{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:NCDPQANYKWA2LZAHGIAKR4LYKW","short_pith_number":"pith:NCDPQANY","schema_version":"1.0","canonical_sha256":"6886f801b85581a5e4073200a8f17855883fb3e6795f4df1b556dc60c6be0b82","source":{"kind":"arxiv","id":"2110.00586","version":1},"attestation_state":"computed","paper":{"title":"The MAVERIC Survey: Variable Jet-Accretion Coupling in Luminous Accreting Neutron Stars in Galactic Globular Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bahramian, C. O. Heinke, E. Tremou, G. R. Sivakoff, J. C. A. Miller-Jones, J. Strader, L. Chomiuk, L. Shishkovsky, R. Urquhart, T. J. Maccarone, T. Panurach, V. Tudor","submitted_at":"2021-10-01T18:00:01Z","abstract_excerpt":"Accreting neutron stars in low-mass X-ray binaries show outflows -- and sometimes jets -- in the general manner of accreting black holes. However, the quantitative link between the accretion flow (traced by X-rays) and outflows and/or jets (traced by radio emission) is much less well-understood for neutron stars than for black holes, other than the general observation that neutron stars are fainter in the radio at a given X-ray luminosity. We use data from the deep MAVERIC radio continuum survey of Galactic globular clusters for a systematic radio and X-ray study of six luminous (L_X > 10^34 e"},"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":"2110.00586","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2021-10-01T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"a4d4294de3c414eb3602d55fe04cb01a3413434393b37e48a7bcb51f414fb9df","abstract_canon_sha256":"f78fe587dd6c7a14b36a2c682c3c12cafd1aff7de9e674b9d6903dde83c6904b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:42:50.615033Z","signature_b64":"cyy5c3YXhNNveX0lxhBDCgxFY6nOYtFLFnR6YCKI7mdTp8pWD0zuCIdzPmPX7pcoib2lnDDejDgiXz+eBb4LAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6886f801b85581a5e4073200a8f17855883fb3e6795f4df1b556dc60c6be0b82","last_reissued_at":"2026-07-05T03:42:50.614570Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:42:50.614570Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The MAVERIC Survey: Variable Jet-Accretion Coupling in Luminous Accreting Neutron Stars in Galactic Globular Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bahramian, C. O. Heinke, E. Tremou, G. R. Sivakoff, J. C. A. Miller-Jones, J. Strader, L. Chomiuk, L. Shishkovsky, R. Urquhart, T. J. Maccarone, T. Panurach, V. Tudor","submitted_at":"2021-10-01T18:00:01Z","abstract_excerpt":"Accreting neutron stars in low-mass X-ray binaries show outflows -- and sometimes jets -- in the general manner of accreting black holes. However, the quantitative link between the accretion flow (traced by X-rays) and outflows and/or jets (traced by radio emission) is much less well-understood for neutron stars than for black holes, other than the general observation that neutron stars are fainter in the radio at a given X-ray luminosity. We use data from the deep MAVERIC radio continuum survey of Galactic globular clusters for a systematic radio and X-ray study of six luminous (L_X > 10^34 e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2110.00586","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/2110.00586/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":"2110.00586","created_at":"2026-07-05T03:42:50.614640+00:00"},{"alias_kind":"arxiv_version","alias_value":"2110.00586v1","created_at":"2026-07-05T03:42:50.614640+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2110.00586","created_at":"2026-07-05T03:42:50.614640+00:00"},{"alias_kind":"pith_short_12","alias_value":"NCDPQANYKWA2","created_at":"2026-07-05T03:42:50.614640+00:00"},{"alias_kind":"pith_short_16","alias_value":"NCDPQANYKWA2LZAH","created_at":"2026-07-05T03:42:50.614640+00:00"},{"alias_kind":"pith_short_8","alias_value":"NCDPQANY","created_at":"2026-07-05T03:42:50.614640+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/NCDPQANYKWA2LZAHGIAKR4LYKW","json":"https://pith.science/pith/NCDPQANYKWA2LZAHGIAKR4LYKW.json","graph_json":"https://pith.science/api/pith-number/NCDPQANYKWA2LZAHGIAKR4LYKW/graph.json","events_json":"https://pith.science/api/pith-number/NCDPQANYKWA2LZAHGIAKR4LYKW/events.json","paper":"https://pith.science/paper/NCDPQANY"},"agent_actions":{"view_html":"https://pith.science/pith/NCDPQANYKWA2LZAHGIAKR4LYKW","download_json":"https://pith.science/pith/NCDPQANYKWA2LZAHGIAKR4LYKW.json","view_paper":"https://pith.science/paper/NCDPQANY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2110.00586&json=true","fetch_graph":"https://pith.science/api/pith-number/NCDPQANYKWA2LZAHGIAKR4LYKW/graph.json","fetch_events":"https://pith.science/api/pith-number/NCDPQANYKWA2LZAHGIAKR4LYKW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NCDPQANYKWA2LZAHGIAKR4LYKW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NCDPQANYKWA2LZAHGIAKR4LYKW/action/storage_attestation","attest_author":"https://pith.science/pith/NCDPQANYKWA2LZAHGIAKR4LYKW/action/author_attestation","sign_citation":"https://pith.science/pith/NCDPQANYKWA2LZAHGIAKR4LYKW/action/citation_signature","submit_replication":"https://pith.science/pith/NCDPQANYKWA2LZAHGIAKR4LYKW/action/replication_record"}},"created_at":"2026-07-05T03:42:50.614640+00:00","updated_at":"2026-07-05T03:42:50.614640+00:00"}