{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:J4TBLM4XV56ZQRQSYCWJEUHTMC","short_pith_number":"pith:J4TBLM4X","schema_version":"1.0","canonical_sha256":"4f2615b397af7d984612c0ac9250f3609e2f5ce385fb0e465e631d4385ab0317","source":{"kind":"arxiv","id":"2309.03715","version":1},"attestation_state":"computed","paper":{"title":"Probing VHE gamma-ray emission from GW events with H.E.S.S","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Fabian Sch\\\"ussler, Francois Brun, Halim Ashkar, Heike Prokoph, Mathieu de Bony de Lavergne, Ruslan Konno, Stefan Ohm, Stephen Fegan, Sylvia J Zhu (for the H.E.S.S. collaboration)","submitted_at":"2023-09-07T13:45:30Z","abstract_excerpt":"Gravitational wave (GW) events, particularly those connected to the merger of compact objects such as neutron stars, are believed to be the primary source of short gamma-ray bursts. To explore the very high energy (VHE) component of the emission from these events, the H.E.S.S. collaboration has dedicated a substantial effort and observing time to follow up on these events. During the second and third GW observing runs, H.E.S.S. was the first ground-based instrument to observe the GW170817 binary neutron star merger. In addition, H.E.S.S. followed four binary black hole mergers. The data acquir"},"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":"2309.03715","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-09-07T13:45:30Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"5e6cec224f923606a462b7b95bb61e6733c6dbf53901db0369173feac4e8fe2c","abstract_canon_sha256":"dcad98254f8be87c56ce5e795d0c3f9af2987e486ea4a7d4f97cc5598cfeda33"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:48:41.073432Z","signature_b64":"V99kaMM3UE5Dy3qJDpa4vPYL8klUijZWNV/3vyrgSt7q96BSYQmco28ABwUgT72scOHnd1VvUQujE0chEFN0CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4f2615b397af7d984612c0ac9250f3609e2f5ce385fb0e465e631d4385ab0317","last_reissued_at":"2026-07-05T06:48:41.072812Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:48:41.072812Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing VHE gamma-ray emission from GW events with H.E.S.S","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Fabian Sch\\\"ussler, Francois Brun, Halim Ashkar, Heike Prokoph, Mathieu de Bony de Lavergne, Ruslan Konno, Stefan Ohm, Stephen Fegan, Sylvia J Zhu (for the H.E.S.S. collaboration)","submitted_at":"2023-09-07T13:45:30Z","abstract_excerpt":"Gravitational wave (GW) events, particularly those connected to the merger of compact objects such as neutron stars, are believed to be the primary source of short gamma-ray bursts. To explore the very high energy (VHE) component of the emission from these events, the H.E.S.S. collaboration has dedicated a substantial effort and observing time to follow up on these events. During the second and third GW observing runs, H.E.S.S. was the first ground-based instrument to observe the GW170817 binary neutron star merger. In addition, H.E.S.S. followed four binary black hole mergers. The data acquir"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.03715","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/2309.03715/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":"2309.03715","created_at":"2026-07-05T06:48:41.072875+00:00"},{"alias_kind":"arxiv_version","alias_value":"2309.03715v1","created_at":"2026-07-05T06:48:41.072875+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2309.03715","created_at":"2026-07-05T06:48:41.072875+00:00"},{"alias_kind":"pith_short_12","alias_value":"J4TBLM4XV56Z","created_at":"2026-07-05T06:48:41.072875+00:00"},{"alias_kind":"pith_short_16","alias_value":"J4TBLM4XV56ZQRQS","created_at":"2026-07-05T06:48:41.072875+00:00"},{"alias_kind":"pith_short_8","alias_value":"J4TBLM4X","created_at":"2026-07-05T06:48:41.072875+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/J4TBLM4XV56ZQRQSYCWJEUHTMC","json":"https://pith.science/pith/J4TBLM4XV56ZQRQSYCWJEUHTMC.json","graph_json":"https://pith.science/api/pith-number/J4TBLM4XV56ZQRQSYCWJEUHTMC/graph.json","events_json":"https://pith.science/api/pith-number/J4TBLM4XV56ZQRQSYCWJEUHTMC/events.json","paper":"https://pith.science/paper/J4TBLM4X"},"agent_actions":{"view_html":"https://pith.science/pith/J4TBLM4XV56ZQRQSYCWJEUHTMC","download_json":"https://pith.science/pith/J4TBLM4XV56ZQRQSYCWJEUHTMC.json","view_paper":"https://pith.science/paper/J4TBLM4X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2309.03715&json=true","fetch_graph":"https://pith.science/api/pith-number/J4TBLM4XV56ZQRQSYCWJEUHTMC/graph.json","fetch_events":"https://pith.science/api/pith-number/J4TBLM4XV56ZQRQSYCWJEUHTMC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J4TBLM4XV56ZQRQSYCWJEUHTMC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J4TBLM4XV56ZQRQSYCWJEUHTMC/action/storage_attestation","attest_author":"https://pith.science/pith/J4TBLM4XV56ZQRQSYCWJEUHTMC/action/author_attestation","sign_citation":"https://pith.science/pith/J4TBLM4XV56ZQRQSYCWJEUHTMC/action/citation_signature","submit_replication":"https://pith.science/pith/J4TBLM4XV56ZQRQSYCWJEUHTMC/action/replication_record"}},"created_at":"2026-07-05T06:48:41.072875+00:00","updated_at":"2026-07-05T06:48:41.072875+00:00"}