{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2005:32KOTSZ6NDM6RUYF2VS5IX4INN","short_pith_number":"pith:32KOTSZ6","canonical_record":{"source":{"id":"astro-ph/0510119","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-10-05T11:46:51Z","cross_cats_sorted":[],"title_canon_sha256":"bae6339f9d46b9ec031afada1f13302be4a14035ce61b52bf35bac05e712bc55","abstract_canon_sha256":"d41ba624ca290abe7642421c7a73d3420a223241c4699baff3a947cab66e7247"},"schema_version":"1.0"},"canonical_sha256":"de94e9cb3e68d9e8d305d565d45f886b5da53867fc93282745a28a749a8b188e","source":{"kind":"arxiv","id":"astro-ph/0510119","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0510119","created_at":"2026-05-18T01:07:25Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0510119v1","created_at":"2026-05-18T01:07:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0510119","created_at":"2026-05-18T01:07:25Z"},{"alias_kind":"pith_short_12","alias_value":"32KOTSZ6NDM6","created_at":"2026-05-18T12:25:52Z"},{"alias_kind":"pith_short_16","alias_value":"32KOTSZ6NDM6RUYF","created_at":"2026-05-18T12:25:52Z"},{"alias_kind":"pith_short_8","alias_value":"32KOTSZ6","created_at":"2026-05-18T12:25:52Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2005:32KOTSZ6NDM6RUYF2VS5IX4INN","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0510119","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-10-05T11:46:51Z","cross_cats_sorted":[],"title_canon_sha256":"bae6339f9d46b9ec031afada1f13302be4a14035ce61b52bf35bac05e712bc55","abstract_canon_sha256":"d41ba624ca290abe7642421c7a73d3420a223241c4699baff3a947cab66e7247"},"schema_version":"1.0"},"canonical_sha256":"de94e9cb3e68d9e8d305d565d45f886b5da53867fc93282745a28a749a8b188e","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:07:25.974365Z","signature_b64":"dSGfW5QxsCJWA8SqFH220IYabkfQ/FOsOwV7WcgwsGMjU8eqfLeJbk6xk7f4ewq26CodGyrehHrv1Ml9wI0SAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"de94e9cb3e68d9e8d305d565d45f886b5da53867fc93282745a28a749a8b188e","last_reissued_at":"2026-05-18T01:07:25.973530Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:07:25.973530Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0510119","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:07:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"EB1apPXynwGf1uTis8o09ks3fqta4IxaNDqAVCIKnTZcyS/JQMlSNSjoici9txRg38gdpcA3LjTsW9+3iqvfBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T04:03:16.988931Z"},"content_sha256":"4594dade931fe8f34146caefaffc41a6abd57b399a9d3e80c3e2b05d1f0715a0","schema_version":"1.0","event_id":"sha256:4594dade931fe8f34146caefaffc41a6abd57b399a9d3e80c3e2b05d1f0715a0"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2005:32KOTSZ6NDM6RUYF2VS5IX4INN","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"ELODIE metallicity-biased search for transiting Hot Jupiters II. A very hot Jupiter transiting the bright K star HD189733","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Claire Moutou (LAM), Damien Segransan, Didier Queloz, Francois Bouchy (LAM, Frederic Pont, Michel Mayor, Nicolas Iribarne (OHP), Nuno Santos, OHP), Ronaldo Da Silva, Sergio Ilovaisky (OHP), Shay Zucker, Stephane Udry","submitted_at":"2005-10-05T11:46:51Z","abstract_excerpt":"Among the 160 known exoplanets, mainly detected in large radial-velocity surveys, only 8 have a characterization of their actual mass and radius thanks to the two complementary methods of detection: radial velocities and photometric transit. We started in March 2004 an exoplanet-search programme biased toward high-metallicity stars which are more frequently host extra-solar planets. This survey aims to detect close-in giant planets, which are most likely to transit their host star. For this programme, high-precision radial velocities are measured with the ELODIE fiber-fed spectrograph on the 