{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:UJ3AENGEAP3Q3FAIXOYPQUXMVM","short_pith_number":"pith:UJ3AENGE","schema_version":"1.0","canonical_sha256":"a2760234c403f70d9408bbb0f852ecab19228b1911d3094a8460079015303a9f","source":{"kind":"arxiv","id":"1210.4257","version":2},"attestation_state":"computed","paper":{"title":"WASP-64b and WASP-72b: two new transiting highly irradiated giant planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Collier-Cameron, A. Fumel, A. H. M. J. Triaud, A. M. S. Smith, A. P. Doyle, B. Smalley, C. Hellier, D. Pollacco, D. Queloz, D. R. Anderson, D. Segransan, E. Jehin, F. Pepe, J. Montalban, J. Southworth, M. Gillon, M. Lendl, P. F. L. Maxted, R. G. West, S. Udry","submitted_at":"2012-10-16T06:12:10Z","abstract_excerpt":"We report the discovery by the WASP transit survey of two new highly irradiated giant planets transiting moderately bright stars. WASP-64b is slightly more massive (1.271+-0.068 M_Jup) and larger (1.271+-0.039 R_Jup) than Jupiter, and is in very-short (a=0.02648+-0.00024 AU, P=1.5732918+-0.0000015 days) circular orbit around a V=12.3 G7-type dwarf (1.004+-0.028 M_Sun, 1.058+-0.025 R_Sun, Teff=5500+-150 K). Its size is typical of hot Jupiters with similar masses. WASP-72b has also a mass a bit higher than Jupiter's (1.461-0.056+0.059 M_Jup) and orbits very close (0.03708+-0.00050 AU, P=2.216742"},"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":"1210.4257","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2012-10-16T06:12:10Z","cross_cats_sorted":[],"title_canon_sha256":"68c9f257d05b45a3e24d1bbaa646335c96b951f6d1be3b6f5ef6c67c4b20bb57","abstract_canon_sha256":"de7c0ae1adb1f5c23536f90339a47bde2d752f4427d96f3a9dc0641020adafe4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:54.699988Z","signature_b64":"rlVUU+yb0nxoNdk0q2v3dBObzQfsexExIfZfPlo3ObgeXxMhytccwgHY8VgE//xMZew0mje8zsGz24QV0KSMBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a2760234c403f70d9408bbb0f852ecab19228b1911d3094a8460079015303a9f","last_reissued_at":"2026-05-18T01:53:54.699404Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:54.699404Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"WASP-64b and WASP-72b: two new transiting highly irradiated giant planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Collier-Cameron, A. Fumel, A. H. M. J. Triaud, A. M. S. Smith, A. P. Doyle, B. Smalley, C. Hellier, D. Pollacco, D. Queloz, D. R. Anderson, D. Segransan, E. Jehin, F. Pepe, J. Montalban, J. Southworth, M. Gillon, M. Lendl, P. F. L. Maxted, R. G. West, S. Udry","submitted_at":"2012-10-16T06:12:10Z","abstract_excerpt":"We report the discovery by the WASP transit survey of two new highly irradiated giant planets transiting moderately bright stars. WASP-64b is slightly more massive (1.271+-0.068 M_Jup) and larger (1.271+-0.039 R_Jup) than Jupiter, and is in very-short (a=0.02648+-0.00024 AU, P=1.5732918+-0.0000015 days) circular orbit around a V=12.3 G7-type dwarf (1.004+-0.028 M_Sun, 1.058+-0.025 R_Sun, Teff=5500+-150 K). Its size is typical of hot Jupiters with similar masses. WASP-72b has also a mass a bit higher than Jupiter's (1.461-0.056+0.059 M_Jup) and orbits very close (0.03708+-0.00050 AU, P=2.216742"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.4257","kind":"arxiv","version":2},"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":"1210.4257","created_at":"2026-05-18T01:53:54.699509+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.4257v2","created_at":"2026-05-18T01:53:54.699509+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.4257","created_at":"2026-05-18T01:53:54.699509+00:00"},{"alias_kind":"pith_short_12","alias_value":"UJ3AENGEAP3Q","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_16","alias_value":"UJ3AENGEAP3Q3FAI","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_8","alias_value":"UJ3AENGE","created_at":"2026-05-18T12:27:23.164592+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/UJ3AENGEAP3Q3FAIXOYPQUXMVM","json":"https://pith.science/pith/UJ3AENGEAP3Q3FAIXOYPQUXMVM.json","graph_json":"https://pith.science/api/pith-number/UJ3AENGEAP3Q3FAIXOYPQUXMVM/graph.json","events_json":"https://pith.science/api/pith-number/UJ3AENGEAP3Q3FAIXOYPQUXMVM/events.json","paper":"https://pith.science/paper/UJ3AENGE"},"agent_actions":{"view_html":"https://pith.science/pith/UJ3AENGEAP3Q3FAIXOYPQUXMVM","download_json":"https://pith.science/pith/UJ3AENGEAP3Q3FAIXOYPQUXMVM.json","view_paper":"https://pith.science/paper/UJ3AENGE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.4257&json=true","fetch_graph":"https://pith.science/api/pith-number/UJ3AENGEAP3Q3FAIXOYPQUXMVM/graph.json","fetch_events":"https://pith.science/api/pith-number/UJ3AENGEAP3Q3FAIXOYPQUXMVM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UJ3AENGEAP3Q3FAIXOYPQUXMVM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UJ3AENGEAP3Q3FAIXOYPQUXMVM/action/storage_attestation","attest_author":"https://pith.science/pith/UJ3AENGEAP3Q3FAIXOYPQUXMVM/action/author_attestation","sign_citation":"https://pith.science/pith/UJ3AENGEAP3Q3FAIXOYPQUXMVM/action/citation_signature","submit_replication":"https://pith.science/pith/UJ3AENGEAP3Q3FAIXOYPQUXMVM/action/replication_record"}},"created_at":"2026-05-18T01:53:54.699509+00:00","updated_at":"2026-05-18T01:53:54.699509+00:00"}