{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:6M7BCIXPYP4CFR7MF3DM7GSUMS","short_pith_number":"pith:6M7BCIXP","canonical_record":{"source":{"id":"1208.0599","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-08-02T20:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"765d209306175eac872de36a67b362c9571b89509a325a252a82ec273d5e247e","abstract_canon_sha256":"cc35b87f3a42bc4316e88290687000131cf4dc755854d2406539025f7053974b"},"schema_version":"1.0"},"canonical_sha256":"f33e1122efc3f822c7ec2ec6cf9a5464b4d79a21b5ad40ea2575f5d7d93d38c1","source":{"kind":"arxiv","id":"1208.0599","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1208.0599","created_at":"2026-05-18T01:55:23Z"},{"alias_kind":"arxiv_version","alias_value":"1208.0599v1","created_at":"2026-05-18T01:55:23Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.0599","created_at":"2026-05-18T01:55:23Z"},{"alias_kind":"pith_short_12","alias_value":"6M7BCIXPYP4C","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_16","alias_value":"6M7BCIXPYP4CFR7M","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_8","alias_value":"6M7BCIXP","created_at":"2026-05-18T12:26:56Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:6M7BCIXPYP4CFR7MF3DM7GSUMS","target":"record","payload":{"canonical_record":{"source":{"id":"1208.0599","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-08-02T20:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"765d209306175eac872de36a67b362c9571b89509a325a252a82ec273d5e247e","abstract_canon_sha256":"cc35b87f3a42bc4316e88290687000131cf4dc755854d2406539025f7053974b"},"schema_version":"1.0"},"canonical_sha256":"f33e1122efc3f822c7ec2ec6cf9a5464b4d79a21b5ad40ea2575f5d7d93d38c1","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:55:23.653201Z","signature_b64":"4C3MpIXxSPOWvqmGv7u5YMoId9SpewhttYOUcE3GB/Ki+yhrJymFItXqvTrruYSvBlOh9dQ8U6YkZREGf8DyCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f33e1122efc3f822c7ec2ec6cf9a5464b4d79a21b5ad40ea2575f5d7d93d38c1","last_reissued_at":"2026-05-18T01:55:23.652577Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:55:23.652577Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1208.0599","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":"2026-05-18T01:55:23Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"D8zBVPQ638mlQjVZhXBKtZEPLK8qyAjRhYB9yhCiVGCMVeIS6ut1f7o5Ytnc1R67vPHzMMK81zdx1ZOd3/RvBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T19:46:51.836702Z"},"content_sha256":"fb530488802999d41d32e16ec058dd7f532a2f194e7907b13a0456f94f009c73","schema_version":"1.0","event_id":"sha256:fb530488802999d41d32e16ec058dd7f532a2f194e7907b13a0456f94f009c73"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:6M7BCIXPYP4CFR7MF3DM7GSUMS","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The G305 star-forming complex: Embedded Massive Star Formation Discovered by Herschel Hi-GAL","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Faimali, J. S. Clark, J. S. Urquhart, L. Hindson, M. A. Thompson, M. Pestalozzi, M. Veneziani, S. Carey, S. Molinari, S. Shenoy","submitted_at":"2012-08-02T20:00:04Z","abstract_excerpt":"We present a Herschel far-infrared study towards the rich massive star- forming complex G305, utilising PACS 70, 160 {\\mu}m and SPIRE 250, 350, and 500 {\\mu}m observations from the Hi-GAL survey of the Galactic plane. The focus of this study is to identify the embedded massive star-forming population within G305, by combining far-infrared data with radio continuum, H2O maser, methanol maser, MIPS, and Red MSX Source survey data available from previous studies. By applying a frequentist technique we are able to identify a sample of the most likely associations within our multi-wavelength datase"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.0599","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":"2026-05-18T01:55:23Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"aWN73PQDj8FXyS0OxO1goHjBHZW30CptFcbJQGvYUGJkPLec6KIZ70rFiP+kpcVB8DlI9pnxgEBfM0DMXbWmCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T19:46:51.837049Z"},"content_sha256":"19b68a84a5e3e8a20da9ade8be2617da5f9ee89e4c2f0b72a510739af94cfa7c","schema_version":"1.0","event_id":"sha256:19b68a84a5e3e8a20da9ade8be2617da5f9ee89e4c2f0b72a510739af94cfa7c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/6M7BCIXPYP4CFR7MF3DM7GSUMS/bundle.json","state_url":"https://pith.science