{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:6FNT2VDYMC6YWCMAJRSSG6WCSK","short_pith_number":"pith:6FNT2VDY","schema_version":"1.0","canonical_sha256":"f15b3d547860bd8b09804c65237ac292905a7e7376528221abcb2002281ec9ff","source":{"kind":"arxiv","id":"1603.04152","version":2},"attestation_state":"computed","paper":{"title":"Alignments of dark matter halos with large-scale tidal fields: mass and redshift dependence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"H.J. Mo, Huiyuan Wang, Jingjing Shi, Sijie Chen","submitted_at":"2016-03-14T06:59:47Z","abstract_excerpt":"Large scale tidal field estimated directly from the distribution of dark matter halos is used to investigate how halo shapes and spin vectors are aligned with the cosmic web. The major, intermediate and minor axes of halos are aligned with the corresponding tidal axes, and halo spin axes tend to be parallel with the intermediate axes and perpendicular to the major axes of tidal field. The strengths of these alignments generally increase with halo mass and redshift, but the dependencies are only through the peak height, {\\nu}. The scaling relations of the alignment strengths with the value of {"},"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":"1603.04152","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-03-14T06:59:47Z","cross_cats_sorted":[],"title_canon_sha256":"6fb060c0c7d4a2c63c9125c45543a286b0c72294929caa3e145b1f1fc5aa6625","abstract_canon_sha256":"a5fd1d414a4ae82905e6d9ce77732a2e0c5ca241ba497408b2f60c7eb1358d1a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:11:31.396659Z","signature_b64":"utz/Vw9u56fAWZpWbqoS2slGNOtSqS8fD+7p1bPouGCE3IZGc1aWqh/Zs9/i6/3IZW2w0/qUwC3qu4vpBy2ICQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f15b3d547860bd8b09804c65237ac292905a7e7376528221abcb2002281ec9ff","last_reissued_at":"2026-05-18T01:11:31.396206Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:11:31.396206Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Alignments of dark matter halos with large-scale tidal fields: mass and redshift dependence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"H.J. Mo, Huiyuan Wang, Jingjing Shi, Sijie Chen","submitted_at":"2016-03-14T06:59:47Z","abstract_excerpt":"Large scale tidal field estimated directly from the distribution of dark matter halos is used to investigate how halo shapes and spin vectors are aligned with the cosmic web. The major, intermediate and minor axes of halos are aligned with the corresponding tidal axes, and halo spin axes tend to be parallel with the intermediate axes and perpendicular to the major axes of tidal field. The strengths of these alignments generally increase with halo mass and redshift, but the dependencies are only through the peak height, {\\nu}. The scaling relations of the alignment strengths with the value of {"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.04152","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":"1603.04152","created_at":"2026-05-18T01:11:31.396268+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.04152v2","created_at":"2026-05-18T01:11:31.396268+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.04152","created_at":"2026-05-18T01:11:31.396268+00:00"},{"alias_kind":"pith_short_12","alias_value":"6FNT2VDYMC6Y","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_16","alias_value":"6FNT2VDYMC6YWCMA","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_8","alias_value":"6FNT2VDY","created_at":"2026-05-18T12:30:01.593930+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/6FNT2VDYMC6YWCMAJRSSG6WCSK","json":"https://pith.science/pith/6FNT2VDYMC6YWCMAJRSSG6WCSK.json","graph_json":"https://pith.science/api/pith-number/6FNT2VDYMC6YWCMAJRSSG6WCSK/graph.json","events_json":"https://pith.science/api/pith-number/6FNT2VDYMC6YWCMAJRSSG6WCSK/events.json","paper":"https://pith.science/paper/6FNT2VDY"},"agent_actions":{"view_html":"https://pith.science/pith/6FNT2VDYMC6YWCMAJRSSG6WCSK","download_json":"https://pith.science/pith/6FNT2VDYMC6YWCMAJRSSG6WCSK.json","view_paper":"https://pith.science/paper/6FNT2VDY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.04152&json=true","fetch_graph":"https://pith.science/api/pith-number/6FNT2VDYMC6YWCMAJRSSG6WCSK/graph.json","fetch_events":"https://pith.science/api/pith-number/6FNT2VDYMC6YWCMAJRSSG6WCSK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6FNT2VDYMC6YWCMAJRSSG6WCSK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6FNT2VDYMC6YWCMAJRSSG6WCSK/action/storage_attestation","attest_author":"https://pith.science/pith/6FNT2VDYMC6YWCMAJRSSG6WCSK/action/author_attestation","sign_citation":"https://pith.science/pith/6FNT2VDYMC6YWCMAJRSSG6WCSK/action/citation_signature","submit_replication":"https://pith.science/pith/6FNT2VDYMC6YWCMAJRSSG6WCSK/action/replication_record"}},"created_at":"2026-05-18T01:11:31.396268+00:00","updated_at":"2026-05-18T01:11:31.396268+00:00"}