{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:J4LS4XJRIDANVZ3X3CSAZ6UDZ7","short_pith_number":"pith:J4LS4XJR","schema_version":"1.0","canonical_sha256":"4f172e5d3140c0dae777d8a40cfa83cff8eff1b94768256ec155de4b35c22bb2","source":{"kind":"arxiv","id":"2307.16107","version":1},"attestation_state":"computed","paper":{"title":"Fermi-LAT detection of A new starburst galaxy candidate: IRAS 13052-5711","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Qingquan Jiang, Xiaofei Lan, Yunchuan Xiang","submitted_at":"2023-07-30T02:15:34Z","abstract_excerpt":"A likely starburst galaxy (SBG), IRAS 13052-5711, which is the most distant SBG candidate discovered to date, was found by analyzing 14.4 years of data from the Fermi large-area telescope (Fermi-LAT). This SBG's significance level is approximately 6.55$\\sigma$ in the 0.1-500 GeV band. Its spatial position is close to that of 4FGL J1308.9-5730, determined from the Fermi large telescope fourth-source Catalog (4FGL). Its power-law spectral index is approximately 2.1, and its light curve (LC) for 14.4 years has no significant variability. These characteristics are highly similar to those of SBGs f"},"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":"2307.16107","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-07-30T02:15:34Z","cross_cats_sorted":[],"title_canon_sha256":"4f65b4dd959edccc2bae2b719ce6ff256966c7ed6a23b017acbaa8b448dfe287","abstract_canon_sha256":"b5f96c9f14f7d671235f11767d9eac6fd4f3a073f41bfec7d041d524e764a306"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:41:21.824175Z","signature_b64":"5NaysRlE7YMkRt5EgjFzyH5rr2HADdGRdWZpp1646m5xCKYxmMKooESt2ColYkPi8wjVFZupaBs3gXiKs/TRBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4f172e5d3140c0dae777d8a40cfa83cff8eff1b94768256ec155de4b35c22bb2","last_reissued_at":"2026-07-05T06:41:21.823725Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:41:21.823725Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fermi-LAT detection of A new starburst galaxy candidate: IRAS 13052-5711","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Qingquan Jiang, Xiaofei Lan, Yunchuan Xiang","submitted_at":"2023-07-30T02:15:34Z","abstract_excerpt":"A likely starburst galaxy (SBG), IRAS 13052-5711, which is the most distant SBG candidate discovered to date, was found by analyzing 14.4 years of data from the Fermi large-area telescope (Fermi-LAT). This SBG's significance level is approximately 6.55$\\sigma$ in the 0.1-500 GeV band. Its spatial position is close to that of 4FGL J1308.9-5730, determined from the Fermi large telescope fourth-source Catalog (4FGL). Its power-law spectral index is approximately 2.1, and its light curve (LC) for 14.4 years has no significant variability. These characteristics are highly similar to those of SBGs f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.16107","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/2307.16107/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":"2307.16107","created_at":"2026-07-05T06:41:21.823788+00:00"},{"alias_kind":"arxiv_version","alias_value":"2307.16107v1","created_at":"2026-07-05T06:41:21.823788+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2307.16107","created_at":"2026-07-05T06:41:21.823788+00:00"},{"alias_kind":"pith_short_12","alias_value":"J4LS4XJRIDAN","created_at":"2026-07-05T06:41:21.823788+00:00"},{"alias_kind":"pith_short_16","alias_value":"J4LS4XJRIDANVZ3X","created_at":"2026-07-05T06:41:21.823788+00:00"},{"alias_kind":"pith_short_8","alias_value":"J4LS4XJR","created_at":"2026-07-05T06:41:21.823788+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/J4LS4XJRIDANVZ3X3CSAZ6UDZ7","json":"https://pith.science/pith/J4LS4XJRIDANVZ3X3CSAZ6UDZ7.json","graph_json":"https://pith.science/api/pith-number/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/graph.json","events_json":"https://pith.science/api/pith-number/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/events.json","paper":"https://pith.science/paper/J4LS4XJR"},"agent_actions":{"view_html":"https://pith.science/pith/J4LS4XJRIDANVZ3X3CSAZ6UDZ7","download_json":"https://pith.science/pith/J4LS4XJRIDANVZ3X3CSAZ6UDZ7.json","view_paper":"https://pith.science/paper/J4LS4XJR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2307.16107&json=true","fetch_graph":"https://pith.science/api/pith-number/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/graph.json","fetch_events":"https://pith.science/api/pith-number/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/action/storage_attestation","attest_author":"https://pith.science/pith/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/action/author_attestation","sign_citation":"https://pith.science/pith/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/action/citation_signature","submit_replication":"https://pith.science/pith/J4LS4XJRIDANVZ3X3CSAZ6UDZ7/action/replication_record"}},"created_at":"2026-07-05T06:41:21.823788+00:00","updated_at":"2026-07-05T06:41:21.823788+00:00"}