{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:JK5MQNWUFOHO3PMFK3KS7N4OBO","short_pith_number":"pith:JK5MQNWU","schema_version":"1.0","canonical_sha256":"4abac836d42b8eedbd8556d52fb78e0b880cfe9043faa79d328e4042dcc7d8af","source":{"kind":"arxiv","id":"1303.3977","version":1},"attestation_state":"computed","paper":{"title":"Hubble Space Telescope ACS Imaging of the GOALS Sample: Quantitative Structural Properties of Nearby Luminous Infrared Galaxies with L_IR > 10^{11.4} L_sun","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Petric, A. S. Evans, D. B. Sanders, D.-C. Kim, G. C. Privon, J. A. Surace, J. H. Howell, J. M. Mazzarella, K. Iwasawa, K. Sheth, L. Armus, S. Haan, T. D\\'iaz-Santos, T. Vavilkin","submitted_at":"2013-03-16T13:29:18Z","abstract_excerpt":"A {\\it Hubble Space Telescope} ({\\it HST}) / Advanced Camera for Surveys (ACS) study of the structural properties of 85 luminous and ultraluminous ($L_{\\rm IR} > 10^{11.4}$ L$_\\odot$) infrared galaxies (LIRGs and ULIRGs) in the Great Observatories All-sky LIRG Survey (GOALS) sample is presented. Two-dimensional GALFIT analysis has been performed on F814W \"{\\it I}-band\" images to decompose each galaxy, as appropriate, into bulge, disk, central PSF and stellar bar components. The fraction of bulge-less disk systems is observed to be higher in LIRGs (35%) than in ULIRGs (20%), with the disk+bulge"},"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":"1303.3977","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-03-16T13:29:18Z","cross_cats_sorted":[],"title_canon_sha256":"ef0f644cf8b9ad7b39ccb88ed6737fe97772e3e2d96cc0e22633d40cd515d173","abstract_canon_sha256":"f6a0a4b4ba9c89e4e8339b279b7357929914da913ab7bb1c8b402b7eb2069571"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:01.566957Z","signature_b64":"6ha/b60MLkAiwIWTiYzElDer6busrMwKSI9czEw78eTJ+WlagZiUA6j39nEElwM5jh6tOROs5iVWnlaj6QDOBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4abac836d42b8eedbd8556d52fb78e0b880cfe9043faa79d328e4042dcc7d8af","last_reissued_at":"2026-05-18T01:51:01.566475Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:01.566475Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hubble Space Telescope ACS Imaging of the GOALS Sample: Quantitative Structural Properties of Nearby Luminous Infrared Galaxies with L_IR > 10^{11.4} L_sun","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Petric, A. S. Evans, D. B. Sanders, D.-C. Kim, G. C. Privon, J. A. Surace, J. H. Howell, J. M. Mazzarella, K. Iwasawa, K. Sheth, L. Armus, S. Haan, T. D\\'iaz-Santos, T. Vavilkin","submitted_at":"2013-03-16T13:29:18Z","abstract_excerpt":"A {\\it Hubble Space Telescope} ({\\it HST}) / Advanced Camera for Surveys (ACS) study of the structural properties of 85 luminous and ultraluminous ($L_{\\rm IR} > 10^{11.4}$ L$_\\odot$) infrared galaxies (LIRGs and ULIRGs) in the Great Observatories All-sky LIRG Survey (GOALS) sample is presented. Two-dimensional GALFIT analysis has been performed on F814W \"{\\it I}-band\" images to decompose each galaxy, as appropriate, into bulge, disk, central PSF and stellar bar components. The fraction of bulge-less disk systems is observed to be higher in LIRGs (35%) than in ULIRGs (20%), with the disk+bulge"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.3977","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":"1303.3977","created_at":"2026-05-18T01:51:01.566550+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.3977v1","created_at":"2026-05-18T01:51:01.566550+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.3977","created_at":"2026-05-18T01:51:01.566550+00:00"},{"alias_kind":"pith_short_12","alias_value":"JK5MQNWUFOHO","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_16","alias_value":"JK5MQNWUFOHO3PMF","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_8","alias_value":"JK5MQNWU","created_at":"2026-05-18T12:27:49.015174+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":57,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO","json":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO.json","graph_json":"https://pith.science/api/pith-number/JK5MQNWUFOHO3PMFK3KS7N4OBO/graph.json","events_json":"https://pith.science/api/pith-number/JK5MQNWUFOHO3PMFK3KS7N4OBO/events.json","paper":"https://pith.science/paper/JK5MQNWU"},"agent_actions":{"view_html":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO","download_json":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO.json","view_paper":"https://pith.science/paper/JK5MQNWU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.3977&json=true","fetch_graph":"https://pith.science/api/pith-number/JK5MQNWUFOHO3PMFK3KS7N4OBO/graph.json","fetch_events":"https://pith.science/api/pith-number/JK5MQNWUFOHO3PMFK3KS7N4OBO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO/action/storage_attestation","attest_author":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO/action/author_attestation","sign_citation":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO/action/citation_signature","submit_replication":"https://pith.science/pith/JK5MQNWUFOHO3PMFK3KS7N4OBO/action/replication_record"}},"created_at":"2026-05-18T01:51:01.566550+00:00","updated_at":"2026-05-18T01:51:01.566550+00:00"}