{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:2WWFPLF3NS2DZFX4B2ZLZMM3AH","short_pith_number":"pith:2WWFPLF3","schema_version":"1.0","canonical_sha256":"d5ac57acbb6cb43c96fc0eb2bcb19b01cc1b572e8e80383e708b27b155358ff7","source":{"kind":"arxiv","id":"1506.05976","version":3},"attestation_state":"computed","paper":{"title":"Neutrino masses and cosmology with Lyman-alpha forest power spectrum","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Arnaud Borde, Christophe Magneville, Christophe Yeche, David Weinberg, Etienne Burtin, Graziano Rossi, James Rich, Jean-Marc LeGoff, Julien Baur, Julien Lesgourgues, Matteo Viel, Nathalie Palanque-Delabrouille","submitted_at":"2015-06-19T12:42:45Z","abstract_excerpt":"We present constraints on neutrino masses, the primordial fluctuation spectrum from inflation, and other parameters of the $\\Lambda$CDM model, using the one-dimensional Ly$\\alpha$-forest power spectrum measured by Palanque-Delabrouille et al. (2013) from SDSS-III/BOSS, complemented by Planck 2015 cosmic microwave background (CMB) data and other cosmological probes. This paper improves on the previous analysis by Palanque-Delabrouille et al. (2015) by using a more powerful set of calibrating hydrodynamical simulations that reduces uncertainties associated with resolution and box size, by adopti"},"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":"1506.05976","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-06-19T12:42:45Z","cross_cats_sorted":[],"title_canon_sha256":"710a80fd239e8ed42d39813a61801be561a6d3b4a78cb2da9f880a90003d913a","abstract_canon_sha256":"cc37198c7ed89a3734a2c1d5d779af871ce2755335121c6326f07eaf1f1227e2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:02:10.251694Z","signature_b64":"eVT1QCYIkLei51gaUr2g5vb3DngoDOHg2Li1+mPZJVQQEtsIHZH4GqlXVDxzIZ3Fg4iYkXWY3xBgsYPaxyJlBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d5ac57acbb6cb43c96fc0eb2bcb19b01cc1b572e8e80383e708b27b155358ff7","last_reissued_at":"2026-07-05T00:02:10.251188Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:02:10.251188Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino masses and cosmology with Lyman-alpha forest power spectrum","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Arnaud Borde, Christophe Magneville, Christophe Yeche, David Weinberg, Etienne Burtin, Graziano Rossi, James Rich, Jean-Marc LeGoff, Julien Baur, Julien Lesgourgues, Matteo Viel, Nathalie Palanque-Delabrouille","submitted_at":"2015-06-19T12:42:45Z","abstract_excerpt":"We present constraints on neutrino masses, the primordial fluctuation spectrum from inflation, and other parameters of the $\\Lambda$CDM model, using the one-dimensional Ly$\\alpha$-forest power spectrum measured by Palanque-Delabrouille et al. (2013) from SDSS-III/BOSS, complemented by Planck 2015 cosmic microwave background (CMB) data and other cosmological probes. This paper improves on the previous analysis by Palanque-Delabrouille et al. (2015) by using a more powerful set of calibrating hydrodynamical simulations that reduces uncertainties associated with resolution and box size, by adopti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.05976","kind":"arxiv","version":3},"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/1506.05976/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":"1506.05976","created_at":"2026-07-05T00:02:10.251248+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.05976v3","created_at":"2026-07-05T00:02:10.251248+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.05976","created_at":"2026-07-05T00:02:10.251248+00:00"},{"alias_kind":"pith_short_12","alias_value":"2WWFPLF3NS2D","created_at":"2026-07-05T00:02:10.251248+00:00"},{"alias_kind":"pith_short_16","alias_value":"2WWFPLF3NS2DZFX4","created_at":"2026-07-05T00:02:10.251248+00:00"},{"alias_kind":"pith_short_8","alias_value":"2WWFPLF3","created_at":"2026-07-05T00:02:10.251248+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2503.14744","citing_title":"Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape","ref_index":33,"is_internal_anchor":false},{"citing_arxiv_id":"1807.06209","citing_title":"Planck 2018 results. VI. Cosmological parameters","ref_index":252,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH","json":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH.json","graph_json":"https://pith.science/api/pith-number/2WWFPLF3NS2DZFX4B2ZLZMM3AH/graph.json","events_json":"https://pith.science/api/pith-number/2WWFPLF3NS2DZFX4B2ZLZMM3AH/events.json","paper":"https://pith.science/paper/2WWFPLF3"},"agent_actions":{"view_html":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH","download_json":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH.json","view_paper":"https://pith.science/paper/2WWFPLF3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.05976&json=true","fetch_graph":"https://pith.science/api/pith-number/2WWFPLF3NS2DZFX4B2ZLZMM3AH/graph.json","fetch_events":"https://pith.science/api/pith-number/2WWFPLF3NS2DZFX4B2ZLZMM3AH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH/action/storage_attestation","attest_author":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH/action/author_attestation","sign_citation":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH/action/citation_signature","submit_replication":"https://pith.science/pith/2WWFPLF3NS2DZFX4B2ZLZMM3AH/action/replication_record"}},"created_at":"2026-07-05T00:02:10.251248+00:00","updated_at":"2026-07-05T00:02:10.251248+00:00"}