/pith/6M7BCIXPYP4CFR7MF3DM7GSUMS/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/6M7BCIXPYP4CFR7MF3DM7GSUMS/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":"2026-06-02T19:46:51Z","links":{"resolver":"https://pith.science/pith/6M7BCIXPYP4CFR7MF3DM7GSUMS","bundle":"https://pith.science/pith/6M7BCIXPYP4CFR7MF3DM7GSUMS/bundle.json","state":"https://pith.science/pith/6M7BCIXPYP4CFR7MF3DM7GSUMS/state.json","well_known_bundle":"https://pith.science/.well-known/pith/6M7BCIXPYP4CFR7MF3DM7GSUMS/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:6M7BCIXPYP4CFR7MF3DM7GSUMS","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":"cc35b87f3a42bc4316e88290687000131cf4dc755854d2406539025f7053974b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-08-02T20:00:04Z","title_canon_sha256":"765d209306175eac872de36a67b362c9571b89509a325a252a82ec273d5e247e"},"schema_version":"1.0","source":{"id":"1208.0599","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1208.0599","created_at":"2026-05-18T01:55:23Z"},{"alias_kind":"arxiv_version","alias_value":"1208.0599v1","created_at":"2026-05-18T01:55:23Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.0599","created_at":"2026-05-18T01:55:23Z"},{"alias_kind":"pith_short_12","alias_value":"6M7BCIXPYP4C","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_16","alias_value":"6M7BCIXPYP4CFR7M","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_8","alias_value":"6M7BCIXP","created_at":"2026-05-18T12:26:56Z"}],"graph_snapshots":[{"event_id":"sha256:19b68a84a5e3e8a20da9ade8be2617da5f9ee89e4c2f0b72a510739af94cfa7c","target":"graph","created_at":"2026-05-18T01:55:23Z","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 Herschel far-infrared study towards the rich massive star- forming complex G305, utilising PACS 70, 160 {\\mu}m and SPIRE 250, 350, and 500 {\\mu}m observations from the Hi-GAL survey of the Galactic plane. The focus of this study is to identify the embedded massive star-forming population within G305, by combining far-infrared data with radio continuum, H2O maser, methanol maser, MIPS, and Red MSX Source survey data available from previous studies. By applying a frequentist technique we are able to identify a sample of the most likely associations within our multi-wavelength datase","authors_text":"A. Faimali, J. S. Clark, J. S. Urquhart, L. Hindson, M. A. Thompson, M. Pestalozzi, M. Veneziani, S. Carey, S. Molinari, S. Shenoy","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-08-02T20:00:04Z","title":"The G305 star-forming complex: Embedded Massive Star Formation Discovered by Herschel Hi-GAL"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.0599","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:fb530488802999d41d32e16ec058dd7f532a2f194e7907b13a0456f94f009c73","target":"record","created_at":"2026-05-18T01:55:23Z","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":"cc35b87f3a42bc4316e88290687000131cf4dc755854d2406539025f7053974b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-08-02T20:00:04Z","title_canon_sha256":"765d209306175eac872de36a67b362c9571b89509a325a252a82ec273d5e247e"},"schema_version":"1.0","source":{"id":"1208.0599","kind":"arxiv","version":1}},"canonical_sha256":"f33e1122efc3f822c7ec2ec6cf9a5464b4d79a21b5ad40ea2575f5d7d93d38c1","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"f33e1122efc3f822c7ec2ec6cf9a5464b4d79a21b5ad40ea2575f5d7d93d38c1","first_computed_at":"2026-05-18T01:55:23.652577Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:55:23.652577Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"4C3MpIXxSPOWvqmGv7u5YMoId9SpewhttYOUcE3GB/Ki+yhrJymFItXqvTrruYSvBlOh9dQ8U6YkZREGf8DyCg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:55:23.653201Z","signed_message":"canonical_sha256_bytes"},"source_id":"1208.0599","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:fb530488802999d41d32e16ec058dd7f532a2f194e7907b13a0456f94f009c73","sha256:19b68a84a5e3e8a20da9ade8be2617da5f9ee89e4c2f0b72a510739af94cfa7c"],"state_sha256":"965c2170f978fe1ec3c12c6b6156b16a09aa472b18d116a2034ed4aa09bc76a5"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"RK9Z/ng/wYWlXiUmctHcl4uhbe3xUCCTV+wNrPCTBKaHw2MOhPbl06pyDJHcf6uFMzaAKQHFIyDbvDbDphhUAA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-02T19:46:51.839015Z","bundle_sha256":"7a63a62a5e10e3f30d4644f5cd01bdb37fe18d4373970d2bc58e3722e00cd398"}}