{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2006:ACYK75KOEJ5WZFOSLYAQSGIPGY","short_pith_number":"pith:ACYK75KO","canonical_record":{"source":{"id":"astro-ph/0605329","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T20:00:09Z","cross_cats_sorted":[],"title_canon_sha256":"ae6dd5da4ceceb3a4723f0b4fa946cd850cfa13cb3a9466aef0cdc75f523cdd3","abstract_canon_sha256":"34e123c5187047be2eab22baf8b449eee611b94a8d4fdc98aef79e6431f5c141"},"schema_version":"1.0"},"canonical_sha256":"00b0aff54e227b6c95d25e0109190f363c85fbc90eeca86dda043643ce1faafa","source":{"kind":"arxiv","id":"astro-ph/0605329","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0605329","created_at":"2026-05-18T04:29:04Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0605329v1","created_at":"2026-05-18T04:29:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0605329","created_at":"2026-05-18T04:29:04Z"},{"alias_kind":"pith_short_12","alias_value":"ACYK75KOEJ5W","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_16","alias_value":"ACYK75KOEJ5WZFOS","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_8","alias_value":"ACYK75KO","created_at":"2026-05-18T12:25:53Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2006:ACYK75KOEJ5WZFOSLYAQSGIPGY","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0605329","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T20:00:09Z","cross_cats_sorted":[],"title_canon_sha256":"ae6dd5da4ceceb3a4723f0b4fa946cd850cfa13cb3a9466aef0cdc75f523cdd3","abstract_canon_sha256":"34e123c5187047be2eab22baf8b449eee611b94a8d4fdc98aef79e6431f5c141"},"schema_version":"1.0"},"canonical_sha256":"00b0aff54e227b6c95d25e0109190f363c85fbc90eeca86dda043643ce1faafa","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:29:04.668352Z","signature_b64":"q5vXv5DLLTSB/EhruekuISm6lD4LdCIwm5r+jameY0A566sCIJ5mzNYw9S1kKKoHk1gmNVJmfMo/C388liWmCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"00b0aff54e227b6c95d25e0109190f363c85fbc90eeca86dda043643ce1faafa","last_reissued_at":"2026-05-18T04:29:04.667859Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:29:04.667859Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0605329","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":"2026-05-18T04:29:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3Gx3wedPfIt2sOiVureNldU9+GFO9GABt6SqODcQyLKSRXI8xN7j1XgBflS34CfQkpHgoBjAGhIKU6b9MUP4Bg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-24T23:18:23.007359Z"},"content_sha256":"176bac9fe491c8f9ea9fac6e0b1f3210fe0f737e8f535e82f998f9db6565a86a","schema_version":"1.0","event_id":"sha256:176bac9fe491c8f9ea9fac6e0b1f3210fe0f737e8f535e82f998f9db6565a86a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2006:ACYK75KOEJ5WZFOSLYAQSGIPGY","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Molecular Line Emission from Gravitationally Unstable Protoplanetary Disks","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Alan Boss (2), Carnegie Institution of Washington), Christopher K. Walker (1) (1: University of Arizona; 2: DTM, Craig Kulesa (1), Desika Narayanan (1)","submitted_at":"2006-05-12T20:00:09Z","abstract_excerpt":"In the era of high resolution submillimeter interferometers, it will soon be possible to observe the neutral circumstellar medium directly involved in gas giant planet (GGP) formation at physical scales previously unattainable. In order to explore possible signatures of gas giant planet formation via disk instabilities, we have combined a 3D, non-local thermodynamic equilibrium (LTE) radiative transfer code with a 3D, finite differences hydrodynamical code to model molecular emission lines from the vicinity of a 1.4 M_J self-gravitating proto-GGP. Here, we explore the properties of rotational "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0605329","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":"2026-05-18T04:29:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"eg9pUjsAVcXAFPOjFPYXj5n6TOfMk2QCCzrVualVmZOsc4u9yHHICZeDElfRvMBT/9OsjDtYWQP0sR4Arsi1AA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-24T23:18:23.007700Z"},"content_sha256":"9d25f2d0efa1a05f4dc57fb43393568eedc74ef2a488b0004182329e395a5c99","schema_version":"1.0","event_id":"sha256:9d25f2d0efa1a05f4dc57fb43393568eedc74ef2a488b0004182329e395a5c99"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ACYK75KOEJ5WZFOSLYAQSGIPGY/bundle.json","state_url":"https://pith.science