{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:JOYZNYXXHVK7RPA5U4IMYAPLRH","short_pith_number":"pith:JOYZNYXX","schema_version":"1.0","canonical_sha256":"4bb196e2f73d55f8bc1da710cc01eb89e4ad79b4b78bb3e4c271009f08e07bbb","source":{"kind":"arxiv","id":"1105.2218","version":1},"attestation_state":"computed","paper":{"title":"A comprehensive approach to analyzing the XMM-Newton data of Seyfert 1 galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"\\'Angeles I. D\\'iaz, Guillermo F. H\\\"agele, Mar\\'ia Santos-Lle\\'o, M\\'onica V. Cardaci, Pedro Rodr\\'iguez-Pascual, Yair Krongold","submitted_at":"2011-05-11T15:18:40Z","abstract_excerpt":"Aims. We seek a comprehensive analysis of all the information provided by the XMM-Newton satellite of the four Seyfert 1 galaxies ESO 359-G19, HE 1143-1810, CTS A08.12, and Mrk 110, including the UV range, to characterize the different components that are emitting and absorbing radiation in the vicinity of the active nucleus.\n  Methods. The continuum emission was studied through the EPIC spectra by taking advantage of the spectral range of these cameras. The high-resolution RGS spectra were analyzed to characterize the absorbing and emission line features that arise in the spectra of the sourc"},"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":"1105.2218","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-05-11T15:18:40Z","cross_cats_sorted":[],"title_canon_sha256":"b0d44a93b2fa3ab7f5f04f4f2109e3c9bbd3af6ffceb04c48e92e7bd6175742f","abstract_canon_sha256":"bae2560ed466c34aa9b5a7c6c5eb90a75aae0589542d34371092c94daa2205c0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:22:21.265259Z","signature_b64":"UD56OhDKl0dyUWobZMER57Dnua7PnlpmF8Jg6qqwb69aG4rNAkVNJqmx7XNVd0k4M7a+b9L7hhUuBLhHed7+CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4bb196e2f73d55f8bc1da710cc01eb89e4ad79b4b78bb3e4c271009f08e07bbb","last_reissued_at":"2026-05-18T04:22:21.264557Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:22:21.264557Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A comprehensive approach to analyzing the XMM-Newton data of Seyfert 1 galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"\\'Angeles I. D\\'iaz, Guillermo F. H\\\"agele, Mar\\'ia Santos-Lle\\'o, M\\'onica V. Cardaci, Pedro Rodr\\'iguez-Pascual, Yair Krongold","submitted_at":"2011-05-11T15:18:40Z","abstract_excerpt":"Aims. We seek a comprehensive analysis of all the information provided by the XMM-Newton satellite of the four Seyfert 1 galaxies ESO 359-G19, HE 1143-1810, CTS A08.12, and Mrk 110, including the UV range, to characterize the different components that are emitting and absorbing radiation in the vicinity of the active nucleus.\n  Methods. The continuum emission was studied through the EPIC spectra by taking advantage of the spectral range of these cameras. The high-resolution RGS spectra were analyzed to characterize the absorbing and emission line features that arise in the spectra of the sourc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1105.2218","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":"1105.2218","created_at":"2026-05-18T04:22:21.264661+00:00"},{"alias_kind":"arxiv_version","alias_value":"1105.2218v1","created_at":"2026-05-18T04:22:21.264661+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1105.2218","created_at":"2026-05-18T04:22:21.264661+00:00"},{"alias_kind":"pith_short_12","alias_value":"JOYZNYXXHVK7","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_16","alias_value":"JOYZNYXXHVK7RPA5","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_8","alias_value":"JOYZNYXX","created_at":"2026-05-18T12:26:32.869790+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/JOYZNYXXHVK7RPA5U4IMYAPLRH","json":"https://pith.science/pith/JOYZNYXXHVK7RPA5U4IMYAPLRH.json","graph_json":"https://pith.science/api/pith-number/JOYZNYXXHVK7RPA5U4IMYAPLRH/graph.json","events_json":"https://pith.science/api/pith-number/JOYZNYXXHVK7RPA5U4IMYAPLRH/events.json","paper":"https://pith.science/paper/JOYZNYXX"},"agent_actions":{"view_html":"https://pith.science/pith/JOYZNYXXHVK7RPA5U4IMYAPLRH","download_json":"https://pith.science/pith/JOYZNYXXHVK7RPA5U4IMYAPLRH.json","view_paper":"https://pith.science/paper/JOYZNYXX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1105.2218&json=true","fetch_graph":"https://pith.science/api/pith-number/JOYZNYXXHVK7RPA5U4IMYAPLRH/graph.json","fetch_events":"https://pith.science/api/pith-number/JOYZNYXXHVK7RPA5U4IMYAPLRH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JOYZNYXXHVK7RPA5U4IMYAPLRH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JOYZNYXXHVK7RPA5U4IMYAPLRH/action/storage_attestation","attest_author":"https://pith.science/pith/JOYZNYXXHVK7RPA5U4IMYAPLRH/action/author_attestation","sign_citation":"https://pith.science/pith/JOYZNYXXHVK7RPA5U4IMYAPLRH/action/citation_signature","submit_replication":"https://pith.science/pith/JOYZNYXXHVK7RPA5U4IMYAPLRH/action/replication_record"}},"created_at":"2026-05-18T04:22:21.264661+00:00","updated_at":"2026-05-18T04:22:21.264661+00:00"}