{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:2DYQNL7F7P3UD37UVBZXMKM4RT","short_pith_number":"pith:2DYQNL7F","canonical_record":{"source":{"id":"1204.3552","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-04-16T16:17:07Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"20c56197ece27a47f1ea06fb566610b7266cad211fd75a0ef27fc23952b5d13e","abstract_canon_sha256":"4486c23f8d167ada914b25a8ffb700f25e69d92dd61607daafb78b9fb997e267"},"schema_version":"1.0"},"canonical_sha256":"d0f106afe5fbf741eff4a87376299c8cdc821505ac36e7b181e21691da331b8e","source":{"kind":"arxiv","id":"1204.3552","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1204.3552","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"arxiv_version","alias_value":"1204.3552v2","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.3552","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"pith_short_12","alias_value":"2DYQNL7F7P3U","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"pith_short_16","alias_value":"2DYQNL7F7P3UD37U","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"pith_short_8","alias_value":"2DYQNL7F","created_at":"2026-07-04T19:56:32Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:2DYQNL7F7P3UD37UVBZXMKM4RT","target":"record","payload":{"canonical_record":{"source":{"id":"1204.3552","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-04-16T16:17:07Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"20c56197ece27a47f1ea06fb566610b7266cad211fd75a0ef27fc23952b5d13e","abstract_canon_sha256":"4486c23f8d167ada914b25a8ffb700f25e69d92dd61607daafb78b9fb997e267"},"schema_version":"1.0"},"canonical_sha256":"d0f106afe5fbf741eff4a87376299c8cdc821505ac36e7b181e21691da331b8e","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T19:56:32.591107Z","signature_b64":"CsfgpApwiYw/97ZpvJSaBAT5yk/tNR/8eUgHx/ulkCM/6H3yGlycH63OBAe30qk/67RY2iLbkZZM1NbsOZewCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d0f106afe5fbf741eff4a87376299c8cdc821505ac36e7b181e21691da331b8e","last_reissued_at":"2026-07-04T19:56:32.590587Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T19:56:32.590587Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1204.3552","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":"2026-07-04T19:56:32Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"iLdQC9n3w+drwx16+XQhiqLJSOry5cwd6qNpGaxqDGtZ5BPA1Gyxy7igYBCknrD5PxrkhO5n6AcLlKrDdtJeAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-06T21:52:25.886551Z"},"content_sha256":"7bc716e6c41fff29df125f4819616c7405cdae2ee09c1faa60691db694ee9ca0","schema_version":"1.0","event_id":"sha256:7bc716e6c41fff29df125f4819616c7405cdae2ee09c1faa60691db694ee9ca0"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:2DYQNL7F7P3UD37UVBZXMKM4RT","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Star Formation in the Milky Way and Nearby Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"Updated prescriptions for calculating star formation rates are presented, along with a review of how these rates relate to gas contents on scales from galaxies to molecular clouds.","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Neal J. Evans II, Robert C. Kennicutt Jr","submitted_at":"2012-04-16T16:17:07Z","abstract_excerpt":"We review progress over the past decade in observations of large-scale star formation, with a focus on the interface between extragalactic and Galactic studies. Methods of measuring gas contents and star formation rates are discussed, and updated prescriptions for calculating star formation rates are provided. We review relations between star formation and gas on scales ranging from entire galaxies to individual molecular clouds."},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"Updated prescriptions for calculating star formation rates are provided. Relations between star formation and gas are reviewed on scales ranging from entire galaxies to individual molecular clouds.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The methods and observations reviewed accurately capture the current understanding of star formation processes without significant biases in measurement techniques.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"Updated prescriptions for calculating star formation rates are presented, along with a review of how these rates relate to gas contents on scales from galaxies to molecular clouds.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"48b2654b1c51e22b8b7f2a93bd1741bc9e84f64022c8afa6cd801b378c5cc047"},"source":{"id":"1204.3552","kind":"arxiv","version":2},"verdict":{"id":"4f2a10d2-6832-426f-b6a7-72741f2d58c4","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-10T20:08:27.759742Z","strongest_claim":"Updated prescriptions for calculating star formation rates are provided. Relations between star formation and gas are reviewed on scales ranging from entire galaxies to individual molecular clouds.","one_line_summary":"A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The methods and observations reviewed accurately capture the current understanding of star formation processes without significant biases in measurement techniques.","pith_extraction_headline":"Updated prescriptions for calculating star formation rates are presented, along with a review of how these rates relate to gas contents on scales from galaxies to molecular clouds."