{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:7JKLOUQMMT2TD2XRXVQVZVUEGC","short_pith_number":"pith:7JKLOUQM","canonical_record":{"source":{"id":"1210.2063","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-10-07T14:54:43Z","cross_cats_sorted":[],"title_canon_sha256":"466dd95c55a164349c45af93e4002f6939c2f613c8cd0d96ccaa103455ad8a5c","abstract_canon_sha256":"9c4549e3f10a9fcbd66ccc7f6ec9af0502e9234dabacc839717d3af3c5acf6bb"},"schema_version":"1.0"},"canonical_sha256":"fa54b7520c64f531eaf1bd615cd6843083dc0b75c2c3016e3d9142dad9d0bb48","source":{"kind":"arxiv","id":"1210.2063","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1210.2063","created_at":"2026-05-18T01:54:04Z"},{"alias_kind":"arxiv_version","alias_value":"1210.2063v1","created_at":"2026-05-18T01:54:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.2063","created_at":"2026-05-18T01:54:04Z"},{"alias_kind":"pith_short_12","alias_value":"7JKLOUQMMT2T","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_16","alias_value":"7JKLOUQMMT2TD2XR","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_8","alias_value":"7JKLOUQM","created_at":"2026-05-18T12:26:56Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:7JKLOUQMMT2TD2XRXVQVZVUEGC","target":"record","payload":{"canonical_record":{"source":{"id":"1210.2063","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-10-07T14:54:43Z","cross_cats_sorted":[],"title_canon_sha256":"466dd95c55a164349c45af93e4002f6939c2f613c8cd0d96ccaa103455ad8a5c","abstract_canon_sha256":"9c4549e3f10a9fcbd66ccc7f6ec9af0502e9234dabacc839717d3af3c5acf6bb"},"schema_version":"1.0"},"canonical_sha256":"fa54b7520c64f531eaf1bd615cd6843083dc0b75c2c3016e3d9142dad9d0bb48","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:04.856577Z","signature_b64":"PSFyGK7eWCJ0AbbI759J49f6mRqXr9xsrOT5uk6+0FsrDDNJo5+hE+WikB6tToNFSh+yuH4vkPrFLepe46WiDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fa54b7520c64f531eaf1bd615cd6843083dc0b75c2c3016e3d9142dad9d0bb48","last_reissued_at":"2026-05-18T01:54:04.856129Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:04.856129Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1210.2063","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":"2026-05-18T01:54:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mxAAynTAnFs1/Vam5x9ZTk9q2+YybZWiWZxepcc9/wmGBCT5PcRsongBaUvw1WFclF6DFgyz9ho0WFHjy9OdDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T16:39:49.256039Z"},"content_sha256":"2637453e3e01904b1be0c3c9f624bbde2ea9b3145d274440be1da5be539ac86b","schema_version":"1.0","event_id":"sha256:2637453e3e01904b1be0c3c9f624bbde2ea9b3145d274440be1da5be539ac86b"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:7JKLOUQMMT2TD2XRXVQVZVUEGC","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Initial phases of massive star formation in high infrared extinction clouds. II. Infall and onset of star formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"((1) Istituto di Astrofisica e Planetologia Spaziali (INAF-IAPS), 2), (2) Max-Planck-Institut fuer Radioastronomie, (3) European Southern Observatory), F. Schuller (3, F. Wyrowski (2), K. L. J. Rygl (1, K. M. Menten (2)","submitted_at":"2012-10-07T14:54:43Z","abstract_excerpt":"The onset of massive star formation is not well understood because of observational and theoretical difficulties. To find the dense and cold clumps where massive star formation can take place, we compiled a sample of high infrared extinction clouds, which were observed previously by us in the 1.2 mm continuum emission and ammonia. We try to understand the star-formation stages of the clumps in these high extinction clouds by studying the infall and outflow properties, the presence of a young stellar object (YSO), and the level of the CO depletion through a molecular line survey with the IRAM 3"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.2063","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":"2026-05-18T01:54:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"6RWRiMEfHAZKvBZwp5rsSdYbrt1w3KgBT1/PE+z8YQ0Yx8dch4LzOUK0hC+WpjNHGDdrqHg6R+JV2mwXb/H1CQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T16:39:49.256782Z"},"content_sha256":"d8ec8523f382d849be2dac4f6a39fc101016b5dfc47e38c84b271f70b78fb814","schema_version":"1.0","event_id":"sha256:d8ec8523f382d849be2dac4f6a39fc101016b5dfc47e38c84b271f70b78fb814"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/7JKLOUQMMT2TD2XRXVQVZVUEGC/bundle.json","state_url":"https://pith.science/pith/7JKLOUQMMT2TD2XRXVQVZVUEGC/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/7JKLOUQMMT2TD2XRXVQVZVUEGC/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":"2026-05-27T16:39:49Z","links":{"resolver":"https://pith.science/pith/7JKLOUQMMT2TD2XRXVQVZVUEGC","bundle":"https://pith.science/pith/7JKLOUQMMT2TD2XRXVQVZVUEGC/bundle.json","state":"https://pith.science/pith/7JKLOUQMMT2TD2XRXVQVZVUEGC/state.json","well_known_bundle":"https://pith.science/.well-known/pith/7JKLOUQMMT2TD2XRXVQVZVUEGC/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:7JKLOUQMMT2TD2XRXVQVZVUEGC","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":"9c4549e3f10a9fcbd66ccc7f6ec9af0502e9234dabacc839717d3af3c5acf6bb","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-10-07T14:54:43Z","title_canon_sha256":"466dd95c55a164349c45af93e4002f6939c2f613c8cd0d96ccaa103455ad8a5c"},"schema_version":"1.0","source":{"id":"1210.2063","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1210.2063","created_at":"2026-05-18T01:54:04Z"},{"alias_kind":"arxiv_version","alias_value":"1210.2063v1","created_at":"2026-05-18T01:54:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.2063","created_at":"2026-05-18T01:54:04Z"},{"alias_kind":"pith_short_12","alias_value":"7JKLOUQMMT2T","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_16","alias_value":"7JKLOUQMMT2TD2XR","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_8","alias_value":"7JKLOUQM","created_at":"2026-05-18T12:26:56Z"}],"graph_snapshots":[{"event_id":"sha256:d8ec8523f382d849be2dac4f6a39fc101016b5dfc47e38c84b271f70b78fb814","target":"graph","created_at":"2026-05-18T01:54:04Z","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":"The onset of massive star formation is not well understood because of observational and theoretical difficulties. To find the dense and cold clumps where massive star formation can take place, we compiled a sample of high infrared extinction clouds, which were observed previously by us in the 1.2 mm continuum emission and ammonia. We try to understand the star-formation stages of the clumps in these high extinction clouds by studying the infall and outflow properties, the presence of a young stellar object (YSO), and the level of the CO depletion through a molecular line survey with the IRAM 3","authors_text":"((1) Istituto di Astrofisica e Planetologia Spaziali (INAF-IAPS), 2), (2) Max-Planck-Institut fuer Radioastronomie, (3) European Southern Observatory), F. Schuller (3, F. Wyrowski (2), K. L. J. Rygl (1, K. M. Menten (2)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-10-07T14:54:43Z","title":"Initial phases of massive star formation in high infrared extinction clouds. II. Infall and onset of star formation"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.2063","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":"sha256:2637453e3e01904b1be0c3c9f624bbde2ea9b3145d274440be1da5be539ac86b","target":"record","created_at":"2026-05-18T01:54:04Z","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":"9c4549e3f10a9fcbd66ccc7f6ec9af0502e9234dabacc839717d3af3c5acf6bb","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-10-07T14:54:43Z","title_canon_sha256":"466dd95c55a164349c45af93e4002f6939c2f613c8cd0d96ccaa103455ad8a5c"},"schema_version":"1.0","source":{"id":"1210.2063","kind":"arxiv","version":1}},"canonical_sha256":"fa54b7520c64f531eaf1bd615cd6843083dc0b75c2c3016e3d9142dad9d0bb48","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"fa54b7520c64f531eaf1bd615cd6843083dc0b75c2c3016e3d9142dad9d0bb48","first_computed_at":"2026-05-18T01:54:04.856129Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:54:04.856129Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"PSFyGK7eWCJ0AbbI759J49f6mRqXr9xsrOT5uk6+0FsrDDNJo5+hE+WikB6tToNFSh+yuH4vkPrFLepe46WiDw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:54:04.856577Z","signed_message":"canonical_sha256_bytes"},"source_id":"1210.2063","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:2637453e3e01904b1be0c3c9f624bbde2ea9b3145d274440be1da5be539ac86b","sha256:d8ec8523f382d849be2dac4f6a39fc101016b5dfc47e38c84b271f70b78fb814"],"state_sha256":"13d55932e83ef327047dab9bf15e6f083e83ac47fee11c6a2c973e2c99f8589a"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ld7BnayJklXi4WgLt/gJXUsYkOaodWHSw7pi3J95IcjmX+PRTtfkmCr0BAFaOUJh4AAsQdzIxM07VhcbhgAUBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T16:39:49.260855Z","bundle_sha256":"0145f8d44192d2bdfb9ae6b48cec573df8094faac2338cee142355663e5045d1"}}