{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:WZXNSO4KNO3QBHY5YBPO6NZTH6","short_pith_number":"pith:WZXNSO4K","schema_version":"1.0","canonical_sha256":"b66ed93b8a6bb7009f1dc05eef37333fa623f1777581fb0018e3e97746f5b1ac","source":{"kind":"arxiv","id":"1305.4938","version":1},"attestation_state":"computed","paper":{"title":"The central kpc of edge-on AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andreas Eckart, Jenz Zuther, Monica Valencia-S., Sebastian Fischer, Semir Smaji\\'c","submitted_at":"2013-05-21T20:00:06Z","abstract_excerpt":"The NIR is less influenced by dust extinction than optical light. This enables us to look to an extent through dusty regions. In addition, it is sensitive to the mass-dominating stellar population. The combination of NIR imaging and spectroscopy of the VLT integral field spectrograph SINFONI gives us the opportunity to analyze several emission and absorption lines and to investigate the stellar population and ionization mechanisms over a field of view (FOV) of 4x4 square arcsec. We detect several emission lines ([Si VI], Pa\\alpha, Br\\gamma, H_2, [Fe II]) and analyze these to disentangle the 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":"1305.4938","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-05-21T20:00:06Z","cross_cats_sorted":[],"title_canon_sha256":"3d9acaa91707c970cdeda69b9dcbcd6285e933b449e668d74d2b7ccd2e377fcf","abstract_canon_sha256":"a9953323d4585649a1b143f7ccc9995153f45257452dcf2a1c5f8d14d50ab6ca"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:25:13.882886Z","signature_b64":"ytSr15UQTnJqRGrTkBpyEoyP3XWrWk1OZY3Vem2ag8Ux27DQ58/+RZ+tc/L2yy9sYFqlYenyeSM5W4YvuQY5CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b66ed93b8a6bb7009f1dc05eef37333fa623f1777581fb0018e3e97746f5b1ac","last_reissued_at":"2026-05-18T03:25:13.882244Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:25:13.882244Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The central kpc of edge-on AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andreas Eckart, Jenz Zuther, Monica Valencia-S., Sebastian Fischer, Semir Smaji\\'c","submitted_at":"2013-05-21T20:00:06Z","abstract_excerpt":"The NIR is less influenced by dust extinction than optical light. This enables us to look to an extent through dusty regions. In addition, it is sensitive to the mass-dominating stellar population. The combination of NIR imaging and spectroscopy of the VLT integral field spectrograph SINFONI gives us the opportunity to analyze several emission and absorption lines and to investigate the stellar population and ionization mechanisms over a field of view (FOV) of 4x4 square arcsec. We detect several emission lines ([Si VI], Pa\\alpha, Br\\gamma, H_2, [Fe II]) and analyze these to disentangle the io"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.4938","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":"1305.4938","created_at":"2026-05-18T03:25:13.882350+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.4938v1","created_at":"2026-05-18T03:25:13.882350+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.4938","created_at":"2026-05-18T03:25:13.882350+00:00"},{"alias_kind":"pith_short_12","alias_value":"WZXNSO4KNO3Q","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_16","alias_value":"WZXNSO4KNO3QBHY5","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_8","alias_value":"WZXNSO4K","created_at":"2026-05-18T12:28:06.772260+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/WZXNSO4KNO3QBHY5YBPO6NZTH6","json":"https://pith.science/pith/WZXNSO4KNO3QBHY5YBPO6NZTH6.json","graph_json":"https://pith.science/api/pith-number/WZXNSO4KNO3QBHY5YBPO6NZTH6/graph.json","events_json":"https://pith.science/api/pith-number/WZXNSO4KNO3QBHY5YBPO6NZTH6/events.json","paper":"https://pith.science/paper/WZXNSO4K"},"agent_actions":{"view_html":"https://pith.science/pith/WZXNSO4KNO3QBHY5YBPO6NZTH6","download_json":"https://pith.science/pith/WZXNSO4KNO3QBHY5YBPO6NZTH6.json","view_paper":"https://pith.science/paper/WZXNSO4K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.4938&json=true","fetch_graph":"https://pith.science/api/pith-number/WZXNSO4KNO3QBHY5YBPO6NZTH6/graph.json","fetch_events":"https://pith.science/api/pith-number/WZXNSO4KNO3QBHY5YBPO6NZTH6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WZXNSO4KNO3QBHY5YBPO6NZTH6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WZXNSO4KNO3QBHY5YBPO6NZTH6/action/storage_attestation","attest_author":"https://pith.science/pith/WZXNSO4KNO3QBHY5YBPO6NZTH6/action/author_attestation","sign_citation":"https://pith.science/pith/WZXNSO4KNO3QBHY5YBPO6NZTH6/action/citation_signature","submit_replication":"https://pith.science/pith/WZXNSO4KNO3QBHY5YBPO6NZTH6/action/replication_record"}},"created_at":"2026-05-18T03:25:13.882350+00:00","updated_at":"2026-05-18T03:25:13.882350+00:00"}