{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:FW74SM5W4K3BW52U5MEGNQZQXP","short_pith_number":"pith:FW74SM5W","canonical_record":{"source":{"id":"1605.08360","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-26T16:48:47Z","cross_cats_sorted":[],"title_canon_sha256":"aa7aa5ea7dd5f804fe447c9debfd6e4ccf69672a088739d975cc951897aaaff7","abstract_canon_sha256":"b692eafb00622f79275e9eb07580e2ba805793430a6cc2974036bd8ba23a798c"},"schema_version":"1.0"},"canonical_sha256":"2dbfc933b6e2b61b7754eb0866c330bbe32d6cf05642aeaff9ed30c29ac087fd","source":{"kind":"arxiv","id":"1605.08360","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1605.08360","created_at":"2026-05-18T01:07:16Z"},{"alias_kind":"arxiv_version","alias_value":"1605.08360v3","created_at":"2026-05-18T01:07:16Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.08360","created_at":"2026-05-18T01:07:16Z"},{"alias_kind":"pith_short_12","alias_value":"FW74SM5W4K3B","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_16","alias_value":"FW74SM5W4K3BW52U","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_8","alias_value":"FW74SM5W","created_at":"2026-05-18T12:30:15Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:FW74SM5W4K3BW52U5MEGNQZQXP","target":"record","payload":{"canonical_record":{"source":{"id":"1605.08360","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-26T16:48:47Z","cross_cats_sorted":[],"title_canon_sha256":"aa7aa5ea7dd5f804fe447c9debfd6e4ccf69672a088739d975cc951897aaaff7","abstract_canon_sha256":"b692eafb00622f79275e9eb07580e2ba805793430a6cc2974036bd8ba23a798c"},"schema_version":"1.0"},"canonical_sha256":"2dbfc933b6e2b61b7754eb0866c330bbe32d6cf05642aeaff9ed30c29ac087fd","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:07:16.316437Z","signature_b64":"OmJI1CwR6f166nAhaT4PtAkr5wPMNLUpPLPRfpr3G6xYXCkqElthsI/5+CDFFx9Bn9VyIhh3+lHADsnYGOU1Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2dbfc933b6e2b61b7754eb0866c330bbe32d6cf05642aeaff9ed30c29ac087fd","last_reissued_at":"2026-05-18T01:07:16.315866Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:07:16.315866Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1605.08360","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:07:16Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"7P2G3HUwuDlcTQVtFfhL0oAHw/YYemaXDPsVfh3wrUIX5Jiw67JRrqx+EtZU22B0fPX8b4EwSt1byTGbXcGoBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T16:12:18.422883Z"},"content_sha256":"7daf1de7808df5e546b528125cb8585d41d0651abf99cd3ee3396127e02bb679","schema_version":"1.0","event_id":"sha256:7daf1de7808df5e546b528125cb8585d41d0651abf99cd3ee3396127e02bb679"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:FW74SM5W4K3BW52U5MEGNQZQXP","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Probing interstellar turbulence in cirrus with deep optical imaging: no sign of energy dissipation at 0.01 pc scale","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"E. Karabal, F. Marleau, J.-C. Cuillandre, M.-A. Miville-Deschenes, P.-A. Duc, P. Didelon, S. Gwyn","submitted_at":"2016-05-26T16:48:47Z","abstract_excerpt":"Diffuse Galactic light has been observed in the optical since the 1930s. We propose that, when observed in the optical with deep imaging surveys, it can be used as a tracer of the turbulent cascade in the diffuse interstellar medium (ISM), down to scales of about 1 arcsec. Here we present a power spectrum analysis of the dust column density of a diffuse cirrus at high Galactic latitude (l ~ 198 deg, b ~ 32 deg) as derived from the combination of a MegaCam g-band image, obtained as part of the MATLAS large programme at the CFHT, with Planck radiance and Wise 12 micron data. The combination of t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.08360","kind":"arxiv","version":3},"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":"2026-05-18T01:07:16Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Uv0ybH20zu5BUIa6NnX54rEDvFM+qi46z+W9WZAJREsLuro6dz7H0rkhOiVj/Y6F7j/XADQ0KUULjTqZQVPOAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T16:12:18.423228Z"},"content_sha256":"10c667917a0c11e1e33693b7ca1f45d94b5fe217e8594bd84bde9e312353d5e5","schema_version":"1.0","event_id":"sha256:10c667917a0c11e1e33693b7ca1f45d94b5fe217e8594bd84bde9e312353d5e5"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/FW74SM5W4K3BW52U5MEGNQZQXP/bundle.json","state_url":"https://pith.science/pith/FW74SM5W