{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:3XCXCFW5BQIYWEEUXG54AWHZIR","short_pith_number":"pith:3XCXCFW5","schema_version":"1.0","canonical_sha256":"ddc57116dd0c118b1094b9bbc058f94449e0a48711d63d9332c531d0d14d0845","source":{"kind":"arxiv","id":"2007.12607","version":2},"attestation_state":"computed","paper":{"title":"Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam D. Myers, Anthony R. Pullen, Ashley J. Ross, Brad W. Lyke, Cheng Zhao, Chia-Hsun Chuang, Etienne Burtin, Graziano Rossi, Jiamin Hou, Richard Neveux, Shadab Alam, Sukhdeep Singh, Yucheng Zhang","submitted_at":"2020-07-24T16:08:10Z","abstract_excerpt":"We test general relativity (GR) at the effective redshift $\\bar{z} \\sim 1.5$ by estimating the statistic $E_G$, a probe of gravity, on cosmological scales $19 - 190\\,h^{-1}{\\rm Mpc}$. This is the highest-redshift and largest-scale estimation of $E_G$ so far. We use the quasar sample with redshifts $0.8 < z < 2.2$ from Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 16 (DR16) as the large-scale structure (LSS) tracer, for which the angular power spectrum $C_\\ell^{qq}$ and the redshift-space distortion (RSD) parameter $\\beta$ are estimated. By cr"},"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":"2007.12607","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2020-07-24T16:08:10Z","cross_cats_sorted":[],"title_canon_sha256":"497db2e147125c5770ab40346f2de83fc4d196a3987a6997bd1d539f8cc18ac3","abstract_canon_sha256":"f2313c92fb504b82d09064e23dd920982dbd01ab509f9c6dc8053f9b068f5700"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:01:13.601278Z","signature_b64":"s4xc6g5xDmWUsZ3rmlUq95LcVgzjDv9ji4N9CE0srXRMjleR4XYOUzf/+3wokTXArulV8px5UJpf6Oi6nFvcCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ddc57116dd0c118b1094b9bbc058f94449e0a48711d63d9332c531d0d14d0845","last_reissued_at":"2026-07-05T02:01:13.600821Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:01:13.600821Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam D. Myers, Anthony R. Pullen, Ashley J. Ross, Brad W. Lyke, Cheng Zhao, Chia-Hsun Chuang, Etienne Burtin, Graziano Rossi, Jiamin Hou, Richard Neveux, Shadab Alam, Sukhdeep Singh, Yucheng Zhang","submitted_at":"2020-07-24T16:08:10Z","abstract_excerpt":"We test general relativity (GR) at the effective redshift $\\bar{z} \\sim 1.5$ by estimating the statistic $E_G$, a probe of gravity, on cosmological scales $19 - 190\\,h^{-1}{\\rm Mpc}$. This is the highest-redshift and largest-scale estimation of $E_G$ so far. We use the quasar sample with redshifts $0.8 < z < 2.2$ from Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 16 (DR16) as the large-scale structure (LSS) tracer, for which the angular power spectrum $C_\\ell^{qq}$ and the redshift-space distortion (RSD) parameter $\\beta$ are estimated. By cr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2007.12607","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/2007.12607/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":"2007.12607","created_at":"2026-07-05T02:01:13.600879+00:00"},{"alias_kind":"arxiv_version","alias_value":"2007.12607v2","created_at":"2026-07-05T02:01:13.600879+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2007.12607","created_at":"2026-07-05T02:01:13.600879+00:00"},{"alias_kind":"pith_short_12","alias_value":"3XCXCFW5BQIY","created_at":"2026-07-05T02:01:13.600879+00:00"},{"alias_kind":"pith_short_16","alias_value":"3XCXCFW5BQIYWEEU","created_at":"2026-07-05T02:01:13.600879+00:00"},{"alias_kind":"pith_short_8","alias_value":"3XCXCFW5","created_at":"2026-07-05T02:01:13.600879+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/3XCXCFW5BQIYWEEUXG54AWHZIR","json":"https://pith.science/pith/3XCXCFW5BQIYWEEUXG54AWHZIR.json","graph_json":"https://pith.science/api/pith-number/3XCXCFW5BQIYWEEUXG54AWHZIR/graph.json","events_json":"https://pith.science/api/pith-number/3XCXCFW5BQIYWEEUXG54AWHZIR/events.json","paper":"https://pith.science/paper/3XCXCFW5"},"agent_actions":{"view_html":"https://pith.science/pith/3XCXCFW5BQIYWEEUXG54AWHZIR","download_json":"https://pith.science/pith/3XCXCFW5BQIYWEEUXG54AWHZIR.json","view_paper":"https://pith.science/paper/3XCXCFW5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2007.12607&json=true","fetch_graph":"https://pith.science/api/pith-number/3XCXCFW5BQIYWEEUXG54AWHZIR/graph.json","fetch_events":"https://pith.science/api/pith-number/3XCXCFW5BQIYWEEUXG54AWHZIR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3XCXCFW5BQIYWEEUXG54AWHZIR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3XCXCFW5BQIYWEEUXG54AWHZIR/action/storage_attestation","attest_author":"https://pith.science/pith/3XCXCFW5BQIYWEEUXG54AWHZIR/action/author_attestation","sign_citation":"https://pith.science/pith/3XCXCFW5BQIYWEEUXG54AWHZIR/action/citation_signature","submit_replication":"https://pith.science/pith/3XCXCFW5BQIYWEEUXG54AWHZIR/action/replication_record"}},"created_at":"2026-07-05T02:01:13.600879+00:00","updated_at":"2026-07-05T02:01:13.600879+00:00"}