{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:4PAP7DHGKM4HMP7QQ2PNGLFFCJ","short_pith_number":"pith:4PAP7DHG","schema_version":"1.0","canonical_sha256":"e3c0ff8ce65338763ff0869ed32ca51247e181a3013d03c3d210f9e63d19fb83","source":{"kind":"arxiv","id":"2003.12190","version":2},"attestation_state":"computed","paper":{"title":"A broadband X-ray study of a sample of AGNs with [OIII] measured inclinations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"M. Ajello, M. Balokovic, S. Marchesi, T. Fischer, X. Zhao","submitted_at":"2020-03-27T00:27:52Z","abstract_excerpt":"In modeling the X-ray spectra of active galactic nuclei (AGNs), the inclination angle is a parameter that can play an important role in analyzing the X-ray spectra of AGN, but it has never been studied in detail. We present a broadband X-ray spectral analysis of the joint NuSTAR-XMM-Newton observations of 13 sources with [OIII] measured inclinations determined by Fischer et al. 2013. By freezing the inclination angles at the [OIII] measured values when modeling the observations, the spectra are well fitted and the geometrical properties of the obscuring structure of the AGNs are slightly bette"},"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":"2003.12190","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-03-27T00:27:52Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"69da3a899b3e5e92f05014dd26e0f9124bc548c32d9ec2f954d87daf369dcae5","abstract_canon_sha256":"357a2cd9492d29457c652884386bd83f4ad220d247bd562f0013ffef78c45501"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:02:13.394931Z","signature_b64":"3PLAsUlsBtIN+BGS8V/AlDMAlG0Y5NveP3bP9H9VvHU6va/8oT7qg6Fo5bKHFwOC5i6ld4IrC5Y0tqeg3NvHAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e3c0ff8ce65338763ff0869ed32ca51247e181a3013d03c3d210f9e63d19fb83","last_reissued_at":"2026-07-05T01:02:13.394523Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:02:13.394523Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A broadband X-ray study of a sample of AGNs with [OIII] measured inclinations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"M. Ajello, M. Balokovic, S. Marchesi, T. Fischer, X. Zhao","submitted_at":"2020-03-27T00:27:52Z","abstract_excerpt":"In modeling the X-ray spectra of active galactic nuclei (AGNs), the inclination angle is a parameter that can play an important role in analyzing the X-ray spectra of AGN, but it has never been studied in detail. We present a broadband X-ray spectral analysis of the joint NuSTAR-XMM-Newton observations of 13 sources with [OIII] measured inclinations determined by Fischer et al. 2013. By freezing the inclination angles at the [OIII] measured values when modeling the observations, the spectra are well fitted and the geometrical properties of the obscuring structure of the AGNs are slightly bette"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2003.12190","kind":"arxiv","version":2},"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/2003.12190/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":"2003.12190","created_at":"2026-07-05T01:02:13.394581+00:00"},{"alias_kind":"arxiv_version","alias_value":"2003.12190v2","created_at":"2026-07-05T01:02:13.394581+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2003.12190","created_at":"2026-07-05T01:02:13.394581+00:00"},{"alias_kind":"pith_short_12","alias_value":"4PAP7DHGKM4H","created_at":"2026-07-05T01:02:13.394581+00:00"},{"alias_kind":"pith_short_16","alias_value":"4PAP7DHGKM4HMP7Q","created_at":"2026-07-05T01:02:13.394581+00:00"},{"alias_kind":"pith_short_8","alias_value":"4PAP7DHG","created_at":"2026-07-05T01:02:13.394581+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/4PAP7DHGKM4HMP7QQ2PNGLFFCJ","json":"https://pith.science/pith/4PAP7DHGKM4HMP7QQ2PNGLFFCJ.json","graph_json":"https://pith.science/api/pith-number/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/graph.json","events_json":"https://pith.science/api/pith-number/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/events.json","paper":"https://pith.science/paper/4PAP7DHG"},"agent_actions":{"view_html":"https://pith.science/pith/4PAP7DHGKM4HMP7QQ2PNGLFFCJ","download_json":"https://pith.science/pith/4PAP7DHGKM4HMP7QQ2PNGLFFCJ.json","view_paper":"https://pith.science/paper/4PAP7DHG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2003.12190&json=true","fetch_graph":"https://pith.science/api/pith-number/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/graph.json","fetch_events":"https://pith.science/api/pith-number/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/action/storage_attestation","attest_author":"https://pith.science/pith/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/action/author_attestation","sign_citation":"https://pith.science/pith/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/action/citation_signature","submit_replication":"https://pith.science/pith/4PAP7DHGKM4HMP7QQ2PNGLFFCJ/action/replication_record"}},"created_at":"2026-07-05T01:02:13.394581+00:00","updated_at":"2026-07-05T01:02:13.394581+00:00"}