{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:IV5BHT32TJGEC2EKOOUKH56URQ","short_pith_number":"pith:IV5BHT32","schema_version":"1.0","canonical_sha256":"457a13cf7a9a4c41688a73a8a3f7d48c0c1f0ebd475d5dc7b13991b941f0846d","source":{"kind":"arxiv","id":"1901.02280","version":1},"attestation_state":"computed","paper":{"title":"AGN torus detectability at sub-millimeter wavelengths: What to expect from ALMA continuum data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alice Pasetto, Cesar Victoria-Ceballos, Donaji Esparza-Arredondo, Mariela Mart\\'inez-Paredes, Natalia Osorio-Clavijo, Omaira Gonz\\'alez-Mart\\'in","submitted_at":"2019-01-08T12:27:47Z","abstract_excerpt":"We study the detectability of the emission associated with the AGN dusty structure at sub-mm wavelengths using ALMA, in a theoretical and observational way. Theoretically, we use the Clumpy models from Nenkova et al. together with the mid-infrared to X-ray and the radio fundamental plane scaling relations. We find that it is more likely to detect bigger and denser dusty tori at the highest ALMA frequency (666 GHz/450 micron). We also find that with 1h at 353 GHz/850 micron and 10h at 666 GHz/450 micron we can detect, with a high detection limit, a 1 mJy torus (characteristic of bright AGN). Th"},"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":"1901.02280","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-01-08T12:27:47Z","cross_cats_sorted":[],"title_canon_sha256":"acf75d850f2475d9e416026271bbe587daec8fe48e711cdccacef26cf63dfc33","abstract_canon_sha256":"80b3dc6440ec5f844ffbbcaa9a26cd05a66d167e11e873d8b6e4155ad4aa652a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:53:23.033435Z","signature_b64":"VFQzviSEUahDSckIgxZuvZkAu38OuWVWx9QxYAGG6z6pRDy2H9Zylvt+rDnXE0yWYRXb0uRn2/EfEYRimb7QDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"457a13cf7a9a4c41688a73a8a3f7d48c0c1f0ebd475d5dc7b13991b941f0846d","last_reissued_at":"2026-05-17T23:53:23.032757Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:53:23.032757Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"AGN torus detectability at sub-millimeter wavelengths: What to expect from ALMA continuum data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alice Pasetto, Cesar Victoria-Ceballos, Donaji Esparza-Arredondo, Mariela Mart\\'inez-Paredes, Natalia Osorio-Clavijo, Omaira Gonz\\'alez-Mart\\'in","submitted_at":"2019-01-08T12:27:47Z","abstract_excerpt":"We study the detectability of the emission associated with the AGN dusty structure at sub-mm wavelengths using ALMA, in a theoretical and observational way. Theoretically, we use the Clumpy models from Nenkova et al. together with the mid-infrared to X-ray and the radio fundamental plane scaling relations. We find that it is more likely to detect bigger and denser dusty tori at the highest ALMA frequency (666 GHz/450 micron). We also find that with 1h at 353 GHz/850 micron and 10h at 666 GHz/450 micron we can detect, with a high detection limit, a 1 mJy torus (characteristic of bright AGN). Th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.02280","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":"1901.02280","created_at":"2026-05-17T23:53:23.032855+00:00"},{"alias_kind":"arxiv_version","alias_value":"1901.02280v1","created_at":"2026-05-17T23:53:23.032855+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1901.02280","created_at":"2026-05-17T23:53:23.032855+00:00"},{"alias_kind":"pith_short_12","alias_value":"IV5BHT32TJGE","created_at":"2026-05-18T12:33:18.533446+00:00"},{"alias_kind":"pith_short_16","alias_value":"IV5BHT32TJGEC2EK","created_at":"2026-05-18T12:33:18.533446+00:00"},{"alias_kind":"pith_short_8","alias_value":"IV5BHT32","created_at":"2026-05-18T12:33:18.533446+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/IV5BHT32TJGEC2EKOOUKH56URQ","json":"https://pith.science/pith/IV5BHT32TJGEC2EKOOUKH56URQ.json","graph_json":"https://pith.science/api/pith-number/IV5BHT32TJGEC2EKOOUKH56URQ/graph.json","events_json":"https://pith.science/api/pith-number/IV5BHT32TJGEC2EKOOUKH56URQ/events.json","paper":"https://pith.science/paper/IV5BHT32"},"agent_actions":{"view_html":"https://pith.science/pith/IV5BHT32TJGEC2EKOOUKH56URQ","download_json":"https://pith.science/pith/IV5BHT32TJGEC2EKOOUKH56URQ.json","view_paper":"https://pith.science/paper/IV5BHT32","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1901.02280&json=true","fetch_graph":"https://pith.science/api/pith-number/IV5BHT32TJGEC2EKOOUKH56URQ/graph.json","fetch_events":"https://pith.science/api/pith-number/IV5BHT32TJGEC2EKOOUKH56URQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IV5BHT32TJGEC2EKOOUKH56URQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IV5BHT32TJGEC2EKOOUKH56URQ/action/storage_attestation","attest_author":"https://pith.science/pith/IV5BHT32TJGEC2EKOOUKH56URQ/action/author_attestation","sign_citation":"https://pith.science/pith/IV5BHT32TJGEC2EKOOUKH56URQ/action/citation_signature","submit_replication":"https://pith.science/pith/IV5BHT32TJGEC2EKOOUKH56URQ/action/replication_record"}},"created_at":"2026-05-17T23:53:23.032855+00:00","updated_at":"2026-05-17T23:53:23.032855+00:00"}