{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:V3Z2AFDHMSEYVCMU6BPLGADQVQ","short_pith_number":"pith:V3Z2AFDH","schema_version":"1.0","canonical_sha256":"aef3a0146764898a8994f05eb30070ac17b3d35158b37f26dce41fd5ec3c401d","source":{"kind":"arxiv","id":"2211.12297","version":1},"attestation_state":"computed","paper":{"title":"The spatially resolved view of star formation in galaxy clusters","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bianca M. Poggianti, the GASP team","submitted_at":"2022-11-22T14:28:49Z","abstract_excerpt":"Integral field spectroscopic studies of galaxies in dense environments, such as clusters and groups of galaxies, have provided new insights for understanding how star formation proceeds, and quenches. I present the spatially resolved view of the star formation activity and its link with the multiphase gas in cluster galaxies based on MUSE and multi-wavelength data of the GASP survey. I discuss the link among the different scales (i.e. the link between the spatially resolved and the global star formation rate-stellar mass relation), the spatially resolved signatures and the quenching histories "},"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":"2211.12297","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-11-22T14:28:49Z","cross_cats_sorted":[],"title_canon_sha256":"8fe6a5d1a537b1a7d56b96486751587c061673ac0ada91d0eb820363fcf2e472","abstract_canon_sha256":"b833d5b112c25ab7ddeefd79bd9902aa451605d7bbb6c41a04fad4b74da92b91"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:25:15.754924Z","signature_b64":"21+KCnUTSMAU3redfTnAcZ45NmVwqJ0Ii7brXFcbuc11eDs81KqsnKU53otRqFb+9hgZPaq1IM4dDzxv38BlCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aef3a0146764898a8994f05eb30070ac17b3d35158b37f26dce41fd5ec3c401d","last_reissued_at":"2026-07-05T06:25:15.754505Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:25:15.754505Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The spatially resolved view of star formation in galaxy clusters","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bianca M. Poggianti, the GASP team","submitted_at":"2022-11-22T14:28:49Z","abstract_excerpt":"Integral field spectroscopic studies of galaxies in dense environments, such as clusters and groups of galaxies, have provided new insights for understanding how star formation proceeds, and quenches. I present the spatially resolved view of the star formation activity and its link with the multiphase gas in cluster galaxies based on MUSE and multi-wavelength data of the GASP survey. I discuss the link among the different scales (i.e. the link between the spatially resolved and the global star formation rate-stellar mass relation), the spatially resolved signatures and the quenching histories "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.12297","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/2211.12297/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":"2211.12297","created_at":"2026-07-05T06:25:15.754560+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.12297v1","created_at":"2026-07-05T06:25:15.754560+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.12297","created_at":"2026-07-05T06:25:15.754560+00:00"},{"alias_kind":"pith_short_12","alias_value":"V3Z2AFDHMSEY","created_at":"2026-07-05T06:25:15.754560+00:00"},{"alias_kind":"pith_short_16","alias_value":"V3Z2AFDHMSEYVCMU","created_at":"2026-07-05T06:25:15.754560+00:00"},{"alias_kind":"pith_short_8","alias_value":"V3Z2AFDH","created_at":"2026-07-05T06:25:15.754560+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.15983","citing_title":"MeerKAT Discovery of an Infalling Cold Gas Tail onto the Nearby Barred Spiral Galaxy, NGC 5643","ref_index":67,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ","json":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ.json","graph_json":"https://pith.science/api/pith-number/V3Z2AFDHMSEYVCMU6BPLGADQVQ/graph.json","events_json":"https://pith.science/api/pith-number/V3Z2AFDHMSEYVCMU6BPLGADQVQ/events.json","paper":"https://pith.science/paper/V3Z2AFDH"},"agent_actions":{"view_html":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ","download_json":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ.json","view_paper":"https://pith.science/paper/V3Z2AFDH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.12297&json=true","fetch_graph":"https://pith.science/api/pith-number/V3Z2AFDHMSEYVCMU6BPLGADQVQ/graph.json","fetch_events":"https://pith.science/api/pith-number/V3Z2AFDHMSEYVCMU6BPLGADQVQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ/action/storage_attestation","attest_author":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ/action/author_attestation","sign_citation":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ/action/citation_signature","submit_replication":"https://pith.science/pith/V3Z2AFDHMSEYVCMU6BPLGADQVQ/action/replication_record"}},"created_at":"2026-07-05T06:25:15.754560+00:00","updated_at":"2026-07-05T06:25:15.754560+00:00"}