{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:TJJAXRJYFLTBINVEPCITOEAJGV","short_pith_number":"pith:TJJAXRJY","canonical_record":{"source":{"id":"1102.0530","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-02-02T18:47:17Z","cross_cats_sorted":[],"title_canon_sha256":"21c9f28e4105dd566d6bd2f3bf54cc1d5ea01a837dfcde4af6c65b80c854136c","abstract_canon_sha256":"5c507d258ff584d825ce1e9d70d694ad1ec429bf629cff778af0c866461b2e39"},"schema_version":"1.0"},"canonical_sha256":"9a520bc5382ae61436a478913710093557d21d1fcb038412559123d43494bc80","source":{"kind":"arxiv","id":"1102.0530","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1102.0530","created_at":"2026-05-18T02:03:17Z"},{"alias_kind":"arxiv_version","alias_value":"1102.0530v2","created_at":"2026-05-18T02:03:17Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.0530","created_at":"2026-05-18T02:03:17Z"},{"alias_kind":"pith_short_12","alias_value":"TJJAXRJYFLTB","created_at":"2026-05-18T12:26:42Z"},{"alias_kind":"pith_short_16","alias_value":"TJJAXRJYFLTBINVE","created_at":"2026-05-18T12:26:42Z"},{"alias_kind":"pith_short_8","alias_value":"TJJAXRJY","created_at":"2026-05-18T12:26:42Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:TJJAXRJYFLTBINVEPCITOEAJGV","target":"record","payload":{"canonical_record":{"source":{"id":"1102.0530","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-02-02T18:47:17Z","cross_cats_sorted":[],"title_canon_sha256":"21c9f28e4105dd566d6bd2f3bf54cc1d5ea01a837dfcde4af6c65b80c854136c","abstract_canon_sha256":"5c507d258ff584d825ce1e9d70d694ad1ec429bf629cff778af0c866461b2e39"},"schema_version":"1.0"},"canonical_sha256":"9a520bc5382ae61436a478913710093557d21d1fcb038412559123d43494bc80","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:17.464245Z","signature_b64":"t6xxd4al+1QJqDG1TKVX6+PI6HPa++Rr5ZEvdtVXTTI0opyDeyM8UgttCKMLHbXs+4HsSqFmUYAI7jIgeCsqBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9a520bc5382ae61436a478913710093557d21d1fcb038412559123d43494bc80","last_reissued_at":"2026-05-18T02:03:17.463695Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:17.463695Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1102.0530","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:03:17Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3P0ef7jrPW8w6SLR7Mf57N0ohV8TMFSL2WOSt4noZkcOK4+RNW8nX9D6FX5ncJQ9xOjBKxwfnCEYV4p+TjJ3Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-23T18:31:40.966134Z"},"content_sha256":"02fd4fc239de025c2aac18d817815180f97d06dbea3af6bed9dd7aabf239d026","schema_version":"1.0","event_id":"sha256:02fd4fc239de025c2aac18d817815180f97d06dbea3af6bed9dd7aabf239d026"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:TJJAXRJYFLTBINVEPCITOEAJGV","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alex de Koter, Carrie Trundle, Chris J. Evans, Ian Hunter, Ines Brott, Jorick S. Vink, Matteo Cantiello, Norbert Langer, Selma E. de Mink","submitted_at":"2011-02-02T18:47:17Z","abstract_excerpt":"We present a dense grid of evolutionary tracks and isochrones of rotating massive main-sequence stars. We provide three grids with different initial compositions tailored to compare with early OB stars in the Small and Large Magellanic Clouds and in the Galaxy. Each grid covers masses ranging from 5 to 60 Msun and initial rotation rates between 0 and about 600 km/s. To calibrate our models we used the results of the VLT-FLAMES Survey of Massive Stars. We determine the amount of convective overshooting by using the observed drop in rotation rates for stars with surface gravities log g < 3.2 to "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.0530","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:03:17Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"klhlUvHSxQMJqf6Gtd9wGCff2nLMEIredff9P2sdb0HB/ynUNoYFXAdmUvC5zWVg0zf0vyJA9iiycSZs8XKvCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-23T18:31:40.966564Z"},"content_sha256":"7bb60c8d0c5b5b373102b9496291ffa7194f3ca1125d7a7a3d80eb55b9fa4359","schema_version":"1.0","event_id":"sha256:7bb60c8d0c5b5b373102b9496291ffa7194f3ca1125d7a7a3d80eb55b9fa4359"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/TJJAXRJYFLTBINVEPCITOEAJGV/bundle.json","state_url":"https://pith.science/pith/TJJAXRJYFLTBINVEPCITOEAJGV/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