{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:GRXXOCJUVP45FYJRLUFHN5ISWL","short_pith_number":"pith:GRXXOCJU","schema_version":"1.0","canonical_sha256":"346f770934abf9d2e1315d0a76f512b2e227f7fc6eaa2531ff56655a6fc0d301","source":{"kind":"arxiv","id":"1712.01043","version":2},"attestation_state":"computed","paper":{"title":"Fermi Large Area Telescope detection of gamma-ray emission from the direction of supernova iPTF14hls","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"2), (2) Ustc, 3), (3) UCAS, (4) KIAA-PKU, (5) UNLV, (6) IHEP), Bing Zhang (5), Hong-Bo Hu (6), Neng-Hui Liao (1), PMO, Qiang Yuan (1, Xiao-Jun Bi (6) ((1), Ye Li (4), Yi-Zhong Fan (1, Yu-Liang Xin (1","submitted_at":"2017-12-04T12:43:21Z","abstract_excerpt":"The remnant of supernova explosion is widely believed to be the acceleration site of high-energy cosmic ray particles. The acceleration timescale is, however, typically very long. Here we report the detection of a variable $\\gamma$-ray source with the Fermi Large Area Telescope, which is positionally and temporally consistent with a peculiar supernova, iPTF14hls. A quasi-stellar object SDSS J092054.04+504251.5, which is probably a blazar according to the infrared data, is found in the error circle of the $\\gamma$-ray source. More data about the $\\gamma$-ray source and SDSS J092054.04+504251.5 "},"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":"1712.01043","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-12-04T12:43:21Z","cross_cats_sorted":[],"title_canon_sha256":"298911b436657b2dfb0e09a287ecc80faca88db5ae433a86eb74802e6c809475","abstract_canon_sha256":"de39bebcc56618187fb022088fabf9020122413a86fbb245e0b9544b19534607"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:50.788685Z","signature_b64":"d6qY12j4gQeR6KspgBng9LIudAzrrq0oSqzWH9eVZEvawtdm0MyU+kD9ePSXt62PcOFFDkv2QGNXEc8BxSacBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"346f770934abf9d2e1315d0a76f512b2e227f7fc6eaa2531ff56655a6fc0d301","last_reissued_at":"2026-05-18T00:22:50.788294Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:50.788294Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fermi Large Area Telescope detection of gamma-ray emission from the direction of supernova iPTF14hls","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"2), (2) Ustc, 3), (3) UCAS, (4) KIAA-PKU, (5) UNLV, (6) IHEP), Bing Zhang (5), Hong-Bo Hu (6), Neng-Hui Liao (1), PMO, Qiang Yuan (1, Xiao-Jun Bi (6) ((1), Ye Li (4), Yi-Zhong Fan (1, Yu-Liang Xin (1","submitted_at":"2017-12-04T12:43:21Z","abstract_excerpt":"The remnant of supernova explosion is widely believed to be the acceleration site of high-energy cosmic ray particles. The acceleration timescale is, however, typically very long. Here we report the detection of a variable $\\gamma$-ray source with the Fermi Large Area Telescope, which is positionally and temporally consistent with a peculiar supernova, iPTF14hls. A quasi-stellar object SDSS J092054.04+504251.5, which is probably a blazar according to the infrared data, is found in the error circle of the $\\gamma$-ray source. More data about the $\\gamma$-ray source and SDSS J092054.04+504251.5 "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.01043","kind":"arxiv","version":2},"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":"1712.01043","created_at":"2026-05-18T00:22:50.788360+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.01043v2","created_at":"2026-05-18T00:22:50.788360+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.01043","created_at":"2026-05-18T00:22:50.788360+00:00"},{"alias_kind":"pith_short_12","alias_value":"GRXXOCJUVP45","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_16","alias_value":"GRXXOCJUVP45FYJR","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_8","alias_value":"GRXXOCJU","created_at":"2026-05-18T12:31:18.294218+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/GRXXOCJUVP45FYJRLUFHN5ISWL","json":"https://pith.science/pith/GRXXOCJUVP45FYJRLUFHN5ISWL.json","graph_json":"https://pith.science/api/pith-number/GRXXOCJUVP45FYJRLUFHN5ISWL/graph.json","events_json":"https://pith.science/api/pith-number/GRXXOCJUVP45FYJRLUFHN5ISWL/events.json","paper":"https://pith.science/paper/GRXXOCJU"},"agent_actions":{"view_html":"https://pith.science/pith/GRXXOCJUVP45FYJRLUFHN5ISWL","download_json":"https://pith.science/pith/GRXXOCJUVP45FYJRLUFHN5ISWL.json","view_paper":"https://pith.science/paper/GRXXOCJU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.01043&json=true","fetch_graph":"https://pith.science/api/pith-number/GRXXOCJUVP45FYJRLUFHN5ISWL/graph.json","fetch_events":"https://pith.science/api/pith-number/GRXXOCJUVP45FYJRLUFHN5ISWL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GRXXOCJUVP45FYJRLUFHN5ISWL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GRXXOCJUVP45FYJRLUFHN5ISWL/action/storage_attestation","attest_author":"https://pith.science/pith/GRXXOCJUVP45FYJRLUFHN5ISWL/action/author_attestation","sign_citation":"https://pith.science/pith/GRXXOCJUVP45FYJRLUFHN5ISWL/action/citation_signature","submit_replication":"https://pith.science/pith/GRXXOCJUVP45FYJRLUFHN5ISWL/action/replication_record"}},"created_at":"2026-05-18T00:22:50.788360+00:00","updated_at":"2026-05-18T00:22:50.788360+00:00"}