{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:LXQJKS6OLWGANCP2OTIJHDPJNZ","short_pith_number":"pith:LXQJKS6O","schema_version":"1.0","canonical_sha256":"5de0954bce5d8c0689fa74d0938de96e76c23e63ff1e60ad8507f3e5cf9cce10","source":{"kind":"arxiv","id":"2207.00470","version":1},"attestation_state":"computed","paper":{"title":"What leads to premature upper cut-off frequencies of auroral radio emission from hot magnetic stars?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Das, P. Chandra, V. Petit","submitted_at":"2022-07-01T14:50:50Z","abstract_excerpt":"Recently a large number of hot magnetic stars have been discovered to produce auroral radio emission by the process of electron cyclotron maser emission (ECME). Such stars have been given the name of Main-sequence Radio Pulse emitters (MRPs). The phenomenon characterizing MRPs is very similar to that exhibited by planets like the Jupiter. However, one important aspect in which the MRPs differ from aurorae exhibited by planets is the upper cut-off frequency of the ECME spectrum. While Jupiter's upper cut-off frequency was found to correspond to its maximum surface magnetic field strength, the s"},"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":"2207.00470","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2022-07-01T14:50:50Z","cross_cats_sorted":[],"title_canon_sha256":"c655700754efb1daf1fb1ab00f1d3481d0517cbf251afe999543f65ddf10ed02","abstract_canon_sha256":"a81571326e92b104a0639928cbbd0e1d3ca26158923604d79b393b4417c39105"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:45:24.641149Z","signature_b64":"RVBprQxstYNwwUm7hH11hn3sqgHMSiGYYh9+HxuICHlnIdHUT2VSuzddFHFtYmkGTF4GIiE70am+CUqXu2TkCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5de0954bce5d8c0689fa74d0938de96e76c23e63ff1e60ad8507f3e5cf9cce10","last_reissued_at":"2026-07-05T04:45:24.640741Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:45:24.640741Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"What leads to premature upper cut-off frequencies of auroral radio emission from hot magnetic stars?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Das, P. Chandra, V. Petit","submitted_at":"2022-07-01T14:50:50Z","abstract_excerpt":"Recently a large number of hot magnetic stars have been discovered to produce auroral radio emission by the process of electron cyclotron maser emission (ECME). Such stars have been given the name of Main-sequence Radio Pulse emitters (MRPs). The phenomenon characterizing MRPs is very similar to that exhibited by planets like the Jupiter. However, one important aspect in which the MRPs differ from aurorae exhibited by planets is the upper cut-off frequency of the ECME spectrum. While Jupiter's upper cut-off frequency was found to correspond to its maximum surface magnetic field strength, the s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2207.00470","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/2207.00470/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":"2207.00470","created_at":"2026-07-05T04:45:24.640798+00:00"},{"alias_kind":"arxiv_version","alias_value":"2207.00470v1","created_at":"2026-07-05T04:45:24.640798+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2207.00470","created_at":"2026-07-05T04:45:24.640798+00:00"},{"alias_kind":"pith_short_12","alias_value":"LXQJKS6OLWGA","created_at":"2026-07-05T04:45:24.640798+00:00"},{"alias_kind":"pith_short_16","alias_value":"LXQJKS6OLWGANCP2","created_at":"2026-07-05T04:45:24.640798+00:00"},{"alias_kind":"pith_short_8","alias_value":"LXQJKS6O","created_at":"2026-07-05T04:45:24.640798+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/LXQJKS6OLWGANCP2OTIJHDPJNZ","json":"https://pith.science/pith/LXQJKS6OLWGANCP2OTIJHDPJNZ.json","graph_json":"https://pith.science/api/pith-number/LXQJKS6OLWGANCP2OTIJHDPJNZ/graph.json","events_json":"https://pith.science/api/pith-number/LXQJKS6OLWGANCP2OTIJHDPJNZ/events.json","paper":"https://pith.science/paper/LXQJKS6O"},"agent_actions":{"view_html":"https://pith.science/pith/LXQJKS6OLWGANCP2OTIJHDPJNZ","download_json":"https://pith.science/pith/LXQJKS6OLWGANCP2OTIJHDPJNZ.json","view_paper":"https://pith.science/paper/LXQJKS6O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2207.00470&json=true","fetch_graph":"https://pith.science/api/pith-number/LXQJKS6OLWGANCP2OTIJHDPJNZ/graph.json","fetch_events":"https://pith.science/api/pith-number/LXQJKS6OLWGANCP2OTIJHDPJNZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LXQJKS6OLWGANCP2OTIJHDPJNZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LXQJKS6OLWGANCP2OTIJHDPJNZ/action/storage_attestation","attest_author":"https://pith.science/pith/LXQJKS6OLWGANCP2OTIJHDPJNZ/action/author_attestation","sign_citation":"https://pith.science/pith/LXQJKS6OLWGANCP2OTIJHDPJNZ/action/citation_signature","submit_replication":"https://pith.science/pith/LXQJKS6OLWGANCP2OTIJHDPJNZ/action/replication_record"}},"created_at":"2026-07-05T04:45:24.640798+00:00","updated_at":"2026-07-05T04:45:24.640798+00:00"}