{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:K4M35ZFTMS5JUZUMCAF5NITCEG","short_pith_number":"pith:K4M35ZFT","schema_version":"1.0","canonical_sha256":"5719bee4b364ba9a668c100bd6a26221811f0d36adf5a8a4519fa9b1a58f2a2f","source":{"kind":"arxiv","id":"1804.06669","version":1},"attestation_state":"computed","paper":{"title":"The Red-Giant Branch Bump Revisited: Constraints on Envelope Overshooting in a Wide Range of Masses and Metallicities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrea Miglio, Beno\\^it Mosser, Guy R. Davies, Josefina Montalb\\'an, L\\'eo Girardi, Oliver J. Hall, Saniya Khan","submitted_at":"2018-04-18T12:06:56Z","abstract_excerpt":"The red-giant branch bump provides valuable information for the investigation of the internal structure of low-mass stars. Because current models are unable to accurately predict the occurrence and efficiency of mixing processes beyond convective boundaries, one can use the luminosity of the bump --- a diagnostic of the maximum extension of the convective envelope during the first-dredge up --- as a calibrator for such processes. By combining asteroseismic and spectroscopic constraints, we expand the analysis of the bump to masses and metallicities beyond those previously accessible using glob"},"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":"1804.06669","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-04-18T12:06:56Z","cross_cats_sorted":[],"title_canon_sha256":"b44fbcc8c9e17936ab42b171f50d31339dc7dc858c745cd3b7f88f777227c95c","abstract_canon_sha256":"6c262fffb8def2f5407ae0f9bcd747db4baa20e38142689c1119f1db38254176"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:12:17.511229Z","signature_b64":"sjEFujqZgY88VBY6X+G4zeWieZTjTe16s0WdUy8hrPAb2DiHRTYsWgc9u/8PrJaOe3c7KBTVTLuU65DdJD59Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5719bee4b364ba9a668c100bd6a26221811f0d36adf5a8a4519fa9b1a58f2a2f","last_reissued_at":"2026-05-18T00:12:17.510549Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:12:17.510549Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Red-Giant Branch Bump Revisited: Constraints on Envelope Overshooting in a Wide Range of Masses and Metallicities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrea Miglio, Beno\\^it Mosser, Guy R. Davies, Josefina Montalb\\'an, L\\'eo Girardi, Oliver J. Hall, Saniya Khan","submitted_at":"2018-04-18T12:06:56Z","abstract_excerpt":"The red-giant branch bump provides valuable information for the investigation of the internal structure of low-mass stars. Because current models are unable to accurately predict the occurrence and efficiency of mixing processes beyond convective boundaries, one can use the luminosity of the bump --- a diagnostic of the maximum extension of the convective envelope during the first-dredge up --- as a calibrator for such processes. By combining asteroseismic and spectroscopic constraints, we expand the analysis of the bump to masses and metallicities beyond those previously accessible using glob"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.06669","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1804.06669","created_at":"2026-05-18T00:12:17.510651+00:00"},{"alias_kind":"arxiv_version","alias_value":"1804.06669v1","created_at":"2026-05-18T00:12:17.510651+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1804.06669","created_at":"2026-05-18T00:12:17.510651+00:00"},{"alias_kind":"pith_short_12","alias_value":"K4M35ZFTMS5J","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_16","alias_value":"K4M35ZFTMS5JUZUM","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_8","alias_value":"K4M35ZFT","created_at":"2026-05-18T12:32:33.847187+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG","json":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG.json","graph_json":"https://pith.science/api/pith-number/K4M35ZFTMS5JUZUMCAF5NITCEG/graph.json","events_json":"https://pith.science/api/pith-number/K4M35ZFTMS5JUZUMCAF5NITCEG/events.json","paper":"https://pith.science/paper/K4M35ZFT"},"agent_actions":{"view_html":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG","download_json":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG.json","view_paper":"https://pith.science/paper/K4M35ZFT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1804.06669&json=true","fetch_graph":"https://pith.science/api/pith-number/K4M35ZFTMS5JUZUMCAF5NITCEG/graph.json","fetch_events":"https://pith.science/api/pith-number/K4M35ZFTMS5JUZUMCAF5NITCEG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG/action/storage_attestation","attest_author":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG/action/author_attestation","sign_citation":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG/action/citation_signature","submit_replication":"https://pith.science/pith/K4M35ZFTMS5JUZUMCAF5NITCEG/action/replication_record"}},"created_at":"2026-05-18T00:12:17.510651+00:00","updated_at":"2026-05-18T00:12:17.510651+00:00"}