{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:3FYJHGLPRKIUC3J6DMZJKZTEQU","short_pith_number":"pith:3FYJHGLP","schema_version":"1.0","canonical_sha256":"d97093996f8a91416d3e1b3295666485028bea5c8c8bebc4204c574f625a335b","source":{"kind":"arxiv","id":"1903.05108","version":2},"attestation_state":"computed","paper":{"title":"A Compact Jet at the Infrared Heart of the Prototypical Low-Luminosity AGN in NGC 1052","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. Asmus, E. Lopez-Rodriguez, J.A. Acosta-Pulido, J.A. Fern\\'andez-Ontiveros, K.R.W. Tristram, M.A. Prieto, N. L\\'opez-Gonzaga","submitted_at":"2019-03-12T18:00:12Z","abstract_excerpt":"The feeble radiative efficiency characteristic of Low-Luminosity Active Galactic Nuclei (LLAGN) is ascribed to a sub-Eddington accretion rate, typically at $\\log(L_{\\rm bol}/L_{\\rm edd}) \\lesssim -3$. At the finest angular resolutions that are attainable nowadays using mid-infrared (mid-IR) interferometry, the prototypical LLAGN in NGC 1052 remains unresolved down to $< 5\\, \\rm{mas}$ ($0.5\\, \\rm{pc}$). This is in line with non-thermal emission from a compact jet, a scenario further supported by a number of evidences: the broken power-law shape of the continuum distribution in the radio-to-UV r"},"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":"1903.05108","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-03-12T18:00:12Z","cross_cats_sorted":[],"title_canon_sha256":"6131669f23eaa17a3589fd0de6c64b8b43fe41f93a5debb47570c8288b9a4230","abstract_canon_sha256":"a95d8bfc8e2939c1406180383bafcde4a9f30e64ea421fe71b83cc568569509d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:50:18.928803Z","signature_b64":"Pkp37wotjpsfln5XecE/uQ5d73ceqG+l0Kw4ImGlc1/Bqi2vemCDzMWrz7c1o1fnSM0Lc2V20zJPG6qZqG02CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d97093996f8a91416d3e1b3295666485028bea5c8c8bebc4204c574f625a335b","last_reissued_at":"2026-05-17T23:50:18.928244Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:50:18.928244Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Compact Jet at the Infrared Heart of the Prototypical Low-Luminosity AGN in NGC 1052","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. Asmus, E. Lopez-Rodriguez, J.A. Acosta-Pulido, J.A. Fern\\'andez-Ontiveros, K.R.W. Tristram, M.A. Prieto, N. L\\'opez-Gonzaga","submitted_at":"2019-03-12T18:00:12Z","abstract_excerpt":"The feeble radiative efficiency characteristic of Low-Luminosity Active Galactic Nuclei (LLAGN) is ascribed to a sub-Eddington accretion rate, typically at $\\log(L_{\\rm bol}/L_{\\rm edd}) \\lesssim -3$. At the finest angular resolutions that are attainable nowadays using mid-infrared (mid-IR) interferometry, the prototypical LLAGN in NGC 1052 remains unresolved down to $< 5\\, \\rm{mas}$ ($0.5\\, \\rm{pc}$). This is in line with non-thermal emission from a compact jet, a scenario further supported by a number of evidences: the broken power-law shape of the continuum distribution in the radio-to-UV r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.05108","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":"1903.05108","created_at":"2026-05-17T23:50:18.928328+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.05108v2","created_at":"2026-05-17T23:50:18.928328+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.05108","created_at":"2026-05-17T23:50:18.928328+00:00"},{"alias_kind":"pith_short_12","alias_value":"3FYJHGLPRKIU","created_at":"2026-05-18T12:33:07.085635+00:00"},{"alias_kind":"pith_short_16","alias_value":"3FYJHGLPRKIUC3J6","created_at":"2026-05-18T12:33:07.085635+00:00"},{"alias_kind":"pith_short_8","alias_value":"3FYJHGLP","created_at":"2026-05-18T12:33:07.085635+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/3FYJHGLPRKIUC3J6DMZJKZTEQU","json":"https://pith.science/pith/3FYJHGLPRKIUC3J6DMZJKZTEQU.json","graph_json":"https://pith.science/api/pith-number/3FYJHGLPRKIUC3J6DMZJKZTEQU/graph.json","events_json":"https://pith.science/api/pith-number/3FYJHGLPRKIUC3J6DMZJKZTEQU/events.json","paper":"https://pith.science/paper/3FYJHGLP"},"agent_actions":{"view_html":"https://pith.science/pith/3FYJHGLPRKIUC3J6DMZJKZTEQU","download_json":"https://pith.science/pith/3FYJHGLPRKIUC3J6DMZJKZTEQU.json","view_paper":"https://pith.science/paper/3FYJHGLP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.05108&json=true","fetch_graph":"https://pith.science/api/pith-number/3FYJHGLPRKIUC3J6DMZJKZTEQU/graph.json","fetch_events":"https://pith.science/api/pith-number/3FYJHGLPRKIUC3J6DMZJKZTEQU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3FYJHGLPRKIUC3J6DMZJKZTEQU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3FYJHGLPRKIUC3J6DMZJKZTEQU/action/storage_attestation","attest_author":"https://pith.science/pith/3FYJHGLPRKIUC3J6DMZJKZTEQU/action/author_attestation","sign_citation":"https://pith.science/pith/3FYJHGLPRKIUC3J6DMZJKZTEQU/action/citation_signature","submit_replication":"https://pith.science/pith/3FYJHGLPRKIUC3J6DMZJKZTEQU/action/replication_record"}},"created_at":"2026-05-17T23:50:18.928328+00:00","updated_at":"2026-05-17T23:50:18.928328+00:00"}