{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:AN6DUSVSKVMKKM7UTKUNJWKCDF","short_pith_number":"pith:AN6DUSVS","schema_version":"1.0","canonical_sha256":"037c3a4ab25558a533f49aa8d4d94219796b9fe9f75fc42557d7205e0d6dcedd","source":{"kind":"arxiv","id":"2606.28210","version":1},"attestation_state":"computed","paper":{"title":"SKAO and Gamma-Ray Synergies","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Adelle J. Goodwin, Alak Ray, Andrea Botteon, Arnau Aguasca-Cabot, Csaba Balazs, Elena Pian, Ettore Carretti, Filippo D'Ammando, Gavin Rowell, Gemma E. Anderson, Gianfranco Brunetti, Gianluca Castignani, Giulia Migliori, James A. Green, Jess W. Broderick, Josep M. Paredes, Lauren Rhodes, Marcello Giroletti, Martin White, Miroslav D. Filipovic, Monica Orienti, Nick Tothill, Philip G. Edwards, Pol Bordas, Roland M. Crocker, Sabrina Einecke, Sanja Lazarevic, Shi Dai, Zachary J. Smeaton","submitted_at":"2026-06-26T16:01:59Z","abstract_excerpt":"A wide variety of Galactic and extragalactic sources are known to emitradiation across the entire electromagnetic spectrum, including both transient and steady-state phenomena. A few hundred of these sources (~300) have been detected even at the highest energies, in the TeV range. The number of known TeV emitters is expected to increase substantially in the coming years with the operation of current and next-generation Cherenkov detectors, such as the Large High Altitude Air Shower Observatory (LHAASO) and the Cherenkov Telescope Array Observatory (CTAO). These sources typically exhibit broad,"},"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":"2606.28210","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-06-26T16:01:59Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"3da6f521a0e2e03a3d32394b0ae9f8a25845aa77f0405649f3d17b74c3de73d2","abstract_canon_sha256":"e892e7f13a1ef148b1912cc3734414fb808f524c7cc31a03b397cc29bb3cb93b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-29T01:15:09.420259Z","signature_b64":"cncbf6pzW9bSDO4/k8ULx6GkH2i3p/MOeQ5ICRuEAJIWHobDXK2p1XSHxSqdDvd7PpEoAzu83NFTJsyGw9v+DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"037c3a4ab25558a533f49aa8d4d94219796b9fe9f75fc42557d7205e0d6dcedd","last_reissued_at":"2026-06-29T01:15:09.419866Z","signature_status":"signed_v1","first_computed_at":"2026-06-29T01:15:09.419866Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SKAO and Gamma-Ray Synergies","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Adelle J. Goodwin, Alak Ray, Andrea Botteon, Arnau Aguasca-Cabot, Csaba Balazs, Elena Pian, Ettore Carretti, Filippo D'Ammando, Gavin Rowell, Gemma E. Anderson, Gianfranco Brunetti, Gianluca Castignani, Giulia Migliori, James A. Green, Jess W. Broderick, Josep M. Paredes, Lauren Rhodes, Marcello Giroletti, Martin White, Miroslav D. Filipovic, Monica Orienti, Nick Tothill, Philip G. Edwards, Pol Bordas, Roland M. Crocker, Sabrina Einecke, Sanja Lazarevic, Shi Dai, Zachary J. Smeaton","submitted_at":"2026-06-26T16:01:59Z","abstract_excerpt":"A wide variety of Galactic and extragalactic sources are known to emitradiation across the entire electromagnetic spectrum, including both transient and steady-state phenomena. A few hundred of these sources (~300) have been detected even at the highest energies, in the TeV range. The number of known TeV emitters is expected to increase substantially in the coming years with the operation of current and next-generation Cherenkov detectors, such as the Large High Altitude Air Shower Observatory (LHAASO) and the Cherenkov Telescope Array Observatory (CTAO). These sources typically exhibit broad,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.28210","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/2606.28210/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":"2606.28210","created_at":"2026-06-29T01:15:09.419921+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.28210v1","created_at":"2026-06-29T01:15:09.419921+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.28210","created_at":"2026-06-29T01:15:09.419921+00:00"},{"alias_kind":"pith_short_12","alias_value":"AN6DUSVSKVMK","created_at":"2026-06-29T01:15:09.419921+00:00"},{"alias_kind":"pith_short_16","alias_value":"AN6DUSVSKVMKKM7U","created_at":"2026-06-29T01:15:09.419921+00:00"},{"alias_kind":"pith_short_8","alias_value":"AN6DUSVS","created_at":"2026-06-29T01:15:09.419921+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/AN6DUSVSKVMKKM7UTKUNJWKCDF","json":"https://pith.science/pith/AN6DUSVSKVMKKM7UTKUNJWKCDF.json","graph_json":"https://pith.science/api/pith-number/AN6DUSVSKVMKKM7UTKUNJWKCDF/graph.json","events_json":"https://pith.science/api/pith-number/AN6DUSVSKVMKKM7UTKUNJWKCDF/events.json","paper":"https://pith.science/paper/AN6DUSVS"},"agent_actions":{"view_html":"https://pith.science/pith/AN6DUSVSKVMKKM7UTKUNJWKCDF","download_json":"https://pith.science/pith/AN6DUSVSKVMKKM7UTKUNJWKCDF.json","view_paper":"https://pith.science/paper/AN6DUSVS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.28210&json=true","fetch_graph":"https://pith.science/api/pith-number/AN6DUSVSKVMKKM7UTKUNJWKCDF/graph.json","fetch_events":"https://pith.science/api/pith-number/AN6DUSVSKVMKKM7UTKUNJWKCDF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AN6DUSVSKVMKKM7UTKUNJWKCDF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AN6DUSVSKVMKKM7UTKUNJWKCDF/action/storage_attestation","attest_author":"https://pith.science/pith/AN6DUSVSKVMKKM7UTKUNJWKCDF/action/author_attestation","sign_citation":"https://pith.science/pith/AN6DUSVSKVMKKM7UTKUNJWKCDF/action/citation_signature","submit_replication":"https://pith.science/pith/AN6DUSVSKVMKKM7UTKUNJWKCDF/action/replication_record"}},"created_at":"2026-06-29T01:15:09.419921+00:00","updated_at":"2026-06-29T01:15:09.419921+00:00"}