{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:ZEALSMW272FDLK2HC4DUGU76LM","short_pith_number":"pith:ZEALSMW2","schema_version":"1.0","canonical_sha256":"c900b932dafe8a35ab4717074353fe5b1777c225645a30c03d209a0c7a6a67c8","source":{"kind":"arxiv","id":"1012.1891","version":1},"attestation_state":"computed","paper":{"title":"Mid-Infrared Spectral Diagnostics of Luminous Infrared Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. O. Petric, A. S. Evans, B. Chan, B. Madore, D. Frayer, D. Kim, D. Sanders, E. Sturm, H. Inami, H. Spoon, J. A. Surace, J. Howell, J. Marshall, J. M. Mazzarella, K. Iwasawa, L. Armus, P. Appleton, S. Haan, S. Lord, S. Stierwalt, S. Veilleux, T. Diaz Santos, T. Vavilkin, V. Charmandaris, V. U","submitted_at":"2010-12-08T23:28:29Z","abstract_excerpt":"We present a statistical analysis of the mid-infrared (MIR) spectra of 248 luminous infrared (IR) galaxies (LIRGs) which comprise the Great Observatories All-sky LIRG Survey (GOALS) observed with the Infrared Spectrograph (IRS) on-board the Spitzer Space Telescope. The GOALS sample enables a direct measurement of the relative contributions of star-formation and active galactic nuclei (AGN) to the total IR emission from a large sample of local LIRGs. The AGN contribution to the MIR emission (f-AGN) is estimated by employing several diagnostics based on the properties of the [NeV], [OIV] and [Ne"},"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":"1012.1891","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-12-08T23:28:29Z","cross_cats_sorted":[],"title_canon_sha256":"4ad399a9b229ae958f417445e65b008efa83aafd5b7839145bf21030295a0279","abstract_canon_sha256":"57ee782e6179a00d6c6c51d6941acf1d05002da0a0d950102327da83d2cad0c3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:31.345416Z","signature_b64":"KdHr8UOTqa/lp+8x0Ir6cSwOwCsRJ6k8xhPikbuXLU+ZHcCAZ6yh2PXpq7O44oMDbkufngvJN3mi66pFuR3UDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c900b932dafe8a35ab4717074353fe5b1777c225645a30c03d209a0c7a6a67c8","last_reissued_at":"2026-05-18T02:04:31.344730Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:31.344730Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Mid-Infrared Spectral Diagnostics of Luminous Infrared Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. O. Petric, A. S. Evans, B. Chan, B. Madore, D. Frayer, D. Kim, D. Sanders, E. Sturm, H. Inami, H. Spoon, J. A. Surace, J. Howell, J. Marshall, J. M. Mazzarella, K. Iwasawa, L. Armus, P. Appleton, S. Haan, S. Lord, S. Stierwalt, S. Veilleux, T. Diaz Santos, T. Vavilkin, V. Charmandaris, V. U","submitted_at":"2010-12-08T23:28:29Z","abstract_excerpt":"We present a statistical analysis of the mid-infrared (MIR) spectra of 248 luminous infrared (IR) galaxies (LIRGs) which comprise the Great Observatories All-sky LIRG Survey (GOALS) observed with the Infrared Spectrograph (IRS) on-board the Spitzer Space Telescope. The GOALS sample enables a direct measurement of the relative contributions of star-formation and active galactic nuclei (AGN) to the total IR emission from a large sample of local LIRGs. The AGN contribution to the MIR emission (f-AGN) is estimated by employing several diagnostics based on the properties of the [NeV], [OIV] and [Ne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.1891","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":"1012.1891","created_at":"2026-05-18T02:04:31.344813+00:00"},{"alias_kind":"arxiv_version","alias_value":"1012.1891v1","created_at":"2026-05-18T02:04:31.344813+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.1891","created_at":"2026-05-18T02:04:31.344813+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZEALSMW272FD","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZEALSMW272FDLK2H","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZEALSMW2","created_at":"2026-05-18T12:26:17.028572+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.19658","citing_title":"The PARADIGM Project II: Characterising Nuclear and Diffuse Radio Components in Local U/LIRGs","ref_index":88,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM","json":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM.json","graph_json":"https://pith.science/api/pith-number/ZEALSMW272FDLK2HC4DUGU76LM/graph.json","events_json":"https://pith.science/api/pith-number/ZEALSMW272FDLK2HC4DUGU76LM/events.json","paper":"https://pith.science/paper/ZEALSMW2"},"agent_actions":{"view_html":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM","download_json":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM.json","view_paper":"https://pith.science/paper/ZEALSMW2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1012.1891&json=true","fetch_graph":"https://pith.science/api/pith-number/ZEALSMW272FDLK2HC4DUGU76LM/graph.json","fetch_events":"https://pith.science/api/pith-number/ZEALSMW272FDLK2HC4DUGU76LM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM/action/storage_attestation","attest_author":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM/action/author_attestation","sign_citation":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM/action/citation_signature","submit_replication":"https://pith.science/pith/ZEALSMW272FDLK2HC4DUGU76LM/action/replication_record"}},"created_at":"2026-05-18T02:04:31.344813+00:00","updated_at":"2026-05-18T02:04:31.344813+00:00"}