{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:SUO7XDXDKQN4DVRBKE3HF6IS4R","short_pith_number":"pith:SUO7XDXD","schema_version":"1.0","canonical_sha256":"951dfb8ee3541bc1d621513672f912e45cf934359d397b43445d5b614b4248da","source":{"kind":"arxiv","id":"1303.3587","version":1},"attestation_state":"computed","paper":{"title":"Identification of Outflows and Candidate Dual Active Galactic Nuclei in SDSS Quasars at z=0.8-1.6","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Claud H. Sandberg Lacy, Daniel Kennefick, Joel C. Berrier, Julia Kennefick, Julia M. Comerford, R. Scott Barrows","submitted_at":"2013-03-14T20:00:06Z","abstract_excerpt":"We present a sample of 131 quasars from the Sloan Digital Sky Survey at redshifts 0.8<z<1.6 with double peaks in either of the high-ionization narrow emission lines [NeV]3426 or [NeIII]3869. These sources were selected with the intention of identifying high-redshift analogs of the z<0.8 active galactic nuclei (AGN) with double-peaked [OIII]5007 lines, which might represent AGN outflows or dual AGN. Lines of high-ionization potential are believed to originate in the inner, highly photoionized portion of the narrow line region (NLR), and we exploit this assumption to investigate the possible kin"},"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":"1303.3587","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-03-14T20:00:06Z","cross_cats_sorted":[],"title_canon_sha256":"f1242ea09eae2d744aa39b6468088dfe4364e68c458f42cf269513c042ab7de3","abstract_canon_sha256":"35ab32ef82cafc4cdcf1d6b74b966f2bf712d2da216211daf5b5bbabbb3c317f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:07.136305Z","signature_b64":"3z2EEdDmikxn0RTFNrTmnSArXS1NRVr/6xwB8cmNhdvAXhN+WV4l22wKEYWiYskgQz1d/NOSdX/feP5uOYNUAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"951dfb8ee3541bc1d621513672f912e45cf934359d397b43445d5b614b4248da","last_reissued_at":"2026-05-18T01:51:07.135748Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:07.135748Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Identification of Outflows and Candidate Dual Active Galactic Nuclei in SDSS Quasars at z=0.8-1.6","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Claud H. Sandberg Lacy, Daniel Kennefick, Joel C. Berrier, Julia Kennefick, Julia M. Comerford, R. Scott Barrows","submitted_at":"2013-03-14T20:00:06Z","abstract_excerpt":"We present a sample of 131 quasars from the Sloan Digital Sky Survey at redshifts 0.8<z<1.6 with double peaks in either of the high-ionization narrow emission lines [NeV]3426 or [NeIII]3869. These sources were selected with the intention of identifying high-redshift analogs of the z<0.8 active galactic nuclei (AGN) with double-peaked [OIII]5007 lines, which might represent AGN outflows or dual AGN. Lines of high-ionization potential are believed to originate in the inner, highly photoionized portion of the narrow line region (NLR), and we exploit this assumption to investigate the possible kin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.3587","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":"1303.3587","created_at":"2026-05-18T01:51:07.135854+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.3587v1","created_at":"2026-05-18T01:51:07.135854+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.3587","created_at":"2026-05-18T01:51:07.135854+00:00"},{"alias_kind":"pith_short_12","alias_value":"SUO7XDXDKQN4","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"SUO7XDXDKQN4DVRB","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"SUO7XDXD","created_at":"2026-05-18T12:27:59.945178+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/SUO7XDXDKQN4DVRBKE3HF6IS4R","json":"https://pith.science/pith/SUO7XDXDKQN4DVRBKE3HF6IS4R.json","graph_json":"https://pith.science/api/pith-number/SUO7XDXDKQN4DVRBKE3HF6IS4R/graph.json","events_json":"https://pith.science/api/pith-number/SUO7XDXDKQN4DVRBKE3HF6IS4R/events.json","paper":"https://pith.science/paper/SUO7XDXD"},"agent_actions":{"view_html":"https://pith.science/pith/SUO7XDXDKQN4DVRBKE3HF6IS4R","download_json":"https://pith.science/pith/SUO7XDXDKQN4DVRBKE3HF6IS4R.json","view_paper":"https://pith.science/paper/SUO7XDXD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.3587&json=true","fetch_graph":"https://pith.science/api/pith-number/SUO7XDXDKQN4DVRBKE3HF6IS4R/graph.json","fetch_events":"https://pith.science/api/pith-number/SUO7XDXDKQN4DVRBKE3HF6IS4R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SUO7XDXDKQN4DVRBKE3HF6IS4R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SUO7XDXDKQN4DVRBKE3HF6IS4R/action/storage_attestation","attest_author":"https://pith.science/pith/SUO7XDXDKQN4DVRBKE3HF6IS4R/action/author_attestation","sign_citation":"https://pith.science/pith/SUO7XDXDKQN4DVRBKE3HF6IS4R/action/citation_signature","submit_replication":"https://pith.science/pith/SUO7XDXDKQN4DVRBKE3HF6IS4R/action/replication_record"}},"created_at":"2026-05-18T01:51:07.135854+00:00","updated_at":"2026-05-18T01:51:07.135854+00:00"}