{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:Y5BVFQA2QIBXOFZYOIGJRARBP3","short_pith_number":"pith:Y5BVFQA2","schema_version":"1.0","canonical_sha256":"c74352c01a8203771738720c9882217eda6ceabc506553b3009fde651e54b3f1","source":{"kind":"arxiv","id":"1411.2604","version":1},"attestation_state":"computed","paper":{"title":"Extended, Dusty Star Formation Fueled by a Residual Cooling Flow in the Cluster of Galaxies Sersic 159-03","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. B. R. Oonk, M. McDonald, N. Werner, S. Veilleux","submitted_at":"2014-11-10T21:02:13Z","abstract_excerpt":"While the cooling of the hot intra-cluster medium (ICM) in the cores of galaxy clusters is mostly counteracted by heating from the central active galactic nucleus (AGN), the balance is not perfect. This can lead to residual cooling flows and low-level star formation, the physics of which is not well understood. Here we present a detailed study of the residual cooling flow in the center of the low mass galaxy cluster Sersic 159-03 (A S1101) using far-ultraviolet imaging from the Hubble Space Telescope and far-infrared (FIR) spectroscopy and photometry from the Herschel space observatory, along "},"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":"1411.2604","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-10T21:02:13Z","cross_cats_sorted":[],"title_canon_sha256":"7bb4f426966e2cafc68bb516cdd5e19c76d76da191687f8a30cd2b96f96dabdc","abstract_canon_sha256":"ee74fb527c97a9e5805adaf758778a5ded6d45339ea10b3a5bbd014b565b9c6e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:33.445302Z","signature_b64":"Fbfup4k8/md7dntk1z+WL4/IFxCSi9Tu62WYZXQIsE/RMdqFeYfYxFDJAZtszQ7vDFtZT+6ZKYmMD2Ew7OE/Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c74352c01a8203771738720c9882217eda6ceabc506553b3009fde651e54b3f1","last_reissued_at":"2026-05-18T01:41:33.444700Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:33.444700Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Extended, Dusty Star Formation Fueled by a Residual Cooling Flow in the Cluster of Galaxies Sersic 159-03","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. B. R. Oonk, M. McDonald, N. Werner, S. Veilleux","submitted_at":"2014-11-10T21:02:13Z","abstract_excerpt":"While the cooling of the hot intra-cluster medium (ICM) in the cores of galaxy clusters is mostly counteracted by heating from the central active galactic nucleus (AGN), the balance is not perfect. This can lead to residual cooling flows and low-level star formation, the physics of which is not well understood. Here we present a detailed study of the residual cooling flow in the center of the low mass galaxy cluster Sersic 159-03 (A S1101) using far-ultraviolet imaging from the Hubble Space Telescope and far-infrared (FIR) spectroscopy and photometry from the Herschel space observatory, along "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.2604","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":"1411.2604","created_at":"2026-05-18T01:41:33.444816+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.2604v1","created_at":"2026-05-18T01:41:33.444816+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.2604","created_at":"2026-05-18T01:41:33.444816+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y5BVFQA2QIBX","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y5BVFQA2QIBXOFZY","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y5BVFQA2","created_at":"2026-05-18T12:28:57.508820+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/Y5BVFQA2QIBXOFZYOIGJRARBP3","json":"https://pith.science/pith/Y5BVFQA2QIBXOFZYOIGJRARBP3.json","graph_json":"https://pith.science/api/pith-number/Y5BVFQA2QIBXOFZYOIGJRARBP3/graph.json","events_json":"https://pith.science/api/pith-number/Y5BVFQA2QIBXOFZYOIGJRARBP3/events.json","paper":"https://pith.science/paper/Y5BVFQA2"},"agent_actions":{"view_html":"https://pith.science/pith/Y5BVFQA2QIBXOFZYOIGJRARBP3","download_json":"https://pith.science/pith/Y5BVFQA2QIBXOFZYOIGJRARBP3.json","view_paper":"https://pith.science/paper/Y5BVFQA2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.2604&json=true","fetch_graph":"https://pith.science/api/pith-number/Y5BVFQA2QIBXOFZYOIGJRARBP3/graph.json","fetch_events":"https://pith.science/api/pith-number/Y5BVFQA2QIBXOFZYOIGJRARBP3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y5BVFQA2QIBXOFZYOIGJRARBP3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y5BVFQA2QIBXOFZYOIGJRARBP3/action/storage_attestation","attest_author":"https://pith.science/pith/Y5BVFQA2QIBXOFZYOIGJRARBP3/action/author_attestation","sign_citation":"https://pith.science/pith/Y5BVFQA2QIBXOFZYOIGJRARBP3/action/citation_signature","submit_replication":"https://pith.science/pith/Y5BVFQA2QIBXOFZYOIGJRARBP3/action/replication_record"}},"created_at":"2026-05-18T01:41:33.444816+00:00","updated_at":"2026-05-18T01:41:33.444816+00:00"}