{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:XQYHVCLIHD2XIRDHHHOAVHZGLD","short_pith_number":"pith:XQYHVCLI","schema_version":"1.0","canonical_sha256":"bc307a896838f574446739dc0a9f2658f73074585919137b0ef2fae9f7f80122","source":{"kind":"arxiv","id":"1209.1296","version":1},"attestation_state":"computed","paper":{"title":"Candidates for detecting exoplanetary radio emissions generated by magnetosphere-ionosphere coupling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"J. D. Nichols","submitted_at":"2012-09-06T14:39:41Z","abstract_excerpt":"In this paper we consider the magnetosphere-ionosphere (M-I) coupling at Jupiter-like exoplanets with internal plasma sources such as volcanic moons, and we have determined the best candidates for detection of these radio emissions by estimating the maximum spectral flux density expected from planets orbiting stars within 25 pc using data listed in the NASA/IPAC/NExScI Star and Exoplanet Database (NStED). In total we identify 91 potential targets, of which 40 already host planets and 51 have stellar X-ray luminosity 100 times the solar value. In general, we find that stronger planetary field 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":"1209.1296","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2012-09-06T14:39:41Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"2abd70d69122f226083a59972c36f4243b3d6d7dbc7c565512f82a792e3d88e7","abstract_canon_sha256":"61358ede7a4b97b5ad1e6c94941677f03385f7a41fb6dece2dd2d4134eeb335d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:39.291823Z","signature_b64":"uLLN2DEW3jxh+mRHcaRFDyzzBkU2x/PphDfvFQIBCf3n8uYY0Gs3Ok+7Sxq4shqNOlCm2CgkoHEmass8lE1iAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bc307a896838f574446739dc0a9f2658f73074585919137b0ef2fae9f7f80122","last_reissued_at":"2026-05-18T01:54:39.291197Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:39.291197Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Candidates for detecting exoplanetary radio emissions generated by magnetosphere-ionosphere coupling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"J. D. Nichols","submitted_at":"2012-09-06T14:39:41Z","abstract_excerpt":"In this paper we consider the magnetosphere-ionosphere (M-I) coupling at Jupiter-like exoplanets with internal plasma sources such as volcanic moons, and we have determined the best candidates for detection of these radio emissions by estimating the maximum spectral flux density expected from planets orbiting stars within 25 pc using data listed in the NASA/IPAC/NExScI Star and Exoplanet Database (NStED). In total we identify 91 potential targets, of which 40 already host planets and 51 have stellar X-ray luminosity 100 times the solar value. In general, we find that stronger planetary field s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1209.1296","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":"1209.1296","created_at":"2026-05-18T01:54:39.291300+00:00"},{"alias_kind":"arxiv_version","alias_value":"1209.1296v1","created_at":"2026-05-18T01:54:39.291300+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1209.1296","created_at":"2026-05-18T01:54:39.291300+00:00"},{"alias_kind":"pith_short_12","alias_value":"XQYHVCLIHD2X","created_at":"2026-05-18T12:27:27.928770+00:00"},{"alias_kind":"pith_short_16","alias_value":"XQYHVCLIHD2XIRDH","created_at":"2026-05-18T12:27:27.928770+00:00"},{"alias_kind":"pith_short_8","alias_value":"XQYHVCLI","created_at":"2026-05-18T12:27:27.928770+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/XQYHVCLIHD2XIRDHHHOAVHZGLD","json":"https://pith.science/pith/XQYHVCLIHD2XIRDHHHOAVHZGLD.json","graph_json":"https://pith.science/api/pith-number/XQYHVCLIHD2XIRDHHHOAVHZGLD/graph.json","events_json":"https://pith.science/api/pith-number/XQYHVCLIHD2XIRDHHHOAVHZGLD/events.json","paper":"https://pith.science/paper/XQYHVCLI"},"agent_actions":{"view_html":"https://pith.science/pith/XQYHVCLIHD2XIRDHHHOAVHZGLD","download_json":"https://pith.science/pith/XQYHVCLIHD2XIRDHHHOAVHZGLD.json","view_paper":"https://pith.science/paper/XQYHVCLI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1209.1296&json=true","fetch_graph":"https://pith.science/api/pith-number/XQYHVCLIHD2XIRDHHHOAVHZGLD/graph.json","fetch_events":"https://pith.science/api/pith-number/XQYHVCLIHD2XIRDHHHOAVHZGLD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XQYHVCLIHD2XIRDHHHOAVHZGLD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XQYHVCLIHD2XIRDHHHOAVHZGLD/action/storage_attestation","attest_author":"https://pith.science/pith/XQYHVCLIHD2XIRDHHHOAVHZGLD/action/author_attestation","sign_citation":"https://pith.science/pith/XQYHVCLIHD2XIRDHHHOAVHZGLD/action/citation_signature","submit_replication":"https://pith.science/pith/XQYHVCLIHD2XIRDHHHOAVHZGLD/action/replication_record"}},"created_at":"2026-05-18T01:54:39.291300+00:00","updated_at":"2026-05-18T01:54:39.291300+00:00"}