{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:M47Z7WXQ2RUVN2HVWOTQ5MCJE7","short_pith_number":"pith:M47Z7WXQ","schema_version":"1.0","canonical_sha256":"673f9fdaf0d46956e8f5b3a70eb04927cca6cebed11dd166cfda262622a1897f","source":{"kind":"arxiv","id":"1908.11381","version":1},"attestation_state":"computed","paper":{"title":"Exploring the mid-infrared SEDs of six AGN dusty torus models I: synthetic spectra","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Pasetto, C. Ramos Almeida, C. Victoria-Ceballos, D. Dultzin, D. Esparza-Arredondo, I. Garc\\'ia-Bernete, I. M\\'arquez, J. Masegosa, J.M. Rodr\\'iguez-Espinosa, M. Mart\\'inez-Paredes, N. Osorio-Clavijo, O. Gonz\\'alez-Mart\\'in","submitted_at":"2019-08-29T18:00:01Z","abstract_excerpt":"At distances from the active galaxy nucleus (AGN) where the ambient temperature falls below ~1500-1800 K, dust is able to survive. It is thus possible to have a large dusty structure present which surrounds the AGN. This is the first of two papers aiming at comparing six dusty torus models with available SEDs, namely Fritz et al. (2006), Nenkova et al. (2008B), Hoenig & Kishimoto (2010), Siebenmorgen et al. (2015), Stalevski et al. (2016), and Hoenig & Kishimoto (2017). In this first paper we use synthetic spectra to explore the discrimination between these models and under which circumstances"},"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":"1908.11381","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-08-29T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"d9110c2b03d2b61bc1ae0db539fe7e2d4167d7d5ce5303b7ecd51544eb2d6fda","abstract_canon_sha256":"c5e84a0b7c8869b48297243678bdb6a60262d58fb7c69699f5c327e01792a933"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:12:05.857063Z","signature_b64":"pUSTXZpiX7+z5YZ8ausCiHlYdDEAGrJUTgf5OAGvKZ1CemAQH6sBLPWMHUwYIh8EO3rzSqHb2+Vt4PWtioWQCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"673f9fdaf0d46956e8f5b3a70eb04927cca6cebed11dd166cfda262622a1897f","last_reissued_at":"2026-07-05T00:12:05.856636Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:12:05.856636Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring the mid-infrared SEDs of six AGN dusty torus models I: synthetic spectra","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Pasetto, C. Ramos Almeida, C. Victoria-Ceballos, D. Dultzin, D. Esparza-Arredondo, I. Garc\\'ia-Bernete, I. M\\'arquez, J. Masegosa, J.M. Rodr\\'iguez-Espinosa, M. Mart\\'inez-Paredes, N. Osorio-Clavijo, O. Gonz\\'alez-Mart\\'in","submitted_at":"2019-08-29T18:00:01Z","abstract_excerpt":"At distances from the active galaxy nucleus (AGN) where the ambient temperature falls below ~1500-1800 K, dust is able to survive. It is thus possible to have a large dusty structure present which surrounds the AGN. This is the first of two papers aiming at comparing six dusty torus models with available SEDs, namely Fritz et al. (2006), Nenkova et al. (2008B), Hoenig & Kishimoto (2010), Siebenmorgen et al. (2015), Stalevski et al. (2016), and Hoenig & Kishimoto (2017). In this first paper we use synthetic spectra to explore the discrimination between these models and under which circumstances"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1908.11381","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1908.11381/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"1908.11381","created_at":"2026-07-05T00:12:05.856695+00:00"},{"alias_kind":"arxiv_version","alias_value":"1908.11381v1","created_at":"2026-07-05T00:12:05.856695+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1908.11381","created_at":"2026-07-05T00:12:05.856695+00:00"},{"alias_kind":"pith_short_12","alias_value":"M47Z7WXQ2RUV","created_at":"2026-07-05T00:12:05.856695+00:00"},{"alias_kind":"pith_short_16","alias_value":"M47Z7WXQ2RUVN2HV","created_at":"2026-07-05T00:12:05.856695+00:00"},{"alias_kind":"pith_short_8","alias_value":"M47Z7WXQ","created_at":"2026-07-05T00:12:05.856695+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/M47Z7WXQ2RUVN2HVWOTQ5MCJE7","json":"https://pith.science/pith/M47Z7WXQ2RUVN2HVWOTQ5MCJE7.json","graph_json":"https://pith.science/api/pith-number/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/graph.json","events_json":"https://pith.science/api/pith-number/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/events.json","paper":"https://pith.science/paper/M47Z7WXQ"},"agent_actions":{"view_html":"https://pith.science/pith/M47Z7WXQ2RUVN2HVWOTQ5MCJE7","download_json":"https://pith.science/pith/M47Z7WXQ2RUVN2HVWOTQ5MCJE7.json","view_paper":"https://pith.science/paper/M47Z7WXQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1908.11381&json=true","fetch_graph":"https://pith.science/api/pith-number/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/graph.json","fetch_events":"https://pith.science/api/pith-number/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/action/storage_attestation","attest_author":"https://pith.science/pith/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/action/author_attestation","sign_citation":"https://pith.science/pith/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/action/citation_signature","submit_replication":"https://pith.science/pith/M47Z7WXQ2RUVN2HVWOTQ5MCJE7/action/replication_record"}},"created_at":"2026-07-05T00:12:05.856695+00:00","updated_at":"2026-07-05T00:12:05.856695+00:00"}