{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:IORIUVXMZ2YTQY5MRQ2ARZ2YAV","short_pith_number":"pith:IORIUVXM","schema_version":"1.0","canonical_sha256":"43a28a56ecceb13863ac8c3408e758057ca49d459bb0aa7a70a83d673dccfd43","source":{"kind":"arxiv","id":"astro-ph/0207551","version":1},"attestation_state":"computed","paper":{"title":"On the correlation between radio and X-ray flux in Low/Hard state Black Holes","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. Gallo, G. Pooley, R. Fender","submitted_at":"2002-07-25T14:14:42Z","abstract_excerpt":"Radio emission from X-ray binary systems (XRBs) has developed in recent years from being peculiar phenomenon to being recognised as an ubiquitous property of several classes of XRBs. In this scenario the synchrotron emission is interpreted as the radiative signature of jet-like outflows, some or all of which may possess relativistic bulk motion. We have analysed a collection of quasi-simultaneous radio/X-ray observations of Black Holes in the Low/Hard X-ray state, finding evidence of a clear correlation between their fluxes over many orders of magnitude in luminosity. Given that the correlatio"},"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":"astro-ph/0207551","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2002-07-25T14:14:42Z","cross_cats_sorted":[],"title_canon_sha256":"8c1851c05a95ab68d9e52fc9feeaf26f2a8c41b6f337b287b437ca567756604c","abstract_canon_sha256":"63cc2e67b82087e2efa17b6399b6040cc334230b3b9f1a52ec224cf6c9397775"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:12:07.847987Z","signature_b64":"XBokfP8OIlEt2b/RTfN8sO3ciR6QVgKQq4tEMW2Z0P6g/mtx5qQQ1BcS96GOH16Sep34PqnAVShtx0u/JQogDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"43a28a56ecceb13863ac8c3408e758057ca49d459bb0aa7a70a83d673dccfd43","last_reissued_at":"2026-07-04T14:12:07.847648Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:12:07.847648Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the correlation between radio and X-ray flux in Low/Hard state Black Holes","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. Gallo, G. Pooley, R. Fender","submitted_at":"2002-07-25T14:14:42Z","abstract_excerpt":"Radio emission from X-ray binary systems (XRBs) has developed in recent years from being peculiar phenomenon to being recognised as an ubiquitous property of several classes of XRBs. In this scenario the synchrotron emission is interpreted as the radiative signature of jet-like outflows, some or all of which may possess relativistic bulk motion. We have analysed a collection of quasi-simultaneous radio/X-ray observations of Black Holes in the Low/Hard X-ray state, finding evidence of a clear correlation between their fluxes over many orders of magnitude in luminosity. Given that the correlatio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0207551","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/astro-ph/0207551/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":"astro-ph/0207551","created_at":"2026-07-04T14:12:07.847704+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0207551v1","created_at":"2026-07-04T14:12:07.847704+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0207551","created_at":"2026-07-04T14:12:07.847704+00:00"},{"alias_kind":"pith_short_12","alias_value":"IORIUVXMZ2YT","created_at":"2026-07-04T14:12:07.847704+00:00"},{"alias_kind":"pith_short_16","alias_value":"IORIUVXMZ2YTQY5M","created_at":"2026-07-04T14:12:07.847704+00:00"},{"alias_kind":"pith_short_8","alias_value":"IORIUVXM","created_at":"2026-07-04T14:12:07.847704+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/IORIUVXMZ2YTQY5MRQ2ARZ2YAV","json":"https://pith.science/pith/IORIUVXMZ2YTQY5MRQ2ARZ2YAV.json","graph_json":"https://pith.science/api/pith-number/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/graph.json","events_json":"https://pith.science/api/pith-number/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/events.json","paper":"https://pith.science/paper/IORIUVXM"},"agent_actions":{"view_html":"https://pith.science/pith/IORIUVXMZ2YTQY5MRQ2ARZ2YAV","download_json":"https://pith.science/pith/IORIUVXMZ2YTQY5MRQ2ARZ2YAV.json","view_paper":"https://pith.science/paper/IORIUVXM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0207551&json=true","fetch_graph":"https://pith.science/api/pith-number/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/graph.json","fetch_events":"https://pith.science/api/pith-number/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/action/storage_attestation","attest_author":"https://pith.science/pith/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/action/author_attestation","sign_citation":"https://pith.science/pith/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/action/citation_signature","submit_replication":"https://pith.science/pith/IORIUVXMZ2YTQY5MRQ2ARZ2YAV/action/replication_record"}},"created_at":"2026-07-04T14:12:07.847704+00:00","updated_at":"2026-07-04T14:12:07.847704+00:00"}