{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:7VAHNRR3GDRJC6ZHL5DY2334IO","short_pith_number":"pith:7VAHNRR3","schema_version":"1.0","canonical_sha256":"fd4076c63b30e2917b275f478d6f7c43aa0c385fa37772a737e1ddc28771cafb","source":{"kind":"arxiv","id":"2408.04504","version":3},"attestation_state":"computed","paper":{"title":"Investigating the effect of hadronic models on IACT images","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Benedetta Bruno, Luan Bonneau Arbeletche, Rodrigo Guedes Lang, Stefan Funk, Vitor de Souza","submitted_at":"2024-08-08T15:02:21Z","abstract_excerpt":"The predictions of hadronic interaction models for cosmic-ray induced air showers contain inherent uncertainties due to limitations of available accelerator data. This leads to differences in shower simulations using each of those models. Many studies have been carried out to track those differences by investigating the shower development or the particle content. In this work, we propose a new approach to search for discrepancies and similarities between the models, via the IACT images resulting from the observations of hadronic air showers. We use simulations of H.E.S.S. as a show-case scenar"},"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":"2408.04504","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-08-08T15:02:21Z","cross_cats_sorted":[],"title_canon_sha256":"2f2ebb3560cfd94efc1f7b1e50bff524acb2f4b648141e525f5ad8f624d10739","abstract_canon_sha256":"a58c27a09040e65d83daad605693079da368317bda0bb71b2c82557180b81898"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:15:18.827680Z","signature_b64":"tgcZmPYn+G+Mo+shqxgsFFuZsPvq/Vok0fC17Kckv/XPdbuuqJWpOEHoUR6LX56uC1fZXaM6icJouLqWgcHUDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fd4076c63b30e2917b275f478d6f7c43aa0c385fa37772a737e1ddc28771cafb","last_reissued_at":"2026-07-05T10:15:18.827193Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:15:18.827193Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigating the effect of hadronic models on IACT images","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Benedetta Bruno, Luan Bonneau Arbeletche, Rodrigo Guedes Lang, Stefan Funk, Vitor de Souza","submitted_at":"2024-08-08T15:02:21Z","abstract_excerpt":"The predictions of hadronic interaction models for cosmic-ray induced air showers contain inherent uncertainties due to limitations of available accelerator data. This leads to differences in shower simulations using each of those models. Many studies have been carried out to track those differences by investigating the shower development or the particle content. In this work, we propose a new approach to search for discrepancies and similarities between the models, via the IACT images resulting from the observations of hadronic air showers. We use simulations of H.E.S.S. as a show-case scenar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.04504","kind":"arxiv","version":3},"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/2408.04504/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":"2408.04504","created_at":"2026-07-05T10:15:18.827243+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.04504v3","created_at":"2026-07-05T10:15:18.827243+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.04504","created_at":"2026-07-05T10:15:18.827243+00:00"},{"alias_kind":"pith_short_12","alias_value":"7VAHNRR3GDRJ","created_at":"2026-07-05T10:15:18.827243+00:00"},{"alias_kind":"pith_short_16","alias_value":"7VAHNRR3GDRJC6ZH","created_at":"2026-07-05T10:15:18.827243+00:00"},{"alias_kind":"pith_short_8","alias_value":"7VAHNRR3","created_at":"2026-07-05T10:15:18.827243+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/7VAHNRR3GDRJC6ZHL5DY2334IO","json":"https://pith.science/pith/7VAHNRR3GDRJC6ZHL5DY2334IO.json","graph_json":"https://pith.science/api/pith-number/7VAHNRR3GDRJC6ZHL5DY2334IO/graph.json","events_json":"https://pith.science/api/pith-number/7VAHNRR3GDRJC6ZHL5DY2334IO/events.json","paper":"https://pith.science/paper/7VAHNRR3"},"agent_actions":{"view_html":"https://pith.science/pith/7VAHNRR3GDRJC6ZHL5DY2334IO","download_json":"https://pith.science/pith/7VAHNRR3GDRJC6ZHL5DY2334IO.json","view_paper":"https://pith.science/paper/7VAHNRR3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.04504&json=true","fetch_graph":"https://pith.science/api/pith-number/7VAHNRR3GDRJC6ZHL5DY2334IO/graph.json","fetch_events":"https://pith.science/api/pith-number/7VAHNRR3GDRJC6ZHL5DY2334IO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7VAHNRR3GDRJC6ZHL5DY2334IO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7VAHNRR3GDRJC6ZHL5DY2334IO/action/storage_attestation","attest_author":"https://pith.science/pith/7VAHNRR3GDRJC6ZHL5DY2334IO/action/author_attestation","sign_citation":"https://pith.science/pith/7VAHNRR3GDRJC6ZHL5DY2334IO/action/citation_signature","submit_replication":"https://pith.science/pith/7VAHNRR3GDRJC6ZHL5DY2334IO/action/replication_record"}},"created_at":"2026-07-05T10:15:18.827243+00:00","updated_at":"2026-07-05T10:15:18.827243+00:00"}