{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:VYOPN6Y2LYVJ54L6I4YNNPAFN2","short_pith_number":"pith:VYOPN6Y2","canonical_record":{"source":{"id":"1005.2128","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-05-12T15:32:51Z","cross_cats_sorted":[],"title_canon_sha256":"abdc1d1515e301a6f3eaada43a09271f9e91d4dc917a1d6400fe4e011292e6a4","abstract_canon_sha256":"298ced827b12bce6fbfcd7e98b2c6d9387023cef87ed472ab57ea7d24f003553"},"schema_version":"1.0"},"canonical_sha256":"ae1cf6fb1a5e2a9ef17e4730d6bc056eaa2dac303a4786bca7255737644443a8","source":{"kind":"arxiv","id":"1005.2128","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1005.2128","created_at":"2026-05-18T02:07:33Z"},{"alias_kind":"arxiv_version","alias_value":"1005.2128v1","created_at":"2026-05-18T02:07:33Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.2128","created_at":"2026-05-18T02:07:33Z"},{"alias_kind":"pith_short_12","alias_value":"VYOPN6Y2LYVJ","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_16","alias_value":"VYOPN6Y2LYVJ54L6","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_8","alias_value":"VYOPN6Y2","created_at":"2026-05-18T12:26:15Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:VYOPN6Y2LYVJ54L6I4YNNPAFN2","target":"record","payload":{"canonical_record":{"source":{"id":"1005.2128","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-05-12T15:32:51Z","cross_cats_sorted":[],"title_canon_sha256":"abdc1d1515e301a6f3eaada43a09271f9e91d4dc917a1d6400fe4e011292e6a4","abstract_canon_sha256":"298ced827b12bce6fbfcd7e98b2c6d9387023cef87ed472ab57ea7d24f003553"},"schema_version":"1.0"},"canonical_sha256":"ae1cf6fb1a5e2a9ef17e4730d6bc056eaa2dac303a4786bca7255737644443a8","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:33.674130Z","signature_b64":"z+xl0xsBzZDh5Ttyy37j+axkTk7tfPPY4odp6uiBQwPzy+TdI/OAuWxjZbBS5mj7Zc4JYMS9QcdtNShybcxdCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ae1cf6fb1a5e2a9ef17e4730d6bc056eaa2dac303a4786bca7255737644443a8","last_reissued_at":"2026-05-18T02:07:33.673678Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:33.673678Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1005.2128","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":"2026-05-18T02:07:33Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"hBLaKSXWQEpOJzMekjNceI5rbn73FrJA7I26y08r9YPdaLWMAV8FiFoGIjgW94k/xWfQ8JJ+bAye3mjnw6YcAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-11T00:09:42.262185Z"},"content_sha256":"defafd946ea589f0d02bd81d3b8d728458b3b7b932c9b0028b276f22d3e69afd","schema_version":"1.0","event_id":"sha256:defafd946ea589f0d02bd81d3b8d728458b3b7b932c9b0028b276f22d3e69afd"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:VYOPN6Y2LYVJ54L6I4YNNPAFN2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A Search for Star-Disk Interaction Among the Strongest X-ray Flaring Stars in the Orion Nebula Cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alicia N. Aarnio, Keivan G. Stassun, Sean P. Matt","submitted_at":"2010-05-12T15:32:51Z","abstract_excerpt":"The Chandra Orion Ultradeep Project observed hundreds of young, low-mass stars undergoing highly energetic X-ray flare events. The 32 most powerful cases have been modeled with the result that the magnetic structures responsible for these flares can be many stellar radii in extent. In this paper, we model the observed spectral energy distributions of these 32 stars in order to determine, in detail for each star, whether there is circumstellar disk material situated in sufficient proximity to the stellar surface for interaction with the large magnetic loops inferred from the observed X-ray flar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.2128","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":"2026-05-18T02:07:33Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"PMUUvSdX1w4C5GJ/rY9io0NByxhE8HlOQKn5uT/Oj2DvWheP5e2EO5icQ2Fif90iyoZpMXXkf7PQp8t2OWKeAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-11T00:09:42.262876Z"},"content_sha256":"13dfe293b3b243a412dc0fde8c830e30b36c63437b84b037da1317019caaed7c","schema_version":"1.0","event_id":"sha256:13dfe293b3b243a412dc0fde8c830e30b36c63437b84b037da1317019caaed7c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/VYOPN6Y2LYVJ54L6I4YNNPAFN2/bundle.json","state_url":"https://pith.science/