/TJJAXRJYFLTBINVEPCITOEAJGV/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":"2026-05-23T18:31:40Z","links":{"resolver":"https://pith.science/pith/TJJAXRJYFLTBINVEPCITOEAJGV","bundle":"https://pith.science/pith/TJJAXRJYFLTBINVEPCITOEAJGV/bundle.json","state":"https://pith.science/pith/TJJAXRJYFLTBINVEPCITOEAJGV/state.json","well_known_bundle":"https://pith.science/.well-known/pith/TJJAXRJYFLTBINVEPCITOEAJGV/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:TJJAXRJYFLTBINVEPCITOEAJGV","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":"5c507d258ff584d825ce1e9d70d694ad1ec429bf629cff778af0c866461b2e39","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-02-02T18:47:17Z","title_canon_sha256":"21c9f28e4105dd566d6bd2f3bf54cc1d5ea01a837dfcde4af6c65b80c854136c"},"schema_version":"1.0","source":{"id":"1102.0530","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1102.0530","created_at":"2026-05-18T02:03:17Z"},{"alias_kind":"arxiv_version","alias_value":"1102.0530v2","created_at":"2026-05-18T02:03:17Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.0530","created_at":"2026-05-18T02:03:17Z"},{"alias_kind":"pith_short_12","alias_value":"TJJAXRJYFLTB","created_at":"2026-05-18T12:26:42Z"},{"alias_kind":"pith_short_16","alias_value":"TJJAXRJYFLTBINVE","created_at":"2026-05-18T12:26:42Z"},{"alias_kind":"pith_short_8","alias_value":"TJJAXRJY","created_at":"2026-05-18T12:26:42Z"}],"graph_snapshots":[{"event_id":"sha256:7bb60c8d0c5b5b373102b9496291ffa7194f3ca1125d7a7a3d80eb55b9fa4359","target":"graph","created_at":"2026-05-18T02:03:17Z","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":"We present a dense grid of evolutionary tracks and isochrones of rotating massive main-sequence stars. We provide three grids with different initial compositions tailored to compare with early OB stars in the Small and Large Magellanic Clouds and in the Galaxy. Each grid covers masses ranging from 5 to 60 Msun and initial rotation rates between 0 and about 600 km/s. To calibrate our models we used the results of the VLT-FLAMES Survey of Massive Stars. We determine the amount of convective overshooting by using the observed drop in rotation rates for stars with surface gravities log g < 3.2 to ","authors_text":"Alex de Koter, Carrie Trundle, Chris J. Evans, Ian Hunter, Ines Brott, Jorick S. Vink, Matteo Cantiello, Norbert Langer, Selma E. de Mink","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-02-02T18:47:17Z","title":"Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.0530","kind":"arxiv","version":2},"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":"sha256:02fd4fc239de025c2aac18d817815180f97d06dbea3af6bed9dd7aabf239d026","target":"record","created_at":"2026-05-18T02:03:17Z","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":"5c507d258ff584d825ce1e9d70d694ad1ec429bf629cff778af0c866461b2e39","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-02-02T18:47:17Z","title_canon_sha256":"21c9f28e4105dd566d6bd2f3bf54cc1d5ea01a837dfcde4af6c65b80c854136c"},"schema_version":"1.0","source":{"id":"1102.0530","kind":"arxiv","version":2}},"canonical_sha256":"9a520bc5382ae61436a478913710093557d21d1fcb038412559123d43494bc80","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"9a520bc5382ae61436a478913710093557d21d1fcb038412559123d43494bc80","first_computed_at":"2026-05-18T02:03:17.463695Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:03:17.463695Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"t6xxd4al+1QJqDG1TKVX6+PI6HPa++Rr5ZEvdtVXTTI0opyDeyM8UgttCKMLHbXs+4HsSqFmUYAI7jIgeCsqBA==","signature_status":"signed_v1","signed_at":"2026-05-18T02:03:17.464245Z","signed_message":"canonical_sha256_bytes"},"source_id":"1102.0530","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:02fd4fc239de025c2aac18d817815180f97d06dbea3af6bed9dd7aabf239d026","sha256:7bb60c8d0c5b5b373102b9496291ffa7194f3ca1125d7a7a3d80eb55b9fa4359"],"state_sha256":"75e204711495de10fc56e1d6c16c04a813d40378899d0c9f9544675a0b3edb8d"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"YOwEbAnAm+ooEmGBpxNsGjgdF/PDFgoY0GpIXpVpcuw9LJr7xRuUWWX7bXjskYqd1lHbZJ3mONmmgEeW0xfqAw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-23T18:31:40.968980Z","bundle_sha256":"25fe42220da5fca4c370f099ceb4968266bc87758ece14bedbea485bf4d14b7c"}}