{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:VMWUVGYHD6MBBZCRXBHE4YJMMV","short_pith_number":"pith:VMWUVGYH","schema_version":"1.0","canonical_sha256":"ab2d4a9b071f9810e451b84e4e612c657c8cac6eea0886cc1a18f0e87593b162","source":{"kind":"arxiv","id":"1501.05520","version":1},"attestation_state":"computed","paper":{"title":"Halo mass distribution reconstruction across the cosmic web","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Charling Tao, Cheng Zhao, Chia-Hsun Chuang, Francisco Prada, Francisco-Shu Kitaura, Gustavo Yepes","submitted_at":"2015-01-22T14:50:10Z","abstract_excerpt":"We study the relation between halo mass and its environment from a probabilistic perspective. We find that halo mass depends not only on local dark matter density, but also on non-local quantities such as the cosmic web environment and the halo-exclusion effect. Given these accurate relations, we have developed the HADRON-code (Halo mAss Distribution ReconstructiON), a technique which permits us to assign halo masses to a distribution of haloes in three-dimensional space. This can be applied to the fast production of mock galaxy catalogues, by assigning halo masses, and reproducing accurately "},"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":"1501.05520","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-01-22T14:50:10Z","cross_cats_sorted":[],"title_canon_sha256":"742f2cd002d0e5da86cb616614e29d10bac9e0b978ba087650be6719e6f8d9ea","abstract_canon_sha256":"bc3ea4180855a9a17c3dde3b40136f7fc5a7ab302fc61fc2664e5fbac27f69fc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:28:54.518769Z","signature_b64":"WswLoDkvCrmejtJPnhgYHV2s6Wp8TbXPFJr5YJ2hXEVERxjHSk5l2Ju9Ha9NI7zHUr/vgh04/wUMj9BxJAv9Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ab2d4a9b071f9810e451b84e4e612c657c8cac6eea0886cc1a18f0e87593b162","last_reissued_at":"2026-05-18T02:28:54.518356Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:28:54.518356Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Halo mass distribution reconstruction across the cosmic web","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Charling Tao, Cheng Zhao, Chia-Hsun Chuang, Francisco Prada, Francisco-Shu Kitaura, Gustavo Yepes","submitted_at":"2015-01-22T14:50:10Z","abstract_excerpt":"We study the relation between halo mass and its environment from a probabilistic perspective. We find that halo mass depends not only on local dark matter density, but also on non-local quantities such as the cosmic web environment and the halo-exclusion effect. Given these accurate relations, we have developed the HADRON-code (Halo mAss Distribution ReconstructiON), a technique which permits us to assign halo masses to a distribution of haloes in three-dimensional space. This can be applied to the fast production of mock galaxy catalogues, by assigning halo masses, and reproducing accurately "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.05520","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":""},"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":"1501.05520","created_at":"2026-05-18T02:28:54.518428+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.05520v1","created_at":"2026-05-18T02:28:54.518428+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.05520","created_at":"2026-05-18T02:28:54.518428+00:00"},{"alias_kind":"pith_short_12","alias_value":"VMWUVGYHD6MB","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_16","alias_value":"VMWUVGYHD6MBBZCR","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_8","alias_value":"VMWUVGYH","created_at":"2026-05-18T12:29:47.479230+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/VMWUVGYHD6MBBZCRXBHE4YJMMV","json":"https://pith.science/pith/VMWUVGYHD6MBBZCRXBHE4YJMMV.json","graph_json":"https://pith.science/api/pith-number/VMWUVGYHD6MBBZCRXBHE4YJMMV/graph.json","events_json":"https://pith.science/api/pith-number/VMWUVGYHD6MBBZCRXBHE4YJMMV/events.json","paper":"https://pith.science/paper/VMWUVGYH"},"agent_actions":{"view_html":"https://pith.science/pith/VMWUVGYHD6MBBZCRXBHE4YJMMV","download_json":"https://pith.science/pith/VMWUVGYHD6MBBZCRXBHE4YJMMV.json","view_paper":"https://pith.science/paper/VMWUVGYH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.05520&json=true","fetch_graph":"https://pith.science/api/pith-number/VMWUVGYHD6MBBZCRXBHE4YJMMV/graph.json","fetch_events":"https://pith.science/api/pith-number/VMWUVGYHD6MBBZCRXBHE4YJMMV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VMWUVGYHD6MBBZCRXBHE4YJMMV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VMWUVGYHD6MBBZCRXBHE4YJMMV/action/storage_attestation","attest_author":"https://pith.science/pith/VMWUVGYHD6MBBZCRXBHE4YJMMV/action/author_attestation","sign_citation":"https://pith.science/pith/VMWUVGYHD6MBBZCRXBHE4YJMMV/action/citation_signature","submit_replication":"https://pith.science/pith/VMWUVGYHD6MBBZCRXBHE4YJMMV/action/replication_record"}},"created_at":"2026-05-18T02:28:54.518428+00:00","updated_at":"2026-05-18T02:28:54.518428+00:00"}