pith/VYOPN6Y2LYVJ54L6I4YNNPAFN2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/VYOPN6Y2LYVJ54L6I4YNNPAFN2/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":"2026-06-11T00:09:42Z","links":{"resolver":"https://pith.science/pith/VYOPN6Y2LYVJ54L6I4YNNPAFN2","bundle":"https://pith.science/pith/VYOPN6Y2LYVJ54L6I4YNNPAFN2/bundle.json","state":"https://pith.science/pith/VYOPN6Y2LYVJ54L6I4YNNPAFN2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/VYOPN6Y2LYVJ54L6I4YNNPAFN2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:VYOPN6Y2LYVJ54L6I4YNNPAFN2","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":"298ced827b12bce6fbfcd7e98b2c6d9387023cef87ed472ab57ea7d24f003553","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-05-12T15:32:51Z","title_canon_sha256":"abdc1d1515e301a6f3eaada43a09271f9e91d4dc917a1d6400fe4e011292e6a4"},"schema_version":"1.0","source":{"id":"1005.2128","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1005.2128","created_at":"2026-05-18T02:07:33Z"},{"alias_kind":"arxiv_version","alias_value":"1005.2128v1","created_at":"2026-05-18T02:07:33Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.2128","created_at":"2026-05-18T02:07:33Z"},{"alias_kind":"pith_short_12","alias_value":"VYOPN6Y2LYVJ","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_16","alias_value":"VYOPN6Y2LYVJ54L6","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_8","alias_value":"VYOPN6Y2","created_at":"2026-05-18T12:26:15Z"}],"graph_snapshots":[{"event_id":"sha256:13dfe293b3b243a412dc0fde8c830e30b36c63437b84b037da1317019caaed7c","target":"graph","created_at":"2026-05-18T02:07:33Z","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":"The Chandra Orion Ultradeep Project observed hundreds of young, low-mass stars undergoing highly energetic X-ray flare events. The 32 most powerful cases have been modeled with the result that the magnetic structures responsible for these flares can be many stellar radii in extent. In this paper, we model the observed spectral energy distributions of these 32 stars in order to determine, in detail for each star, whether there is circumstellar disk material situated in sufficient proximity to the stellar surface for interaction with the large magnetic loops inferred from the observed X-ray flar","authors_text":"Alicia N. Aarnio, Keivan G. Stassun, Sean P. Matt","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-05-12T15:32:51Z","title":"A Search for Star-Disk Interaction Among the Strongest X-ray Flaring Stars in the Orion Nebula Cluster"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.2128","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:defafd946ea589f0d02bd81d3b8d728458b3b7b932c9b0028b276f22d3e69afd","target":"record","created_at":"2026-05-18T02:07:33Z","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":"298ced827b12bce6fbfcd7e98b2c6d9387023cef87ed472ab57ea7d24f003553","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-05-12T15:32:51Z","title_canon_sha256":"abdc1d1515e301a6f3eaada43a09271f9e91d4dc917a1d6400fe4e011292e6a4"},"schema_version":"1.0","source":{"id":"1005.2128","kind":"arxiv","version":1}},"canonical_sha256":"ae1cf6fb1a5e2a9ef17e4730d6bc056eaa2dac303a4786bca7255737644443a8","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"ae1cf6fb1a5e2a9ef17e4730d6bc056eaa2dac303a4786bca7255737644443a8","first_computed_at":"2026-05-18T02:07:33.673678Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:07:33.673678Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"z+xl0xsBzZDh5Ttyy37j+axkTk7tfPPY4odp6uiBQwPzy+TdI/OAuWxjZbBS5mj7Zc4JYMS9QcdtNShybcxdCg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:07:33.674130Z","signed_message":"canonical_sha256_bytes"},"source_id":"1005.2128","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:defafd946ea589f0d02bd81d3b8d728458b3b7b932c9b0028b276f22d3e69afd","sha256:13dfe293b3b243a412dc0fde8c830e30b36c63437b84b037da1317019caaed7c"],"state_sha256":"2a22d4822036f5096f88e6e605125d1b0cf67cfd23d5765d5b6783b80ca9e518"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3BKdqMATI4MPaca1f2ExLqw5xjXqdiSM06l7qFr0oWm1cgTJ1XDeqYlKsv2tSRRBP6e93pH7M4m8spzU+uEEDA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-11T00:09:42.266720Z","bundle_sha256":"d251e82b9a26b305b5c1265f71ef2b8dfee6a92ba6c566770ba6c6404b27d986"}}