{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:4E3QHIV6EMPFYBFALZITYT77CP","short_pith_number":"pith:4E3QHIV6","schema_version":"1.0","canonical_sha256":"e13703a2be231e5c04a05e513c4fff13f4e1c3c18d956fdd9ca3df0c712cd5f2","source":{"kind":"arxiv","id":"2605.28662","version":1},"attestation_state":"computed","paper":{"title":"Testing cosmic anisotropy with the Combo correlation of gamma-ray bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Dong Zhao, Hao-Ran Duan, Jun-Qing Xia","submitted_at":"2026-05-27T15:58:58Z","abstract_excerpt":"We employ the sample of 244 gamma-ray bursts (GRBs; i.e., C244) with the Combo correlation to test cosmic anisotropy. Meanwhile, the Pantheon sample is introduced to verify whether the GRB sample can suppress the fake anisotropic signals induced by inhomogeneous spatial distributions. In the dipole fitting (DF) method, under the dipole-modulated $\\Lambda$CDM model, the C244 sample shifts the best-fitting longitude $l$ derived from the Pantheon sample by $54.09^\\circ$ and reduces the uncertainty in $l$ by approximately $40\\%$. Compared to the 118 GRBs (i.e., A118) with the $E_\\mathrm{p}$-$E_\\ma"},"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":"2605.28662","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-27T15:58:58Z","cross_cats_sorted":[],"title_canon_sha256":"cc5a7160b1b6aa5b3c8bfb833351342f942eaf86400026d9830fac8eb3a3eecc","abstract_canon_sha256":"d25bfd5c5bccce52d3209a22c738488822795b6e66b145143b7c50d4f208199b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-28T02:04:59.200294Z","signature_b64":"rPKJZ7cGWc8XyIAnE/EqW20NjPBxDrQQbD+fgGx0fe+Z9tVMByEAclXUEqqkhf7GNlm4zA031EeTkAUvjTncCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e13703a2be231e5c04a05e513c4fff13f4e1c3c18d956fdd9ca3df0c712cd5f2","last_reissued_at":"2026-05-28T02:04:59.199877Z","signature_status":"signed_v1","first_computed_at":"2026-05-28T02:04:59.199877Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing cosmic anisotropy with the Combo correlation of gamma-ray bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Dong Zhao, Hao-Ran Duan, Jun-Qing Xia","submitted_at":"2026-05-27T15:58:58Z","abstract_excerpt":"We employ the sample of 244 gamma-ray bursts (GRBs; i.e., C244) with the Combo correlation to test cosmic anisotropy. Meanwhile, the Pantheon sample is introduced to verify whether the GRB sample can suppress the fake anisotropic signals induced by inhomogeneous spatial distributions. In the dipole fitting (DF) method, under the dipole-modulated $\\Lambda$CDM model, the C244 sample shifts the best-fitting longitude $l$ derived from the Pantheon sample by $54.09^\\circ$ and reduces the uncertainty in $l$ by approximately $40\\%$. Compared to the 118 GRBs (i.e., A118) with the $E_\\mathrm{p}$-$E_\\ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.28662","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/2605.28662/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":"2605.28662","created_at":"2026-05-28T02:04:59.199940+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.28662v1","created_at":"2026-05-28T02:04:59.199940+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.28662","created_at":"2026-05-28T02:04:59.199940+00:00"},{"alias_kind":"pith_short_12","alias_value":"4E3QHIV6EMPF","created_at":"2026-05-28T02:04:59.199940+00:00"},{"alias_kind":"pith_short_16","alias_value":"4E3QHIV6EMPFYBFA","created_at":"2026-05-28T02:04:59.199940+00:00"},{"alias_kind":"pith_short_8","alias_value":"4E3QHIV6","created_at":"2026-05-28T02:04:59.199940+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/4E3QHIV6EMPFYBFALZITYT77CP","json":"https://pith.science/pith/4E3QHIV6EMPFYBFALZITYT77CP.json","graph_json":"https://pith.science/api/pith-number/4E3QHIV6EMPFYBFALZITYT77CP/graph.json","events_json":"https://pith.science/api/pith-number/4E3QHIV6EMPFYBFALZITYT77CP/events.json","paper":"https://pith.science/paper/4E3QHIV6"},"agent_actions":{"view_html":"https://pith.science/pith/4E3QHIV6EMPFYBFALZITYT77CP","download_json":"https://pith.science/pith/4E3QHIV6EMPFYBFALZITYT77CP.json","view_paper":"https://pith.science/paper/4E3QHIV6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.28662&json=true","fetch_graph":"https://pith.science/api/pith-number/4E3QHIV6EMPFYBFALZITYT77CP/graph.json","fetch_events":"https://pith.science/api/pith-number/4E3QHIV6EMPFYBFALZITYT77CP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4E3QHIV6EMPFYBFALZITYT77CP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4E3QHIV6EMPFYBFALZITYT77CP/action/storage_attestation","attest_author":"https://pith.science/pith/4E3QHIV6EMPFYBFALZITYT77CP/action/author_attestation","sign_citation":"https://pith.science/pith/4E3QHIV6EMPFYBFALZITYT77CP/action/citation_signature","submit_replication":"https://pith.science/pith/4E3QHIV6EMPFYBFALZITYT77CP/action/replication_record"}},"created_at":"2026-05-28T02:04:59.199940+00:00","updated_at":"2026-05-28T02:04:59.199940+00:00"}