{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:RP3SR4CYV26SIDVWOEQ7NNFOVU","short_pith_number":"pith:RP3SR4CY","schema_version":"1.0","canonical_sha256":"8bf728f058aebd240eb67121f6b4aead1e1278a7ca3287bb361359d2da017a74","source":{"kind":"arxiv","id":"2103.12081","version":2},"attestation_state":"computed","paper":{"title":"Radiative Driving of the AGN Outflows in the Narrow-Line Seyfert 1 Galaxy NGC 4051","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Beena Meena, D. Michael Crenshaw, Dzhuliya Dashtamirova, Garrett E. Polack, Henrique R. Schmitt, Mitchell Revalski, Steven B. Kraemer, Travis C. Fischer","submitted_at":"2021-03-22T18:00:04Z","abstract_excerpt":"We explore the properties of ionized gas in the nuclear and circumnuclear environment of the narrow-line Seyfert 1 galaxy NGC 4051 using spectroscopic and imaging observations from the Hubble Space Telescope (HST) and Apache Point Observatory (APO)'s ARC 3.5m Telescope. We identify an unresolved moderate-density intermediate width component and a high-density broad component in the optical emission lines from the active nucleus, as well as spatially-resolved emission extending up to $\\sim$1 kpc in the AGN ionized narrow-line region (NLR) and $\\sim$8 kpc in the stellar ionized host galaxy. The "},"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":"2103.12081","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2021-03-22T18:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"3fc0ad4ce0d9b4fb7f894b8b39111909348d8c5da24b508ee9769278de34890b","abstract_canon_sha256":"f5f4ae1f4ec77c15a1b38ab4f0c0b8d8ae11dae62856682d546b3acb294b274a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:19:07.036217Z","signature_b64":"dGe0a7+RKuoC8+04v+u55IM/eobk+D3snhmPCfyE9ejsf2sa0gic+6ITXUwZ5HBVTHDl+U4LyXoj0WNYl5rXCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8bf728f058aebd240eb67121f6b4aead1e1278a7ca3287bb361359d2da017a74","last_reissued_at":"2026-07-05T03:19:07.035676Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:19:07.035676Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radiative Driving of the AGN Outflows in the Narrow-Line Seyfert 1 Galaxy NGC 4051","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Beena Meena, D. Michael Crenshaw, Dzhuliya Dashtamirova, Garrett E. Polack, Henrique R. Schmitt, Mitchell Revalski, Steven B. Kraemer, Travis C. Fischer","submitted_at":"2021-03-22T18:00:04Z","abstract_excerpt":"We explore the properties of ionized gas in the nuclear and circumnuclear environment of the narrow-line Seyfert 1 galaxy NGC 4051 using spectroscopic and imaging observations from the Hubble Space Telescope (HST) and Apache Point Observatory (APO)'s ARC 3.5m Telescope. We identify an unresolved moderate-density intermediate width component and a high-density broad component in the optical emission lines from the active nucleus, as well as spatially-resolved emission extending up to $\\sim$1 kpc in the AGN ionized narrow-line region (NLR) and $\\sim$8 kpc in the stellar ionized host galaxy. The "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2103.12081","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/2103.12081/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":"2103.12081","created_at":"2026-07-05T03:19:07.035758+00:00"},{"alias_kind":"arxiv_version","alias_value":"2103.12081v2","created_at":"2026-07-05T03:19:07.035758+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2103.12081","created_at":"2026-07-05T03:19:07.035758+00:00"},{"alias_kind":"pith_short_12","alias_value":"RP3SR4CYV26S","created_at":"2026-07-05T03:19:07.035758+00:00"},{"alias_kind":"pith_short_16","alias_value":"RP3SR4CYV26SIDVW","created_at":"2026-07-05T03:19:07.035758+00:00"},{"alias_kind":"pith_short_8","alias_value":"RP3SR4CY","created_at":"2026-07-05T03:19:07.035758+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/RP3SR4CYV26SIDVWOEQ7NNFOVU","json":"https://pith.science/pith/RP3SR4CYV26SIDVWOEQ7NNFOVU.json","graph_json":"https://pith.science/api/pith-number/RP3SR4CYV26SIDVWOEQ7NNFOVU/graph.json","events_json":"https://pith.science/api/pith-number/RP3SR4CYV26SIDVWOEQ7NNFOVU/events.json","paper":"https://pith.science/paper/RP3SR4CY"},"agent_actions":{"view_html":"https://pith.science/pith/RP3SR4CYV26SIDVWOEQ7NNFOVU","download_json":"https://pith.science/pith/RP3SR4CYV26SIDVWOEQ7NNFOVU.json","view_paper":"https://pith.science/paper/RP3SR4CY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2103.12081&json=true","fetch_graph":"https://pith.science/api/pith-number/RP3SR4CYV26SIDVWOEQ7NNFOVU/graph.json","fetch_events":"https://pith.science/api/pith-number/RP3SR4CYV26SIDVWOEQ7NNFOVU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RP3SR4CYV26SIDVWOEQ7NNFOVU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RP3SR4CYV26SIDVWOEQ7NNFOVU/action/storage_attestation","attest_author":"https://pith.science/pith/RP3SR4CYV26SIDVWOEQ7NNFOVU/action/author_attestation","sign_citation":"https://pith.science/pith/RP3SR4CYV26SIDVWOEQ7NNFOVU/action/citation_signature","submit_replication":"https://pith.science/pith/RP3SR4CYV26SIDVWOEQ7NNFOVU/action/replication_record"}},"created_at":"2026-07-05T03:19:07.035758+00:00","updated_at":"2026-07-05T03:19:07.035758+00:00"}