{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:G3GSYH7P4EZ4YKZKTBVNR52YAW","short_pith_number":"pith:G3GSYH7P","canonical_record":{"source":{"id":"1607.04445","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-07-15T10:31:10Z","cross_cats_sorted":[],"title_canon_sha256":"7ce000b371ec85f83c658fc9e6dbff711be46ada0df4dfb4daccc14f2d5e6aae","abstract_canon_sha256":"5ce40216f0e8403ea6541b0d4b4a1e86e16a77f5d3309ce31047a4b29610bab9"},"schema_version":"1.0"},"canonical_sha256":"36cd2c1fefe133cc2b2a986ad8f7580597956a150dceacc78003d7a60d39c443","source":{"kind":"arxiv","id":"1607.04445","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1607.04445","created_at":"2026-05-18T01:03:18Z"},{"alias_kind":"arxiv_version","alias_value":"1607.04445v1","created_at":"2026-05-18T01:03:18Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.04445","created_at":"2026-05-18T01:03:18Z"},{"alias_kind":"pith_short_12","alias_value":"G3GSYH7P4EZ4","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_16","alias_value":"G3GSYH7P4EZ4YKZK","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_8","alias_value":"G3GSYH7P","created_at":"2026-05-18T12:30:15Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:G3GSYH7P4EZ4YKZKTBVNR52YAW","target":"record","payload":{"canonical_record":{"source":{"id":"1607.04445","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-07-15T10:31:10Z","cross_cats_sorted":[],"title_canon_sha256":"7ce000b371ec85f83c658fc9e6dbff711be46ada0df4dfb4daccc14f2d5e6aae","abstract_canon_sha256":"5ce40216f0e8403ea6541b0d4b4a1e86e16a77f5d3309ce31047a4b29610bab9"},"schema_version":"1.0"},"canonical_sha256":"36cd2c1fefe133cc2b2a986ad8f7580597956a150dceacc78003d7a60d39c443","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:18.050134Z","signature_b64":"abEaInSR4S6KeoVO/SJJQZkP6TJYagKAX3s9sFGuLYhWuTX5ffsGBtdN2AqfIs4YbWEihnLAlX/a1YFM5RHTBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"36cd2c1fefe133cc2b2a986ad8f7580597956a150dceacc78003d7a60d39c443","last_reissued_at":"2026-05-18T01:03:18.049528Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:18.049528Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1607.04445","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":"2026-05-18T01:03:18Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"M8bw7b8SlbwioM6B1q87RY5zjUI7fdMiRRw2jgrwXLPwbMnR4HgncG+Vqu8zUTxddwOUjMiBM3E96BvF412HDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T04:57:38.739860Z"},"content_sha256":"750029be33e05b5ad4ae3de616b11011915f313f085bd215de173350a82b43f5","schema_version":"1.0","event_id":"sha256:750029be33e05b5ad4ae3de616b11011915f313f085bd215de173350a82b43f5"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:G3GSYH7P4EZ4YKZKTBVNR52YAW","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Stellar wind models of subluminous hot stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"I. Krtickova, J. Krticka, J. Kubat","submitted_at":"2016-07-15T10:31:10Z","abstract_excerpt":"Mass-loss rate is one of the most important stellar parameters. We aim to provide mass-loss rates as a function of subdwarf parameters and to apply the formula for individual subdwarfs, to predict the wind terminal velocities, to estimate the influence of the magnetic field and X-ray ionization on the stellar wind, and to study the interaction of subdwarf wind with mass loss from Be and cool companions. We used our kinetic equilibrium (NLTE) wind models with the radiative force determined from the radiative transfer equation in the comoving frame (CMF) to predict the wind structure of sublumin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.04445","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":"2026-05-18T01:03:18Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"zdhS9/7mDpMnwhJ0ZH8Xdo4oT9BKOrNbGGdNES8sBKonSB2jBvY2Xh7K751rbV6Kto80jcYG0s7MBeq+liBmCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T04:57:38.740572Z"},"content_sha256":"14fcaf72df564ef806698ac030ed41e769b6854392f721c3f50178aea6064214","schema_version":"1.0","event_id":"sha256:14fcaf72df564ef806698ac030ed41e769b6854392f721c3f50178aea6064214"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/G3GSYH7P4EZ4YKZKTBVNR52YAW/bundle.json","state_url":"https://pith.science/pith/G3GSYH7P4EZ4YKZKTBVNR52YAW/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/G3GSYH7P4EZ4YKZKTBVNR52YAW/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":"2026-06-05T04:57:38Z","links":{"resolver":"https://pith.science/pith/G3GSYH7P4EZ4YKZKTBVNR52YAW","bundle":"https://pith.science/pith/G3GSYH7P4EZ4YKZKTBVNR52YAW/bundle.json","state":"https://pith.science/pith/G3GSYH7P4EZ4YKZKTBVNR52YAW/state.json","well_known_bundle":"https://pith.science/.well-known/pith/G3GSYH7P4EZ4YKZKTBVNR52YAW/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:G3GSYH7P4EZ4YKZKTBVNR52YAW","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":"5ce40216f0e8403ea6541b0d4b4a1e86e16a77f5d3309ce31047a4b29610bab9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-07-15T10:31:10Z","title_canon_sha256":"7ce000b371ec85f83c658fc9e6dbff711be46ada0df4dfb4daccc14f2d5e6aae"},"schema_version":"1.0","source":{"id":"1607.04445","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1607.04445","created_at":"2026-05-18T01:03:18Z"},{"alias_kind":"arxiv_version","alias_value":"1607.04445v1","created_at":"2026-05-18T01:03:18Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.04445","created_at":"2026-05-18T01:03:18Z"},{"alias_kind":"pith_short_12","alias_value":"G3GSYH7P4EZ4","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_16","alias_value":"G3GSYH7P4EZ4YKZK","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_8","alias_value":"G3GSYH7P","created_at":"2026-05-18T12:30:15Z"}],"graph_snapshots":[{"event_id":"sha256:14fcaf72df564ef806698ac030ed41e769b6854392f721c3f50178aea6064214","target":"graph","created_at":"2026-05-18T01:03:18Z","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":"Mass-loss rate is one of the most important stellar parameters. We aim to provide mass-loss rates as a function of subdwarf parameters and to apply the formula for individual subdwarfs, to predict the wind terminal velocities, to estimate the influence of the magnetic field and X-ray ionization on the stellar wind, and to study the interaction of subdwarf wind with mass loss from Be and cool companions. We used our kinetic equilibrium (NLTE) wind models with the radiative force determined from the radiative transfer equation in the comoving frame (CMF) to predict the wind structure of sublumin","authors_text":"I. Krtickova, J. Krticka, J. Kubat","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-07-15T10:31:10Z","title":"Stellar wind models of subluminous hot stars"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.04445","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":"sha256:750029be33e05b5ad4ae3de616b11011915f313f085bd215de173350a82b43f5","target":"record","created_at":"2026-05-18T01:03:18Z","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":"5ce40216f0e8403ea6541b0d4b4a1e86e16a77f5d3309ce31047a4b29610bab9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-07-15T10:31:10Z","title_canon_sha256":"7ce000b371ec85f83c658fc9e6dbff711be46ada0df4dfb4daccc14f2d5e6aae"},"schema_version":"1.0","source":{"id":"1607.04445","kind":"arxiv","version":1}},"canonical_sha256":"36cd2c1fefe133cc2b2a986ad8f7580597956a150dceacc78003d7a60d39c443","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"36cd2c1fefe133cc2b2a986ad8f7580597956a150dceacc78003d7a60d39c443","first_computed_at":"2026-05-18T01:03:18.049528Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:03:18.049528Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"abEaInSR4S6KeoVO/SJJQZkP6TJYagKAX3s9sFGuLYhWuTX5ffsGBtdN2AqfIs4YbWEihnLAlX/a1YFM5RHTBg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:03:18.050134Z","signed_message":"canonical_sha256_bytes"},"source_id":"1607.04445","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:750029be33e05b5ad4ae3de616b11011915f313f085bd215de173350a82b43f5","sha256:14fcaf72df564ef806698ac030ed41e769b6854392f721c3f50178aea6064214"],"state_sha256":"43cc1b5dc1cc84e64f5fd8d77257607bab2441c13a39cc57adce1006ff612866"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"rC2w6qYHtZAh/Ad6QA2pvP7NHGT9mqx91chU2Vzb31Lc6iJuU4MhTLynBqg03D1PL3vjPbNqKL1m2h9MHA6LDw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-05T04:57:38.744171Z","bundle_sha256":"06383d520f3c9082f7b5de793019b5e145e7412c327545db9b1f7544fc2ece9c"}}