{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:AYGKIM73LDTXZHN763F27QEUEH","short_pith_number":"pith:AYGKIM73","canonical_record":{"source":{"id":"1201.4798","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-01-23T18:21:55Z","cross_cats_sorted":[],"title_canon_sha256":"49d350e41d1f3aa0d8cd9f51a498e714907c24a8e64b7d12a34964c782976620","abstract_canon_sha256":"948574b5fc74ad5835301872d4976ede82ef9fa1e15fc7b82f6b5bd6ca7a8fc6"},"schema_version":"1.0"},"canonical_sha256":"060ca433fb58e77c9dbff6cbafc09421eee4b55da4693ed955fb927d87b5638d","source":{"kind":"arxiv","id":"1201.4798","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1201.4798","created_at":"2026-05-18T01:58:43Z"},{"alias_kind":"arxiv_version","alias_value":"1201.4798v1","created_at":"2026-05-18T01:58:43Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.4798","created_at":"2026-05-18T01:58:43Z"},{"alias_kind":"pith_short_12","alias_value":"AYGKIM73LDTX","created_at":"2026-05-18T12:26:58Z"},{"alias_kind":"pith_short_16","alias_value":"AYGKIM73LDTXZHN7","created_at":"2026-05-18T12:26:58Z"},{"alias_kind":"pith_short_8","alias_value":"AYGKIM73","created_at":"2026-05-18T12:26:58Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:AYGKIM73LDTXZHN763F27QEUEH","target":"record","payload":{"canonical_record":{"source":{"id":"1201.4798","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-01-23T18:21:55Z","cross_cats_sorted":[],"title_canon_sha256":"49d350e41d1f3aa0d8cd9f51a498e714907c24a8e64b7d12a34964c782976620","abstract_canon_sha256":"948574b5fc74ad5835301872d4976ede82ef9fa1e15fc7b82f6b5bd6ca7a8fc6"},"schema_version":"1.0"},"canonical_sha256":"060ca433fb58e77c9dbff6cbafc09421eee4b55da4693ed955fb927d87b5638d","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:43.311057Z","signature_b64":"yBmddOBEcUmdkJsFXFcqpf4g87qaJ9Z1EIvSA7cvNz0fr1qJTCTuKZEG6IyG89jz/eS7Ez1YGSIVD1/WF7cfDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"060ca433fb58e77c9dbff6cbafc09421eee4b55da4693ed955fb927d87b5638d","last_reissued_at":"2026-05-18T01:58:43.310386Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:43.310386Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1201.4798","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":"2026-05-18T01:58:43Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"pkyyOQ+GSc/Nel1V05qzRe25kvlYYyFFnVo5ZKxmjRDMHNj9lQtFuP/GjmaC862pL+EnpzGUIZnJ126FdkYhDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T09:46:47.442536Z"},"content_sha256":"9f9a6e302e2824914af86be811a894323c0ca26bb7cd9d589a9639e7bf31e04b","schema_version":"1.0","event_id":"sha256:9f9a6e302e2824914af86be811a894323c0ca26bb7cd9d589a9639e7bf31e04b"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:AYGKIM73LDTXZHN763F27QEUEH","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A spectral line survey of the starless and proto-stellar cores detected by BLAST toward the Vela-D molecular cloud","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Dario Lorenzetti, Davide Elia, Fabrizio Massi, Francesco Strafella, Jorge L. Morales Ortiz, Luca Olmi, Massimo De Luca, Michael Burton, Teresa Giannini","submitted_at":"2012-01-23T18:21:55Z","abstract_excerpt":"We present a 3-mm and 1.3-cm spectral line survey conducted with the Mopra 22-m and Parkes 64-m radio telescopes of a sample of 40 cold dust cores, previously observed with BLAST, including both starless and proto-stellar sources. 20 objects were also mapped using molecular tracers of dense gas. To trace the dense gas we used the molecular species NH3, N2H+, HNC, HCO+, H13CO+, HCN and H13CN, where some of them trace the more quiescent gas, while others are sensitive to more dynamical processes. The selected cores have a wide variety of morphological types and also show physical and chemical va"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.4798","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":"2026-05-18T01:58:43Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dLrr4vhN5urTcyVD6Si6kw53xtNFTvvuwx75frdq9/HBKILQicb+APGUbQ2Ux5h+KWcOnkJlAzLND+ftzJ/XCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T09:46:47.443209Z"},"content_sha256":"d8962bc0298b3007680d5d5174b519eebfd4260ece8a2a5d7fbddface87b8175","schema_version":"1.0","event_id":"sha256:d8962bc0298b3007680d5d5174b519eebfd4260ece8a2a5d7fbddface87b8175"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/AYGKIM73LDTXZHN763F27QEUEH/bundle.json","state_url":"https://pith.science/pith/AYGKIM73LDTXZHN763F27QEUEH/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/AYGKIM73LDTXZHN763F27QEUEH/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":"2026-05-26T09:46:47Z","links":{"resolver":"https://pith.science/pith/AYGKIM73LDTXZHN763F27QEUEH","bundle":"https://pith.science/pith/AYGKIM73LDTXZHN763F27QEUEH/bundle.json","state":"https://pith.science/pith/AYGKIM73LDTXZHN763F27QEUEH/state.json","well_known_bundle":"https://pith.science/.well-known/pith/AYGKIM73LDTXZHN763F27QEUEH/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:AYGKIM73LDTXZHN763F27QEUEH","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":"948574b5fc74ad5835301872d4976ede82ef9fa1e15fc7b82f6b5bd6ca7a8fc6","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-01-23T18:21:55Z","title_canon_sha256":"49d350e41d1f3aa0d8cd9f51a498e714907c24a8e64b7d12a34964c782976620"},"schema_version":"1.0","source":{"id":"1201.4798","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1201.4798","created_at":"2026-05-18T01:58:43Z"},{"alias_kind":"arxiv_version","alias_value":"1201.4798v1","created_at":"2026-05-18T01:58:43Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.4798","created_at":"2026-05-18T01:58:43Z"},{"alias_kind":"pith_short_12","alias_value":"AYGKIM73LDTX","created_at":"2026-05-18T12:26:58Z"},{"alias_kind":"pith_short_16","alias_value":"AYGKIM73LDTXZHN7","created_at":"2026-05-18T12:26:58Z"},{"alias_kind":"pith_short_8","alias_value":"AYGKIM73","created_at":"2026-05-18T12:26:58Z"}],"graph_snapshots":[{"event_id":"sha256:d8962bc0298b3007680d5d5174b519eebfd4260ece8a2a5d7fbddface87b8175","target":"graph","created_at":"2026-05-18T01:58:43Z","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":"We present a 3-mm and 1.3-cm spectral line survey conducted with the Mopra 22-m and Parkes 64-m radio telescopes of a sample of 40 cold dust cores, previously observed with BLAST, including both starless and proto-stellar sources. 20 objects were also mapped using molecular tracers of dense gas. To trace the dense gas we used the molecular species NH3, N2H+, HNC, HCO+, H13CO+, HCN and H13CN, where some of them trace the more quiescent gas, while others are sensitive to more dynamical processes. The selected cores have a wide variety of morphological types and also show physical and chemical va","authors_text":"Dario Lorenzetti, Davide Elia, Fabrizio Massi, Francesco Strafella, Jorge L. Morales Ortiz, Luca Olmi, Massimo De Luca, Michael Burton, Teresa Giannini","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-01-23T18:21:55Z","title":"A spectral line survey of the starless and proto-stellar cores detected by BLAST toward the Vela-D molecular cloud"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.4798","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":"sha256:9f9a6e302e2824914af86be811a894323c0ca26bb7cd9d589a9639e7bf31e04b","target":"record","created_at":"2026-05-18T01:58:43Z","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":"948574b5fc74ad5835301872d4976ede82ef9fa1e15fc7b82f6b5bd6ca7a8fc6","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-01-23T18:21:55Z","title_canon_sha256":"49d350e41d1f3aa0d8cd9f51a498e714907c24a8e64b7d12a34964c782976620"},"schema_version":"1.0","source":{"id":"1201.4798","kind":"arxiv","version":1}},"canonical_sha256":"060ca433fb58e77c9dbff6cbafc09421eee4b55da4693ed955fb927d87b5638d","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"060ca433fb58e77c9dbff6cbafc09421eee4b55da4693ed955fb927d87b5638d","first_computed_at":"2026-05-18T01:58:43.310386Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:58:43.310386Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"yBmddOBEcUmdkJsFXFcqpf4g87qaJ9Z1EIvSA7cvNz0fr1qJTCTuKZEG6IyG89jz/eS7Ez1YGSIVD1/WF7cfDQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:58:43.311057Z","signed_message":"canonical_sha256_bytes"},"source_id":"1201.4798","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:9f9a6e302e2824914af86be811a894323c0ca26bb7cd9d589a9639e7bf31e04b","sha256:d8962bc0298b3007680d5d5174b519eebfd4260ece8a2a5d7fbddface87b8175"],"state_sha256":"462496b3497de3cf5b6a2a29b218a7b8ac4f422c7b56dd0f7b8a8498ac349e2b"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"lAGZBRvYVPriuWe5LEPD43bAhYnCFQuvzHJpNM+WNF4P5aitAhmoyvmju+1M9YXPsiViHtPzeGGVtDO0x1a9Bw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T09:46:47.446769Z","bundle_sha256":"7017982a394c49cf0c66ff1a277ea63c138cccce68a6138d4f3e30557aafcaf7"}}