{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:AGPFJXEIR3RVPZM7LCONXVQ4DC","short_pith_number":"pith:AGPFJXEI","schema_version":"1.0","canonical_sha256":"019e54dc888ee357e59f589cdbd61c1893032468de7a5b31417bfb48b6fb19f1","source":{"kind":"arxiv","id":"1501.02653","version":1},"attestation_state":"computed","paper":{"title":"Improved parameters of seven Kepler giant companions characterized with SOPHIE and HARPS-N","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Santerne, A. S. Bonomo, A. Sozzetti, C. Moutou, G. Bruno, G. H\\'ebrard, J.-M. Almenara, M. Deleuil, R. F. D\\'iaz","submitted_at":"2015-01-12T14:18:45Z","abstract_excerpt":"Radial-velocity observations of Kepler candidates obtained with the SOPHIE and HARPS-N spectrographs have permitted unveiling the nature of the five giant planets Kepler-41b, Kepler-43b, Kepler-44b, Kepler-74b, and Kepler-75b, the massive companion Kepler-39b, and the brown dwarf KOI-205b. These companions were previously characterized with long-cadence (LC) Kepler data. Here we aim at refining the parameters of these transiting systems by i) modelling the published radial velocities (RV) and Kepler short-cadence (SC) data that provide a much better sampling of the transits, ii) performing new"},"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":"1501.02653","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-01-12T14:18:45Z","cross_cats_sorted":[],"title_canon_sha256":"15c58caffe60f648464b9d9da574510bfeca94a802aed6fd148363265f4063ea","abstract_canon_sha256":"e76248af10ffb897db52c6923a79ed5f4fdecd0c1eada6381caa8a25a7992562"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:25:40.706140Z","signature_b64":"2TIEPmRJvTcKA79KU9fsqbPi21KfOg77nmSaC/qHf8B8cdFTkusc27a2h3rnkQeHBezRySobMnc2Lo5po9iECA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"019e54dc888ee357e59f589cdbd61c1893032468de7a5b31417bfb48b6fb19f1","last_reissued_at":"2026-05-18T02:25:40.705694Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:25:40.705694Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Improved parameters of seven Kepler giant companions characterized with SOPHIE and HARPS-N","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Santerne, A. S. Bonomo, A. Sozzetti, C. Moutou, G. Bruno, G. H\\'ebrard, J.-M. Almenara, M. Deleuil, R. F. D\\'iaz","submitted_at":"2015-01-12T14:18:45Z","abstract_excerpt":"Radial-velocity observations of Kepler candidates obtained with the SOPHIE and HARPS-N spectrographs have permitted unveiling the nature of the five giant planets Kepler-41b, Kepler-43b, Kepler-44b, Kepler-74b, and Kepler-75b, the massive companion Kepler-39b, and the brown dwarf KOI-205b. These companions were previously characterized with long-cadence (LC) Kepler data. Here we aim at refining the parameters of these transiting systems by i) modelling the published radial velocities (RV) and Kepler short-cadence (SC) data that provide a much better sampling of the transits, ii) performing new"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.02653","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":"1501.02653","created_at":"2026-05-18T02:25:40.705774+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.02653v1","created_at":"2026-05-18T02:25:40.705774+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.02653","created_at":"2026-05-18T02:25:40.705774+00:00"},{"alias_kind":"pith_short_12","alias_value":"AGPFJXEIR3RV","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_16","alias_value":"AGPFJXEIR3RVPZM7","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_8","alias_value":"AGPFJXEI","created_at":"2026-05-18T12:29:10.953037+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/AGPFJXEIR3RVPZM7LCONXVQ4DC","json":"https://pith.science/pith/AGPFJXEIR3RVPZM7LCONXVQ4DC.json","graph_json":"https://pith.science/api/pith-number/AGPFJXEIR3RVPZM7LCONXVQ4DC/graph.json","events_json":"https://pith.science/api/pith-number/AGPFJXEIR3RVPZM7LCONXVQ4DC/events.json","paper":"https://pith.science/paper/AGPFJXEI"},"agent_actions":{"view_html":"https://pith.science/pith/AGPFJXEIR3RVPZM7LCONXVQ4DC","download_json":"https://pith.science/pith/AGPFJXEIR3RVPZM7LCONXVQ4DC.json","view_paper":"https://pith.science/paper/AGPFJXEI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.02653&json=true","fetch_graph":"https://pith.science/api/pith-number/AGPFJXEIR3RVPZM7LCONXVQ4DC/graph.json","fetch_events":"https://pith.science/api/pith-number/AGPFJXEIR3RVPZM7LCONXVQ4DC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AGPFJXEIR3RVPZM7LCONXVQ4DC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AGPFJXEIR3RVPZM7LCONXVQ4DC/action/storage_attestation","attest_author":"https://pith.science/pith/AGPFJXEIR3RVPZM7LCONXVQ4DC/action/author_attestation","sign_citation":"https://pith.science/pith/AGPFJXEIR3RVPZM7LCONXVQ4DC/action/citation_signature","submit_replication":"https://pith.science/pith/AGPFJXEIR3RVPZM7LCONXVQ4DC/action/replication_record"}},"created_at":"2026-05-18T02:25:40.705774+00:00","updated_at":"2026-05-18T02:25:40.705774+00:00"}