{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:QQQF3RYBM24AZXEUGM5UO25MEX","short_pith_number":"pith:QQQF3RYB","schema_version":"1.0","canonical_sha256":"84205dc70166b80cdc94333b476bac25c0221001d5fedf8fe97501259ac976e9","source":{"kind":"arxiv","id":"2310.19928","version":2},"attestation_state":"computed","paper":{"title":"Characterising HOD in filaments and nodes of the cosmic web","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andr\\'es N. Ruiz, Facundo Rodriguez, Georgina Coldwell, Ignacio G. Alfaro, Luis A. Pereyra, Noelia R. Perez","submitted_at":"2023-10-30T18:44:38Z","abstract_excerpt":"The standard paradigm for the formation of the Universe suggests that large structures are formed from hierarchical clustering by the continuous accretion of less massive galaxy systems through filaments. In this context, filamentary structures play an important role in the properties and evolution of galaxies by connecting high-density regions, such as nodes, and being surrounded by low-density regions, such as cosmic voids. The availability of the filament and point critic catalogues extracted by \\textsc{DisPerSE} from the \\textsc{Illustris} TNG300-1 hydrodynamic simulation allows a detailed"},"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":"2310.19928","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-10-30T18:44:38Z","cross_cats_sorted":[],"title_canon_sha256":"95aaab8057c5a3d06a7c2a4513fda15ef1d41684d93e980aba40293bf182ae9b","abstract_canon_sha256":"634d3f89942db86d002b51c362c8732cd07041797a78933e2a378fc0a6f93953"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:28:11.890236Z","signature_b64":"Ds3XD5UmcfnvkbDmm2xGtwdABdGPWxl//98iRv4Ywbl1nuaMMIHXpYRZNUlBUvgUkllVNQR8HUeJ/N0kXtUoAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"84205dc70166b80cdc94333b476bac25c0221001d5fedf8fe97501259ac976e9","last_reissued_at":"2026-07-05T07:28:11.889793Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:28:11.889793Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Characterising HOD in filaments and nodes of the cosmic web","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andr\\'es N. Ruiz, Facundo Rodriguez, Georgina Coldwell, Ignacio G. Alfaro, Luis A. Pereyra, Noelia R. Perez","submitted_at":"2023-10-30T18:44:38Z","abstract_excerpt":"The standard paradigm for the formation of the Universe suggests that large structures are formed from hierarchical clustering by the continuous accretion of less massive galaxy systems through filaments. In this context, filamentary structures play an important role in the properties and evolution of galaxies by connecting high-density regions, such as nodes, and being surrounded by low-density regions, such as cosmic voids. The availability of the filament and point critic catalogues extracted by \\textsc{DisPerSE} from the \\textsc{Illustris} TNG300-1 hydrodynamic simulation allows a detailed"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.19928","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/2310.19928/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":"2310.19928","created_at":"2026-07-05T07:28:11.889846+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.19928v2","created_at":"2026-07-05T07:28:11.889846+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.19928","created_at":"2026-07-05T07:28:11.889846+00:00"},{"alias_kind":"pith_short_12","alias_value":"QQQF3RYBM24A","created_at":"2026-07-05T07:28:11.889846+00:00"},{"alias_kind":"pith_short_16","alias_value":"QQQF3RYBM24AZXEU","created_at":"2026-07-05T07:28:11.889846+00:00"},{"alias_kind":"pith_short_8","alias_value":"QQQF3RYB","created_at":"2026-07-05T07:28:11.889846+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/QQQF3RYBM24AZXEUGM5UO25MEX","json":"https://pith.science/pith/QQQF3RYBM24AZXEUGM5UO25MEX.json","graph_json":"https://pith.science/api/pith-number/QQQF3RYBM24AZXEUGM5UO25MEX/graph.json","events_json":"https://pith.science/api/pith-number/QQQF3RYBM24AZXEUGM5UO25MEX/events.json","paper":"https://pith.science/paper/QQQF3RYB"},"agent_actions":{"view_html":"https://pith.science/pith/QQQF3RYBM24AZXEUGM5UO25MEX","download_json":"https://pith.science/pith/QQQF3RYBM24AZXEUGM5UO25MEX.json","view_paper":"https://pith.science/paper/QQQF3RYB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.19928&json=true","fetch_graph":"https://pith.science/api/pith-number/QQQF3RYBM24AZXEUGM5UO25MEX/graph.json","fetch_events":"https://pith.science/api/pith-number/QQQF3RYBM24AZXEUGM5UO25MEX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QQQF3RYBM24AZXEUGM5UO25MEX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QQQF3RYBM24AZXEUGM5UO25MEX/action/storage_attestation","attest_author":"https://pith.science/pith/QQQF3RYBM24AZXEUGM5UO25MEX/action/author_attestation","sign_citation":"https://pith.science/pith/QQQF3RYBM24AZXEUGM5UO25MEX/action/citation_signature","submit_replication":"https://pith.science/pith/QQQF3RYBM24AZXEUGM5UO25MEX/action/replication_record"}},"created_at":"2026-07-05T07:28:11.889846+00:00","updated_at":"2026-07-05T07:28:11.889846+00:00"}