{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:NFM32TMAQ4IXYGAKLE5ZM6VX7M","short_pith_number":"pith:NFM32TMA","canonical_record":{"source":{"id":"1203.5335","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-03-23T20:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"30b34e90aad13189643a00d4ad7a2fa207d65a027c6587618e41cfda25ce1661","abstract_canon_sha256":"beffefe3006b165aa49770051d46232975fadd7270ae44ce90c40508dd16d507"},"schema_version":"1.0"},"canonical_sha256":"6959bd4d8087117c180a593b967ab7fb11c5745f8ea40c5a5332b3d3613bb44a","source":{"kind":"arxiv","id":"1203.5335","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1203.5335","created_at":"2026-05-18T01:58:02Z"},{"alias_kind":"arxiv_version","alias_value":"1203.5335v2","created_at":"2026-05-18T01:58:02Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.5335","created_at":"2026-05-18T01:58:02Z"},{"alias_kind":"pith_short_12","alias_value":"NFM32TMAQ4IX","created_at":"2026-05-18T12:27:16Z"},{"alias_kind":"pith_short_16","alias_value":"NFM32TMAQ4IXYGAK","created_at":"2026-05-18T12:27:16Z"},{"alias_kind":"pith_short_8","alias_value":"NFM32TMA","created_at":"2026-05-18T12:27:16Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:NFM32TMAQ4IXYGAKLE5ZM6VX7M","target":"record","payload":{"canonical_record":{"source":{"id":"1203.5335","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-03-23T20:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"30b34e90aad13189643a00d4ad7a2fa207d65a027c6587618e41cfda25ce1661","abstract_canon_sha256":"beffefe3006b165aa49770051d46232975fadd7270ae44ce90c40508dd16d507"},"schema_version":"1.0"},"canonical_sha256":"6959bd4d8087117c180a593b967ab7fb11c5745f8ea40c5a5332b3d3613bb44a","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:02.343895Z","signature_b64":"nZk+e4uJO5ufAtFp3wCgrIaObtSd6agc05Z16pTsVTUsBdURafWd06YgeNVhSl4JHX7iHTf2JhR2O7ptIX55Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6959bd4d8087117c180a593b967ab7fb11c5745f8ea40c5a5332b3d3613bb44a","last_reissued_at":"2026-05-18T01:58:02.343394Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:02.343394Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1203.5335","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:58:02Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"cGA/CdkTf9dJgZOm3wTK8PeziAXk2+H8ogPLfnHeNi7NRZ6HrXqn85R9XNhlwLCt41kE9YdM5DBL1GvqQbojDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T14:10:06.085093Z"},"content_sha256":"d674dc4313959e284837c469a914e667c3941c439c35032c3ed90ba17f1e6d6f","schema_version":"1.0","event_id":"sha256:d674dc4313959e284837c469a914e667c3941c439c35032c3ed90ba17f1e6d6f"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:NFM32TMAQ4IXYGAKLE5ZM6VX7M","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The effects of halo alignment and shape on the clustering of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"2), Leiden University), Marcel P. van Daalen (1, Raul E. Angulo (1), Simon D. M. White (1) ((1) Max Planck Institute for Astrophysics (2) Leiden Observatory","submitted_at":"2012-03-23T20:00:00Z","abstract_excerpt":"We investigate the effects of halo shape and its alignment with larger scale structure on the galaxy correlation function. We base our analysis on the galaxy formation models of Guo et al., run on the Millennium Simulations. We quantify the importance of these effects by randomizing the angular positions of satellite galaxies within haloes, either coherently or individually, while keeping the distance to their respective central galaxies fixed. We find that the effect of disrupting the alignment with larger scale structure is a ~2 per cent decrease in the galaxy correlation function around r=1"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.5335","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:58:02Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"HgmUt+xAOv7SBUGZB5M4ZzheRmZe6pCDqTJ/fzAdy9IA2yCLUSoyzBx0wiNUU95Q8W/W/V97HGbxAPPQKDqxCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T14:10:06.085463Z"},"content_sha256":"e34fb559b18472b65ec1219c7d28847c2b611d6165117969166df474fc561733","schema_version":"1.0","event_id":"sha256:e34fb559b18472b65ec1219c7d28847c2b611d6165117969166df474fc561733"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/NFM32TMAQ4IXYGAKLE5ZM6VX7M/bundle.json","state_url":"https://pith.science/pith/NFM32TMAQ4