{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:OXVJDPJTR65FE5CGREYYI57ZPL","short_pith_number":"pith:OXVJDPJT","canonical_record":{"source":{"id":"1310.4350","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-10-16T12:35:53Z","cross_cats_sorted":[],"title_canon_sha256":"e2fc2d9c9dffe6e812919ab4914b22b85b5041b0a1decc5a2adb8a4170b4ec5b","abstract_canon_sha256":"6ebe396cc26c2a6e5547f6530fcbe60fa901230835bb469788cd26674a97ccf3"},"schema_version":"1.0"},"canonical_sha256":"75ea91bd338fba52744689318477f97ac873bd111c8dfe39b84e7c05b7136f80","source":{"kind":"arxiv","id":"1310.4350","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1310.4350","created_at":"2026-05-18T03:10:23Z"},{"alias_kind":"arxiv_version","alias_value":"1310.4350v1","created_at":"2026-05-18T03:10:23Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.4350","created_at":"2026-05-18T03:10:23Z"},{"alias_kind":"pith_short_12","alias_value":"OXVJDPJTR65F","created_at":"2026-05-18T12:27:54Z"},{"alias_kind":"pith_short_16","alias_value":"OXVJDPJTR65FE5CG","created_at":"2026-05-18T12:27:54Z"},{"alias_kind":"pith_short_8","alias_value":"OXVJDPJT","created_at":"2026-05-18T12:27:54Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:OXVJDPJTR65FE5CGREYYI57ZPL","target":"record","payload":{"canonical_record":{"source":{"id":"1310.4350","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-10-16T12:35:53Z","cross_cats_sorted":[],"title_canon_sha256":"e2fc2d9c9dffe6e812919ab4914b22b85b5041b0a1decc5a2adb8a4170b4ec5b","abstract_canon_sha256":"6ebe396cc26c2a6e5547f6530fcbe60fa901230835bb469788cd26674a97ccf3"},"schema_version":"1.0"},"canonical_sha256":"75ea91bd338fba52744689318477f97ac873bd111c8dfe39b84e7c05b7136f80","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:10:23.084548Z","signature_b64":"TEo+cZ6dB18a3SZDfDSHCYsFPqUwvJTSq3mWMaryETjLMHCBOwmH89iL8Q99cIUGRW0aQPdl+aie91mGKyrHAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"75ea91bd338fba52744689318477f97ac873bd111c8dfe39b84e7c05b7136f80","last_reissued_at":"2026-05-18T03:10:23.083793Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:10:23.083793Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1310.4350","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":"2026-05-18T03:10:23Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3/EwaZlQwF1eB+c//WdZkE0fSDvZnIZ8Emg/LW9tphWeN5ASvkVqYdh3jujH/CS+ud5NmsdUBsjQFf87B6D9CQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T19:26:52.928039Z"},"content_sha256":"937fdb270adf0bf10c6d83ed55c828de468f7bc991c068788b43d8a8f1a242f3","schema_version":"1.0","event_id":"sha256:937fdb270adf0bf10c6d83ed55c828de468f7bc991c068788b43d8a8f1a242f3"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:OXVJDPJTR65FE5CGREYYI57ZPL","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Review of important reactions for the nitrogen chemistry in the interstellar medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bergeat, D. Talbi, I. W. M. Smith, J.-C. Loison, K. M. Hickson, S. J. Klippenstein, V. Wakelam, W. D. Geppert","submitted_at":"2013-10-16T12:35:53Z","abstract_excerpt":"Predictions of astrochemical models depend strongly on the reaction rate coefficients used in the simulations. We reviewed a number of key reactions for the chemistry of nitrogen-bearing species in the dense interstellar medium and proposed new reaction rate coefficients for those reactions. The details of the reviews are given in the form of a datasheet associated with each reaction. The new recommended rate coefficients are given with an uncertainty and a temperature range of validity and will be included in KIDA (http://kida.obs.u-bordeaux1.fr)."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.4350","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":"2026-05-18T03:10:23Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"khMnXVUILOJ9pn3aH7nTOqt4G6gTf5Ww+x9eB1fKn0ZO14DuyRPiweGQt7cSCjEeNws3az99+hQm5aEtMhmrDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T19:26:52.928397Z"},"content_sha256":"07994780a5055c6685090f45e947257e9917dc0c9e96b2647e0f424f927feac3","schema_version":"1.0","event_id":"sha256:07994780a5055c6685090f45e947257e9917dc0c9e96b2647e0f424f927feac3"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/OXVJDPJTR65FE5CGREYYI57ZPL/bundle.json","state_url":"https://pith.science/pith/OXVJDPJTR65