{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:MN357F5VYOJYXSR4WVBJBYI6Z3","short_pith_number":"pith:MN357F5V","schema_version":"1.0","canonical_sha256":"6377df97b5c3938bca3cb54290e11ecec3a75e81c0c12399fec3c8a4df837772","source":{"kind":"arxiv","id":"2004.12033","version":1},"attestation_state":"computed","paper":{"title":"Ram pressure stripping candidates in the Coma Cluster: Evidence for enhanced star formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ian D. Roberts, Laura C. Parker","submitted_at":"2020-04-25T01:21:29Z","abstract_excerpt":"The Coma cluster is the nearest massive ($M \\gtrsim 10^{15}\\,\\mathrm{M_\\odot}$) galaxy cluster, making it an excellent laboratory to probe the influence of the cluster environment on galaxy star formation. Here, we present a sample of 41 galaxies with disturbed morphologies consistent with ram pressure stripping. These galaxies are identified visually using high-quality, multi-band imaging from the Canada-France-Hawaii telescope covering ~9 $\\mathrm{deg^2}$ of the Coma cluster. These \"stripping candidates\" are clear outliers in common quantitative morphological measures, such as concentration-"},"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":"2004.12033","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-04-25T01:21:29Z","cross_cats_sorted":[],"title_canon_sha256":"e8a71a151a46c19631edc80b6323dc64ae53346518ebe6b1d4c85582fdcd4585","abstract_canon_sha256":"87db327c5d1be94c3d4846a4ffb6f2e69aa0b26d309fed85d67c88f901adf1a3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:02:17.486980Z","signature_b64":"HRSbRMGEh1U5a3LzM8FLUuTBUsWoZ7YKCHdKxr82i3T2tCbHItmOpaMmffnVwsCZX0AqEVEPJBSK9Ppq9igjAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6377df97b5c3938bca3cb54290e11ecec3a75e81c0c12399fec3c8a4df837772","last_reissued_at":"2026-07-05T01:02:17.486567Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:02:17.486567Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Ram pressure stripping candidates in the Coma Cluster: Evidence for enhanced star formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ian D. Roberts, Laura C. Parker","submitted_at":"2020-04-25T01:21:29Z","abstract_excerpt":"The Coma cluster is the nearest massive ($M \\gtrsim 10^{15}\\,\\mathrm{M_\\odot}$) galaxy cluster, making it an excellent laboratory to probe the influence of the cluster environment on galaxy star formation. Here, we present a sample of 41 galaxies with disturbed morphologies consistent with ram pressure stripping. These galaxies are identified visually using high-quality, multi-band imaging from the Canada-France-Hawaii telescope covering ~9 $\\mathrm{deg^2}$ of the Coma cluster. These \"stripping candidates\" are clear outliers in common quantitative morphological measures, such as concentration-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2004.12033","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/2004.12033/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":"2004.12033","created_at":"2026-07-05T01:02:17.486622+00:00"},{"alias_kind":"arxiv_version","alias_value":"2004.12033v1","created_at":"2026-07-05T01:02:17.486622+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2004.12033","created_at":"2026-07-05T01:02:17.486622+00:00"},{"alias_kind":"pith_short_12","alias_value":"MN357F5VYOJY","created_at":"2026-07-05T01:02:17.486622+00:00"},{"alias_kind":"pith_short_16","alias_value":"MN357F5VYOJYXSR4","created_at":"2026-07-05T01:02:17.486622+00:00"},{"alias_kind":"pith_short_8","alias_value":"MN357F5V","created_at":"2026-07-05T01:02:17.486622+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/MN357F5VYOJYXSR4WVBJBYI6Z3","json":"https://pith.science/pith/MN357F5VYOJYXSR4WVBJBYI6Z3.json","graph_json":"https://pith.science/api/pith-number/MN357F5VYOJYXSR4WVBJBYI6Z3/graph.json","events_json":"https://pith.science/api/pith-number/MN357F5VYOJYXSR4WVBJBYI6Z3/events.json","paper":"https://pith.science/paper/MN357F5V"},"agent_actions":{"view_html":"https://pith.science/pith/MN357F5VYOJYXSR4WVBJBYI6Z3","download_json":"https://pith.science/pith/MN357F5VYOJYXSR4WVBJBYI6Z3.json","view_paper":"https://pith.science/paper/MN357F5V","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2004.12033&json=true","fetch_graph":"https://pith.science/api/pith-number/MN357F5VYOJYXSR4WVBJBYI6Z3/graph.json","fetch_events":"https://pith.science/api/pith-number/MN357F5VYOJYXSR4WVBJBYI6Z3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MN357F5VYOJYXSR4WVBJBYI6Z3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MN357F5VYOJYXSR4WVBJBYI6Z3/action/storage_attestation","attest_author":"https://pith.science/pith/MN357F5VYOJYXSR4WVBJBYI6Z3/action/author_attestation","sign_citation":"https://pith.science/pith/MN357F5VYOJYXSR4WVBJBYI6Z3/action/citation_signature","submit_replication":"https://pith.science/pith/MN357F5VYOJYXSR4WVBJBYI6Z3/action/replication_record"}},"created_at":"2026-07-05T01:02:17.486622+00:00","updated_at":"2026-07-05T01:02:17.486622+00:00"}