{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:5Z2E2TR64KCFI2DVA7UJWRGVKZ","short_pith_number":"pith:5Z2E2TR6","schema_version":"1.0","canonical_sha256":"ee744d4e3ee28454687507e89b44d5564adcfac3329e3fc9727fb54f043e1c7a","source":{"kind":"arxiv","id":"2107.13019","version":1},"attestation_state":"computed","paper":{"title":"A broadband radio view of transient jet ejecta in the black hole candidate X-ray binary MAXI J1535-571","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bahramian, A. Paduano, C. Flynn, C. M. Trott, D. Altamirano, D. L. Kaplan, G. E. Anderson, G. R. Sivakoff, H. A. Krimm, J. C. A. Miller-Jones, J. Chauhan, M. Johnston-Hollitt, M. Sokolowski, N. Hurley-Walker, P. J. Hancock, R. B. Wayth, R. Soria, S. Croft, S. J. Tingay, S. W. Duchesne, T. D. Russell, V. Gupta","submitted_at":"2021-07-27T18:00:47Z","abstract_excerpt":"We present a broadband radio study of the transient jets ejected from the black hole candidate X-ray binary MAXI J1535-571, which underwent a prolonged outburst beginning on 2 September 2017. We monitored MAXI J1535-571 with the Murchison Widefield Array (MWA) at frequencies from 119 to 186 MHz over six epochs from 20 September to 14 October 2017. The source was quasi-simultaneously observed over the frequency range 0.84-19 GHz by UTMOST (the upgraded Molonglo Observatory Synthesis Telescope), the Australian Square Kilometre Array Pathfinder, the Australia Telescope Compact Array (ATCA), and t"},"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":"2107.13019","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2021-07-27T18:00:47Z","cross_cats_sorted":[],"title_canon_sha256":"d99ac09960b0aa2291f65bc026104d2b678b0d680916da26b0e9bd07f230bc78","abstract_canon_sha256":"7f8b32d5ecfc1a6692ed59155c5a857ddc5843901dd66bd18eba73322217151d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:14:24.214792Z","signature_b64":"hEM/nONFpRqVRGQkLC6wuQs2/9PT1h1eE211CAf23c+NdlrA9w5QaOs4RipQu+kEa4ggeGWKwdlIDLLtPWGYAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ee744d4e3ee28454687507e89b44d5564adcfac3329e3fc9727fb54f043e1c7a","last_reissued_at":"2026-07-05T03:14:24.214354Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:14:24.214354Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A broadband radio view of transient jet ejecta in the black hole candidate X-ray binary MAXI J1535-571","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bahramian, A. Paduano, C. Flynn, C. M. Trott, D. Altamirano, D. L. Kaplan, G. E. Anderson, G. R. Sivakoff, H. A. Krimm, J. C. A. Miller-Jones, J. Chauhan, M. Johnston-Hollitt, M. Sokolowski, N. Hurley-Walker, P. J. Hancock, R. B. Wayth, R. Soria, S. Croft, S. J. Tingay, S. W. Duchesne, T. D. Russell, V. Gupta","submitted_at":"2021-07-27T18:00:47Z","abstract_excerpt":"We present a broadband radio study of the transient jets ejected from the black hole candidate X-ray binary MAXI J1535-571, which underwent a prolonged outburst beginning on 2 September 2017. We monitored MAXI J1535-571 with the Murchison Widefield Array (MWA) at frequencies from 119 to 186 MHz over six epochs from 20 September to 14 October 2017. The source was quasi-simultaneously observed over the frequency range 0.84-19 GHz by UTMOST (the upgraded Molonglo Observatory Synthesis Telescope), the Australian Square Kilometre Array Pathfinder, the Australia Telescope Compact Array (ATCA), and t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2107.13019","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/2107.13019/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":"2107.13019","created_at":"2026-07-05T03:14:24.214411+00:00"},{"alias_kind":"arxiv_version","alias_value":"2107.13019v1","created_at":"2026-07-05T03:14:24.214411+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2107.13019","created_at":"2026-07-05T03:14:24.214411+00:00"},{"alias_kind":"pith_short_12","alias_value":"5Z2E2TR64KCF","created_at":"2026-07-05T03:14:24.214411+00:00"},{"alias_kind":"pith_short_16","alias_value":"5Z2E2TR64KCFI2DV","created_at":"2026-07-05T03:14:24.214411+00:00"},{"alias_kind":"pith_short_8","alias_value":"5Z2E2TR6","created_at":"2026-07-05T03:14:24.214411+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.03024","citing_title":"Rapid Response Triggering for Radio Transients with the SKA Observatory","ref_index":97,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ","json":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ.json","graph_json":"https://pith.science/api/pith-number/5Z2E2TR64KCFI2DVA7UJWRGVKZ/graph.json","events_json":"https://pith.science/api/pith-number/5Z2E2TR64KCFI2DVA7UJWRGVKZ/events.json","paper":"https://pith.science/paper/5Z2E2TR6"},"agent_actions":{"view_html":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ","download_json":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ.json","view_paper":"https://pith.science/paper/5Z2E2TR6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2107.13019&json=true","fetch_graph":"https://pith.science/api/pith-number/5Z2E2TR64KCFI2DVA7UJWRGVKZ/graph.json","fetch_events":"https://pith.science/api/pith-number/5Z2E2TR64KCFI2DVA7UJWRGVKZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ/action/storage_attestation","attest_author":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ/action/author_attestation","sign_citation":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ/action/citation_signature","submit_replication":"https://pith.science/pith/5Z2E2TR64KCFI2DVA7UJWRGVKZ/action/replication_record"}},"created_at":"2026-07-05T03:14:24.214411+00:00","updated_at":"2026-07-05T03:14:24.214411+00:00"}