{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:5VGULQ6H42LHC7FVFDMJUETUHJ","short_pith_number":"pith:5VGULQ6H","schema_version":"1.0","canonical_sha256":"ed4d45c3c7e696717cb528d89a12743a78fc0dcf969a6ed02b9cb816f3260ee1","source":{"kind":"arxiv","id":"1701.07298","version":1},"attestation_state":"computed","paper":{"title":"Coexistence of a non thermal jet and a complex ultra fast X-ray outflow in a moderately luminous AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"2 - INAF/IAPS, 3 - CONACYT, 4 - UNAM, 5 - ESAC, 6), 6 - ISAS, 7 - SRON), A.L. Longinotti (3), E. Costantini (7), F. Panessa (2), M. Giroletti (1), M. Guainazzi (5, M. Santos-Lleo (5) (1 - INAF/IRA, Y. Krongold (4)","submitted_at":"2017-01-25T13:19:45Z","abstract_excerpt":"Context: Recent XMM-Newton observations have revealed that IRAS 17020+4544 is a very unusual example of black hole wind-produced feedback by a moderately luminous AGN in a spiral galaxy. Aims: Since the source is known for being a radio emitter, we investigated about the presence and the properties of a non-thermal component. Methods: We observed IRAS 17020+4544 with the Very Long Baseline Array at 5, 8, 15, and 24 GHz within a month of the 2014 XMM-Newton observations. We further analysed archival data taken in 2000 and 2012. Results: We detect the source at 5 GHz and on short baselines at 8 "},"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":"1701.07298","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-01-25T13:19:45Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"1851cb761f41e113707c3792c1cdd7b7504540cec2cfb1acf1e0fe36ad59e504","abstract_canon_sha256":"06b17a7aa94382cc715db64e8bfa30c087c37f0244c3791b40a1df23e29734c3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:46:37.813181Z","signature_b64":"kFXbK/R0EGzGi+mlN8SdSZDsAHkuqN1zZw/uhRVl2N+fdDXAN5EYl/cGKl462KLI4THx/eQ3LoQFUzKVnVgFBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ed4d45c3c7e696717cb528d89a12743a78fc0dcf969a6ed02b9cb816f3260ee1","last_reissued_at":"2026-05-18T00:46:37.812565Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:46:37.812565Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Coexistence of a non thermal jet and a complex ultra fast X-ray outflow in a moderately luminous AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"2 - INAF/IAPS, 3 - CONACYT, 4 - UNAM, 5 - ESAC, 6), 6 - ISAS, 7 - SRON), A.L. Longinotti (3), E. Costantini (7), F. Panessa (2), M. Giroletti (1), M. Guainazzi (5, M. Santos-Lleo (5) (1 - INAF/IRA, Y. Krongold (4)","submitted_at":"2017-01-25T13:19:45Z","abstract_excerpt":"Context: Recent XMM-Newton observations have revealed that IRAS 17020+4544 is a very unusual example of black hole wind-produced feedback by a moderately luminous AGN in a spiral galaxy. Aims: Since the source is known for being a radio emitter, we investigated about the presence and the properties of a non-thermal component. Methods: We observed IRAS 17020+4544 with the Very Long Baseline Array at 5, 8, 15, and 24 GHz within a month of the 2014 XMM-Newton observations. We further analysed archival data taken in 2000 and 2012. Results: We detect the source at 5 GHz and on short baselines at 8 "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.07298","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":"1701.07298","created_at":"2026-05-18T00:46:37.812659+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.07298v1","created_at":"2026-05-18T00:46:37.812659+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.07298","created_at":"2026-05-18T00:46:37.812659+00:00"},{"alias_kind":"pith_short_12","alias_value":"5VGULQ6H42LH","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_16","alias_value":"5VGULQ6H42LHC7FV","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_8","alias_value":"5VGULQ6H","created_at":"2026-05-18T12:31:00.734936+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/5VGULQ6H42LHC7FVFDMJUETUHJ","json":"https://pith.science/pith/5VGULQ6H42LHC7FVFDMJUETUHJ.json","graph_json":"https://pith.science/api/pith-number/5VGULQ6H42LHC7FVFDMJUETUHJ/graph.json","events_json":"https://pith.science/api/pith-number/5VGULQ6H42LHC7FVFDMJUETUHJ/events.json","paper":"https://pith.science/paper/5VGULQ6H"},"agent_actions":{"view_html":"https://pith.science/pith/5VGULQ6H42LHC7FVFDMJUETUHJ","download_json":"https://pith.science/pith/5VGULQ6H42LHC7FVFDMJUETUHJ.json","view_paper":"https://pith.science/paper/5VGULQ6H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.07298&json=true","fetch_graph":"https://pith.science/api/pith-number/5VGULQ6H42LHC7FVFDMJUETUHJ/graph.json","fetch_events":"https://pith.science/api/pith-number/5VGULQ6H42LHC7FVFDMJUETUHJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5VGULQ6H42LHC7FVFDMJUETUHJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5VGULQ6H42LHC7FVFDMJUETUHJ/action/storage_attestation","attest_author":"https://pith.science/pith/5VGULQ6H42LHC7FVFDMJUETUHJ/action/author_attestation","sign_citation":"https://pith.science/pith/5VGULQ6H42LHC7FVFDMJUETUHJ/action/citation_signature","submit_replication":"https://pith.science/pith/5VGULQ6H42LHC7FVFDMJUETUHJ/action/replication_record"}},"created_at":"2026-05-18T00:46:37.812659+00:00","updated_at":"2026-05-18T00:46:37.812659+00:00"}