{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:VBZCIKWQNK3GIBI4A3ELJRE75J","short_pith_number":"pith:VBZCIKWQ","schema_version":"1.0","canonical_sha256":"a872242ad06ab664051c06c8b4c49fea5e5353588e3a77bb677bda08965fec8a","source":{"kind":"arxiv","id":"2209.11238","version":2},"attestation_state":"computed","paper":{"title":"Cosmicflows-4","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Alexandra Dupuy, Benjamin E. Stahl, Cullan Howlett, Daniel Guinet, Daniel Pomar\\`ede, Daniel Scolnic, David Rubin, Dillon Brout, Ehsan Kourkchi, Gagandeep S. Anand, H\\'el\\`ene M. Courtois, John P. Blakeslee, Joseph B. Jensen, Khaled Said, Luca Rizzi, R. Brent Tully, Thomas de Jaeger","submitted_at":"2022-09-22T18:00:01Z","abstract_excerpt":"With Cosmicflows-4, distances are compiled for 55,877 galaxies gathered into 38,065 groups. Eight methodologies are employed, with the largest numbers coming from the correlations between the photometric and kinematic properties of spiral galaxies (TF) and elliptical galaxies (FP). Supernovae that arise from degenerate progenitors (type Ia Sne) are an important overlapping component. Smaller contributions come from distance estimates from the surface brightness fluctuations of elliptical galaxies and the luminosities and expansion rates of core collapse supernovae (SNII). Cepheid period-lumino"},"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":"2209.11238","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2022-09-22T18:00:01Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"edee9d05160d432c4ee1e9bbe3b3a102c3bad43156b55391443d4ddbc8db221d","abstract_canon_sha256":"cb2eca81e765e19a335e639b6103143b64af00bfd27817daf9aced7742a902a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:43:56.821685Z","signature_b64":"kBPey8wijlgWlnY0nAkPgmm/7uRz7YDiYUX1UrcM033Z0TLOQB5+ctckJ/nwCQtB0EWXfrQs8AgxDoKuCH2ECw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a872242ad06ab664051c06c8b4c49fea5e5353588e3a77bb677bda08965fec8a","last_reissued_at":"2026-07-05T05:43:56.821179Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:43:56.821179Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmicflows-4","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Alexandra Dupuy, Benjamin E. Stahl, Cullan Howlett, Daniel Guinet, Daniel Pomar\\`ede, Daniel Scolnic, David Rubin, Dillon Brout, Ehsan Kourkchi, Gagandeep S. Anand, H\\'el\\`ene M. Courtois, John P. Blakeslee, Joseph B. Jensen, Khaled Said, Luca Rizzi, R. Brent Tully, Thomas de Jaeger","submitted_at":"2022-09-22T18:00:01Z","abstract_excerpt":"With Cosmicflows-4, distances are compiled for 55,877 galaxies gathered into 38,065 groups. Eight methodologies are employed, with the largest numbers coming from the correlations between the photometric and kinematic properties of spiral galaxies (TF) and elliptical galaxies (FP). Supernovae that arise from degenerate progenitors (type Ia Sne) are an important overlapping component. Smaller contributions come from distance estimates from the surface brightness fluctuations of elliptical galaxies and the luminosities and expansion rates of core collapse supernovae (SNII). Cepheid period-lumino"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.11238","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2209.11238/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":"2209.11238","created_at":"2026-07-05T05:43:56.821239+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.11238v2","created_at":"2026-07-05T05:43:56.821239+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.11238","created_at":"2026-07-05T05:43:56.821239+00:00"},{"alias_kind":"pith_short_12","alias_value":"VBZCIKWQNK3G","created_at":"2026-07-05T05:43:56.821239+00:00"},{"alias_kind":"pith_short_16","alias_value":"VBZCIKWQNK3GIBI4","created_at":"2026-07-05T05:43:56.821239+00:00"},{"alias_kind":"pith_short_8","alias_value":"VBZCIKWQ","created_at":"2026-07-05T05:43:56.821239+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07821","citing_title":"Multipolar structure of the local expansion rate from incomplete sky data","ref_index":76,"is_internal_anchor":true},{"citing_arxiv_id":"2606.05539","citing_title":"Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2605.30305","citing_title":"Augmented Correlation Functions for Spectroscopic Galaxy Surveys","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16426","citing_title":"Expected redshift drift for tilted observers","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2512.02526","citing_title":"Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4","ref_index":34,"is_internal_anchor":false},{"citing_arxiv_id":"2603.20963","citing_title":"Redshift Dipoles from Non-Geodesic Observer Congruences in Covariant Cosmology","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2604.03769","citing_title":"Dispersion Measure Distribution of Unlocalized Fast Radio Bursts as a Probe of the Hubble Constant","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19922","citing_title":"Measuring neutrino mass and asymmetry through galaxy pairwise peculiar velocity","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06361","citing_title":"Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB","ref_index":47,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J","json":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J.json","graph_json":"https://pith.science/api/pith-number/VBZCIKWQNK3GIBI4A3ELJRE75J/graph.json","events_json":"https://pith.science/api/pith-number/VBZCIKWQNK3GIBI4A3ELJRE75J/events.json","paper":"https://pith.science/paper/VBZCIKWQ"},"agent_actions":{"view_html":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J","download_json":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J.json","view_paper":"https://pith.science/paper/VBZCIKWQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.11238&json=true","fetch_graph":"https://pith.science/api/pith-number/VBZCIKWQNK3GIBI4A3ELJRE75J/graph.json","fetch_events":"https://pith.science/api/pith-number/VBZCIKWQNK3GIBI4A3ELJRE75J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J/action/storage_attestation","attest_author":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J/action/author_attestation","sign_citation":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J/action/citation_signature","submit_replication":"https://pith.science/pith/VBZCIKWQNK3GIBI4A3ELJRE75J/action/replication_record"}},"created_at":"2026-07-05T05:43:56.821239+00:00","updated_at":"2026-07-05T05:43:56.821239+00:00"}