{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:KUPVHITHMQYHRJVOZAUODNZSTE","short_pith_number":"pith:KUPVHITH","schema_version":"1.0","canonical_sha256":"551f53a267643078a6aec828e1b732990be0d6529ffede163535565c163e9f45","source":{"kind":"arxiv","id":"1104.1444","version":2},"attestation_state":"computed","paper":{"title":"SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Conley, A. M. Mourao, C. Balland, C. J. Pritchet, C. Lidmam, D. A. Howell, D. Balam, D. Fouchez, D. Hardin, E. Hsiao, E. S. Walker, H. K. Fakhouri, I. M. Hook, J. D. Neill, J. Guy, J. Rich, K. M. Perrett, M. J. Hudson, M. L. Graham, M. Sullivan, N. Fourmanoit, N. Palanque-Delabrouille, N. Regnault, N. Suzuki, P. Astier, P. Ripoche, R. G. Carlberg, R. Pain, R. S. Ellis, S. Basa, S. Baumont, S. Fabbro, S. Gonzalez-Gaitan, S. Perlmutter, T. Kronborg, V. Ruhlmann-Kleider","submitted_at":"2011-04-07T20:53:03Z","abstract_excerpt":"We present observational constraints on the nature of dark energy using the Supernova Legacy Survey three year sample (SNLS3) of Guy et al. (2010) and Conley et al. (2011). We use the 472 SNe Ia in this sample, accounting for recently discovered correlations between SN Ia luminosity and host galaxy properties, and include the effects of all identified systematic uncertainties directly in the cosmological fits. Combining the SNLS3 data with the full WMAP7 power spectrum, the Sloan Digital Sky Survey luminous red galaxy power spectrum, and a prior on the Hubble constant H0 from SHOES, in a flat "},"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":"1104.1444","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-04-07T20:53:03Z","cross_cats_sorted":[],"title_canon_sha256":"236c8a8f8d533a98badb4a97a0ee5936482cb4b1e16ca6c6d0057acfe0b4b816","abstract_canon_sha256":"02a60b2ed693a715ae10da0a1862114d974c68714384d51ba8221f2d25ef8991"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:15:49.843472Z","signature_b64":"DGVlLft7tACW2x8J55BO+4HEEj8J+xNdSKej1GV/kgQ21s/xorBD9BwnQI5j9jb77eEEMpitXs6Kdcw62pvEBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"551f53a267643078a6aec828e1b732990be0d6529ffede163535565c163e9f45","last_reissued_at":"2026-05-18T04:15:49.842919Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:15:49.842919Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Conley, A. M. Mourao, C. Balland, C. J. Pritchet, C. Lidmam, D. A. Howell, D. Balam, D. Fouchez, D. Hardin, E. Hsiao, E. S. Walker, H. K. Fakhouri, I. M. Hook, J. D. Neill, J. Guy, J. Rich, K. M. Perrett, M. J. Hudson, M. L. Graham, M. Sullivan, N. Fourmanoit, N. Palanque-Delabrouille, N. Regnault, N. Suzuki, P. Astier, P. Ripoche, R. G. Carlberg, R. Pain, R. S. Ellis, S. Basa, S. Baumont, S. Fabbro, S. Gonzalez-Gaitan, S. Perlmutter, T. Kronborg, V. Ruhlmann-Kleider","submitted_at":"2011-04-07T20:53:03Z","abstract_excerpt":"We present observational constraints on the nature of dark energy using the Supernova Legacy Survey three year sample (SNLS3) of Guy et al. (2010) and Conley et al. (2011). We use the 472 SNe Ia in this sample, accounting for recently discovered correlations between SN Ia luminosity and host galaxy properties, and include the effects of all identified systematic uncertainties directly in the cosmological fits. Combining the SNLS3 data with the full WMAP7 power spectrum, the Sloan Digital Sky Survey luminous red galaxy power spectrum, and a prior on the Hubble constant H0 from SHOES, in a flat "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1104.1444","kind":"arxiv","version":2},"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":"1104.1444","created_at":"2026-05-18T04:15:49.843010+00:00"},{"alias_kind":"arxiv_version","alias_value":"1104.1444v2","created_at":"2026-05-18T04:15:49.843010+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1104.1444","created_at":"2026-05-18T04:15:49.843010+00:00"},{"alias_kind":"pith_short_12","alias_value":"KUPVHITHMQYH","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_16","alias_value":"KUPVHITHMQYHRJVO","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_8","alias_value":"KUPVHITH","created_at":"2026-05-18T12:26:34.985390+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"1611.00036","citing_title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","ref_index":112,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE","json":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE.json","graph_json":"https://pith.science/api/pith-number/KUPVHITHMQYHRJVOZAUODNZSTE/graph.json","events_json":"https://pith.science/api/pith-number/KUPVHITHMQYHRJVOZAUODNZSTE/events.json","paper":"https://pith.science/paper/KUPVHITH"},"agent_actions":{"view_html":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE","download_json":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE.json","view_paper":"https://pith.science/paper/KUPVHITH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1104.1444&json=true","fetch_graph":"https://pith.science/api/pith-number/KUPVHITHMQYHRJVOZAUODNZSTE/graph.json","fetch_events":"https://pith.science/api/pith-number/KUPVHITHMQYHRJVOZAUODNZSTE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE/action/storage_attestation","attest_author":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE/action/author_attestation","sign_citation":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE/action/citation_signature","submit_replication":"https://pith.science/pith/KUPVHITHMQYHRJVOZAUODNZSTE/action/replication_record"}},"created_at":"2026-05-18T04:15:49.843010+00:00","updated_at":"2026-05-18T04:15:49.843010+00:00"}