{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:DHLUCRC3CQ32D5OQAWLOWDXBCP","short_pith_number":"pith:DHLUCRC3","schema_version":"1.0","canonical_sha256":"19d741445b1437a1f5d00596eb0ee113f7ea1500f821ff8c6edbd353842e1dad","source":{"kind":"arxiv","id":"1611.09862","version":2},"attestation_state":"computed","paper":{"title":"Testing $\\Lambda$CDM at the lowest redshifts with SN Ia and galaxy velocities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Daniel L. Shafer, Daniel Scolnic, Dragan Huterer, Fabian Schmidt","submitted_at":"2016-11-29T21:00:02Z","abstract_excerpt":"Peculiar velocities of objects in the nearby universe are correlated due to the gravitational pull of large-scale structure. By measuring these velocities, we have a unique opportunity to test the cosmological model at the lowest redshifts. We perform this test, using current data to constrain the amplitude of the \"signal\" covariance matrix describing the velocities and their correlations. We consider a new, well-calibrated \"Supercal\" set of low-redshift SNe Ia as well as a set of distances derived from the fundamental plane relation of 6dFGS galaxies. Analyzing the SN and galaxy data separate"},"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":"1611.09862","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-11-29T21:00:02Z","cross_cats_sorted":["astro-ph.GA","gr-qc"],"title_canon_sha256":"8484dcba96058efe67b18be576c76cdc130d00e503ffdddd375fc1934b02a927","abstract_canon_sha256":"e2dd4f9f8598ad16cff1cd15df5645f12dbb7791cdbd728efd0ef01a63eb2feb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:44:51.962407Z","signature_b64":"ft76lCY01M7iBPio+qAKlN9qBK4VwlanUbZHZSdK7Rxtjn/UNtVUUgcBjs+eNbv3GfXGTRniLaOUT2ELLeQwDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"19d741445b1437a1f5d00596eb0ee113f7ea1500f821ff8c6edbd353842e1dad","last_reissued_at":"2026-05-18T00:44:51.961858Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:44:51.961858Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing $\\Lambda$CDM at the lowest redshifts with SN Ia and galaxy velocities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Daniel L. Shafer, Daniel Scolnic, Dragan Huterer, Fabian Schmidt","submitted_at":"2016-11-29T21:00:02Z","abstract_excerpt":"Peculiar velocities of objects in the nearby universe are correlated due to the gravitational pull of large-scale structure. By measuring these velocities, we have a unique opportunity to test the cosmological model at the lowest redshifts. We perform this test, using current data to constrain the amplitude of the \"signal\" covariance matrix describing the velocities and their correlations. We consider a new, well-calibrated \"Supercal\" set of low-redshift SNe Ia as well as a set of distances derived from the fundamental plane relation of 6dFGS galaxies. Analyzing the SN and galaxy data separate"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.09862","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1611.09862","created_at":"2026-05-18T00:44:51.961942+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.09862v2","created_at":"2026-05-18T00:44:51.961942+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.09862","created_at":"2026-05-18T00:44:51.961942+00:00"},{"alias_kind":"pith_short_12","alias_value":"DHLUCRC3CQ32","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_16","alias_value":"DHLUCRC3CQ32D5OQ","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_8","alias_value":"DHLUCRC3","created_at":"2026-05-18T12:30:12.583610+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2105.13549","citing_title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","ref_index":57,"is_internal_anchor":true},{"citing_arxiv_id":"2508.19106","citing_title":"Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid","ref_index":37,"is_internal_anchor":true},{"citing_arxiv_id":"2604.06361","citing_title":"Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"1807.06209","citing_title":"Planck 2018 results. VI. Cosmological parameters","ref_index":187,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP","json":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP.json","graph_json":"https://pith.science/api/pith-number/DHLUCRC3CQ32D5OQAWLOWDXBCP/graph.json","events_json":"https://pith.science/api/pith-number/DHLUCRC3CQ32D5OQAWLOWDXBCP/events.json","paper":"https://pith.science/paper/DHLUCRC3"},"agent_actions":{"view_html":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP","download_json":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP.json","view_paper":"https://pith.science/paper/DHLUCRC3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.09862&json=true","fetch_graph":"https://pith.science/api/pith-number/DHLUCRC3CQ32D5OQAWLOWDXBCP/graph.json","fetch_events":"https://pith.science/api/pith-number/DHLUCRC3CQ32D5OQAWLOWDXBCP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP/action/storage_attestation","attest_author":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP/action/author_attestation","sign_citation":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP/action/citation_signature","submit_replication":"https://pith.science/pith/DHLUCRC3CQ32D5OQAWLOWDXBCP/action/replication_record"}},"created_at":"2026-05-18T00:44:51.961942+00:00","updated_at":"2026-05-18T00:44:51.961942+00:00"}