{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:ZRLZWUZWXRALR5XNGUVRZUY4DA","short_pith_number":"pith:ZRLZWUZW","schema_version":"1.0","canonical_sha256":"cc579b5336bc40b8f6ed352b1cd31c18010f308b05422d7741f08c435428314a","source":{"kind":"arxiv","id":"1307.2906","version":2},"attestation_state":"computed","paper":{"title":"Redshift Space Distortion Reconstruction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alberto Vallinotto, Eric V. Linder","submitted_at":"2013-07-10T20:01:14Z","abstract_excerpt":"Redshift space distortions of the matter density power spectrum carry information on the growth rate of cosmic structure but require accurate modeling of nonlinear and velocity effects on the density field. We test and advance the reconstruction function of Kwan, Lewis, Linder (2012) in several ways. First, we compare to the distribution function perturbative approach of Seljak & McDonald (2012), deriving the mapping between them and showing how the KLL form can extend the validity of the latter. Second, using cosmological simulations rather than perturbation theory we calibrate the free funct"},"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":"1307.2906","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-07-10T20:01:14Z","cross_cats_sorted":[],"title_canon_sha256":"582e8db91b14a21fc0f090c6f62f056002e30a824e1578182582c000c53570c8","abstract_canon_sha256":"5879fddfa58222c2ce7e92917838b48ac4816d2db9261cbb67bcf03f03f4464a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:18:07.714135Z","signature_b64":"g919dKnhAvJbG51I8B4yvAC5U2ivz/CZmcCpj38vRCXhNk0/fQwbtWwYTkmIDs3hdvXM1FcuJl5Z6ds01UwyBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc579b5336bc40b8f6ed352b1cd31c18010f308b05422d7741f08c435428314a","last_reissued_at":"2026-05-18T03:18:07.713583Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:18:07.713583Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Redshift Space Distortion Reconstruction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alberto Vallinotto, Eric V. Linder","submitted_at":"2013-07-10T20:01:14Z","abstract_excerpt":"Redshift space distortions of the matter density power spectrum carry information on the growth rate of cosmic structure but require accurate modeling of nonlinear and velocity effects on the density field. We test and advance the reconstruction function of Kwan, Lewis, Linder (2012) in several ways. First, we compare to the distribution function perturbative approach of Seljak & McDonald (2012), deriving the mapping between them and showing how the KLL form can extend the validity of the latter. Second, using cosmological simulations rather than perturbation theory we calibrate the free funct"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.2906","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":"1307.2906","created_at":"2026-05-18T03:18:07.713669+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.2906v2","created_at":"2026-05-18T03:18:07.713669+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.2906","created_at":"2026-05-18T03:18:07.713669+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZRLZWUZWXRAL","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZRLZWUZWXRALR5XN","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZRLZWUZW","created_at":"2026-05-18T12:28:09.283467+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA","json":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA.json","graph_json":"https://pith.science/api/pith-number/ZRLZWUZWXRALR5XNGUVRZUY4DA/graph.json","events_json":"https://pith.science/api/pith-number/ZRLZWUZWXRALR5XNGUVRZUY4DA/events.json","paper":"https://pith.science/paper/ZRLZWUZW"},"agent_actions":{"view_html":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA","download_json":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA.json","view_paper":"https://pith.science/paper/ZRLZWUZW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.2906&json=true","fetch_graph":"https://pith.science/api/pith-number/ZRLZWUZWXRALR5XNGUVRZUY4DA/graph.json","fetch_events":"https://pith.science/api/pith-number/ZRLZWUZWXRALR5XNGUVRZUY4DA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA/action/storage_attestation","attest_author":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA/action/author_attestation","sign_citation":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA/action/citation_signature","submit_replication":"https://pith.science/pith/ZRLZWUZWXRALR5XNGUVRZUY4DA/action/replication_record"}},"created_at":"2026-05-18T03:18:07.713669+00:00","updated_at":"2026-05-18T03:18:07.713669+00:00"}