{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:N5FZMNWMLADAEAXRGWEVPUXIBA","short_pith_number":"pith:N5FZMNWM","canonical_record":{"source":{"id":"1602.00541","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-01T14:37:09Z","cross_cats_sorted":[],"title_canon_sha256":"39213b95c5eb70e2109b92bed93a34dc8967798fb09ca3b1bce22b8f4cc90257","abstract_canon_sha256":"16e315f36be5655af2ab1e6867023d79d95ce32d336dbea456fcaa9afb51bef1"},"schema_version":"1.0"},"canonical_sha256":"6f4b9636cc58060202f1358957d2e8080cd82439157ac129fc5996b1f208a09c","source":{"kind":"arxiv","id":"1602.00541","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1602.00541","created_at":"2026-05-18T01:19:01Z"},{"alias_kind":"arxiv_version","alias_value":"1602.00541v1","created_at":"2026-05-18T01:19:01Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.00541","created_at":"2026-05-18T01:19:01Z"},{"alias_kind":"pith_short_12","alias_value":"N5FZMNWMLADA","created_at":"2026-05-18T12:30:32Z"},{"alias_kind":"pith_short_16","alias_value":"N5FZMNWMLADAEAXR","created_at":"2026-05-18T12:30:32Z"},{"alias_kind":"pith_short_8","alias_value":"N5FZMNWM","created_at":"2026-05-18T12:30:32Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:N5FZMNWMLADAEAXRGWEVPUXIBA","target":"record","payload":{"canonical_record":{"source":{"id":"1602.00541","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-01T14:37:09Z","cross_cats_sorted":[],"title_canon_sha256":"39213b95c5eb70e2109b92bed93a34dc8967798fb09ca3b1bce22b8f4cc90257","abstract_canon_sha256":"16e315f36be5655af2ab1e6867023d79d95ce32d336dbea456fcaa9afb51bef1"},"schema_version":"1.0"},"canonical_sha256":"6f4b9636cc58060202f1358957d2e8080cd82439157ac129fc5996b1f208a09c","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:19:01.127869Z","signature_b64":"iGR2n+umlhr6ThykgsLMoZ8rpRymtQULBqmVby3ANvbTiY0nN5Wc+NRigL3ZsakRHpw8/onMh8i+cuO6ip+gAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6f4b9636cc58060202f1358957d2e8080cd82439157ac129fc5996b1f208a09c","last_reissued_at":"2026-05-18T01:19:01.127447Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:19:01.127447Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1602.00541","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":"2026-05-18T01:19:01Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ZKdFrEg1rCESZju0TosxVaGGRA4yUWPXYbK8o3Y9nwcARbmLuMivQZxEGst1iGGJmLvJCwKNF7UVH9njZN9YBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T23:04:45.105155Z"},"content_sha256":"bc399d7a12afaa5163f66e5aca010623bd518df4da86006081fdbc9b567f4d21","schema_version":"1.0","event_id":"sha256:bc399d7a12afaa5163f66e5aca010623bd518df4da86006081fdbc9b567f4d21"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:N5FZMNWMLADAEAXRGWEVPUXIBA","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Mantle formation, coagulation and the origin of cloud/core-shine: II. Comparison with observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A.P. Jones, E. Dartois, L. Gavilan, M. Godard, M. Koehler, N. Ysard","submitted_at":"2016-02-01T14:37:09Z","abstract_excerpt":"Many dense interstellar clouds are observable in emission in the near-IR, commonly referred to as \"Cloudshine\", and in the mid-IR, the so-called \"Coreshine\". These C-shine observations have usually been explained with grain growth but no model has yet been able to self-consistently explain the dust spectral energy distribution from the near-IR to the submm. We want to demonstrate the ability of our new core/mantle evolutionary dust model THEMIS (The Heterogeneous dust Evolution Model at the IaS), which has been shown to be valid in the far-IR and submm, to reproduce the C-shine observations. O"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.00541","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":"2026-05-18T01:19:01Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"DhZxftGlbs45oWQ3R253Xh2aYILwu24IiAUukP7bqlzOcuax0qA57mtJjW7d5aR1o/buo4YcsKBsiMWQE9ORCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T23:04:45.105931Z"},"content_sha256":"323b152d2a6385b5f30aad3a4778a7cdc18939fa5f8422fa617c5de27deef15a","schema_version":"1.0","event_id":"sha256:323b152d2a6385b5f30aad3a4778a7cdc18939fa5f8422fa617c5de27deef15a"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/N5FZMNWMLADAEAXRGWEVPUXIBA/bundle.json","state_url":"https://pith.science/pith/N