{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:JWKWHTAAZHS4WS57KZ2MTFK37W","short_pith_number":"pith:JWKWHTAA","schema_version":"1.0","canonical_sha256":"4d9563cc00c9e5cb4bbf5674c9955bfdbbd1d1f5b3cc2c56e592fc15564f43b4","source":{"kind":"arxiv","id":"1503.08634","version":1},"attestation_state":"computed","paper":{"title":"Radio monitoring of the hard state jets in the 2011 outburst of MAXI J1836-194","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"(10) Oxford University, (11) U Wisconsin-Madison, (12) SRON, 13, (13) CfA, 14), (14) Radboud U, (15) NASA/GSFC, 16), (16) USRA, (17) Wheaton College, (18) U Amsterdam, (19) Cambridge, (20) U Barcelona, (21) MIT, (22) NRC, 23), (23) NRAO, (24) U Virginia, (25) ISS, (26) CSIRO), (2) U Southampton, (3) AIM/CEA-Saclay, 4), (4) Observatoire de Paris, (5) U Cape Town, (6) NYU Abu Dhabi, 7), (7) Shanghai Astronomical Observatory, (8) U Alberta, (9) INAF, A. J. Tetarenko (8), A. K. Tzioumis (26) ((1) ICRAR/Curtin University, A. Moin (6, C. L. Sarazin (24), D. Altamirano (2), D. Maitra (17), D. M. Russell (6), E. G. Kording (14), G. R. Sivakoff (8), H. A. Krimm (15, M. A. P. Torres (12, M. Coriat (5), M. Middleton (19), M. P. Rupen (22, P. A. Curran (1), P. G. Jonker (12, R. A. Remillard (21), R. P. Fender (10), R. Soria (1), S. Corbel (3, S. Heinz (11), S. Markoff (18), S. Migliari (20), T. D. Russell (1) J. C. A. Miller-Jones (1), T. J. Slaven-Blair (1), T. M. Belloni (9), V. Tudose (25)","submitted_at":"2015-03-30T10:55:56Z","abstract_excerpt":"MAXI J1836-194 is a Galactic black hole candidate X-ray binary that was discovered in 2011 when it went into outburst. In this paper, we present the full radio monitoring of this system during its `failed' outburst, in which the source did not complete a full set of state changes, only transitioning as far as the hard intermediate state. Observations with the Karl G. Jansky Very Large Array (VLA) and Australia Telescope Compact Array (ATCA) show that the jet properties changed significantly during the outburst. The VLA observations detected linearly polarised emission at a level of ~1% early 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":"1503.08634","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-03-30T10:55:56Z","cross_cats_sorted":[],"title_canon_sha256":"0d8497962bb3a6a1404eee7b3a8bbded4cd6b35696f027d7b0ebb5c2f48a115a","abstract_canon_sha256":"6e5b642580635aba173aaf159d02e9cf7332c72dcbd037687578d9d6e7c197a9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:49.519441Z","signature_b64":"PPeChsBBIJtN13ek4SBBpDA37oqZW7vXIl+N7TW4FBi/DOEkIB6+Xbcsafxsu9f7xtlIm9DDFfCh1aB+A+IzCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4d9563cc00c9e5cb4bbf5674c9955bfdbbd1d1f5b3cc2c56e592fc15564f43b4","last_reissued_at":"2026-05-18T01:40:49.518736Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:49.518736Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radio monitoring of the hard state jets in the 2011 outburst of MAXI J1836-194","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"(10) Oxford University, (11) U Wisconsin-Madison, (12) SRON, 13, (13) CfA, 14), (14) Radboud U, (15) NASA/GSFC, 16), (16) USRA, (17) Wheaton College, (18) U Amsterdam, (19) Cambridge, (20) U Barcelona, (21) MIT, (22) NRC, 23), (23) NRAO, (24) U Virginia, (25) ISS, (26) CSIRO), (2) U Southampton, (3) AIM/CEA-Saclay, 4), (4) Observatoire de Paris, (5) U Cape