},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1204.3552/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":300,"sample":[{"doi":"","year":1968,"title":"Bishop WH, Richards FM. 1968. Isoelectric point of a protein in the crosslinked crystalline state. J. Mol. Biol. 33:415--21","work_id":"66bd7eb8-6cdd-4cf8-aa85-76a7d4720cd6","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1983,"title":"Connolly ML. 1983. Analytical molecular surface calculation. J. Appl. Crystallogr. 16:548--58","work_id":"09e68218-1fc9-49f8-8e27-a78fb6102fcc","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1963,"title":"Doscher MS, Richards FM. 1963. The activity of an enzyme in the crystalline state: Ribonuclease-S. J. Biol. Chem. 238:2399--406","work_id":"e0672fe3-2626-4b99-b0f4-e43469a7bb70","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1974,"title":"Heitzmann H, Richards FM. 1974. Use of the avidin-biotin complex for specific staining of biological membranes in electron microscopy. Proc. Natl. Acad. Sci. USA 71:3537--41","work_id":"70571c8f-c0eb-4b4d-afdf-965b536a5b35","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1994,"title":"Hellinga HW, Richards FM. 1994. An analysis of packing in the protein folding problem. Optimal sequence selection in proteins of known structure by simulated evolution. Proc. Natl. Acad. Sci. USA. 91:","work_id":"bedc6702-a30e-4607-861d-ae00384f66ca","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":300,"snapshot_sha256":"ac982a98b279289c817c68f225da09693db81b427d7ca13762b443604aab01d8","internal_anchors":0},"formal_canon":{"evidence_count":2,"snapshot_sha256":"3042437677482dcd62e563559ae89ee8847b212392a0d3b42926914ee48e40b1"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":"4f2a10d2-6832-426f-b6a7-72741f2d58c4"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T19:56:32Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"zrk/eGzNLBVxdpy11UlL5zJFkRDWLMV2ks4G1q7SWUTzKjvx7qytkaEq1OtzxV3WWR+9zId8ppYBrLkWBXJRAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-06T21:52:25.888045Z"},"content_sha256":"0e26f20656c72ba72267eebe37a7cc77bcd69c9501d4e4b883dfe846817cde12","schema_version":"1.0","event_id":"sha256:0e26f20656c72ba72267eebe37a7cc77bcd69c9501d4e4b883dfe846817cde12"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/2DYQNL7F7P3UD37UVBZXMKM4RT/bundle.json","state_url":"https://pith.science/pith/2DYQNL7F7P3UD37UVBZXMKM4RT/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/2DYQNL7F7P3UD37UVBZXMKM4RT/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":"2026-08-06T21:52:25Z","links":{"resolver":"https://pith.science/pith/2DYQNL7F7P3UD37UVBZXMKM4RT","bundle":"https://pith.science/pith/2DYQNL7F7P3UD37UVBZXMKM4RT/bundle.json","state":"https://pith.science/pith/2DYQNL7F7P3UD37UVBZXMKM4RT/state.json","well_known_bundle":"https://pith.science/.well-known/pith/2DYQNL7F7P3UD37UVBZXMKM4RT/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:2DYQNL7F7P3UD37UVBZXMKM4RT","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":"4486c23f8d167ada914b25a8ffb700f25e69d92dd61607daafb78b9fb997e267","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-04-16T16:17:07Z","title_canon_sha256":"20c56197ece27a47f1ea06fb566610b7266cad211fd75a0ef27fc23952b5d13e"},"schema_version":"1.0","source":{"id":"1204.3552","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1204.3552","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"arxiv_version","alias_value":"1204.3552v2","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.3552","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"pith_short_12","alias_value":"2DYQNL7F7P3U","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"pith_short_16","alias_value":"2DYQNL7F7P3UD37U","created_at":"2026-07-04T19:56:32Z"},{"alias_kind":"pith_short_8","alias_value":"2DYQNL7F","created_at":"2026-07-04T19:56:32Z"}],"graph_snapshots":[{"event_id":"sha256:0e26f20656c72ba72267eebe37a7cc77bcd69c9501d4e4b883dfe846817cde12","target":"graph","created_at":"2026-07-04T19:56:32Z","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":4,"items":[{"attestation":"unclaimed","claim_id":"C1","kind":"strongest_claim","source":"verdict.strongest_claim","status":"machine_extracted","text":"Updated prescriptions for calculating star formation rates are provided. Relations between star formation and gas are reviewed on scales ranging from entire galaxies to individual molecular clouds."},{"attestation":"unclaimed","claim_id":"C2","kind":"weakest_assumption","source":"verdict.weakest_assumption","status":"machine_extracted","text":"The methods and observations reviewed accurately capture the current understanding of star formation processes without significant biases in measurement techniques."},{"attestation":"unclaimed","claim_id":"C3","kind":"one_line_summary","source":"verdict.one_line_summary","status":"machine_extracted","text":"A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions."},{"attestation":"unclaimed","claim_id":"C4","kind":"headline","source":"verdict.pith_extraction.headline","status":"machine_extracted","text":"Updated prescriptions for calculating star formation rates are presented, along with a review of how these rates relate to gas contents on scales from galaxies to molecular clouds."