{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:2YXWL2HAR3CIKE5MD3RXIFUOCX","short_pith_number":"pith:2YXWL2HA","schema_version":"1.0","canonical_sha256":"d62f65e8e08ec48513ac1ee374168e15ed6223b1be5e868c28bceda33818674c","source":{"kind":"arxiv","id":"2308.12118","version":1},"attestation_state":"computed","paper":{"title":"Dense Forests of Microshots in Bursts from FRB 20220912A","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Akshatha Gopinath, Daniela Huppenkothen, Dant\\'e M. Hewitt, Isma\\\"el Cognard, Jason W. T. Hessels, Kenzie Nimmo6, Lucas Guillemot, Mark P. Snelders, Omar S. Ould-Boukattine, Pragya Chawla","submitted_at":"2023-08-23T13:13:07Z","abstract_excerpt":"We report on exceptionally bright bursts (>400 Jy ms) detected from the repeating fast radio burst source FRB 20220912A using the Nan\\c{c}ay Radio Telescope (NRT), as part of the ECLAT (Extragalactic Coherent Light from Astrophysical Transients) monitoring campaign. These bursts exhibit extremely luminous, broadband, short-duration structures (~ 16 microseconds), which we term 'microshots' and which can be especially well studied in the NRT data given the excellent signal-to-noise and dynamic range (32-bit samples). The estimated peak flux density of the brightest microshot is 450 Jy. We show "},"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":"2308.12118","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-08-23T13:13:07Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"434ea0ad42ab73ecb8d9dfe6a168ebbe67fa768aa132b0bcd0adad2a45702052","abstract_canon_sha256":"2d57bf33b7e2cd3d83478442f958f906425d1084db581ada574e0c630b894bce"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:43:59.760654Z","signature_b64":"sIHmeRw9L6mq1GpH24I/IEkAu9zn+F1aDiKpWZgzxdyhki//7obfVKBRKj2in5ttMAKNLEK4iOremCIGzPvDDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d62f65e8e08ec48513ac1ee374168e15ed6223b1be5e868c28bceda33818674c","last_reissued_at":"2026-07-05T06:43:59.760144Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:43:59.760144Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dense Forests of Microshots in Bursts from FRB 20220912A","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Akshatha Gopinath, Daniela Huppenkothen, Dant\\'e M. Hewitt, Isma\\\"el Cognard, Jason W. T. Hessels, Kenzie Nimmo6, Lucas Guillemot, Mark P. Snelders, Omar S. Ould-Boukattine, Pragya Chawla","submitted_at":"2023-08-23T13:13:07Z","abstract_excerpt":"We report on exceptionally bright bursts (>400 Jy ms) detected from the repeating fast radio burst source FRB 20220912A using the Nan\\c{c}ay Radio Telescope (NRT), as part of the ECLAT (Extragalactic Coherent Light from Astrophysical Transients) monitoring campaign. These bursts exhibit extremely luminous, broadband, short-duration structures (~ 16 microseconds), which we term 'microshots' and which can be especially well studied in the NRT data given the excellent signal-to-noise and dynamic range (32-bit samples). The estimated peak flux density of the brightest microshot is 450 Jy. We show "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.12118","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/2308.12118/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":"2308.12118","created_at":"2026-07-05T06:43:59.760207+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.12118v1","created_at":"2026-07-05T06:43:59.760207+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.12118","created_at":"2026-07-05T06:43:59.760207+00:00"},{"alias_kind":"pith_short_12","alias_value":"2YXWL2HAR3CI","created_at":"2026-07-05T06:43:59.760207+00:00"},{"alias_kind":"pith_short_16","alias_value":"2YXWL2HAR3CIKE5M","created_at":"2026-07-05T06:43:59.760207+00:00"},{"alias_kind":"pith_short_8","alias_value":"2YXWL2HA","created_at":"2026-07-05T06:43:59.760207+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/2YXWL2HAR3CIKE5MD3RXIFUOCX","json":"https://pith.science/pith/2YXWL2HAR3CIKE5MD3RXIFUOCX.json","graph_json":"https://pith.science/api/pith-number/2YXWL2HAR3CIKE5MD3RXIFUOCX/graph.json","events_json":"https://pith.science/api/pith-number/2YXWL2HAR3CIKE5MD3RXIFUOCX/events.json","paper":"https://pith.science/paper/2YXWL2HA"},"agent_actions":{"view_html":"https://pith.science/pith/2YXWL2HAR3CIKE5MD3RXIFUOCX","download_json":"https://pith.science/pith/2YXWL2HAR3CIKE5MD3RXIFUOCX.json","view_paper":"https://pith.science/paper/2YXWL2HA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.12118&json=true","fetch_graph":"https://pith.science/api/pith-number/2YXWL2HAR3CIKE5MD3RXIFUOCX/graph.json","fetch_events":"https://pith.science/api/pith-number/2YXWL2HAR3CIKE5MD3RXIFUOCX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2YXWL2HAR3CIKE5MD3RXIFUOCX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2YXWL2HAR3CIKE5MD3RXIFUOCX/action/storage_attestation","attest_author":"https://pith.science/pith/2YXWL2HAR3CIKE5MD3RXIFUOCX/action/author_attestation","sign_citation":"https://pith.science/pith/2YXWL2HAR3CIKE5MD3RXIFUOCX/action/citation_signature","submit_replication":"https://pith.science/pith/2YXWL2HAR3CIKE5MD3RXIFUOCX/action/replication_record"}},"created_at":"2026-07-05T06:43:59.760207+00:00","updated_at":"2026-07-05T06:43:59.760207+00:00"}