{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:LYX7H2HTITO62GO2UKXASH2CU3","short_pith_number":"pith:LYX7H2HT","schema_version":"1.0","canonical_sha256":"5e2ff3e8f344dded19daa2ae091f42a6d2503371144697c39c4362b89dfdb3da","source":{"kind":"arxiv","id":"1007.1638","version":1},"attestation_state":"computed","paper":{"title":"The broad-band X-ray spectrum of the Seyfert 1 galaxy, MCG+8-11-11","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alessandra De Rosa, Elena Jim\\'enez Bail\\'on, Enrico Piconcelli, Giorgio Matt, Ilaria De Angelis, Paola Grandi, Stefano Bianchi, Valentina La Parola","submitted_at":"2010-07-09T17:49:18Z","abstract_excerpt":"We present a long (100 ks) Suzaku observation of one of the X-ray brightest AGN, MCG+8-11-11. These data were complemented with the 54-month Swift BAT spectrum, allowing us to perform a broad-band fit in the 0.6-150 keV range. The fits performed in the 0.6-10 keV band give consistent results with respect to a previous XMM-Newton observation, i.e. the lack of a soft excess, warm absorption along the line of sight, a large Compton reflection component (R~1) and the absence of a relativistic component of the neutral iron K$\\alpha$ emission line. However, when the PIN and Swift BAT data are includ"},"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":"1007.1638","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-07-09T17:49:18Z","cross_cats_sorted":[],"title_canon_sha256":"cd5fe5b859c087dd72e7f525ebc9742db2c5bd0e3d4fb1b636d8c39585dd5f1c","abstract_canon_sha256":"3c6ab470f5528792ae081db4e7d1e4d5579f81e6e57a879fce5c57bcb71d5781"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:06:23.315286Z","signature_b64":"iR+B4btP8vh30AmTeMSAK56ZOpuWy15w0q7Gk/GDGpz+VArlBR3HBkHRQ6M+1BI/6eSEESP6i9iLi97YGAJGCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5e2ff3e8f344dded19daa2ae091f42a6d2503371144697c39c4362b89dfdb3da","last_reissued_at":"2026-05-18T02:06:23.314714Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:06:23.314714Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The broad-band X-ray spectrum of the Seyfert 1 galaxy, MCG+8-11-11","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alessandra De Rosa, Elena Jim\\'enez Bail\\'on, Enrico Piconcelli, Giorgio Matt, Ilaria De Angelis, Paola Grandi, Stefano Bianchi, Valentina La Parola","submitted_at":"2010-07-09T17:49:18Z","abstract_excerpt":"We present a long (100 ks) Suzaku observation of one of the X-ray brightest AGN, MCG+8-11-11. These data were complemented with the 54-month Swift BAT spectrum, allowing us to perform a broad-band fit in the 0.6-150 keV range. The fits performed in the 0.6-10 keV band give consistent results with respect to a previous XMM-Newton observation, i.e. the lack of a soft excess, warm absorption along the line of sight, a large Compton reflection component (R~1) and the absence of a relativistic component of the neutral iron K$\\alpha$ emission line. However, when the PIN and Swift BAT data are includ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1007.1638","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":"1007.1638","created_at":"2026-05-18T02:06:23.314778+00:00"},{"alias_kind":"arxiv_version","alias_value":"1007.1638v1","created_at":"2026-05-18T02:06:23.314778+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1007.1638","created_at":"2026-05-18T02:06:23.314778+00:00"},{"alias_kind":"pith_short_12","alias_value":"LYX7H2HTITO6","created_at":"2026-05-18T12:26:10.704358+00:00"},{"alias_kind":"pith_short_16","alias_value":"LYX7H2HTITO62GO2","created_at":"2026-05-18T12:26:10.704358+00:00"},{"alias_kind":"pith_short_8","alias_value":"LYX7H2HT","created_at":"2026-05-18T12:26:10.704358+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/LYX7H2HTITO62GO2UKXASH2CU3","json":"https://pith.science/pith/LYX7H2HTITO62GO2UKXASH2CU3.json","graph_json":"https://pith.science/api/pith-number/LYX7H2HTITO62GO2UKXASH2CU3/graph.json","events_json":"https://pith.science/api/pith-number/LYX7H2HTITO62GO2UKXASH2CU3/events.json","paper":"https://pith.science/paper/LYX7H2HT"},"agent_actions":{"view_html":"https://pith.science/pith/LYX7H2HTITO62GO2UKXASH2CU3","download_json":"https://pith.science/pith/LYX7H2HTITO62GO2UKXASH2CU3.json","view_paper":"https://pith.science/paper/LYX7H2HT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1007.1638&json=true","fetch_graph":"https://pith.science/api/pith-number/LYX7H2HTITO62GO2UKXASH2CU3/graph.json","fetch_events":"https://pith.science/api/pith-number/LYX7H2HTITO62GO2UKXASH2CU3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LYX7H2HTITO62GO2UKXASH2CU3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LYX7H2HTITO62GO2UKXASH2CU3/action/storage_attestation","attest_author":"https://pith.science/pith/LYX7H2HTITO62GO2UKXASH2CU3/action/author_attestation","sign_citation":"https://pith.science/pith/LYX7H2HTITO62GO2UKXASH2CU3/action/citation_signature","submit_replication":"https://pith.science/pith/LYX7H2HTITO62GO2UKXASH2CU3/action/replication_record"}},"created_at":"2026-05-18T02:06:23.314778+00:00","updated_at":"2026-05-18T02:06:23.314778+00:00"}