{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:QVUIWGVHEFCWUR4QM3ZQED4PXM","short_pith_number":"pith:QVUIWGVH","schema_version":"1.0","canonical_sha256":"85688b1aa721456a479066f3020f8fbb21a3ff1c9c80c21af991264c3112f2e3","source":{"kind":"arxiv","id":"1010.5484","version":1},"attestation_state":"computed","paper":{"title":"A Halo Model of Local IRAS Galaxies Selected at 60 Micron Using Conditional Luminosity Functions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Asantha Cooray, Lingyu Wang, Seb Oliver","submitted_at":"2010-10-26T19:03:41Z","abstract_excerpt":"Using conditional luminosity functions (CLFs) which encode the luminosity distribution of galaxies as a function of halo mass, we construct a halo model of IRAS galaxies selected at 60 micron. An abundance matching technique is used to link galaxy luminosity to the host halo mass. The shape of the mass - light relation at 60 micron is different from those derived at r-, K- and B-band. This is because the 60 micron LF can not be fitted by a Schechter function with a sharp exponential cutoff. We then seek the parameters in the CLFs that best fit the LF and power spectrum. We find that the predic"},"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":"1010.5484","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-10-26T19:03:41Z","cross_cats_sorted":[],"title_canon_sha256":"61328777394e0484af1501607661c8d7bc7b8594ee5d4503e5c5c952e8805191","abstract_canon_sha256":"b45bf93f833cc34d716d2ed2e1a5d042854dba0872e10e5dea487f2f0c756e60"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:38:38.635489Z","signature_b64":"cF3TZEIoRmlJB/vNSCRh8Oc1uGCZjowiGopwyr/nCqGcLL+XqvWCSvWybzO98wQZBhoy+iAlOIx5/XQlJY24Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"85688b1aa721456a479066f3020f8fbb21a3ff1c9c80c21af991264c3112f2e3","last_reissued_at":"2026-05-18T04:38:38.634683Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:38:38.634683Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Halo Model of Local IRAS Galaxies Selected at 60 Micron Using Conditional Luminosity Functions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Asantha Cooray, Lingyu Wang, Seb Oliver","submitted_at":"2010-10-26T19:03:41Z","abstract_excerpt":"Using conditional luminosity functions (CLFs) which encode the luminosity distribution of galaxies as a function of halo mass, we construct a halo model of IRAS galaxies selected at 60 micron. An abundance matching technique is used to link galaxy luminosity to the host halo mass. The shape of the mass - light relation at 60 micron is different from those derived at r-, K- and B-band. This is because the 60 micron LF can not be fitted by a Schechter function with a sharp exponential cutoff. We then seek the parameters in the CLFs that best fit the LF and power spectrum. We find that the predic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.5484","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":"1010.5484","created_at":"2026-05-18T04:38:38.634838+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.5484v1","created_at":"2026-05-18T04:38:38.634838+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.5484","created_at":"2026-05-18T04:38:38.634838+00:00"},{"alias_kind":"pith_short_12","alias_value":"QVUIWGVHEFCW","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_16","alias_value":"QVUIWGVHEFCWUR4Q","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_8","alias_value":"QVUIWGVH","created_at":"2026-05-18T12:26:13.927090+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/QVUIWGVHEFCWUR4QM3ZQED4PXM","json":"https://pith.science/pith/QVUIWGVHEFCWUR4QM3ZQED4PXM.json","graph_json":"https://pith.science/api/pith-number/QVUIWGVHEFCWUR4QM3ZQED4PXM/graph.json","events_json":"https://pith.science/api/pith-number/QVUIWGVHEFCWUR4QM3ZQED4PXM/events.json","paper":"https://pith.science/paper/QVUIWGVH"},"agent_actions":{"view_html":"https://pith.science/pith/QVUIWGVHEFCWUR4QM3ZQED4PXM","download_json":"https://pith.science/pith/QVUIWGVHEFCWUR4QM3ZQED4PXM.json","view_paper":"https://pith.science/paper/QVUIWGVH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.5484&json=true","fetch_graph":"https://pith.science/api/pith-number/QVUIWGVHEFCWUR4QM3ZQED4PXM/graph.json","fetch_events":"https://pith.science/api/pith-number/QVUIWGVHEFCWUR4QM3ZQED4PXM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QVUIWGVHEFCWUR4QM3ZQED4PXM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QVUIWGVHEFCWUR4QM3ZQED4PXM/action/storage_attestation","attest_author":"https://pith.science/pith/QVUIWGVHEFCWUR4QM3ZQED4PXM/action/author_attestation","sign_citation":"https://pith.science/pith/QVUIWGVHEFCWUR4QM3ZQED4PXM/action/citation_signature","submit_replication":"https://pith.science/pith/QVUIWGVHEFCWUR4QM3ZQED4PXM/action/replication_record"}},"created_at":"2026-05-18T04:38:38.634838+00:00","updated_at":"2026-05-18T04:38:38.634838+00:00"}