{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:5YUGDKTCHFP4EVFT3OH6CLL3FL","short_pith_number":"pith:5YUGDKTC","schema_version":"1.0","canonical_sha256":"ee2861aa62395fc254b3db8fe12d7b2afa97f3f4f3ee994a1a3df71db372a9f6","source":{"kind":"arxiv","id":"astro-ph/0602198","version":1},"attestation_state":"computed","paper":{"title":"The AGN Contribution to the Mid-IR Emission of Luminous Infrared Galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Dey, B. T. Jannuzi, B. T. Soifer, C. Papovich, D. Weedman, E. Le Floc'h, H. A. Smith, K. Brand, M. J. I. Brown, P. Eisenhardt, R. J. Cool, S. P. Willner, V. Desai, V. Gorjian","submitted_at":"2006-02-08T21:11:12Z","abstract_excerpt":"We determine the contribution of AGN to the mid-IR emission of luminous infrared galaxies (LIRGs) at z>0.6 by measuring the mid-IR dust continuum slope of 20,039 mid-IR sources. The 24 micron sources are selected from a Spitzer/MIPS survey of the NOAO Deep Wide-Field Survey Bo\\\"otes field and have corresponding 8 micron data from the IRAC Shallow Survey. There is a clear bimodal distribution in the 24 micron to 8 micron flux ratio. The X-ray detected sources fall within the peak corresponding to a flat spectrum in nufnu, implying that it is populated by AGN-dominated LIRGs, whereas the peak co"},"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":"astro-ph/0602198","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-02-08T21:11:12Z","cross_cats_sorted":[],"title_canon_sha256":"cbf7b13643057d232e27a8bb82821537a03676dcfdbe2eb383e39d7c3db3780c","abstract_canon_sha256":"4c83771d504847f407f1e4b70cc1eebbbe33cede31a77cfb9d45daf52fee860f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:57:56.942194Z","signature_b64":"nXhhEZdSVIZI1O9tVo+2rVS/EY0qIy16j2YKTpOYGWcVYlMLdOB2N89YCso3qphb5PzEnqiDyu3djCiEbAeNBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ee2861aa62395fc254b3db8fe12d7b2afa97f3f4f3ee994a1a3df71db372a9f6","last_reissued_at":"2026-07-04T16:57:56.941658Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:57:56.941658Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The AGN Contribution to the Mid-IR Emission of Luminous Infrared Galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Dey, B. T. Jannuzi, B. T. Soifer, C. Papovich, D. Weedman, E. Le Floc'h, H. A. Smith, K. Brand, M. J. I. Brown, P. Eisenhardt, R. J. Cool, S. P. Willner, V. Desai, V. Gorjian","submitted_at":"2006-02-08T21:11:12Z","abstract_excerpt":"We determine the contribution of AGN to the mid-IR emission of luminous infrared galaxies (LIRGs) at z>0.6 by measuring the mid-IR dust continuum slope of 20,039 mid-IR sources. The 24 micron sources are selected from a Spitzer/MIPS survey of the NOAO Deep Wide-Field Survey Bo\\\"otes field and have corresponding 8 micron data from the IRAC Shallow Survey. There is a clear bimodal distribution in the 24 micron to 8 micron flux ratio. The X-ray detected sources fall within the peak corresponding to a flat spectrum in nufnu, implying that it is populated by AGN-dominated LIRGs, whereas the peak co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0602198","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/astro-ph/0602198/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":"astro-ph/0602198","created_at":"2026-07-04T16:57:56.941716+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0602198v1","created_at":"2026-07-04T16:57:56.941716+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0602198","created_at":"2026-07-04T16:57:56.941716+00:00"},{"alias_kind":"pith_short_12","alias_value":"5YUGDKTCHFP4","created_at":"2026-07-04T16:57:56.941716+00:00"},{"alias_kind":"pith_short_16","alias_value":"5YUGDKTCHFP4EVFT","created_at":"2026-07-04T16:57:56.941716+00:00"},{"alias_kind":"pith_short_8","alias_value":"5YUGDKTC","created_at":"2026-07-04T16:57:56.941716+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/5YUGDKTCHFP4EVFT3OH6CLL3FL","json":"https://pith.science/pith/5YUGDKTCHFP4EVFT3OH6CLL3FL.json","graph_json":"https://pith.science/api/pith-number/5YUGDKTCHFP4EVFT3OH6CLL3FL/graph.json","events_json":"https://pith.science/api/pith-number/5YUGDKTCHFP4EVFT3OH6CLL3FL/events.json","paper":"https://pith.science/paper/5YUGDKTC"},"agent_actions":{"view_html":"https://pith.science/pith/5YUGDKTCHFP4EVFT3OH6CLL3FL","download_json":"https://pith.science/pith/5YUGDKTCHFP4EVFT3OH6CLL3FL.json","view_paper":"https://pith.science/paper/5YUGDKTC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0602198&json=true","fetch_graph":"https://pith.science/api/pith-number/5YUGDKTCHFP4EVFT3OH6CLL3FL/graph.json","fetch_events":"https://pith.science/api/pith-number/5YUGDKTCHFP4EVFT3OH6CLL3FL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5YUGDKTCHFP4EVFT3OH6CLL3FL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5YUGDKTCHFP4EVFT3OH6CLL3FL/action/storage_attestation","attest_author":"https://pith.science/pith/5YUGDKTCHFP4EVFT3OH6CLL3FL/action/author_attestation","sign_citation":"https://pith.science/pith/5YUGDKTCHFP4EVFT3OH6CLL3FL/action/citation_signature","submit_replication":"https://pith.science/pith/5YUGDKTCHFP4EVFT3OH6CLL3FL/action/replication_record"}},"created_at":"2026-07-04T16:57:56.941716+00:00","updated_at":"2026-07-04T16:57:56.941716+00:00"}