{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:7DMMHK67NIN3C7QQXVE63QJDHH","short_pith_number":"pith:7DMMHK67","schema_version":"1.0","canonical_sha256":"f8d8c3abdf6a1bb17e10bd49edc12339fafcc346d5f3eeca089d35ac34e30414","source":{"kind":"arxiv","id":"astro-ph/0610088","version":1},"attestation_state":"computed","paper":{"title":"Ram Pressure Stripping in Clusters and Groups","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"J. A. Hester","submitted_at":"2006-10-03T18:39:50Z","abstract_excerpt":"Ram pressure stripping is an important process in the evolution of both dwarf galaxies and large spirals. Large spirals are severely stripped in rich clusters and may be mildly stripped in groups. Dwarf galaxies can be severely stripped in both clusters and groups. A model is developed that describes the stripping of a satellite galaxy's outer H \\textsc{i} disk and hot galactic halo. The model can be applied to a wide range of environments and satellite galaxy masses. Whether ram pressure stripping of the outer disk or hot galactic halo occurs is found to depend primarily on the ratio of the s"},"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":"astro-ph/0610088","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-10-03T18:39:50Z","cross_cats_sorted":[],"title_canon_sha256":"ea8751d5a74fa587bc447121dfbd184ced0b86f5e7560a5575a660cca4df6cad","abstract_canon_sha256":"85752d06b97e1f62bc2b8c76da0349feaf585861bea3cf7dcba9fba67365705d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:28:57.518293Z","signature_b64":"oIpTue+A4jJww7jiVSkKrt/Tre2qnl7TrThIE3A+8rWsqalLPYu+2bFfRoDvZrtoE4hZl9NdVkPy/djdmp7nAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f8d8c3abdf6a1bb17e10bd49edc12339fafcc346d5f3eeca089d35ac34e30414","last_reissued_at":"2026-05-18T04:28:57.517923Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:28:57.517923Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Ram Pressure Stripping in Clusters and Groups","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"J. A. Hester","submitted_at":"2006-10-03T18:39:50Z","abstract_excerpt":"Ram pressure stripping is an important process in the evolution of both dwarf galaxies and large spirals. Large spirals are severely stripped in rich clusters and may be mildly stripped in groups. Dwarf galaxies can be severely stripped in both clusters and groups. A model is developed that describes the stripping of a satellite galaxy's outer H \\textsc{i} disk and hot galactic halo. The model can be applied to a wide range of environments and satellite galaxy masses. Whether ram pressure stripping of the outer disk or hot galactic halo occurs is found to depend primarily on the ratio of the s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0610088","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":"astro-ph/0610088","created_at":"2026-05-18T04:28:57.517982+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0610088v1","created_at":"2026-05-18T04:28:57.517982+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0610088","created_at":"2026-05-18T04:28:57.517982+00:00"},{"alias_kind":"pith_short_12","alias_value":"7DMMHK67NIN3","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"7DMMHK67NIN3C7QQ","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"7DMMHK67","created_at":"2026-05-18T12:25:53.939244+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.18229","citing_title":"An extreme ram-pressure stripping event in a protocluster at redshift 4.3","ref_index":6,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH","json":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH.json","graph_json":"https://pith.science/api/pith-number/7DMMHK67NIN3C7QQXVE63QJDHH/graph.json","events_json":"https://pith.science/api/pith-number/7DMMHK67NIN3C7QQXVE63QJDHH/events.json","paper":"https://pith.science/paper/7DMMHK67"},"agent_actions":{"view_html":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH","download_json":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH.json","view_paper":"https://pith.science/paper/7DMMHK67","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0610088&json=true","fetch_graph":"https://pith.science/api/pith-number/7DMMHK67NIN3C7QQXVE63QJDHH/graph.json","fetch_events":"https://pith.science/api/pith-number/7DMMHK67NIN3C7QQXVE63QJDHH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH/action/storage_attestation","attest_author":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH/action/author_attestation","sign_citation":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH/action/citation_signature","submit_replication":"https://pith.science/pith/7DMMHK67NIN3C7QQXVE63QJDHH/action/replication_record"}},"created_at":"2026-05-18T04:28:57.517982+00:00","updated_at":"2026-05-18T04:28:57.517982+00:00"}