{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:B2YROMOWGH3C35AHMHD7OZWR4H","short_pith_number":"pith:B2YROMOW","schema_version":"1.0","canonical_sha256":"0eb11731d631f62df40761c7f766d1e1f9bdc26d91e3e6ce76fcc5802afcb81e","source":{"kind":"arxiv","id":"1705.03657","version":1},"attestation_state":"computed","paper":{"title":"Search for GeV counterparts to fast radio bursts with Fermi","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Fang-Kun Peng, Pak-Hin Thomas Tam (SYSU), Shao-Qiang Xi (NJU), Xiang-Yu Wang (NJU)","submitted_at":"2017-05-10T08:25:52Z","abstract_excerpt":"The non-repeating fast radio bursts (FRBs) could arise from catastrophic stellar explosions or magnetar giant flares, so relativistic blast waves might be produced in these events. Motivated by this, we here search for GeV counterparts to all non-repeating FRBs with Fermi Large Area Telescope (LAT), including FRB 131104 that is claimed to be possibly associated with a gamma-ray transient candidate detected by Swift Burst Alert Telescope (BAT). FRB 131104 enters the field of view (FoV) of LAT ~5000s after the burst time, so we are only able to search for the GeV afterglow emission during this p"},"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":"1705.03657","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-10T08:25:52Z","cross_cats_sorted":[],"title_canon_sha256":"c600089b3ae28d3f51fd4e9c64a79e7802635ba77970fca0381f2ca567756d9f","abstract_canon_sha256":"de9b2b1a9f17f013b77df86dfdab9e27c188ff1d9948a51db44c0f4c8f44b023"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:41:32.878858Z","signature_b64":"0H2nE9pnj5KZ8Y0fTuAEm+Lnh+zDfVvNoWfWIzDp76/PEojnGQMFyznkIlAzqlzlL2lGieaYok7tGpgnRHrTBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0eb11731d631f62df40761c7f766d1e1f9bdc26d91e3e6ce76fcc5802afcb81e","last_reissued_at":"2026-05-18T00:41:32.878246Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:41:32.878246Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for GeV counterparts to fast radio bursts with Fermi","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Fang-Kun Peng, Pak-Hin Thomas Tam (SYSU), Shao-Qiang Xi (NJU), Xiang-Yu Wang (NJU)","submitted_at":"2017-05-10T08:25:52Z","abstract_excerpt":"The non-repeating fast radio bursts (FRBs) could arise from catastrophic stellar explosions or magnetar giant flares, so relativistic blast waves might be produced in these events. Motivated by this, we here search for GeV counterparts to all non-repeating FRBs with Fermi Large Area Telescope (LAT), including FRB 131104 that is claimed to be possibly associated with a gamma-ray transient candidate detected by Swift Burst Alert Telescope (BAT). FRB 131104 enters the field of view (FoV) of LAT ~5000s after the burst time, so we are only able to search for the GeV afterglow emission during this p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.03657","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":"1705.03657","created_at":"2026-05-18T00:41:32.878364+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.03657v1","created_at":"2026-05-18T00:41:32.878364+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.03657","created_at":"2026-05-18T00:41:32.878364+00:00"},{"alias_kind":"pith_short_12","alias_value":"B2YROMOWGH3C","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_16","alias_value":"B2YROMOWGH3C35AH","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_8","alias_value":"B2YROMOW","created_at":"2026-05-18T12:31:08.081275+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/B2YROMOWGH3C35AHMHD7OZWR4H","json":"https://pith.science/pith/B2YROMOWGH3C35AHMHD7OZWR4H.json","graph_json":"https://pith.science/api/pith-number/B2YROMOWGH3C35AHMHD7OZWR4H/graph.json","events_json":"https://pith.science/api/pith-number/B2YROMOWGH3C35AHMHD7OZWR4H/events.json","paper":"https://pith.science/paper/B2YROMOW"},"agent_actions":{"view_html":"https://pith.science/pith/B2YROMOWGH3C35AHMHD7OZWR4H","download_json":"https://pith.science/pith/B2YROMOWGH3C35AHMHD7OZWR4H.json","view_paper":"https://pith.science/paper/B2YROMOW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.03657&json=true","fetch_graph":"https://pith.science/api/pith-number/B2YROMOWGH3C35AHMHD7OZWR4H/graph.json","fetch_events":"https://pith.science/api/pith-number/B2YROMOWGH3C35AHMHD7OZWR4H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B2YROMOWGH3C35AHMHD7OZWR4H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B2YROMOWGH3C35AHMHD7OZWR4H/action/storage_attestation","attest_author":"https://pith.science/pith/B2YROMOWGH3C35AHMHD7OZWR4H/action/author_attestation","sign_citation":"https://pith.science/pith/B2YROMOWGH3C35AHMHD7OZWR4H/action/citation_signature","submit_replication":"https://pith.science/pith/B2YROMOWGH3C35AHMHD7OZWR4H/action/replication_record"}},"created_at":"2026-05-18T00:41:32.878364+00:00","updated_at":"2026-05-18T00:41:32.878364+00:00"}