{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:Y5DQMRIAMGJJHFOQLQKEOIBZIR","short_pith_number":"pith:Y5DQMRIA","schema_version":"1.0","canonical_sha256":"c74706450061929395d05c14472039447372befa472901fb7bbaa4ef0c556981","source":{"kind":"arxiv","id":"1208.5356","version":1},"attestation_state":"computed","paper":{"title":"Dark Matter and Fundamental Physics with the Cherenkov Telescope Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.IM","authors_text":"A. Gonzalez-Munoz, A. Jacholkowska, A. Moralejo, A. Stamerra, A.Viana, C. Jahn, D. Emmanoulopoulos, D. Horns, D. Nieto, E. Birsin, E. Moulin, G. Spengler, H. Sandaker, H. S. Zechlin, J. A. Barrio, J. Bolmont, J. Conrad, J. F. Glicenstein, J. L. Contreras, J. Ripken, M. A. Sanchez-Conde, M. Doro, M. Fornasa, M. Gaug, M. K. Daniel, N. Mirabal, P. Brun, R. Mazini, S. Colafrancesco, S. H. Connell, S. Zimmer (for the CTA collaboration), T. Hassan, U. Schwanke","submitted_at":"2012-08-27T10:55:04Z","abstract_excerpt":"The Cherenkov Telescope Array (CTA) is a project for a next-generation observatory for very high energy (GeV-TeV) ground-based gamma-ray astronomy, currently in its design phase, and foreseen to be operative a few years from now. Several tens of telescopes of 2-3 different sizes, distributed over a large area, will allow for a sensitivity about a factor 10 better than current instruments such as H.E.S.S, MAGIC and VERITAS, an energy coverage from a few tens of GeV to several tens of TeV, and a field of view of up to 10 deg. In the following study, we investigate the prospects for CTA to study "},"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":"1208.5356","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2012-08-27T10:55:04Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"5e71c22e1ba1c9cc07cafafd82056e7c7260a6e2c1cc998bf2e100214c4a5d0b","abstract_canon_sha256":"3b44980404ca88ce54feff6a3c3de3cb0e29d5f96e14dd1236202807ec22dcf1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T23:53:42.926797Z","signature_b64":"uiD7/SmCF58eMI/IL5dgu6Df/ZjlWWtLQWk3ZCtr79CaXsQyAKC3lAPhcwcktH/41DFSRXOw4dkESlv24DqZBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c74706450061929395d05c14472039447372befa472901fb7bbaa4ef0c556981","last_reissued_at":"2026-07-04T23:53:42.926383Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T23:53:42.926383Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Matter and Fundamental Physics with the Cherenkov Telescope Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.IM","authors_text":"A. Gonzalez-Munoz, A. Jacholkowska, A. Moralejo, A. Stamerra, A.Viana, C. Jahn, D. Emmanoulopoulos, D. Horns, D. Nieto, E. Birsin, E. Moulin, G. Spengler, H. Sandaker, H. S. Zechlin, J. A. Barrio, J. Bolmont, J. Conrad, J. F. Glicenstein, J. L. Contreras, J. Ripken, M. A. Sanchez-Conde, M. Doro, M. Fornasa, M. Gaug, M. K. Daniel, N. Mirabal, P. Brun, R. Mazini, S. Colafrancesco, S. H. Connell, S. Zimmer (for the CTA collaboration), T. Hassan, U. Schwanke","submitted_at":"2012-08-27T10:55:04Z","abstract_excerpt":"The Cherenkov Telescope Array (CTA) is a project for a next-generation observatory for very high energy (GeV-TeV) ground-based gamma-ray astronomy, currently in its design phase, and foreseen to be operative a few years from now. Several tens of telescopes of 2-3 different sizes, distributed over a large area, will allow for a sensitivity about a factor 10 better than current instruments such as H.E.S.S, MAGIC and VERITAS, an energy coverage from a few tens of GeV to several tens of TeV, and a field of view of up to 10 deg. In the following study, we investigate the prospects for CTA to study "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.5356","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/1208.5356/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":"1208.5356","created_at":"2026-07-04T23:53:42.926444+00:00"},{"alias_kind":"arxiv_version","alias_value":"1208.5356v1","created_at":"2026-07-04T23:53:42.926444+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.5356","created_at":"2026-07-04T23:53:42.926444+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y5DQMRIAMGJJ","created_at":"2026-07-04T23:53:42.926444+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y5DQMRIAMGJJHFOQ","created_at":"2026-07-04T23:53:42.926444+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y5DQMRIA","created_at":"2026-07-04T23:53:42.926444+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/Y5DQMRIAMGJJHFOQLQKEOIBZIR","json":"https://pith.science/pith/Y5DQMRIAMGJJHFOQLQKEOIBZIR.json","graph_json":"https://pith.science/api/pith-number/Y5DQMRIAMGJJHFOQLQKEOIBZIR/graph.json","events_json":"https://pith.science/api/pith-number/Y5DQMRIAMGJJHFOQLQKEOIBZIR/events.json","paper":"https://pith.science/paper/Y5DQMRIA"},"agent_actions":{"view_html":"https://pith.science/pith/Y5DQMRIAMGJJHFOQLQKEOIBZIR","download_json":"https://pith.science/pith/Y5DQMRIAMGJJHFOQLQKEOIBZIR.json","view_paper":"https://pith.science/paper/Y5DQMRIA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1208.5356&json=true","fetch_graph":"https://pith.science/api/pith-number/Y5DQMRIAMGJJHFOQLQKEOIBZIR/graph.json","fetch_events":"https://pith.science/api/pith-number/Y5DQMRIAMGJJHFOQLQKEOIBZIR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y5DQMRIAMGJJHFOQLQKEOIBZIR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y5DQMRIAMGJJHFOQLQKEOIBZIR/action/storage_attestation","attest_author":"https://pith.science/pith/Y5DQMRIAMGJJHFOQLQKEOIBZIR/action/author_attestation","sign_citation":"https://pith.science/pith/Y5DQMRIAMGJJHFOQLQKEOIBZIR/action/citation_signature","submit_replication":"https://pith.science/pith/Y5DQMRIAMGJJHFOQLQKEOIBZIR/action/replication_record"}},"created_at":"2026-07-04T23:53:42.926444+00:00","updated_at":"2026-07-04T23:53:42.926444+00:00"}