5FZMNWMLADAEAXRGWEVPUXIBA/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/N5FZMNWMLADAEAXRGWEVPUXIBA/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":"2026-05-31T23:04:45Z","links":{"resolver":"https://pith.science/pith/N5FZMNWMLADAEAXRGWEVPUXIBA","bundle":"https://pith.science/pith/N5FZMNWMLADAEAXRGWEVPUXIBA/bundle.json","state":"https://pith.science/pith/N5FZMNWMLADAEAXRGWEVPUXIBA/state.json","well_known_bundle":"https://pith.science/.well-known/pith/N5FZMNWMLADAEAXRGWEVPUXIBA/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:N5FZMNWMLADAEAXRGWEVPUXIBA","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":"16e315f36be5655af2ab1e6867023d79d95ce32d336dbea456fcaa9afb51bef1","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-01T14:37:09Z","title_canon_sha256":"39213b95c5eb70e2109b92bed93a34dc8967798fb09ca3b1bce22b8f4cc90257"},"schema_version":"1.0","source":{"id":"1602.00541","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1602.00541","created_at":"2026-05-18T01:19:01Z"},{"alias_kind":"arxiv_version","alias_value":"1602.00541v1","created_at":"2026-05-18T01:19:01Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.00541","created_at":"2026-05-18T01:19:01Z"},{"alias_kind":"pith_short_12","alias_value":"N5FZMNWMLADA","created_at":"2026-05-18T12:30:32Z"},{"alias_kind":"pith_short_16","alias_value":"N5FZMNWMLADAEAXR","created_at":"2026-05-18T12:30:32Z"},{"alias_kind":"pith_short_8","alias_value":"N5FZMNWM","created_at":"2026-05-18T12:30:32Z"}],"graph_snapshots":[{"event_id":"sha256:323b152d2a6385b5f30aad3a4778a7cdc18939fa5f8422fa617c5de27deef15a","target":"graph","created_at":"2026-05-18T01:19:01Z","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":"Many dense interstellar clouds are observable in emission in the near-IR, commonly referred to as \"Cloudshine\", and in the mid-IR, the so-called \"Coreshine\". These C-shine observations have usually been explained with grain growth but no model has yet been able to self-consistently explain the dust spectral energy distribution from the near-IR to the submm. We want to demonstrate the ability of our new core/mantle evolutionary dust model THEMIS (The Heterogeneous dust Evolution Model at the IaS), which has been shown to be valid in the far-IR and submm, to reproduce the C-shine observations. O","authors_text":"A.P. Jones, E. Dartois, L. Gavilan, M. Godard, M. Koehler, N. Ysard","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-01T14:37:09Z","title":"Mantle formation, coagulation and the origin of cloud/core-shine: II. Comparison with observations"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.00541","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:bc399d7a12afaa5163f66e5aca010623bd518df4da86006081fdbc9b567f4d21","target":"record","created_at":"2026-05-18T01:19:01Z","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":"16e315f36be5655af2ab1e6867023d79d95ce32d336dbea456fcaa9afb51bef1","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-01T14:37:09Z","title_canon_sha256":"39213b95c5eb70e2109b92bed93a34dc8967798fb09ca3b1bce22b8f4cc90257"},"schema_version":"1.0","source":{"id":"1602.00541","kind":"arxiv","version":1}},"canonical_sha256":"6f4b9636cc58060202f1358957d2e8080cd82439157ac129fc5996b1f208a09c","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"6f4b9636cc58060202f1358957d2e8080cd82439157ac129fc5996b1f208a09c","first_computed_at":"2026-05-18T01:19:01.127447Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:19:01.127447Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"iGR2n+umlhr6ThykgsLMoZ8rpRymtQULBqmVby3ANvbTiY0nN5Wc+NRigL3ZsakRHpw8/onMh8i+cuO6ip+gAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:19:01.127869Z","signed_message":"canonical_sha256_bytes"},"source_id":"1602.00541","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:bc399d7a12afaa5163f66e5aca010623bd518df4da86006081fdbc9b567f4d21","sha256:323b152d2a6385b5f30aad3a4778a7cdc18939fa5f8422fa617c5de27deef15a"],"state_sha256":"a045085522ca0f855de1b7f91c154a21ef4edf199da54862b4137f5cf58eeed6"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"CU1H7fAR5ovweuvS++4VyvAc7znetdGi+/xhX0M+ENVs7z6QK/RECCqBNfANXSTSBdCY6BqmrYNIFLBRLBO9Cg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-31T23:04:45.110262Z","bundle_sha256":"2933a789a123b34cb18d01acd83b093847044cd0407960a7bd3d9531dba055ff"}}