{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:4ZW65XBLT27ESKUCL567HMT5EO","short_pith_number":"pith:4ZW65XBL","schema_version":"1.0","canonical_sha256":"e66deedc2b9ebe492a825f7df3b27d23bb853d097bc2ba39008f02f278d893f2","source":{"kind":"arxiv","id":"1710.02904","version":2},"attestation_state":"computed","paper":{"title":"Fast $\\gamma$-ray variability in blazars beyond redsift 3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Neng-Hui Liao, Shang Li, Yi-Zhong Fan, Yun-Feng Liang, Zi-Qing Xia","submitted_at":"2017-10-09T01:00:31Z","abstract_excerpt":"High-redshift blazars are one of the most powerful monsters in the universe and $\\gamma$-ray variability carries crucial information of their relativistic jets. In this work we present results of the first systematical temporal analysis of {\\it Fermi}-LAT data of all known seven $\\gamma$-ray blazars beyond redshift 3. Significant long-term $\\gamma$-ray variability is found from five sources in monthly $\\gamma$-ray light curves, in which three of them are reported for the first time. Furthermore, intraday $\\gamma$-ray variations are detected from NVSS J053954$-$283956 and NVSS J080518$+$614423."},"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":"1710.02904","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-09T01:00:31Z","cross_cats_sorted":[],"title_canon_sha256":"977a53cd890ba1781bd38f296ac21fdeabe60a97510cceb3624cafe52d73c8b4","abstract_canon_sha256":"317e15ea86b9315dcf7ea17b115bc014c3009f64a1aaacbbbcc4f0e165e90a40"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:23:32.664888Z","signature_b64":"noHnIXw+PSi8+++dblUQsZLG8ktVs61CbBuUsotFQgpyXsYy6jjtza6egz0eYuxgeDWV6RzYH+sAkwZV8Yr+Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e66deedc2b9ebe492a825f7df3b27d23bb853d097bc2ba39008f02f278d893f2","last_reissued_at":"2026-05-18T00:23:32.664148Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:23:32.664148Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fast $\\gamma$-ray variability in blazars beyond redsift 3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Neng-Hui Liao, Shang Li, Yi-Zhong Fan, Yun-Feng Liang, Zi-Qing Xia","submitted_at":"2017-10-09T01:00:31Z","abstract_excerpt":"High-redshift blazars are one of the most powerful monsters in the universe and $\\gamma$-ray variability carries crucial information of their relativistic jets. In this work we present results of the first systematical temporal analysis of {\\it Fermi}-LAT data of all known seven $\\gamma$-ray blazars beyond redshift 3. Significant long-term $\\gamma$-ray variability is found from five sources in monthly $\\gamma$-ray light curves, in which three of them are reported for the first time. Furthermore, intraday $\\gamma$-ray variations are detected from NVSS J053954$-$283956 and NVSS J080518$+$614423."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.02904","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":"1710.02904","created_at":"2026-05-18T00:23:32.664255+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.02904v2","created_at":"2026-05-18T00:23:32.664255+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.02904","created_at":"2026-05-18T00:23:32.664255+00:00"},{"alias_kind":"pith_short_12","alias_value":"4ZW65XBLT27E","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_16","alias_value":"4ZW65XBLT27ESKUC","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_8","alias_value":"4ZW65XBL","created_at":"2026-05-18T12:31:00.734936+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/4ZW65XBLT27ESKUCL567HMT5EO","json":"https://pith.science/pith/4ZW65XBLT27ESKUCL567HMT5EO.json","graph_json":"https://pith.science/api/pith-number/4ZW65XBLT27ESKUCL567HMT5EO/graph.json","events_json":"https://pith.science/api/pith-number/4ZW65XBLT27ESKUCL567HMT5EO/events.json","paper":"https://pith.science/paper/4ZW65XBL"},"agent_actions":{"view_html":"https://pith.science/pith/4ZW65XBLT27ESKUCL567HMT5EO","download_json":"https://pith.science/pith/4ZW65XBLT27ESKUCL567HMT5EO.json","view_paper":"https://pith.science/paper/4ZW65XBL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.02904&json=true","fetch_graph":"https://pith.science/api/pith-number/4ZW65XBLT27ESKUCL567HMT5EO/graph.json","fetch_events":"https://pith.science/api/pith-number/4ZW65XBLT27ESKUCL567HMT5EO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4ZW65XBLT27ESKUCL567HMT5EO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4ZW65XBLT27ESKUCL567HMT5EO/action/storage_attestation","attest_author":"https://pith.science/pith/4ZW65XBLT27ESKUCL567HMT5EO/action/author_attestation","sign_citation":"https://pith.science/pith/4ZW65XBLT27ESKUCL567HMT5EO/action/citation_signature","submit_replication":"https://pith.science/pith/4ZW65XBLT27ESKUCL567HMT5EO/action/replication_record"}},"created_at":"2026-05-18T00:23:32.664255+00:00","updated_at":"2026-05-18T00:23:32.664255+00:00"}