{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:CBZYCKMJGNWLEKTX46HGMQYOGI","short_pith_number":"pith:CBZYCKMJ","schema_version":"1.0","canonical_sha256":"1073812989336cb22a77e78e66430e322ca4f47c9bd7f2198666b4e3e8c5816f","source":{"kind":"arxiv","id":"0902.4594","version":1},"attestation_state":"computed","paper":{"title":"Monitoring of Bright Blazars with MAGIC in the 2007/2008 Season","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Antonio Stamerra, Ching-Cheng Hsu, Elina Lindfors, Elisa Bernardini, Florian Goebel, Giacomo Bonnoli, Konstancja Satalecka, Nicola Galante, Pratik Majumdar, Robert Wagner (MAGIC collaboration)","submitted_at":"2009-02-26T14:57:17Z","abstract_excerpt":"Because of the short duty-cycles and observation-time constraints, studies of bright TeV (E>100 GeV) blazars are mostly restricted to flaring episodes or rather short (days to few weeks) multiwavelength campaigns. At the same time, long-term studies of these objects are essential to gain a more complete understanding of the blazar phenomenon and to constrain theoretical models concerning jet physics. Only unbiased long-term studies are adequate for the determination of flaring state probabilities and for estimating the statistical significance of possible correlations between TeV flaring state"},"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":"0902.4594","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-02-26T14:57:17Z","cross_cats_sorted":[],"title_canon_sha256":"898ba7cfc907afe7bc4c0f45e13e233027429ef9a087327837a06adbc00abda1","abstract_canon_sha256":"e0326332227750bb583b0c327b60714d927e23c0c43e81c20224ebdb62e47154"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:33:40.026790Z","signature_b64":"dWMR1OQ+xQXEHRaXJuYAoM9tk9e8E132TGC0KrhZ6neoRgRXvotFfu+mH0znLfr43BsQcg34Ei3Ow0ffJ+hTDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1073812989336cb22a77e78e66430e322ca4f47c9bd7f2198666b4e3e8c5816f","last_reissued_at":"2026-05-18T04:33:40.026257Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:33:40.026257Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Monitoring of Bright Blazars with MAGIC in the 2007/2008 Season","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Antonio Stamerra, Ching-Cheng Hsu, Elina Lindfors, Elisa Bernardini, Florian Goebel, Giacomo Bonnoli, Konstancja Satalecka, Nicola Galante, Pratik Majumdar, Robert Wagner (MAGIC collaboration)","submitted_at":"2009-02-26T14:57:17Z","abstract_excerpt":"Because of the short duty-cycles and observation-time constraints, studies of bright TeV (E>100 GeV) blazars are mostly restricted to flaring episodes or rather short (days to few weeks) multiwavelength campaigns. At the same time, long-term studies of these objects are essential to gain a more complete understanding of the blazar phenomenon and to constrain theoretical models concerning jet physics. Only unbiased long-term studies are adequate for the determination of flaring state probabilities and for estimating the statistical significance of possible correlations between TeV flaring state"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0902.4594","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":""},"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":"0902.4594","created_at":"2026-05-18T04:33:40.026355+00:00"},{"alias_kind":"arxiv_version","alias_value":"0902.4594v1","created_at":"2026-05-18T04:33:40.026355+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0902.4594","created_at":"2026-05-18T04:33:40.026355+00:00"},{"alias_kind":"pith_short_12","alias_value":"CBZYCKMJGNWL","created_at":"2026-05-18T12:25:59.703012+00:00"},{"alias_kind":"pith_short_16","alias_value":"CBZYCKMJGNWLEKTX","created_at":"2026-05-18T12:25:59.703012+00:00"},{"alias_kind":"pith_short_8","alias_value":"CBZYCKMJ","created_at":"2026-05-18T12:25:59.703012+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/CBZYCKMJGNWLEKTX46HGMQYOGI","json":"https://pith.science/pith/CBZYCKMJGNWLEKTX46HGMQYOGI.json","graph_json":"https://pith.science/api/pith-number/CBZYCKMJGNWLEKTX46HGMQYOGI/graph.json","events_json":"https://pith.science/api/pith-number/CBZYCKMJGNWLEKTX46HGMQYOGI/events.json","paper":"https://pith.science/paper/CBZYCKMJ"},"agent_actions":{"view_html":"https://pith.science/pith/CBZYCKMJGNWLEKTX46HGMQYOGI","download_json":"https://pith.science/pith/CBZYCKMJGNWLEKTX46HGMQYOGI.json","view_paper":"https://pith.science/paper/CBZYCKMJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0902.4594&json=true","fetch_graph":"https://pith.science/api/pith-number/CBZYCKMJGNWLEKTX46HGMQYOGI/graph.json","fetch_events":"https://pith.science/api/pith-number/CBZYCKMJGNWLEKTX46HGMQYOGI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CBZYCKMJGNWLEKTX46HGMQYOGI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CBZYCKMJGNWLEKTX46HGMQYOGI/action/storage_attestation","attest_author":"https://pith.science/pith/CBZYCKMJGNWLEKTX46HGMQYOGI/action/author_attestation","sign_citation":"https://pith.science/pith/CBZYCKMJGNWLEKTX46HGMQYOGI/action/citation_signature","submit_replication":"https://pith.science/pith/CBZYCKMJGNWLEKTX46HGMQYOGI/action/replication_record"}},"created_at":"2026-05-18T04:33:40.026355+00:00","updated_at":"2026-05-18T04:33:40.026355+00:00"}