{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:ROLPKNG4XTTUBV3QAQLNZ4H4CW","short_pith_number":"pith:ROLPKNG4","schema_version":"1.0","canonical_sha256":"8b96f534dcbce740d7700416dcf0fc159d64f768e7276c5fa3ad68ee6f32abee","source":{"kind":"arxiv","id":"2211.02059","version":2},"attestation_state":"computed","paper":{"title":"Evidence for multiple shocks from the $\\gamma$-ray emission of RS Ophiuchi","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Brian D. Metzger, Damiano Caprioli, Elias Aydi, Indrek Vurm, Laura Chomiuk, Rebecca Diesing, Siddhartha Gupta","submitted_at":"2022-11-03T18:00:03Z","abstract_excerpt":"In August of 2021, Fermi-LAT, H.E.S.S., and MAGIC detected GeV and TeV $\\gamma$-ray emission from an outburst of recurrent nova RS Ophiuchi. This detection represents the first very high energy $\\gamma$-rays observed from a nova, and opens a new window to study particle acceleration. Both H.E.S.S. and MAGIC described the observed $\\gamma$-rays as arising from a single, external shock. In this paper, we perform detailed, multi-zone modeling of RS Ophiuchi's 2021 outburst including a self-consistent prescription for particle acceleration and magnetic field amplification. We demonstrate that, con"},"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":"2211.02059","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-11-03T18:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"c48553540173fc0fe8e9294a1cb565ec683b0a311b6702329d3f164d1c90cf5d","abstract_canon_sha256":"2e7a5631c5bc8aec97f3d9ea298d68f98df2adce7bbeb4e9e3d96972d1192cba"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:08:38.383203Z","signature_b64":"kI7Zt71h2Z8vSaNuKf/KoRvmZ0GmR0nG38gAWiU0YThyI/8CffWkA5VVeUet2XuBcRiyiZE+m/tp7po1LmhIDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b96f534dcbce740d7700416dcf0fc159d64f768e7276c5fa3ad68ee6f32abee","last_reissued_at":"2026-07-05T06:08:38.382753Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:08:38.382753Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evidence for multiple shocks from the $\\gamma$-ray emission of RS Ophiuchi","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Brian D. Metzger, Damiano Caprioli, Elias Aydi, Indrek Vurm, Laura Chomiuk, Rebecca Diesing, Siddhartha Gupta","submitted_at":"2022-11-03T18:00:03Z","abstract_excerpt":"In August of 2021, Fermi-LAT, H.E.S.S., and MAGIC detected GeV and TeV $\\gamma$-ray emission from an outburst of recurrent nova RS Ophiuchi. This detection represents the first very high energy $\\gamma$-rays observed from a nova, and opens a new window to study particle acceleration. Both H.E.S.S. and MAGIC described the observed $\\gamma$-rays as arising from a single, external shock. In this paper, we perform detailed, multi-zone modeling of RS Ophiuchi's 2021 outburst including a self-consistent prescription for particle acceleration and magnetic field amplification. We demonstrate that, con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.02059","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2211.02059/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":"2211.02059","created_at":"2026-07-05T06:08:38.382823+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.02059v2","created_at":"2026-07-05T06:08:38.382823+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.02059","created_at":"2026-07-05T06:08:38.382823+00:00"},{"alias_kind":"pith_short_12","alias_value":"ROLPKNG4XTTU","created_at":"2026-07-05T06:08:38.382823+00:00"},{"alias_kind":"pith_short_16","alias_value":"ROLPKNG4XTTUBV3Q","created_at":"2026-07-05T06:08:38.382823+00:00"},{"alias_kind":"pith_short_8","alias_value":"ROLPKNG4","created_at":"2026-07-05T06:08:38.382823+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/ROLPKNG4XTTUBV3QAQLNZ4H4CW","json":"https://pith.science/pith/ROLPKNG4XTTUBV3QAQLNZ4H4CW.json","graph_json":"https://pith.science/api/pith-number/ROLPKNG4XTTUBV3QAQLNZ4H4CW/graph.json","events_json":"https://pith.science/api/pith-number/ROLPKNG4XTTUBV3QAQLNZ4H4CW/events.json","paper":"https://pith.science/paper/ROLPKNG4"},"agent_actions":{"view_html":"https://pith.science/pith/ROLPKNG4XTTUBV3QAQLNZ4H4CW","download_json":"https://pith.science/pith/ROLPKNG4XTTUBV3QAQLNZ4H4CW.json","view_paper":"https://pith.science/paper/ROLPKNG4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.02059&json=true","fetch_graph":"https://pith.science/api/pith-number/ROLPKNG4XTTUBV3QAQLNZ4H4CW/graph.json","fetch_events":"https://pith.science/api/pith-number/ROLPKNG4XTTUBV3QAQLNZ4H4CW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ROLPKNG4XTTUBV3QAQLNZ4H4CW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ROLPKNG4XTTUBV3QAQLNZ4H4CW/action/storage_attestation","attest_author":"https://pith.science/pith/ROLPKNG4XTTUBV3QAQLNZ4H4CW/action/author_attestation","sign_citation":"https://pith.science/pith/ROLPKNG4XTTUBV3QAQLNZ4H4CW/action/citation_signature","submit_replication":"https://pith.science/pith/ROLPKNG4XTTUBV3QAQLNZ4H4CW/action/replication_record"}},"created_at":"2026-07-05T06:08:38.382823+00:00","updated_at":"2026-07-05T06:08:38.382823+00:00"}