{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:N7NHSATOJ73PVQ3BWXUOWPPTX2","short_pith_number":"pith:N7NHSATO","schema_version":"1.0","canonical_sha256":"6fda79026e4ff6fac361b5e8eb3df3bebf04900f6e4427a4d127f1c7e77f4527","source":{"kind":"arxiv","id":"2506.22431","version":1},"attestation_state":"computed","paper":{"title":"Gravitational redshift from large-scale structure: nonlinearities, anti-symmetries, and the dipole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Camille Bonvin, Lawrence Dam","submitted_at":"2025-06-27T17:58:34Z","abstract_excerpt":"Gravitational redshift imprints a slight asymmetry in the observed clustering of galaxies, producing odd multipoles (e.g.\\ the dipole) in the cross-correlation function. But there are other sources of asymmetry which must also be considered in any model which aims to measure gravitational redshift from large-scale structure. In this work we develop a nonlinear model of the redshift-space correlation function complete down to these subleading, asymmetric effects. In addition to gravitational redshift and the well-known redshift-space distortions, our model, given by a compact nonperturbative fo"},"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":"2506.22431","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-06-27T17:58:34Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"90fedc31118c3461da5b6863bd5f058efff7d47ef97d6d43b68deb15cb655ade","abstract_canon_sha256":"72720e05810e6e79c0fe90974df4ce9ac242cccd22c20f1436f9f702597c3512"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:38:30.836886Z","signature_b64":"kLF53Zl3I1AULCbm624teHhTj1M8qGczv+/GmPqhXVtmT2xvuRvOEPcSak9Oqum3CcMD+sAB4s2E2spka+7KDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6fda79026e4ff6fac361b5e8eb3df3bebf04900f6e4427a4d127f1c7e77f4527","last_reissued_at":"2026-07-05T11:38:30.836388Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:38:30.836388Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational redshift from large-scale structure: nonlinearities, anti-symmetries, and the dipole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Camille Bonvin, Lawrence Dam","submitted_at":"2025-06-27T17:58:34Z","abstract_excerpt":"Gravitational redshift imprints a slight asymmetry in the observed clustering of galaxies, producing odd multipoles (e.g.\\ the dipole) in the cross-correlation function. But there are other sources of asymmetry which must also be considered in any model which aims to measure gravitational redshift from large-scale structure. In this work we develop a nonlinear model of the redshift-space correlation function complete down to these subleading, asymmetric effects. In addition to gravitational redshift and the well-known redshift-space distortions, our model, given by a compact nonperturbative fo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.22431","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2506.22431/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2506.22431","created_at":"2026-07-05T11:38:30.836447+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.22431v1","created_at":"2026-07-05T11:38:30.836447+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.22431","created_at":"2026-07-05T11:38:30.836447+00:00"},{"alias_kind":"pith_short_12","alias_value":"N7NHSATOJ73P","created_at":"2026-07-05T11:38:30.836447+00:00"},{"alias_kind":"pith_short_16","alias_value":"N7NHSATOJ73PVQ3B","created_at":"2026-07-05T11:38:30.836447+00:00"},{"alias_kind":"pith_short_8","alias_value":"N7NHSATO","created_at":"2026-07-05T11:38:30.836447+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.05203","citing_title":"Non-conservation and time non-locality of biased tracers","ref_index":150,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2","json":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2.json","graph_json":"https://pith.science/api/pith-number/N7NHSATOJ73PVQ3BWXUOWPPTX2/graph.json","events_json":"https://pith.science/api/pith-number/N7NHSATOJ73PVQ3BWXUOWPPTX2/events.json","paper":"https://pith.science/paper/N7NHSATO"},"agent_actions":{"view_html":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2","download_json":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2.json","view_paper":"https://pith.science/paper/N7NHSATO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.22431&json=true","fetch_graph":"https://pith.science/api/pith-number/N7NHSATOJ73PVQ3BWXUOWPPTX2/graph.json","fetch_events":"https://pith.science/api/pith-number/N7NHSATOJ73PVQ3BWXUOWPPTX2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2/action/storage_attestation","attest_author":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2/action/author_attestation","sign_citation":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2/action/citation_signature","submit_replication":"https://pith.science/pith/N7NHSATOJ73PVQ3BWXUOWPPTX2/action/replication_record"}},"created_at":"2026-07-05T11:38:30.836447+00:00","updated_at":"2026-07-05T11:38:30.836447+00:00"}