{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:3O5BO7KLDAJAF6LJZNYXVKGHZQ","short_pith_number":"pith:3O5BO7KL","schema_version":"1.0","canonical_sha256":"dbba177d4b181202f969cb717aa8c7cc2af2a274d5752ed48465d4e9cf6a4b75","source":{"kind":"arxiv","id":"2303.01591","version":1},"attestation_state":"computed","paper":{"title":"High-accuracy emulators for observables in $\\Lambda$CDM, $N_\\mathrm{eff}$, $\\Sigma m_\\nu$, and $w$ cosmologies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alessio Spurio Mancini, Boris Bolliet, Erminia Calabrese, Hidde T. Jense, J. Colin Hill, Jo Dunkley, Mathew Madhavacheril","submitted_at":"2023-03-02T21:28:21Z","abstract_excerpt":"We use the emulation framework CosmoPower to construct and publicly release neural network emulators of cosmological observables, including the Cosmic Microwave Background (CMB) temperature and polarization power spectra, matter power spectrum, distance-redshift relation, baryon acoustic oscillation (BAO) and redshift-space distortion (RSD) observables, and derived parameters. We train our emulators on Einstein-Boltzmann calculations obtained with high-precision numerical convergence settings, for a wide range of cosmological models including $\\Lambda$CDM, $w$CDM, $\\Lambda$CDM+$N_\\mathrm{eff}$"},"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":"2303.01591","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-03-02T21:28:21Z","cross_cats_sorted":[],"title_canon_sha256":"5cb3ac4c6a01f59ff6c6475ae41b8eb6b96d005b398ac0dd599aaf990fda0a02","abstract_canon_sha256":"5ef971ae3c4bd51535992053c30d8f2bb7871540b45218ff9b393eb416461611"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:47:36.163539Z","signature_b64":"Rqt/VgHNIxI7IgfKB1xdpv7ODQHuM2g0oqaBPvR580VjENS+54QXcxahaJ9g1hjGC66WvoVQAWkERxph3zidDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dbba177d4b181202f969cb717aa8c7cc2af2a274d5752ed48465d4e9cf6a4b75","last_reissued_at":"2026-07-05T05:47:36.162990Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:47:36.162990Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-accuracy emulators for observables in $\\Lambda$CDM, $N_\\mathrm{eff}$, $\\Sigma m_\\nu$, and $w$ cosmologies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alessio Spurio Mancini, Boris Bolliet, Erminia Calabrese, Hidde T. Jense, J. Colin Hill, Jo Dunkley, Mathew Madhavacheril","submitted_at":"2023-03-02T21:28:21Z","abstract_excerpt":"We use the emulation framework CosmoPower to construct and publicly release neural network emulators of cosmological observables, including the Cosmic Microwave Background (CMB) temperature and polarization power spectra, matter power spectrum, distance-redshift relation, baryon acoustic oscillation (BAO) and redshift-space distortion (RSD) observables, and derived parameters. We train our emulators on Einstein-Boltzmann calculations obtained with high-precision numerical convergence settings, for a wide range of cosmological models including $\\Lambda$CDM, $w$CDM, $\\Lambda$CDM+$N_\\mathrm{eff}$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.01591","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/2303.01591/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":"2303.01591","created_at":"2026-07-05T05:47:36.163044+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.01591v1","created_at":"2026-07-05T05:47:36.163044+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.01591","created_at":"2026-07-05T05:47:36.163044+00:00"},{"alias_kind":"pith_short_12","alias_value":"3O5BO7KLDAJA","created_at":"2026-07-05T05:47:36.163044+00:00"},{"alias_kind":"pith_short_16","alias_value":"3O5BO7KLDAJAF6LJ","created_at":"2026-07-05T05:47:36.163044+00:00"},{"alias_kind":"pith_short_8","alias_value":"3O5BO7KL","created_at":"2026-07-05T05:47:36.163044+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.06410","citing_title":"The Atacama Cosmology Telescope: Probing new signatures of ultralight axions with gravitational lensing","ref_index":90,"is_internal_anchor":false},{"citing_arxiv_id":"2506.20707","citing_title":"SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field","ref_index":102,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ","json":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ.json","graph_json":"https://pith.science/api/pith-number/3O5BO7KLDAJAF6LJZNYXVKGHZQ/graph.json","events_json":"https://pith.science/api/pith-number/3O5BO7KLDAJAF6LJZNYXVKGHZQ/events.json","paper":"https://pith.science/paper/3O5BO7KL"},"agent_actions":{"view_html":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ","download_json":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ.json","view_paper":"https://pith.science/paper/3O5BO7KL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.01591&json=true","fetch_graph":"https://pith.science/api/pith-number/3O5BO7KLDAJAF6LJZNYXVKGHZQ/graph.json","fetch_events":"https://pith.science/api/pith-number/3O5BO7KLDAJAF6LJZNYXVKGHZQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ/action/storage_attestation","attest_author":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ/action/author_attestation","sign_citation":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ/action/citation_signature","submit_replication":"https://pith.science/pith/3O5BO7KLDAJAF6LJZNYXVKGHZQ/action/replication_record"}},"created_at":"2026-07-05T05:47:36.163044+00:00","updated_at":"2026-07-05T05:47:36.163044+00:00"}