/pith/ACYK75KOEJ5WZFOSLYAQSGIPGY/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ACYK75KOEJ5WZFOSLYAQSGIPGY/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":"2026-06-24T23:18:23Z","links":{"resolver":"https://pith.science/pith/ACYK75KOEJ5WZFOSLYAQSGIPGY","bundle":"https://pith.science/pith/ACYK75KOEJ5WZFOSLYAQSGIPGY/bundle.json","state":"https://pith.science/pith/ACYK75KOEJ5WZFOSLYAQSGIPGY/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ACYK75KOEJ5WZFOSLYAQSGIPGY/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2006:ACYK75KOEJ5WZFOSLYAQSGIPGY","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":"34e123c5187047be2eab22baf8b449eee611b94a8d4fdc98aef79e6431f5c141","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T20:00:09Z","title_canon_sha256":"ae6dd5da4ceceb3a4723f0b4fa946cd850cfa13cb3a9466aef0cdc75f523cdd3"},"schema_version":"1.0","source":{"id":"astro-ph/0605329","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0605329","created_at":"2026-05-18T04:29:04Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0605329v1","created_at":"2026-05-18T04:29:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0605329","created_at":"2026-05-18T04:29:04Z"},{"alias_kind":"pith_short_12","alias_value":"ACYK75KOEJ5W","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_16","alias_value":"ACYK75KOEJ5WZFOS","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_8","alias_value":"ACYK75KO","created_at":"2026-05-18T12:25:53Z"}],"graph_snapshots":[{"event_id":"sha256:9d25f2d0efa1a05f4dc57fb43393568eedc74ef2a488b0004182329e395a5c99","target":"graph","created_at":"2026-05-18T04:29:04Z","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":"In the era of high resolution submillimeter interferometers, it will soon be possible to observe the neutral circumstellar medium directly involved in gas giant planet (GGP) formation at physical scales previously unattainable. In order to explore possible signatures of gas giant planet formation via disk instabilities, we have combined a 3D, non-local thermodynamic equilibrium (LTE) radiative transfer code with a 3D, finite differences hydrodynamical code to model molecular emission lines from the vicinity of a 1.4 M_J self-gravitating proto-GGP. Here, we explore the properties of rotational ","authors_text":"Alan Boss (2), Carnegie Institution of Washington), Christopher K. Walker (1) (1: University of Arizona; 2: DTM, Craig Kulesa (1), Desika Narayanan (1)","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T20:00:09Z","title":"Molecular Line Emission from Gravitationally Unstable Protoplanetary Disks"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0605329","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":"sha256:176bac9fe491c8f9ea9fac6e0b1f3210fe0f737e8f535e82f998f9db6565a86a","target":"record","created_at":"2026-05-18T04:29:04Z","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":"34e123c5187047be2eab22baf8b449eee611b94a8d4fdc98aef79e6431f5c141","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T20:00:09Z","title_canon_sha256":"ae6dd5da4ceceb3a4723f0b4fa946cd850cfa13cb3a9466aef0cdc75f523cdd3"},"schema_version":"1.0","source":{"id":"astro-ph/0605329","kind":"arxiv","version":1}},"canonical_sha256":"00b0aff54e227b6c95d25e0109190f363c85fbc90eeca86dda043643ce1faafa","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"00b0aff54e227b6c95d25e0109190f363c85fbc90eeca86dda043643ce1faafa","first_computed_at":"2026-05-18T04:29:04.667859Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:29:04.667859Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"q5vXv5DLLTSB/EhruekuISm6lD4LdCIwm5r+jameY0A566sCIJ5mzNYw9S1kKKoHk1gmNVJmfMo/C388liWmCQ==","signature_status":"signed_v1","signed_at":"2026-05-18T04:29:04.668352Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0605329","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:176bac9fe491c8f9ea9fac6e0b1f3210fe0f737e8f535e82f998f9db6565a86a","sha256:9d25f2d0efa1a05f4dc57fb43393568eedc74ef2a488b0004182329e395a5c99"],"state_sha256":"007f30cc6008e30a21c311e7074991a96331b9f392981bb40d43949bc2335c7f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"scd+5bHO/UO4kBaL88AcJ7iOgwb+ISTmT8geZSxghc9H4mm9P6Y5lmXzTzk3BCZ7JjPKE4zdcwZk/Fj8RJIOBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-24T23:18:23.009582Z","bundle_sha256":"9294e853f95f895e78a7849ce77ed11af9c74032e90bb55b823ab760e9c78900"}}