{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:LVU45R6P32ZEWX6UCFY42WNORS","short_pith_number":"pith:LVU45R6P","canonical_record":{"source":{"id":"1709.01027","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-09-04T16:28:47Z","cross_cats_sorted":[],"title_canon_sha256":"94a50fbff55ec31be5dd7f46890342e2845887a1bf865f72b0afb0aa85c8abc7","abstract_canon_sha256":"e041271aeedf3e9f1d454bbd0b779c9e046e1765237b17c6df9b31245535cf59"},"schema_version":"1.0"},"canonical_sha256":"5d69cec7cfdeb24b5fd41171cd59ae8c80e02ae5c7beec7ca23e0f0000da60a7","source":{"kind":"arxiv","id":"1709.01027","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1709.01027","created_at":"2026-05-18T00:36:04Z"},{"alias_kind":"arxiv_version","alias_value":"1709.01027v1","created_at":"2026-05-18T00:36:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.01027","created_at":"2026-05-18T00:36:04Z"},{"alias_kind":"pith_short_12","alias_value":"LVU45R6P32ZE","created_at":"2026-05-18T12:31:28Z"},{"alias_kind":"pith_short_16","alias_value":"LVU45R6P32ZEWX6U","created_at":"2026-05-18T12:31:28Z"},{"alias_kind":"pith_short_8","alias_value":"LVU45R6P","created_at":"2026-05-18T12:31:28Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:LVU45R6P32ZEWX6UCFY42WNORS","target":"record","payload":{"canonical_record":{"source":{"id":"1709.01027","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-09-04T16:28:47Z","cross_cats_sorted":[],"title_canon_sha256":"94a50fbff55ec31be5dd7f46890342e2845887a1bf865f72b0afb0aa85c8abc7","abstract_canon_sha256":"e041271aeedf3e9f1d454bbd0b779c9e046e1765237b17c6df9b31245535cf59"},"schema_version":"1.0"},"canonical_sha256":"5d69cec7cfdeb24b5fd41171cd59ae8c80e02ae5c7beec7ca23e0f0000da60a7","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:36:04.470034Z","signature_b64":"ONyXJiaGkj0X/LjHaeWOia+LOPp8DGZfD/aj8/X9/Adgsih/4IdnAMEFwBJGzk3y5FJO/VnCLDLScI5fJTEGCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5d69cec7cfdeb24b5fd41171cd59ae8c80e02ae5c7beec7ca23e0f0000da60a7","last_reissued_at":"2026-05-18T00:36:04.469382Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:36:04.469382Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1709.01027","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":"2026-05-18T00:36:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"DEj6vXtldod1A++M7lpIfml60NszFc5LFvCC8UvkUsB9qBV8g5AhncnPTT7eDuErWjwua6zS1jCJfshPsRWGDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T18:56:41.082646Z"},"content_sha256":"c052de570a3576c35b36470972083175a54fa27dbdbadb9b21ccc2cf56c4e8ec","schema_version":"1.0","event_id":"sha256:c052de570a3576c35b36470972083175a54fa27dbdbadb9b21ccc2cf56c4e8ec"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:LVU45R6P32ZEWX6UCFY42WNORS","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The Influence of Coronal Mass Ejections on the Mass-loss Rates of Hot-Jupiters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. A. Cherenkov, C. M\\\"ostl, D. V. Bisikalo, L. Fossati","submitted_at":"2017-09-04T16:28:47Z","abstract_excerpt":"Hot-Jupiters are subject to extreme radiation and plasma flows coming from their host stars. Past ultraviolet Hubble Space Telescope observations, supported by hydrodynamic models, confirmed that these factors lead to the formation of an extended envelope, part of which lies beyond the Roche lobe. We use gas-dynamic simulations to study the impact of time variations in the parameters of the stellar wind, namely that of coronal mass ejections (CMEs), on the envelope of the typical hot-Jupiter HD 209458b. We consider three CMEs characterized by different velocities and densities, taking their pa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.01027","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":"2026-05-18T00:36:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"qhXbXHCzuMRwhuKFJne8lbZpK+u4Mg4S2oPkJX4x2DL65/K4RTQieQ73YWtISN++/Yv6z/+SueeNz+ULqDjlBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T18:56:41.083296Z"},"content_sha256":"80834d48ada31ec9286cbb8740debd4ed242ce5e52f45010f7534087e1833f70","schema_version":"1.0","event_id":"sha256:80834d48ada31ec9286cbb8740debd4ed242ce5e52f45010f7534087e1833f70"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/LVU45R6P32ZEWX6UCFY42WNORS/bundle.json","state_url":"https://pith.science/pith/LVU45R6P32ZEWX6UCFY42WNORS/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/LVU45R6P32ZEWX6UCFY42WNORS/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":"2026-06-06T18:56:41Z","links":{"resolver":"https://pith.science/pith/LVU45R6P32ZEWX6UCFY42WNORS","bundle":"https://pith.science/pith/LVU45R6P32ZEWX6UCFY42WNORS/bundle.json","state":"https://pith.science/pith/LVU45R6P32ZEWX6UCFY42WNORS/state.json","well_known_bundle":"https://pith.science/.well-known/pith/LVU45R6P32ZEWX6UCFY42WNORS/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:LVU45R6P32ZEWX6UCFY42WNORS","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":"e041271aeedf3e9f1d454bbd0b779c9e046e1765237b17c6df9b31245535cf59","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-09-04T16:28:47Z","title_canon_sha256":"94a50fbff55ec31be5dd7f46890342e2845887a1bf865f72b0afb0aa85c8abc7"},"schema_version":"1.0","source":{"id":"1709.01027","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1709.01027","created_at":"2026-05-18T00:36:04Z"},{"alias_kind":"arxiv_version","alias_value":"1709.01027v1","created_at":"2026-05-18T00:36:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.01027","created_at":"2026-05-18T00:36:04Z"},{"alias_kind":"pith_short_12","alias_value":"LVU45R6P32ZE","created_at":"2026-05-18T12:31:28Z"},{"alias_kind":"pith_short_16","alias_value":"LVU45R6P32ZEWX6U","created_at":"2026-05-18T12:31:28Z"},{"alias_kind":"pith_short_8","alias_value":"LVU45R6P","created_at":"2026-05-18T12:31:28Z"}],"graph_snapshots":[{"event_id":"sha256:80834d48ada31ec9286cbb8740debd4ed242ce5e52f45010f7534087e1833f70","target":"graph","created_at":"2026-05-18T00:36:04Z","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":"Hot-Jupiters are subject to extreme radiation and plasma flows coming from their host stars. Past ultraviolet Hubble Space Telescope observations, supported by hydrodynamic models, confirmed that these factors lead to the formation of an extended envelope, part of which lies beyond the Roche lobe. We use gas-dynamic simulations to study the impact of time variations in the parameters of the stellar wind, namely that of coronal mass ejections (CMEs), on the envelope of the typical hot-Jupiter HD 209458b. We consider three CMEs characterized by different velocities and densities, taking their pa","authors_text":"A. A. Cherenkov, C. M\\\"ostl, D. V. Bisikalo, L. Fossati","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-09-04T16:28:47Z","title":"The Influence of Coronal Mass Ejections on the Mass-loss Rates of Hot-Jupiters"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.01027","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:c052de570a3576c35b36470972083175a54fa27dbdbadb9b21ccc2cf56c4e8ec","target":"record","created_at":"2026-05-18T00:36:04Z","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":"e041271aeedf3e9f1d454bbd0b779c9e046e1765237b17c6df9b31245535cf59","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-09-04T16:28:47Z","title_canon_sha256":"94a50fbff55ec31be5dd7f46890342e2845887a1bf865f72b0afb0aa85c8abc7"},"schema_version":"1.0","source":{"id":"1709.01027","kind":"arxiv","version":1}},"canonical_sha256":"5d69cec7cfdeb24b5fd41171cd59ae8c80e02ae5c7beec7ca23e0f0000da60a7","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"5d69cec7cfdeb24b5fd41171cd59ae8c80e02ae5c7beec7ca23e0f0000da60a7","first_computed_at":"2026-05-18T00:36:04.469382Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:36:04.469382Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"ONyXJiaGkj0X/LjHaeWOia+LOPp8DGZfD/aj8/X9/Adgsih/4IdnAMEFwBJGzk3y5FJO/VnCLDLScI5fJTEGCA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:36:04.470034Z","signed_message":"canonical_sha256_bytes"},"source_id":"1709.01027","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:c052de570a3576c35b36470972083175a54fa27dbdbadb9b21ccc2cf56c4e8ec","sha256:80834d48ada31ec9286cbb8740debd4ed242ce5e52f45010f7534087e1833f70"],"state_sha256":"8aef763f2dd1c52384876009208552e30d0f91f2c9b5d813cea15659e4604954"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"JE8BqrBCc2nbLOG1Em+t3YcnP1gg9X2gheJTgcJkop9j3doB16ZOOJRFc+//5SecqyBhugP68wUNRYD333PFBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-06T18:56:41.086421Z","bundle_sha256":"462cdbd78f83e66e0d8bc6d6477174b29a4973f283a8c8f9801e78e11d9f20d1"}}