{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:C2YOJPA74EVWUCTMRTYHDXQKXH","short_pith_number":"pith:C2YOJPA7","schema_version":"1.0","canonical_sha256":"16b0e4bc1fe12b6a0a6c8cf071de0ab9f193a09d9bef59ddde124217f3598d38","source":{"kind":"arxiv","id":"1807.00548","version":1},"attestation_state":"computed","paper":{"title":"A new powerful and highly variable disk wind in an AGN-star forming galaxy, the case of MCG-03-58-007","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Caccianiga, C. Cicone, G. A. Matzeu, J. N. Reeves, L. Ballo, P. Severgnini, R. Della Ceca, S. Campana, T. J. Turner, V. Braito","submitted_at":"2018-07-02T09:12:35Z","abstract_excerpt":"We present the discovery of a new candidate for a fast disk wind, in the nearby Seyfert 2 galaxy MCG-03-58-007. This wind is discovered in a deep Suzaku observation that was performed in 2010. Overall the X-ray spectrum of MCG-03-58-007 is highly absorbed by a neutral column density of NH~10^23 cm^-2, in agreement with the optical classification as a type 2 AGN. In addition, this observation unveiled the presence of two deep absorption troughs at E = 7.4 +- 0.1 keV and E = 8.5 +- 0.2 keV. If associated with blue-shifted FeXXVI, these features can be explained with the presence of two highly io"},"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":"1807.00548","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-07-02T09:12:35Z","cross_cats_sorted":[],"title_canon_sha256":"702fc84e95fc57d5604ef1446f8d8e8ecd7704c73f4de0124f5983946608d340","abstract_canon_sha256":"11bf9139ef483ee8d3f40d3d3d0ad164859812a6652a27e7a68949cce14fd565"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:04.114424Z","signature_b64":"JVPVaT4g52+f3Znf4RUd5kHTq7HGNqD3UzO7FeDk36E+FdU4tGvkp/i8ptMAratRWn68gP49eEoj60hYxPjqBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"16b0e4bc1fe12b6a0a6c8cf071de0ab9f193a09d9bef59ddde124217f3598d38","last_reissued_at":"2026-05-18T00:11:04.113729Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:04.113729Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A new powerful and highly variable disk wind in an AGN-star forming galaxy, the case of MCG-03-58-007","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Caccianiga, C. Cicone, G. A. Matzeu, J. N. Reeves, L. Ballo, P. Severgnini, R. Della Ceca, S. Campana, T. J. Turner, V. Braito","submitted_at":"2018-07-02T09:12:35Z","abstract_excerpt":"We present the discovery of a new candidate for a fast disk wind, in the nearby Seyfert 2 galaxy MCG-03-58-007. This wind is discovered in a deep Suzaku observation that was performed in 2010. Overall the X-ray spectrum of MCG-03-58-007 is highly absorbed by a neutral column density of NH~10^23 cm^-2, in agreement with the optical classification as a type 2 AGN. In addition, this observation unveiled the presence of two deep absorption troughs at E = 7.4 +- 0.1 keV and E = 8.5 +- 0.2 keV. If associated with blue-shifted FeXXVI, these features can be explained with the presence of two highly io"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.00548","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":"1807.00548","created_at":"2026-05-18T00:11:04.113831+00:00"},{"alias_kind":"arxiv_version","alias_value":"1807.00548v1","created_at":"2026-05-18T00:11:04.113831+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.00548","created_at":"2026-05-18T00:11:04.113831+00:00"},{"alias_kind":"pith_short_12","alias_value":"C2YOJPA74EVW","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_16","alias_value":"C2YOJPA74EVWUCTM","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_8","alias_value":"C2YOJPA7","created_at":"2026-05-18T12:32:16.446611+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/C2YOJPA74EVWUCTMRTYHDXQKXH","json":"https://pith.science/pith/C2YOJPA74EVWUCTMRTYHDXQKXH.json","graph_json":"https://pith.science/api/pith-number/C2YOJPA74EVWUCTMRTYHDXQKXH/graph.json","events_json":"https://pith.science/api/pith-number/C2YOJPA74EVWUCTMRTYHDXQKXH/events.json","paper":"https://pith.science/paper/C2YOJPA7"},"agent_actions":{"view_html":"https://pith.science/pith/C2YOJPA74EVWUCTMRTYHDXQKXH","download_json":"https://pith.science/pith/C2YOJPA74EVWUCTMRTYHDXQKXH.json","view_paper":"https://pith.science/paper/C2YOJPA7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1807.00548&json=true","fetch_graph":"https://pith.science/api/pith-number/C2YOJPA74EVWUCTMRTYHDXQKXH/graph.json","fetch_events":"https://pith.science/api/pith-number/C2YOJPA74EVWUCTMRTYHDXQKXH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/C2YOJPA74EVWUCTMRTYHDXQKXH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/C2YOJPA74EVWUCTMRTYHDXQKXH/action/storage_attestation","attest_author":"https://pith.science/pith/C2YOJPA74EVWUCTMRTYHDXQKXH/action/author_attestation","sign_citation":"https://pith.science/pith/C2YOJPA74EVWUCTMRTYHDXQKXH/action/citation_signature","submit_replication":"https://pith.science/pith/C2YOJPA74EVWUCTMRTYHDXQKXH/action/replication_record"}},"created_at":"2026-05-18T00:11:04.113831+00:00","updated_at":"2026-05-18T00:11:04.113831+00:00"}