{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:RBACARQF533YCBOOESHYRHS35R","short_pith_number":"pith:RBACARQF","schema_version":"1.0","canonical_sha256":"8840204605eef78105ce248f889e5bec5532d0ccddc765b265cf5b54211fe5e0","source":{"kind":"arxiv","id":"2402.17581","version":2},"attestation_state":"computed","paper":{"title":"CosmoMIA: Cosmic Web-based redshift space halo distribution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Daniel Forero-S\\'anchez, Francesco Sinigaglia, Francisco-Shu Kitaura, Jean-Paul Kneib, Jose Mar\\'ia Coloma-Nadal","submitted_at":"2024-02-27T15:13:34Z","abstract_excerpt":"Modern galaxy surveys demand extensive survey volumes and resolutions surpassing current dark matter-only simulations' capabilities. To address this, many methods employ effective bias models on the dark matter field to approximate object counts on a grid. However, realistic catalogs necessitate specific coordinates and velocities for a comprehensive understanding of the Universe. In this research, we explore sub-grid modeling to create accurate catalogs, beginning with coarse grid number counts at resolutions of approximately $5.5\\,h^{-1}\\rm Mpc$ per side. These resolutions strike a balance b"},"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":"2402.17581","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-02-27T15:13:34Z","cross_cats_sorted":[],"title_canon_sha256":"48b9efc27c73f7ebff17bba119ace71250833e188f82ff984c1c88fdbca48080","abstract_canon_sha256":"95de3fea01aecf26e77fcefcb35661a30262aa026f7a2c7ebd98ee3fa751427c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:16:08.671681Z","signature_b64":"950Y+ft1WUYmOxwpnmG8ncmxGYxynEuKxxRTc9t5gHrp6FzubRQDBePHg2BbvxsbcNAstey2dKOvoHM0UeukAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8840204605eef78105ce248f889e5bec5532d0ccddc765b265cf5b54211fe5e0","last_reissued_at":"2026-07-05T08:16:08.671177Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:16:08.671177Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CosmoMIA: Cosmic Web-based redshift space halo distribution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Daniel Forero-S\\'anchez, Francesco Sinigaglia, Francisco-Shu Kitaura, Jean-Paul Kneib, Jose Mar\\'ia Coloma-Nadal","submitted_at":"2024-02-27T15:13:34Z","abstract_excerpt":"Modern galaxy surveys demand extensive survey volumes and resolutions surpassing current dark matter-only simulations' capabilities. To address this, many methods employ effective bias models on the dark matter field to approximate object counts on a grid. However, realistic catalogs necessitate specific coordinates and velocities for a comprehensive understanding of the Universe. In this research, we explore sub-grid modeling to create accurate catalogs, beginning with coarse grid number counts at resolutions of approximately $5.5\\,h^{-1}\\rm Mpc$ per side. These resolutions strike a balance b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.17581","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2402.17581/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":"2402.17581","created_at":"2026-07-05T08:16:08.671241+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.17581v2","created_at":"2026-07-05T08:16:08.671241+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.17581","created_at":"2026-07-05T08:16:08.671241+00:00"},{"alias_kind":"pith_short_12","alias_value":"RBACARQF533Y","created_at":"2026-07-05T08:16:08.671241+00:00"},{"alias_kind":"pith_short_16","alias_value":"RBACARQF533YCBOO","created_at":"2026-07-05T08:16:08.671241+00:00"},{"alias_kind":"pith_short_8","alias_value":"RBACARQF","created_at":"2026-07-05T08:16:08.671241+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2509.15890","citing_title":"Fast and accurate Gaia-unWISE quasar mock catalogs from LPT and Eulerian bias","ref_index":66,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R","json":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R.json","graph_json":"https://pith.science/api/pith-number/RBACARQF533YCBOOESHYRHS35R/graph.json","events_json":"https://pith.science/api/pith-number/RBACARQF533YCBOOESHYRHS35R/events.json","paper":"https://pith.science/paper/RBACARQF"},"agent_actions":{"view_html":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R","download_json":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R.json","view_paper":"https://pith.science/paper/RBACARQF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.17581&json=true","fetch_graph":"https://pith.science/api/pith-number/RBACARQF533YCBOOESHYRHS35R/graph.json","fetch_events":"https://pith.science/api/pith-number/RBACARQF533YCBOOESHYRHS35R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R/action/storage_attestation","attest_author":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R/action/author_attestation","sign_citation":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R/action/citation_signature","submit_replication":"https://pith.science/pith/RBACARQF533YCBOOESHYRHS35R/action/replication_record"}},"created_at":"2026-07-05T08:16:08.671241+00:00","updated_at":"2026-07-05T08:16:08.671241+00:00"}