{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:V2CTSH3VW2BAEKJC5DKL7JJ2C2","short_pith_number":"pith:V2CTSH3V","schema_version":"1.0","canonical_sha256":"ae85391f75b682022922e8d4bfa53a169f6d8fd6f87ba85bcbf10ea2dfe22153","source":{"kind":"arxiv","id":"1407.8230","version":1},"attestation_state":"computed","paper":{"title":"On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"R. J. Brunner, Yiran Wang","submitted_at":"2014-07-30T22:17:35Z","abstract_excerpt":"We analyze the clustering of photometrically selected galaxy pairs by using the halo-occupation distribution (HOD) model. We measure the angular two-point auto-correlation function, $\\omega(\\theta)$, for galaxies and galaxy pairs in three volume-limited samples and develop an HOD to model their clustering. Our results are successfully fit by these HOD models, and we see the separation of \"1-halo\" and \"2-halo\" clustering terms for both single galaxies and galaxy pairs. Our clustering measurements and HOD model fits for the single galaxy samples are consistent with previous results. We find that"},"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":"1407.8230","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-30T22:17:35Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"bb37c6e953108e6575c41edeeb25257754d4d79c369ecfd9d3862719435b5e7d","abstract_canon_sha256":"bada57b9afcddfc41ab5d61a6173bfa99b640a7e59203fb303d0dcf8503be414"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:27.059768Z","signature_b64":"8qpA7Nc0cuiIT2hG+xT+y4IZWr22rBzic/3T1L0LfEadj5uhO7zzl7gpOpk8sjLDzaqx/LMngq5YBsO5m8gyAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ae85391f75b682022922e8d4bfa53a169f6d8fd6f87ba85bcbf10ea2dfe22153","last_reissued_at":"2026-05-18T01:42:27.059216Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:27.059216Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"R. J. Brunner, Yiran Wang","submitted_at":"2014-07-30T22:17:35Z","abstract_excerpt":"We analyze the clustering of photometrically selected galaxy pairs by using the halo-occupation distribution (HOD) model. We measure the angular two-point auto-correlation function, $\\omega(\\theta)$, for galaxies and galaxy pairs in three volume-limited samples and develop an HOD to model their clustering. Our results are successfully fit by these HOD models, and we see the separation of \"1-halo\" and \"2-halo\" clustering terms for both single galaxies and galaxy pairs. Our clustering measurements and HOD model fits for the single galaxy samples are consistent with previous results. We find that"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.8230","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":"1407.8230","created_at":"2026-05-18T01:42:27.059304+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.8230v1","created_at":"2026-05-18T01:42:27.059304+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.8230","created_at":"2026-05-18T01:42:27.059304+00:00"},{"alias_kind":"pith_short_12","alias_value":"V2CTSH3VW2BA","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_16","alias_value":"V2CTSH3VW2BAEKJC","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_8","alias_value":"V2CTSH3V","created_at":"2026-05-18T12:28:52.271510+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/V2CTSH3VW2BAEKJC5DKL7JJ2C2","json":"https://pith.science/pith/V2CTSH3VW2BAEKJC5DKL7JJ2C2.json","graph_json":"https://pith.science/api/pith-number/V2CTSH3VW2BAEKJC5DKL7JJ2C2/graph.json","events_json":"https://pith.science/api/pith-number/V2CTSH3VW2BAEKJC5DKL7JJ2C2/events.json","paper":"https://pith.science/paper/V2CTSH3V"},"agent_actions":{"view_html":"https://pith.science/pith/V2CTSH3VW2BAEKJC5DKL7JJ2C2","download_json":"https://pith.science/pith/V2CTSH3VW2BAEKJC5DKL7JJ2C2.json","view_paper":"https://pith.science/paper/V2CTSH3V","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.8230&json=true","fetch_graph":"https://pith.science/api/pith-number/V2CTSH3VW2BAEKJC5DKL7JJ2C2/graph.json","fetch_events":"https://pith.science/api/pith-number/V2CTSH3VW2BAEKJC5DKL7JJ2C2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V2CTSH3VW2BAEKJC5DKL7JJ2C2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V2CTSH3VW2BAEKJC5DKL7JJ2C2/action/storage_attestation","attest_author":"https://pith.science/pith/V2CTSH3VW2BAEKJC5DKL7JJ2C2/action/author_attestation","sign_citation":"https://pith.science/pith/V2CTSH3VW2BAEKJC5DKL7JJ2C2/action/citation_signature","submit_replication":"https://pith.science/pith/V2CTSH3VW2BAEKJC5DKL7JJ2C2/action/replication_record"}},"created_at":"2026-05-18T01:42:27.059304+00:00","updated_at":"2026-05-18T01:42:27.059304+00:00"}