FE5CGREYYI57ZPL/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/OXVJDPJTR65FE5CGREYYI57ZPL/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":"2026-06-02T19:26:52Z","links":{"resolver":"https://pith.science/pith/OXVJDPJTR65FE5CGREYYI57ZPL","bundle":"https://pith.science/pith/OXVJDPJTR65FE5CGREYYI57ZPL/bundle.json","state":"https://pith.science/pith/OXVJDPJTR65FE5CGREYYI57ZPL/state.json","well_known_bundle":"https://pith.science/.well-known/pith/OXVJDPJTR65FE5CGREYYI57ZPL/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:OXVJDPJTR65FE5CGREYYI57ZPL","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":"6ebe396cc26c2a6e5547f6530fcbe60fa901230835bb469788cd26674a97ccf3","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-10-16T12:35:53Z","title_canon_sha256":"e2fc2d9c9dffe6e812919ab4914b22b85b5041b0a1decc5a2adb8a4170b4ec5b"},"schema_version":"1.0","source":{"id":"1310.4350","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1310.4350","created_at":"2026-05-18T03:10:23Z"},{"alias_kind":"arxiv_version","alias_value":"1310.4350v1","created_at":"2026-05-18T03:10:23Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.4350","created_at":"2026-05-18T03:10:23Z"},{"alias_kind":"pith_short_12","alias_value":"OXVJDPJTR65F","created_at":"2026-05-18T12:27:54Z"},{"alias_kind":"pith_short_16","alias_value":"OXVJDPJTR65FE5CG","created_at":"2026-05-18T12:27:54Z"},{"alias_kind":"pith_short_8","alias_value":"OXVJDPJT","created_at":"2026-05-18T12:27:54Z"}],"graph_snapshots":[{"event_id":"sha256:07994780a5055c6685090f45e947257e9917dc0c9e96b2647e0f424f927feac3","target":"graph","created_at":"2026-05-18T03:10:23Z","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":"Predictions of astrochemical models depend strongly on the reaction rate coefficients used in the simulations. We reviewed a number of key reactions for the chemistry of nitrogen-bearing species in the dense interstellar medium and proposed new reaction rate coefficients for those reactions. The details of the reviews are given in the form of a datasheet associated with each reaction. The new recommended rate coefficients are given with an uncertainty and a temperature range of validity and will be included in KIDA (http://kida.obs.u-bordeaux1.fr).","authors_text":"A. Bergeat, D. Talbi, I. W. M. Smith, J.-C. Loison, K. M. Hickson, S. J. Klippenstein, V. Wakelam, W. D. Geppert","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-10-16T12:35:53Z","title":"Review of important reactions for the nitrogen chemistry in the interstellar medium"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.4350","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":"sha256:937fdb270adf0bf10c6d83ed55c828de468f7bc991c068788b43d8a8f1a242f3","target":"record","created_at":"2026-05-18T03:10:23Z","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":"6ebe396cc26c2a6e5547f6530fcbe60fa901230835bb469788cd26674a97ccf3","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-10-16T12:35:53Z","title_canon_sha256":"e2fc2d9c9dffe6e812919ab4914b22b85b5041b0a1decc5a2adb8a4170b4ec5b"},"schema_version":"1.0","source":{"id":"1310.4350","kind":"arxiv","version":1}},"canonical_sha256":"75ea91bd338fba52744689318477f97ac873bd111c8dfe39b84e7c05b7136f80","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"75ea91bd338fba52744689318477f97ac873bd111c8dfe39b84e7c05b7136f80","first_computed_at":"2026-05-18T03:10:23.083793Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:10:23.083793Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"TEo+cZ6dB18a3SZDfDSHCYsFPqUwvJTSq3mWMaryETjLMHCBOwmH89iL8Q99cIUGRW0aQPdl+aie91mGKyrHAw==","signature_status":"signed_v1","signed_at":"2026-05-18T03:10:23.084548Z","signed_message":"canonical_sha256_bytes"},"source_id":"1310.4350","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:937fdb270adf0bf10c6d83ed55c828de468f7bc991c068788b43d8a8f1a242f3","sha256:07994780a5055c6685090f45e947257e9917dc0c9e96b2647e0f424f927feac3"],"state_sha256":"ac618187cf591ca6e77ada1979e9493a4aa658015c2858d604f60a8a220f9e88"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"HpXFSb+rrI4B0HMtS4h2BoWqF4QOWQIarSQg9OXWQg9ggHGaDLa3PEnCcQRu5x2IKvkQe3nQEnjxtD3C8tq/AA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-02T19:26:52.930283Z","bundle_sha256":"6701b63bb5ed11258627d1bddb95c106eda89413fec874bb559c474013ae8283"}}