IXYGAKLE5ZM6VX7M/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/NFM32TMAQ4IXYGAKLE5ZM6VX7M/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-30T14:10:06Z","links":{"resolver":"https://pith.science/pith/NFM32TMAQ4IXYGAKLE5ZM6VX7M","bundle":"https://pith.science/pith/NFM32TMAQ4IXYGAKLE5ZM6VX7M/bundle.json","state":"https://pith.science/pith/NFM32TMAQ4IXYGAKLE5ZM6VX7M/state.json","well_known_bundle":"https://pith.science/.well-known/pith/NFM32TMAQ4IXYGAKLE5ZM6VX7M/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:NFM32TMAQ4IXYGAKLE5ZM6VX7M","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"beffefe3006b165aa49770051d46232975fadd7270ae44ce90c40508dd16d507","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-03-23T20:00:00Z","title_canon_sha256":"30b34e90aad13189643a00d4ad7a2fa207d65a027c6587618e41cfda25ce1661"},"schema_version":"1.0","source":{"id":"1203.5335","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1203.5335","created_at":"2026-05-18T01:58:02Z"},{"alias_kind":"arxiv_version","alias_value":"1203.5335v2","created_at":"2026-05-18T01:58:02Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.5335","created_at":"2026-05-18T01:58:02Z"},{"alias_kind":"pith_short_12","alias_value":"NFM32TMAQ4IX","created_at":"2026-05-18T12:27:16Z"},{"alias_kind":"pith_short_16","alias_value":"NFM32TMAQ4IXYGAK","created_at":"2026-05-18T12:27:16Z"},{"alias_kind":"pith_short_8","alias_value":"NFM32TMA","created_at":"2026-05-18T12:27:16Z"}],"graph_snapshots":[{"event_id":"sha256:e34fb559b18472b65ec1219c7d28847c2b611d6165117969166df474fc561733","target":"graph","created_at":"2026-05-18T01:58:02Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We investigate the effects of halo shape and its alignment with larger scale structure on the galaxy correlation function. We base our analysis on the galaxy formation models of Guo et al., run on the Millennium Simulations. We quantify the importance of these effects by randomizing the angular positions of satellite galaxies within haloes, either coherently or individually, while keeping the distance to their respective central galaxies fixed. We find that the effect of disrupting the alignment with larger scale structure is a ~2 per cent decrease in the galaxy correlation function around r=1","authors_text":"2), Leiden University), Marcel P. van Daalen (1, Raul E. Angulo (1), Simon D. M. White (1) ((1) Max Planck Institute for Astrophysics (2) Leiden Observatory","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-03-23T20:00:00Z","title":"The effects of halo alignment and shape on the clustering of galaxies"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.5335","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:d674dc4313959e284837c469a914e667c3941c439c35032c3ed90ba17f1e6d6f","target":"record","created_at":"2026-05-18T01:58:02Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"beffefe3006b165aa49770051d46232975fadd7270ae44ce90c40508dd16d507","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-03-23T20:00:00Z","title_canon_sha256":"30b34e90aad13189643a00d4ad7a2fa207d65a027c6587618e41cfda25ce1661"},"schema_version":"1.0","source":{"id":"1203.5335","kind":"arxiv","version":2}},"canonical_sha256":"6959bd4d8087117c180a593b967ab7fb11c5745f8ea40c5a5332b3d3613bb44a","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"6959bd4d8087117c180a593b967ab7fb11c5745f8ea40c5a5332b3d3613bb44a","first_computed_at":"2026-05-18T01:58:02.343394Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:58:02.343394Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"nZk+e4uJO5ufAtFp3wCgrIaObtSd6agc05Z16pTsVTUsBdURafWd06YgeNVhSl4JHX7iHTf2JhR2O7ptIX55Dw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:58:02.343895Z","signed_message":"canonical_sha256_bytes"},"source_id":"1203.5335","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:d674dc4313959e284837c469a914e667c3941c439c35032c3ed90ba17f1e6d6f","sha256:e34fb559b18472b65ec1219c7d28847c2b611d6165117969166df474fc561733"],"state_sha256":"bf9eacb0dca7093dfc2d3d55e522e9ec5e0c8db2ed5cdb63eab3bb4b0872a3eb"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Qz46L6EKC4Lr25tamAs42w8hN+PP4HhKpcMTUQFIvcvsmon/nGbPt7pPNLJWKwHLorEWEdgUZM9gFUxZrDz0CQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-30T14:10:06.087945Z","bundle_sha256":"06346cc2fc790ea77d604824026db8fcae944ac0aaef9a78c3c0f89cf5e133fd"}}