4K3BW52U5MEGNQZQXP/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/FW74SM5W4K3BW52U5MEGNQZQXP/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":"2026-05-26T16:12:18Z","links":{"resolver":"https://pith.science/pith/FW74SM5W4K3BW52U5MEGNQZQXP","bundle":"https://pith.science/pith/FW74SM5W4K3BW52U5MEGNQZQXP/bundle.json","state":"https://pith.science/pith/FW74SM5W4K3BW52U5MEGNQZQXP/state.json","well_known_bundle":"https://pith.science/.well-known/pith/FW74SM5W4K3BW52U5MEGNQZQXP/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:FW74SM5W4K3BW52U5MEGNQZQXP","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":"b692eafb00622f79275e9eb07580e2ba805793430a6cc2974036bd8ba23a798c","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-26T16:48:47Z","title_canon_sha256":"aa7aa5ea7dd5f804fe447c9debfd6e4ccf69672a088739d975cc951897aaaff7"},"schema_version":"1.0","source":{"id":"1605.08360","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1605.08360","created_at":"2026-05-18T01:07:16Z"},{"alias_kind":"arxiv_version","alias_value":"1605.08360v3","created_at":"2026-05-18T01:07:16Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.08360","created_at":"2026-05-18T01:07:16Z"},{"alias_kind":"pith_short_12","alias_value":"FW74SM5W4K3B","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_16","alias_value":"FW74SM5W4K3BW52U","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_8","alias_value":"FW74SM5W","created_at":"2026-05-18T12:30:15Z"}],"graph_snapshots":[{"event_id":"sha256:10c667917a0c11e1e33693b7ca1f45d94b5fe217e8594bd84bde9e312353d5e5","target":"graph","created_at":"2026-05-18T01:07:16Z","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":"Diffuse Galactic light has been observed in the optical since the 1930s. We propose that, when observed in the optical with deep imaging surveys, it can be used as a tracer of the turbulent cascade in the diffuse interstellar medium (ISM), down to scales of about 1 arcsec. Here we present a power spectrum analysis of the dust column density of a diffuse cirrus at high Galactic latitude (l ~ 198 deg, b ~ 32 deg) as derived from the combination of a MegaCam g-band image, obtained as part of the MATLAS large programme at the CFHT, with Planck radiance and Wise 12 micron data. The combination of t","authors_text":"E. Karabal, F. Marleau, J.-C. Cuillandre, M.-A. Miville-Deschenes, P.-A. Duc, P. Didelon, S. Gwyn","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-26T16:48:47Z","title":"Probing interstellar turbulence in cirrus with deep optical imaging: no sign of energy dissipation at 0.01 pc scale"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.08360","kind":"arxiv","version":3},"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":"sha256:7daf1de7808df5e546b528125cb8585d41d0651abf99cd3ee3396127e02bb679","target":"record","created_at":"2026-05-18T01:07:16Z","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":"b692eafb00622f79275e9eb07580e2ba805793430a6cc2974036bd8ba23a798c","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-26T16:48:47Z","title_canon_sha256":"aa7aa5ea7dd5f804fe447c9debfd6e4ccf69672a088739d975cc951897aaaff7"},"schema_version":"1.0","source":{"id":"1605.08360","kind":"arxiv","version":3}},"canonical_sha256":"2dbfc933b6e2b61b7754eb0866c330bbe32d6cf05642aeaff9ed30c29ac087fd","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"2dbfc933b6e2b61b7754eb0866c330bbe32d6cf05642aeaff9ed30c29ac087fd","first_computed_at":"2026-05-18T01:07:16.315866Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:07:16.315866Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"OmJI1CwR6f166nAhaT4PtAkr5wPMNLUpPLPRfpr3G6xYXCkqElthsI/5+CDFFx9Bn9VyIhh3+lHADsnYGOU1Bw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:07:16.316437Z","signed_message":"canonical_sha256_bytes"},"source_id":"1605.08360","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:7daf1de7808df5e546b528125cb8585d41d0651abf99cd3ee3396127e02bb679","sha256:10c667917a0c11e1e33693b7ca1f45d94b5fe217e8594bd84bde9e312353d5e5"],"state_sha256":"b32f9ef74e20c2f618851d089289ee56828bbb298f18a87db5ac80ef5c4a147f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"pvYSYLyb+ApTE/K09FqmnOaJhL9lQQfyDN91zUJFqI0tSFYR1U265FO/EesNBf46SLCNdhPcCbFnbqL/zyi5Dw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T16:12:18.425399Z","bundle_sha256":"1aa295b69d609004a05e81b89905d527bf34d276e3c277121cdbe3b787312206"}}