Town, (6) NYU Abu Dhabi, 7), (7) Shanghai Astronomical Observatory, (8) U Alberta, (9) INAF, A. J. Tetarenko (8), A. K. Tzioumis (26) ((1) ICRAR/Curtin University, A. Moin (6, C. L. Sarazin (24), D. Altamirano (2), D. Maitra (17), D. M. Russell (6), E. G. Kording (14), G. R. Sivakoff (8), H. A. Krimm (15, M. A. P. Torres (12, M. Coriat (5), M. Middleton (19), M. P. Rupen (22, P. A. Curran (1), P. G. Jonker (12, R. A. Remillard (21), R. P. Fender (10), R. Soria (1), S. Corbel (3, S. Heinz (11), S. Markoff (18), S. Migliari (20), T. D. Russell (1) J. C. A. Miller-Jones (1), T. J. Slaven-Blair (1), T. M. Belloni (9), V. Tudose (25)","submitted_at":"2015-03-30T10:55:56Z","abstract_excerpt":"MAXI J1836-194 is a Galactic black hole candidate X-ray binary that was discovered in 2011 when it went into outburst. In this paper, we present the full radio monitoring of this system during its `failed' outburst, in which the source did not complete a full set of state changes, only transitioning as far as the hard intermediate state. Observations with the Karl G. Jansky Very Large Array (VLA) and Australia Telescope Compact Array (ATCA) show that the jet properties changed significantly during the outburst. The VLA observations detected linearly polarised emission at a level of ~1% early i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1503.08634","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":""},"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":"1503.08634","created_at":"2026-05-18T01:40:49.518878+00:00"},{"alias_kind":"arxiv_version","alias_value":"1503.08634v1","created_at":"2026-05-18T01:40:49.518878+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1503.08634","created_at":"2026-05-18T01:40:49.518878+00:00"},{"alias_kind":"pith_short_12","alias_value":"JWKWHTAAZHS4","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"JWKWHTAAZHS4WS57","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"JWKWHTAA","created_at":"2026-05-18T12:29:27.538025+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/JWKWHTAAZHS4WS57KZ2MTFK37W","json":"https://pith.science/pith/JWKWHTAAZHS4WS57KZ2MTFK37W.json","graph_json":"https://pith.science/api/pith-number/JWKWHTAAZHS4WS57KZ2MTFK37W/graph.json","events_json":"https://pith.science/api/pith-number/JWKWHTAAZHS4WS57KZ2MTFK37W/events.json","paper":"https://pith.science/paper/JWKWHTAA"},"agent_actions":{"view_html":"https://pith.science/pith/JWKWHTAAZHS4WS57KZ2MTFK37W","download_json":"https://pith.science/pith/JWKWHTAAZHS4WS57KZ2MTFK37W.json","view_paper":"https://pith.science/paper/JWKWHTAA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1503.08634&json=true","fetch_graph":"https://pith.science/api/pith-number/JWKWHTAAZHS4WS57KZ2MTFK37W/graph.json","fetch_events":"https://pith.science/api/pith-number/JWKWHTAAZHS4WS57KZ2MTFK37W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JWKWHTAAZHS4WS57KZ2MTFK37W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JWKWHTAAZHS4WS57KZ2MTFK37W/action/storage_attestation","attest_author":"https://pith.science/pith/JWKWHTAAZHS4WS57KZ2MTFK37W/action/author_attestation","sign_citation":"https://pith.science/pith/JWKWHTAAZHS4WS57KZ2MTFK37W/action/citation_signature","submit_replication":"https://pith.science/pith/JWKWHTAAZHS4WS57KZ2MTFK37W/action/replication_record"}},"created_at":"2026-05-18T01:40:49.518878+00:00","updated_at":"2026-05-18T01:40:49.518878+00:00"}