{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:QHGDFYPMFZQQUPMHGKCPYUXPWC","short_pith_number":"pith:QHGDFYPM","schema_version":"1.0","canonical_sha256":"81cc32e1ec2e610a3d873284fc52efb099e6e5cc7438f63f08beacfc85b6c14b","source":{"kind":"arxiv","id":"2509.10275","version":1},"attestation_state":"computed","paper":{"title":"A MeerKAT view of the parsec-scale jets in the black-hole X-ray binary GRS 1758-258","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"I. Heywood, I. Mariani, J.H. Matthews, J. Mart\\'i, P. Atri, P. L. Luque-Escamilla, R.P. Fender, S.E. Motta","submitted_at":"2025-09-12T14:18:32Z","abstract_excerpt":"Jets from accreting black hole (BH) X-ray binaries (XRBs) are powerful outflows that release a large fraction of the accretion energy to the surrounding environment, providing a feedback mechanism that may alter the interstellar medium (ISM) properties. Studying accretion and feedback together enables estimates of matter and energy input/output around accreting BHs. We focus on the extended jet structures of the BH-XRB GRS1758-258. First seen in VLA data, these parsec-scale jets arise from jet-ISM interaction and show a Z-shaped morphology. Using the MeerKAT telescope we observed GRS1758-258 i"},"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":"2509.10275","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-09-12T14:18:32Z","cross_cats_sorted":[],"title_canon_sha256":"f653cd711e07fa6b5ea8f3e24db2e3fddc1cf212add4c8cc1012cba14d17845c","abstract_canon_sha256":"57395c26c52a80ce4b7b395231a096868cce7001238c71182012d853f7523396"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T12:11:06.127597Z","signature_b64":"lWwAdMsXob9Cb26dD6k94XxYf7On75AfkuTopBKLgUdqZG1mQW/qeY7cci+b2h5HSSAyqjYLHq8gcanJRIjLDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"81cc32e1ec2e610a3d873284fc52efb099e6e5cc7438f63f08beacfc85b6c14b","last_reissued_at":"2026-07-05T12:11:06.127032Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T12:11:06.127032Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A MeerKAT view of the parsec-scale jets in the black-hole X-ray binary GRS 1758-258","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"I. Heywood, I. Mariani, J.H. Matthews, J. Mart\\'i, P. Atri, P. L. Luque-Escamilla, R.P. Fender, S.E. Motta","submitted_at":"2025-09-12T14:18:32Z","abstract_excerpt":"Jets from accreting black hole (BH) X-ray binaries (XRBs) are powerful outflows that release a large fraction of the accretion energy to the surrounding environment, providing a feedback mechanism that may alter the interstellar medium (ISM) properties. Studying accretion and feedback together enables estimates of matter and energy input/output around accreting BHs. We focus on the extended jet structures of the BH-XRB GRS1758-258. First seen in VLA data, these parsec-scale jets arise from jet-ISM interaction and show a Z-shaped morphology. Using the MeerKAT telescope we observed GRS1758-258 i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2509.10275","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/2509.10275/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":"2509.10275","created_at":"2026-07-05T12:11:06.127094+00:00"},{"alias_kind":"arxiv_version","alias_value":"2509.10275v1","created_at":"2026-07-05T12:11:06.127094+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2509.10275","created_at":"2026-07-05T12:11:06.127094+00:00"},{"alias_kind":"pith_short_12","alias_value":"QHGDFYPMFZQQ","created_at":"2026-07-05T12:11:06.127094+00:00"},{"alias_kind":"pith_short_16","alias_value":"QHGDFYPMFZQQUPMH","created_at":"2026-07-05T12:11:06.127094+00:00"},{"alias_kind":"pith_short_8","alias_value":"QHGDFYPM","created_at":"2026-07-05T12:11:06.127094+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/QHGDFYPMFZQQUPMHGKCPYUXPWC","json":"https://pith.science/pith/QHGDFYPMFZQQUPMHGKCPYUXPWC.json","graph_json":"https://pith.science/api/pith-number/QHGDFYPMFZQQUPMHGKCPYUXPWC/graph.json","events_json":"https://pith.science/api/pith-number/QHGDFYPMFZQQUPMHGKCPYUXPWC/events.json","paper":"https://pith.science/paper/QHGDFYPM"},"agent_actions":{"view_html":"https://pith.science/pith/QHGDFYPMFZQQUPMHGKCPYUXPWC","download_json":"https://pith.science/pith/QHGDFYPMFZQQUPMHGKCPYUXPWC.json","view_paper":"https://pith.science/paper/QHGDFYPM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2509.10275&json=true","fetch_graph":"https://pith.science/api/pith-number/QHGDFYPMFZQQUPMHGKCPYUXPWC/graph.json","fetch_events":"https://pith.science/api/pith-number/QHGDFYPMFZQQUPMHGKCPYUXPWC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QHGDFYPMFZQQUPMHGKCPYUXPWC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QHGDFYPMFZQQUPMHGKCPYUXPWC/action/storage_attestation","attest_author":"https://pith.science/pith/QHGDFYPMFZQQUPMHGKCPYUXPWC/action/author_attestation","sign_citation":"https://pith.science/pith/QHGDFYPMFZQQUPMHGKCPYUXPWC/action/citation_signature","submit_replication":"https://pith.science/pith/QHGDFYPMFZQQUPMHGKCPYUXPWC/action/replication_record"}},"created_at":"2026-07-05T12:11:06.127094+00:00","updated_at":"2026-07-05T12:11:06.127094+00:00"}