{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:SW6NRB2NZ4F4INIL6AI3I6WXKA","short_pith_number":"pith:SW6NRB2N","schema_version":"1.0","canonical_sha256":"95bcd8874dcf0bc4350bf011b47ad7503d68239e31676ee04c8133ca7b2bfdbd","source":{"kind":"arxiv","id":"0906.4885","version":2},"attestation_state":"computed","paper":{"title":"The 3-5 micron Spectrum of NGC 1068 at High Angular Resolution: Distribution of Emission and Absorption Features across the Nuclear Continuum Source","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Rodr\\'iguez-Ardila, D.J. Axon, R.E. Mason, T.R. Geballe","submitted_at":"2009-06-26T09:32:32Z","abstract_excerpt":"We report moderate resolution 3-5 micron spectroscopy of the nucleus of NGC 1068 obtained at 0.3 arcsec (20 pc) resolution with the spectrograph slit aligned approximately along the ionization cones of the AGN. The deconvolved FWHM of the nuclear continuum source in this direction is 0.3 arcsec. Four coronal lines of widely different excitations were detected; the intensity of each peaks near radio knot C, approximately 0.3 arcsec north of the infrared continuum peak, where the radio jet changes direction. Together with the broadened line profiles observed near that location, this suggests tha"},"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":"0906.4885","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-06-26T09:32:32Z","cross_cats_sorted":[],"title_canon_sha256":"8577b9ad96cc0e1a3aa9c3ff6703ca0ba9a9a6cae99cce8cfa371538e2838496","abstract_canon_sha256":"a9823c473ef7e97690fa94df27542ece1da4e1af3d7c030aa26637b72cd053e7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:29:42.584016Z","signature_b64":"puGQaj93+jeydQVf3YMMZ6RnLD7SUzdydH5bEtfVAK4IaCHkG4M4SxDdZNpPKXDFEYftw1k25OEbZf2mMuavBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"95bcd8874dcf0bc4350bf011b47ad7503d68239e31676ee04c8133ca7b2bfdbd","last_reissued_at":"2026-05-18T04:29:42.583576Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:29:42.583576Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The 3-5 micron Spectrum of NGC 1068 at High Angular Resolution: Distribution of Emission and Absorption Features across the Nuclear Continuum Source","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Rodr\\'iguez-Ardila, D.J. Axon, R.E. Mason, T.R. Geballe","submitted_at":"2009-06-26T09:32:32Z","abstract_excerpt":"We report moderate resolution 3-5 micron spectroscopy of the nucleus of NGC 1068 obtained at 0.3 arcsec (20 pc) resolution with the spectrograph slit aligned approximately along the ionization cones of the AGN. The deconvolved FWHM of the nuclear continuum source in this direction is 0.3 arcsec. Four coronal lines of widely different excitations were detected; the intensity of each peaks near radio knot C, approximately 0.3 arcsec north of the infrared continuum peak, where the radio jet changes direction. Together with the broadened line profiles observed near that location, this suggests tha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0906.4885","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":""},"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":"0906.4885","created_at":"2026-05-18T04:29:42.583642+00:00"},{"alias_kind":"arxiv_version","alias_value":"0906.4885v2","created_at":"2026-05-18T04:29:42.583642+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0906.4885","created_at":"2026-05-18T04:29:42.583642+00:00"},{"alias_kind":"pith_short_12","alias_value":"SW6NRB2NZ4F4","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"SW6NRB2NZ4F4INIL","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"SW6NRB2N","created_at":"2026-05-18T12:26:01.383474+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/SW6NRB2NZ4F4INIL6AI3I6WXKA","json":"https://pith.science/pith/SW6NRB2NZ4F4INIL6AI3I6WXKA.json","graph_json":"https://pith.science/api/pith-number/SW6NRB2NZ4F4INIL6AI3I6WXKA/graph.json","events_json":"https://pith.science/api/pith-number/SW6NRB2NZ4F4INIL6AI3I6WXKA/events.json","paper":"https://pith.science/paper/SW6NRB2N"},"agent_actions":{"view_html":"https://pith.science/pith/SW6NRB2NZ4F4INIL6AI3I6WXKA","download_json":"https://pith.science/pith/SW6NRB2NZ4F4INIL6AI3I6WXKA.json","view_paper":"https://pith.science/paper/SW6NRB2N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0906.4885&json=true","fetch_graph":"https://pith.science/api/pith-number/SW6NRB2NZ4F4INIL6AI3I6WXKA/graph.json","fetch_events":"https://pith.science/api/pith-number/SW6NRB2NZ4F4INIL6AI3I6WXKA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SW6NRB2NZ4F4INIL6AI3I6WXKA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SW6NRB2NZ4F4INIL6AI3I6WXKA/action/storage_attestation","attest_author":"https://pith.science/pith/SW6NRB2NZ4F4INIL6AI3I6WXKA/action/author_attestation","sign_citation":"https://pith.science/pith/SW6NRB2NZ4F4INIL6AI3I6WXKA/action/citation_signature","submit_replication":"https://pith.science/pith/SW6NRB2NZ4F4INIL6AI3I6WXKA/action/replication_record"}},"created_at":"2026-05-18T04:29:42.583642+00:00","updated_at":"2026-05-18T04:29:42.583642+00:00"}