1"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0510119","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:07:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"VAH+SloUrPOv89LdMkgrpvSpdWknXhY4EGRm2B6mdv5yDm0c1MpD5WRan8qjHxvsG6Q9PdD81KSwaZQjEoGLAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T04:03:16.989523Z"},"content_sha256":"d2841b893af2829f734fe46fb0d821f5394cf1a61a70cd1a51c6eb62516820c5","schema_version":"1.0","event_id":"sha256:d2841b893af2829f734fe46fb0d821f5394cf1a61a70cd1a51c6eb62516820c5"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/32KOTSZ6NDM6RUYF2VS5IX4INN/bundle.json","state_url":"https://pith.science/pith/32KOTSZ6NDM6RUYF2VS5IX4INN/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/32KOTSZ6NDM6RUYF2VS5IX4INN/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-26T04:03:16Z","links":{"resolver":"https://pith.science/pith/32KOTSZ6NDM6RUYF2VS5IX4INN","bundle":"https://pith.science/pith/32KOTSZ6NDM6RUYF2VS5IX4INN/bundle.json","state":"https://pith.science/pith/32KOTSZ6NDM6RUYF2VS5IX4INN/state.json","well_known_bundle":"https://pith.science/.well-known/pith/32KOTSZ6NDM6RUYF2VS5IX4INN/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2005:32KOTSZ6NDM6RUYF2VS5IX4INN","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"d41ba624ca290abe7642421c7a73d3420a223241c4699baff3a947cab66e7247","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2005-10-05T11:46:51Z","title_canon_sha256":"bae6339f9d46b9ec031afada1f13302be4a14035ce61b52bf35bac05e712bc55"},"schema_version":"1.0","source":{"id":"astro-ph/0510119","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0510119","created_at":"2026-05-18T01:07:25Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0510119v1","created_at":"2026-05-18T01:07:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0510119","created_at":"2026-05-18T01:07:25Z"},{"alias_kind":"pith_short_12","alias_value":"32KOTSZ6NDM6","created_at":"2026-05-18T12:25:52Z"},{"alias_kind":"pith_short_16","alias_value":"32KOTSZ6NDM6RUYF","created_at":"2026-05-18T12:25:52Z"},{"alias_kind":"pith_short_8","alias_value":"32KOTSZ6","created_at":"2026-05-18T12:25:52Z"}],"graph_snapshots":[{"event_id":"sha256:d2841b893af2829f734fe46fb0d821f5394cf1a61a70cd1a51c6eb62516820c5","target":"graph","created_at":"2026-05-18T01:07:25Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Among the 160 known exoplanets, mainly detected in large radial-velocity surveys, only 8 have a characterization of their actual mass and radius thanks to the two complementary methods of detection: radial velocities and photometric transit. We started in March 2004 an exoplanet-search programme biased toward high-metallicity stars which are more frequently host extra-solar planets. This survey aims to detect close-in giant planets, which are most likely to transit their host star. For this programme, high-precision radial velocities are measured with the ELODIE fiber-fed spectrograph on the 1","authors_text":"Claire Moutou (LAM), Damien Segransan, Didier Queloz, Francois Bouchy (LAM, Frederic Pont, Michel Mayor, Nicolas Iribarne (OHP), Nuno Santos, OHP), Ronaldo Da Silva, Sergio Ilovaisky (OHP), Shay Zucker, Stephane Udry","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2005-10-05T11:46:51Z","title":"ELODIE metallicity-biased search for transiting Hot Jupiters II. A very hot Jupiter transiting the bright K star HD189733"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0510119","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:4594dade931fe8f34146caefaffc41a6abd57b399a9d3e80c3e2b05d1f0715a0","target":"record","created_at":"2026-05-18T01:07:25Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"d41ba624ca290abe7642421c7a73d3420a223241c4699baff3a947cab66e7247","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2005-10-05T11:46:51Z","title_canon_sha256":"bae6339f9d46b9ec031afada1f13302be4a14035ce61b52bf35bac05e712bc55"},"schema_version":"1.0","source":{"id":"astro-ph/0510119","kind":"arxiv","version":1}},"canonical_sha256":"de94e9cb3e68d9e8d305d565d45f886b5da53867fc93282745a28a749a8b188e","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"de94e9cb3e68d9e8d305d565d45f886b5da53867fc93282745a28a749a8b188e","first_computed_at":"2026-05-18T01:07:25.973530Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:07:25.973530Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"dSGfW5QxsCJWA8SqFH220IYabkfQ/FOsOwV7WcgwsGMjU8eqfLeJbk6xk7f4ewq26CodGyrehHrv1Ml9wI0SAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:07:25.974365Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0510119","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:4594dade931fe8f34146caefaffc41a6abd57b399a9d3e80c3e2b05d1f0715a0","sha256:d2841b893af2829f734fe46fb0d821f5394cf1a61a70cd1a51c6eb62516820c5"],"state_sha256":"bac9cfe746a9fbab2b246bb7058f3b4aa4a6dc49edd101c92d301a0d6bdf9230"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"fpWM+ZMk4eIkBUAhXO31wcmUDHgs3ytK0YWKoRQHC6xLTzkXUIFR7G0d7HzgZOfl+Wd5z8HJQ9KX1qZxoGG5Bg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T04:03:16.993170Z","bundle_sha256":"829c8a34079ad66310acc14a5292d008a42c8a010f4bf83f87b7c9075fad53e2"}}