{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:2ANRZWEALHWCK2CUWYHUPAJNX4","short_pith_number":"pith:2ANRZWEA","schema_version":"1.0","canonical_sha256":"d01b1cd88059ec256854b60f47812dbf2367330ea0f0fc6b3238a6aaba345999","source":{"kind":"arxiv","id":"1708.07704","version":3},"attestation_state":"computed","paper":{"title":"Extragalactic source population studies at very high energies in the Cherenkov Telescope Array era","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"A. Dom\\'inguez, A. Zech (for the CTA Consortium), D. Mazin, J. Lefaucheur, S. Pita, T. Hassan","submitted_at":"2017-08-25T11:59:57Z","abstract_excerpt":"The Cherenkov Telescope Array (CTA) is the next generation ground-based $\\gamma$-ray observatory. It will provide an order of magnitude better sensitivity and an extended energy coverage, 20 GeV - 300 TeV, relative to current Imaging Atmospheric Cherenkov Telescopes (IACTs). IACTs, despite featuring an excellent sensitivity, are characterized by a limited field of view that makes the blind search of new sources very time inefficient. Fortunately, the $\\textit{Fermi}$-LAT collaboration recently released a new catalog of 1,556 sources detected in the 10 GeV - 2 TeV range by the Large Area Telesc"},"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":"1708.07704","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-08-25T11:59:57Z","cross_cats_sorted":["astro-ph.CO","astro-ph.IM"],"title_canon_sha256":"b90aba586979e26fba4c7261df5af4fe0da56fb214a39d7d410c5f49f929b7aa","abstract_canon_sha256":"564603173d04dc4f6ebf7d39a3df2cad36289c482a4ce670bf4e8b3c9664c8d6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:25:34.050147Z","signature_b64":"YxW+PbrdXYpxKaTYEpeobgaGU8gEmmmw3aD/sH8Il/McQcJVwOF1OZqEg0xGqCa2ucwzkfXH7vU2wezVdyoYBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d01b1cd88059ec256854b60f47812dbf2367330ea0f0fc6b3238a6aaba345999","last_reissued_at":"2026-05-18T00:25:34.049447Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:25:34.049447Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Extragalactic source population studies at very high energies in the Cherenkov Telescope Array era","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"A. Dom\\'inguez, A. Zech (for the CTA Consortium), D. Mazin, J. Lefaucheur, S. Pita, T. Hassan","submitted_at":"2017-08-25T11:59:57Z","abstract_excerpt":"The Cherenkov Telescope Array (CTA) is the next generation ground-based $\\gamma$-ray observatory. It will provide an order of magnitude better sensitivity and an extended energy coverage, 20 GeV - 300 TeV, relative to current Imaging Atmospheric Cherenkov Telescopes (IACTs). IACTs, despite featuring an excellent sensitivity, are characterized by a limited field of view that makes the blind search of new sources very time inefficient. Fortunately, the $\\textit{Fermi}$-LAT collaboration recently released a new catalog of 1,556 sources detected in the 10 GeV - 2 TeV range by the Large Area Telesc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.07704","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":""},"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":"1708.07704","created_at":"2026-05-18T00:25:34.049569+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.07704v3","created_at":"2026-05-18T00:25:34.049569+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.07704","created_at":"2026-05-18T00:25:34.049569+00:00"},{"alias_kind":"pith_short_12","alias_value":"2ANRZWEALHWC","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_16","alias_value":"2ANRZWEALHWCK2CU","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_8","alias_value":"2ANRZWEA","created_at":"2026-05-18T12:30:55.937587+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/2ANRZWEALHWCK2CUWYHUPAJNX4","json":"https://pith.science/pith/2ANRZWEALHWCK2CUWYHUPAJNX4.json","graph_json":"https://pith.science/api/pith-number/2ANRZWEALHWCK2CUWYHUPAJNX4/graph.json","events_json":"https://pith.science/api/pith-number/2ANRZWEALHWCK2CUWYHUPAJNX4/events.json","paper":"https://pith.science/paper/2ANRZWEA"},"agent_actions":{"view_html":"https://pith.science/pith/2ANRZWEALHWCK2CUWYHUPAJNX4","download_json":"https://pith.science/pith/2ANRZWEALHWCK2CUWYHUPAJNX4.json","view_paper":"https://pith.science/paper/2ANRZWEA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.07704&json=true","fetch_graph":"https://pith.science/api/pith-number/2ANRZWEALHWCK2CUWYHUPAJNX4/graph.json","fetch_events":"https://pith.science/api/pith-number/2ANRZWEALHWCK2CUWYHUPAJNX4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2ANRZWEALHWCK2CUWYHUPAJNX4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2ANRZWEALHWCK2CUWYHUPAJNX4/action/storage_attestation","attest_author":"https://pith.science/pith/2ANRZWEALHWCK2CUWYHUPAJNX4/action/author_attestation","sign_citation":"https://pith.science/pith/2ANRZWEALHWCK2CUWYHUPAJNX4/action/citation_signature","submit_replication":"https://pith.science/pith/2ANRZWEALHWCK2CUWYHUPAJNX4/action/replication_record"}},"created_at":"2026-05-18T00:25:34.049569+00:00","updated_at":"2026-05-18T00:25:34.049569+00:00"}