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To identify their origins, we compare planetary nebulae and neutral hydrogen with faint fuzzy positions and line-of-sight velocities in NGC1023. In this way, we rule out scenarios in which these objects are associated with an on-going merger or with a spheroid population in NGC1023. Their kinematics are indistinguishable from the stellar disk population in this galaxy, and we conclude that faint fuzzies are most likely just remnant open clust"},"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":"1310.4508","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-16T20:03:26Z","cross_cats_sorted":[],"title_canon_sha256":"d163732fe7225ea4a21484f6ddaa5fe5ed8cbb0d6fc6f95971264e52214aa3a1","abstract_canon_sha256":"5293410282c24c04f991f43343b59058d94d3c71642bfc54fc716eba025e491f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:58.652580Z","signature_b64":"JmF37AirMk05KHwC/bHJRenQanO2gp5RZA96goJzPnVXONwnC+zsGxMXVWpNDd0uGKTE+5tb9TmiDOcbLCSDAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"78515f9da58fde20feba4df76748a699017351a2ac1b9f341a7914cc4d3a3ed9","last_reissued_at":"2026-05-18T01:46:58.651972Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:58.651972Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Nature of Faint Fuzzies from the Kinematics of NGC1023","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. 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