump stars, -0.053 and 0"},"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":"1304.2530","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-04-09T11:01:42Z","cross_cats_sorted":[],"title_canon_sha256":"cee6b2b7b929dde5d57871901ce62c64e0c875bcca59edd95d6b7967b8233c47","abstract_canon_sha256":"f3b6e2535f3bdfc4ce60dbf96da2a22483c555af59eb2f9bb73e204b46d28809"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:41.173765Z","signature_b64":"wuRF1vm17wOdERBhHR1e6Pz90Yo4cJ/UhTS64N64GjS3No/yRoOrPYT/UVQF/NicF0wC0bottjxC3S9WPRA7Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5362754b16cdab16e357cec53e38e0d5e05c60af9f804cb3ad484fa59c9a75e8","last_reissued_at":"2026-05-18T01:50:41.173185Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:41.173185Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Absolute Magnitude Calibration for Red Clump Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"E. 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