}],"snapshot_sha256":"48b2654b1c51e22b8b7f2a93bd1741bc9e84f64022c8afa6cd801b378c5cc047"},"formal_canon":{"evidence_count":2,"snapshot_sha256":"3042437677482dcd62e563559ae89ee8847b212392a0d3b42926914ee48e40b1"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/1204.3552/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We review progress over the past decade in observations of large-scale star formation, with a focus on the interface between extragalactic and Galactic studies. Methods of measuring gas contents and star formation rates are discussed, and updated prescriptions for calculating star formation rates are provided. We review relations between star formation and gas on scales ranging from entire galaxies to individual molecular clouds.","authors_text":"Neal J. Evans II, Robert C. Kennicutt Jr","cross_cats":["astro-ph.CO"],"headline":"Updated prescriptions for calculating star formation rates are presented, along with a review of how these rates relate to gas contents on scales from galaxies to molecular clouds.","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-04-16T16:17:07Z","title":"Star Formation in the Milky Way and Nearby Galaxies"},"references":{"count":300,"internal_anchors":0,"resolved_work":300,"sample":[{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":1,"title":"Bishop WH, Richards FM. 1968. Isoelectric point of a protein in the crosslinked crystalline state. J. Mol. Biol. 33:415--21","work_id":"66bd7eb8-6cdd-4cf8-aa85-76a7d4720cd6","year":1968},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":2,"title":"Connolly ML. 1983. Analytical molecular surface calculation. J. Appl. Crystallogr. 16:548--58","work_id":"09e68218-1fc9-49f8-8e27-a78fb6102fcc","year":1983},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":3,"title":"Doscher MS, Richards FM. 1963. The activity of an enzyme in the crystalline state: Ribonuclease-S. J. Biol. Chem. 238:2399--406","work_id":"e0672fe3-2626-4b99-b0f4-e43469a7bb70","year":1963},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":4,"title":"Heitzmann H, Richards FM. 1974. Use of the avidin-biotin complex for specific staining of biological membranes in electron microscopy. Proc. Natl. Acad. Sci. USA 71:3537--41","work_id":"70571c8f-c0eb-4b4d-afdf-965b536a5b35","year":1974},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":5,"title":"Hellinga HW, Richards FM. 1994. An analysis of packing in the protein folding problem. Optimal sequence selection in proteins of known structure by simulated evolution. Proc. Natl. Acad. Sci. USA. 91:","work_id":"bedc6702-a30e-4607-861d-ae00384f66ca","year":1994}],"snapshot_sha256":"ac982a98b279289c817c68f225da09693db81b427d7ca13762b443604aab01d8"},"source":{"id":"1204.3552","kind":"arxiv","version":2},"verdict":{"created_at":"2026-05-10T20:08:27.759742Z","id":"4f2a10d2-6832-426f-b6a7-72741f2d58c4","model_set":{"reader":"grok-4.3"},"one_line_summary":"A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"Updated prescriptions for calculating star formation rates are presented, along with a review of how these rates relate to gas contents on scales from galaxies to molecular clouds.","strongest_claim":"Updated prescriptions for calculating star formation rates are provided. Relations between star formation and gas are reviewed on scales ranging from entire galaxies to individual molecular clouds.","weakest_assumption":"The methods and observations reviewed accurately capture the current understanding of star formation processes without significant biases in measurement techniques."}},"verdict_id":"4f2a10d2-6832-426f-b6a7-72741f2d58c4"}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:7bc716e6c41fff29df125f4819616c7405cdae2ee09c1faa60691db694ee9ca0","target":"record","created_at":"2026-07-04T19:56:32Z","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":"4486c23f8d167ada914b25a8ffb700f25e69d92dd61607daafb78b9fb997e267","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-04-16T16:17:07Z","title_canon_sha256":"20c56197ece27a47f1ea06fb566610b7266cad211fd75a0ef27fc23952b5d13e"},"schema_version":"1.0","source":{"id":"1204.3552","kind":"arxiv","version":2}},"canonical_sha256":"d0f106afe5fbf741eff4a87376299c8cdc821505ac36e7b181e21691da331b8e","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"d0f106afe5fbf741eff4a87376299c8cdc821505ac36e7b181e21691da331b8e","first_computed_at":"2026-07-04T19:56:32.590587Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T19:56:32.590587Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"CsfgpApwiYw/97ZpvJSaBAT5yk/tNR/8eUgHx/ulkCM/6H3yGlycH63OBAe30qk/67RY2iLbkZZM1NbsOZewCw==","signature_status":"signed_v1","signed_at":"2026-07-04T19:56:32.591107Z","signed_message":"canonical_sha256_bytes"},"source_id":"1204.3552","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:7bc716e6c41fff29df125f4819616c7405cdae2ee09c1faa60691db694ee9ca0","sha256:0e26f20656c72ba72267eebe37a7cc77bcd69c9501d4e4b883dfe846817cde12"],"state_sha256":"0f77f1efb10cafda6c7f98f2e3b185c315cc6484342b3450ee121b9779747ff6"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"nyXtyNroKnYfMnmG9/He9SD1p8jhIZS39n88mOWeLwrOKGOA+oW/RcRbT1Y4RcM013jTPX68e5hKP55mMMGrAQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-06T21:52:25.894849Z","bundle_sha256":"bbab3623b14a7c9635b703398c758eaaae4095a7ce2cf53b0e0a61b760405929"}}