{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:77EFIJQUZRI2TY7QKLNQZLBDIR","short_pith_number":"pith:77EFIJQU","schema_version":"1.0","canonical_sha256":"ffc8542614cc51a9e3f052db0cac23446786cfdc7cefd48cffcf9402c48b99cc","source":{"kind":"arxiv","id":"2308.01931","version":1},"attestation_state":"computed","paper":{"title":"Identifying parent bodies of meteorites among near-Earth asteroids","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Albino Carbognani, Marco Fenucci","submitted_at":"2023-08-02T15:48:39Z","abstract_excerpt":"Meteorites provide an important source of information about the formation and composition of asteroids, because the level of accuracy of studies and analyses performed in a laboratory cannot be achieved by any ground or space based observation. To better understand what asteroid types a meteorite represents, it is crucial to identify the body they originated from. In this paper, we aim to determine possible parent bodies for the known meteorite falls among the known population of near-Earth asteroids (NEAs). By using the similarity criterion $D_N$, based on geocentric quantities, we found 20 p"},"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":"2308.01931","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-08-02T15:48:39Z","cross_cats_sorted":[],"title_canon_sha256":"38caaa5871ba67b8183afdfafcffd150786476c7cb56a6a14c54bfa2470a0ea9","abstract_canon_sha256":"2c62ed00b0dbb28670c2b6a7717f04763afcb7121cf0911dbe31a69c06722cda"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:39:54.936544Z","signature_b64":"cJTOLV3ZSr8gpKrSA92Zjbqevx59ZnwIWil7BdFQWKzG317BxfDP9ui7pAkXnQvqoBOajXjn6YQNgQTl/Aj8DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ffc8542614cc51a9e3f052db0cac23446786cfdc7cefd48cffcf9402c48b99cc","last_reissued_at":"2026-07-05T06:39:54.936113Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:39:54.936113Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Identifying parent bodies of meteorites among near-Earth asteroids","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Albino Carbognani, Marco Fenucci","submitted_at":"2023-08-02T15:48:39Z","abstract_excerpt":"Meteorites provide an important source of information about the formation and composition of asteroids, because the level of accuracy of studies and analyses performed in a laboratory cannot be achieved by any ground or space based observation. To better understand what asteroid types a meteorite represents, it is crucial to identify the body they originated from. In this paper, we aim to determine possible parent bodies for the known meteorite falls among the known population of near-Earth asteroids (NEAs). By using the similarity criterion $D_N$, based on geocentric quantities, we found 20 p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.01931","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2308.01931/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2308.01931","created_at":"2026-07-05T06:39:54.936178+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.01931v1","created_at":"2026-07-05T06:39:54.936178+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.01931","created_at":"2026-07-05T06:39:54.936178+00:00"},{"alias_kind":"pith_short_12","alias_value":"77EFIJQUZRI2","created_at":"2026-07-05T06:39:54.936178+00:00"},{"alias_kind":"pith_short_16","alias_value":"77EFIJQUZRI2TY7Q","created_at":"2026-07-05T06:39:54.936178+00:00"},{"alias_kind":"pith_short_8","alias_value":"77EFIJQU","created_at":"2026-07-05T06:39:54.936178+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.09712","citing_title":"The fall of asteroid 2024 XA$_1$ and the location of possible meteorites","ref_index":7,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR","json":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR.json","graph_json":"https://pith.science/api/pith-number/77EFIJQUZRI2TY7QKLNQZLBDIR/graph.json","events_json":"https://pith.science/api/pith-number/77EFIJQUZRI2TY7QKLNQZLBDIR/events.json","paper":"https://pith.science/paper/77EFIJQU"},"agent_actions":{"view_html":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR","download_json":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR.json","view_paper":"https://pith.science/paper/77EFIJQU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.01931&json=true","fetch_graph":"https://pith.science/api/pith-number/77EFIJQUZRI2TY7QKLNQZLBDIR/graph.json","fetch_events":"https://pith.science/api/pith-number/77EFIJQUZRI2TY7QKLNQZLBDIR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR/action/storage_attestation","attest_author":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR/action/author_attestation","sign_citation":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR/action/citation_signature","submit_replication":"https://pith.science/pith/77EFIJQUZRI2TY7QKLNQZLBDIR/action/replication_record"}},"created_at":"2026-07-05T06:39:54.936178+00:00","updated_at":"2026-07-05T06:39:54.936178+00:00"}