{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:6YQZ64A2IEH2QIJSWLRBURTKYO","short_pith_number":"pith:6YQZ64A2","schema_version":"1.0","canonical_sha256":"f6219f701a410fa82132b2e21a466ac3b91fd4a98c7aacea37b5e19b972525ae","source":{"kind":"arxiv","id":"2605.24174","version":1},"attestation_state":"computed","paper":{"title":"The Sensitivity of Substructure Lensing to SIDM Core-collapse Model Variation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Andrew Benson, Annika H. G. Peter, Birendra Dhanasingham, Charlie Mace, Francis-Yan Cyr-Racine, Xiaolong Du, Zhichao Carton Zeng","submitted_at":"2026-05-22T19:48:35Z","abstract_excerpt":"Strong gravitational lensing has emerged as a powerful probe of dark matter substructure, and shows particularly strong promise as a test of self-interacting dark matter (SIDM). The compact halos produced by SIDM can leave distinct imprints on lensing observations, but the core-collapse timeline for subhalos is difficult to model accurately. This difficulty is an obstacle to accurate substructure lensing predictions, where small variations in core-collapsing subhalos can lead to significant differences in the lensing power. To quantify this problem and inform future lensing analyses, we test v"},"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":"2605.24174","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-22T19:48:35Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"698b985b036bbbe12dfa5744dfda291716267c5b61b1c8229f6761174895aebc","abstract_canon_sha256":"1f40577c6bb51456a0c45bc2e69a50418085e9be5a10502b6e37f5604876bf1b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-26T01:02:50.641191Z","signature_b64":"UE4pP+TDEHDT8y353P5bvBoRZbU/7qq8AkE8q8myBsYWoyNosfu+UJ9fZHgux9OvEczR8uTIXlaJNPUBF2jQAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f6219f701a410fa82132b2e21a466ac3b91fd4a98c7aacea37b5e19b972525ae","last_reissued_at":"2026-05-26T01:02:50.640332Z","signature_status":"signed_v1","first_computed_at":"2026-05-26T01:02:50.640332Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Sensitivity of Substructure Lensing to SIDM Core-collapse Model Variation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Andrew Benson, Annika H. G. Peter, Birendra Dhanasingham, Charlie Mace, Francis-Yan Cyr-Racine, Xiaolong Du, Zhichao Carton Zeng","submitted_at":"2026-05-22T19:48:35Z","abstract_excerpt":"Strong gravitational lensing has emerged as a powerful probe of dark matter substructure, and shows particularly strong promise as a test of self-interacting dark matter (SIDM). The compact halos produced by SIDM can leave distinct imprints on lensing observations, but the core-collapse timeline for subhalos is difficult to model accurately. This difficulty is an obstacle to accurate substructure lensing predictions, where small variations in core-collapsing subhalos can lead to significant differences in the lensing power. To quantify this problem and inform future lensing analyses, we test v"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.24174","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/2605.24174/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":"2605.24174","created_at":"2026-05-26T01:02:50.640474+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.24174v1","created_at":"2026-05-26T01:02:50.640474+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.24174","created_at":"2026-05-26T01:02:50.640474+00:00"},{"alias_kind":"pith_short_12","alias_value":"6YQZ64A2IEH2","created_at":"2026-05-26T01:02:50.640474+00:00"},{"alias_kind":"pith_short_16","alias_value":"6YQZ64A2IEH2QIJS","created_at":"2026-05-26T01:02:50.640474+00:00"},{"alias_kind":"pith_short_8","alias_value":"6YQZ64A2","created_at":"2026-05-26T01:02:50.640474+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/6YQZ64A2IEH2QIJSWLRBURTKYO","json":"https://pith.science/pith/6YQZ64A2IEH2QIJSWLRBURTKYO.json","graph_json":"https://pith.science/api/pith-number/6YQZ64A2IEH2QIJSWLRBURTKYO/graph.json","events_json":"https://pith.science/api/pith-number/6YQZ64A2IEH2QIJSWLRBURTKYO/events.json","paper":"https://pith.science/paper/6YQZ64A2"},"agent_actions":{"view_html":"https://pith.science/pith/6YQZ64A2IEH2QIJSWLRBURTKYO","download_json":"https://pith.science/pith/6YQZ64A2IEH2QIJSWLRBURTKYO.json","view_paper":"https://pith.science/paper/6YQZ64A2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.24174&json=true","fetch_graph":"https://pith.science/api/pith-number/6YQZ64A2IEH2QIJSWLRBURTKYO/graph.json","fetch_events":"https://pith.science/api/pith-number/6YQZ64A2IEH2QIJSWLRBURTKYO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6YQZ64A2IEH2QIJSWLRBURTKYO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6YQZ64A2IEH2QIJSWLRBURTKYO/action/storage_attestation","attest_author":"https://pith.science/pith/6YQZ64A2IEH2QIJSWLRBURTKYO/action/author_attestation","sign_citation":"https://pith.science/pith/6YQZ64A2IEH2QIJSWLRBURTKYO/action/citation_signature","submit_replication":"https://pith.science/pith/6YQZ64A2IEH2QIJSWLRBURTKYO/action/replication_record"}},"created_at":"2026-05-26T01:02:50.640474+00:00","updated_at":"2026-05-26T01:02:50.640474+00:00"}