{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:FCNT3DI7A2N7JV2HMOLUEGPOZQ","short_pith_number":"pith:FCNT3DI7","schema_version":"1.0","canonical_sha256":"289b3d8d1f069bf4d74763974219eecc3325823f4d1bd4a30b1e2de3e0ae52d0","source":{"kind":"arxiv","id":"1010.2085","version":1},"attestation_state":"computed","paper":{"title":"Suzaku and SWIFT-BAT observations of a newly discovered Compton-thick AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"A. Caccianiga, A. Moretti, C. Vignali, P. Severgnini, R. Della Ceca, V. Braito, V. La Parola","submitted_at":"2010-10-11T12:33:47Z","abstract_excerpt":"Obscured AGN are fundamental to understand the history of Super Massive Black Hole growth and their influence on galaxy formation. However, the Compton-thick AGN (NH>1e24 cm^-2) population is basically unconstrained, with less than few dozen confirmed Compton-thick AGN found and studied so far. A way to select heavily obscured AGN is to compare the X-ray emission below 10 keV (which is strongly depressed) with the emission from other bands less affected by the absorption, i.e. the IR band. To this end, we have cross-correlated the 2XMM catalogue with the IRAS Point Source catalogue and, by usi"},"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":"1010.2085","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-10-11T12:33:47Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"8b4f268755cd57b70e2c058a2223c75c7f8eee7e64ca705c25ff1d52856a3973","abstract_canon_sha256":"db27cf51dcb7de36fc80bdd211074db715ff8e90ff015058d758707553aa1ede"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:06.713580Z","signature_b64":"AvGmQ9AkyQjJ4WBs70NK7+ujCmE/GOctO1DHWtfHSJV0ejo2hONJpKUjzZSblMkxIClBw7xH8Ikct4/wuiAwDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"289b3d8d1f069bf4d74763974219eecc3325823f4d1bd4a30b1e2de3e0ae52d0","last_reissued_at":"2026-05-18T02:05:06.712674Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:06.712674Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Suzaku and SWIFT-BAT observations of a newly discovered Compton-thick AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"A. Caccianiga, A. Moretti, C. Vignali, P. Severgnini, R. Della Ceca, V. Braito, V. La Parola","submitted_at":"2010-10-11T12:33:47Z","abstract_excerpt":"Obscured AGN are fundamental to understand the history of Super Massive Black Hole growth and their influence on galaxy formation. However, the Compton-thick AGN (NH>1e24 cm^-2) population is basically unconstrained, with less than few dozen confirmed Compton-thick AGN found and studied so far. A way to select heavily obscured AGN is to compare the X-ray emission below 10 keV (which is strongly depressed) with the emission from other bands less affected by the absorption, i.e. the IR band. To this end, we have cross-correlated the 2XMM catalogue with the IRAS Point Source catalogue and, by usi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.2085","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":"1010.2085","created_at":"2026-05-18T02:05:06.712814+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.2085v1","created_at":"2026-05-18T02:05:06.712814+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.2085","created_at":"2026-05-18T02:05:06.712814+00:00"},{"alias_kind":"pith_short_12","alias_value":"FCNT3DI7A2N7","created_at":"2026-05-18T12:26:06.534383+00:00"},{"alias_kind":"pith_short_16","alias_value":"FCNT3DI7A2N7JV2H","created_at":"2026-05-18T12:26:06.534383+00:00"},{"alias_kind":"pith_short_8","alias_value":"FCNT3DI7","created_at":"2026-05-18T12:26:06.534383+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/FCNT3DI7A2N7JV2HMOLUEGPOZQ","json":"https://pith.science/pith/FCNT3DI7A2N7JV2HMOLUEGPOZQ.json","graph_json":"https://pith.science/api/pith-number/FCNT3DI7A2N7JV2HMOLUEGPOZQ/graph.json","events_json":"https://pith.science/api/pith-number/FCNT3DI7A2N7JV2HMOLUEGPOZQ/events.json","paper":"https://pith.science/paper/FCNT3DI7"},"agent_actions":{"view_html":"https://pith.science/pith/FCNT3DI7A2N7JV2HMOLUEGPOZQ","download_json":"https://pith.science/pith/FCNT3DI7A2N7JV2HMOLUEGPOZQ.json","view_paper":"https://pith.science/paper/FCNT3DI7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.2085&json=true","fetch_graph":"https://pith.science/api/pith-number/FCNT3DI7A2N7JV2HMOLUEGPOZQ/graph.json","fetch_events":"https://pith.science/api/pith-number/FCNT3DI7A2N7JV2HMOLUEGPOZQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FCNT3DI7A2N7JV2HMOLUEGPOZQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FCNT3DI7A2N7JV2HMOLUEGPOZQ/action/storage_attestation","attest_author":"https://pith.science/pith/FCNT3DI7A2N7JV2HMOLUEGPOZQ/action/author_attestation","sign_citation":"https://pith.science/pith/FCNT3DI7A2N7JV2HMOLUEGPOZQ/action/citation_signature","submit_replication":"https://pith.science/pith/FCNT3DI7A2N7JV2HMOLUEGPOZQ/action/replication_record"}},"created_at":"2026-05-18T02:05:06.712814+00:00","updated_at":"2026-05-18T02:05:06.712814+00:00"}