{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:5HBVV6JKHYUZFQE3SL4VQL6CFN","short_pith_number":"pith:5HBVV6JK","schema_version":"1.0","canonical_sha256":"e9c35af92a3e2992c09b92f9582fc22b64742a0bf0594fc544c2cebc863b3d54","source":{"kind":"arxiv","id":"astro-ph/0109504","version":1},"attestation_state":"computed","paper":{"title":"Images of an equatorial outflow in SS433","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Amy Mioduszewski (NRAO Socorro), Katherine Blundell (Oxford), Michael Rupen (NRAO Socorro), Philipp Podsiadlowski (Oxford), Tom Muxlow (Jodrell Bank Observatory)","submitted_at":"2001-09-27T09:19:35Z","abstract_excerpt":"We have imaged the X-ray binary SS433 with unprecedented Fourier-plane coverage at 6cm using simultaneously the VLBA, MERLIN, and the VLA, and also at 20cm with the VLBA. At both wavelengths we have securely detected smooth, low-surface brightness emission having the appearance of a `ruff' or collar attached perpendicularly to the well-studied knotty jets in this system, extending over at least a few hundred AU. We interpret this smooth emission as a wind-like outflow from the binary, and discuss its implications for the present evolutionary stage of this system."},"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/0109504","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-09-27T09:19:35Z","cross_cats_sorted":[],"title_canon_sha256":"5dea93cd42d89ac3b3e3d26922ad6b53121f3b0ebccff36151c76b88fb404ffe","abstract_canon_sha256":"e268a6f97e1a9798541aafbfb3a3bce6add5b8d917d887257884baef3c6e0921"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:24:11.800185Z","signature_b64":"f+K5lqHYbzdEvLTugEWTHOlmnrvUa1m1mLBRkWQ8GB42xDEypwsfUzMq+ABzRPM9xY7yTxW9whrg1cw523umAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e9c35af92a3e2992c09b92f9582fc22b64742a0bf0594fc544c2cebc863b3d54","last_reissued_at":"2026-07-04T16:24:11.799817Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:24:11.799817Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Images of an equatorial outflow in SS433","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Amy Mioduszewski (NRAO Socorro), Katherine Blundell (Oxford), Michael Rupen (NRAO Socorro), Philipp Podsiadlowski (Oxford), Tom Muxlow (Jodrell Bank Observatory)","submitted_at":"2001-09-27T09:19:35Z","abstract_excerpt":"We have imaged the X-ray binary SS433 with unprecedented Fourier-plane coverage at 6cm using simultaneously the VLBA, MERLIN, and the VLA, and also at 20cm with the VLBA. At both wavelengths we have securely detected smooth, low-surface brightness emission having the appearance of a `ruff' or collar attached perpendicularly to the well-studied knotty jets in this system, extending over at least a few hundred AU. We interpret this smooth emission as a wind-like outflow from the binary, and discuss its implications for the present evolutionary stage of this system."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0109504","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/0109504/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/0109504","created_at":"2026-07-04T16:24:11.799879+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0109504v1","created_at":"2026-07-04T16:24:11.799879+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0109504","created_at":"2026-07-04T16:24:11.799879+00:00"},{"alias_kind":"pith_short_12","alias_value":"5HBVV6JKHYUZ","created_at":"2026-07-04T16:24:11.799879+00:00"},{"alias_kind":"pith_short_16","alias_value":"5HBVV6JKHYUZFQE3","created_at":"2026-07-04T16:24:11.799879+00:00"},{"alias_kind":"pith_short_8","alias_value":"5HBVV6JK","created_at":"2026-07-04T16:24:11.799879+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/5HBVV6JKHYUZFQE3SL4VQL6CFN","json":"https://pith.science/pith/5HBVV6JKHYUZFQE3SL4VQL6CFN.json","graph_json":"https://pith.science/api/pith-number/5HBVV6JKHYUZFQE3SL4VQL6CFN/graph.json","events_json":"https://pith.science/api/pith-number/5HBVV6JKHYUZFQE3SL4VQL6CFN/events.json","paper":"https://pith.science/paper/5HBVV6JK"},"agent_actions":{"view_html":"https://pith.science/pith/5HBVV6JKHYUZFQE3SL4VQL6CFN","download_json":"https://pith.science/pith/5HBVV6JKHYUZFQE3SL4VQL6CFN.json","view_paper":"https://pith.science/paper/5HBVV6JK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0109504&json=true","fetch_graph":"https://pith.science/api/pith-number/5HBVV6JKHYUZFQE3SL4VQL6CFN/graph.json","fetch_events":"https://pith.science/api/pith-number/5HBVV6JKHYUZFQE3SL4VQL6CFN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5HBVV6JKHYUZFQE3SL4VQL6CFN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5HBVV6JKHYUZFQE3SL4VQL6CFN/action/storage_attestation","attest_author":"https://pith.science/pith/5HBVV6JKHYUZFQE3SL4VQL6CFN/action/author_attestation","sign_citation":"https://pith.science/pith/5HBVV6JKHYUZFQE3SL4VQL6CFN/action/citation_signature","submit_replication":"https://pith.science/pith/5HBVV6JKHYUZFQE3SL4VQL6CFN/action/replication_record"}},"created_at":"2026-07-04T16:24:11.799879+00:00","updated_at":"2026-07-04T16:24:11.799879+00:00"}