{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:VJGC2ZTPUGJGIFR63LCQGPGPGG","short_pith_number":"pith:VJGC2ZTP","canonical_record":{"source":{"id":"1406.1176","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-04T20:00:04Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"4f6eccb5203eff50e730d4e5b686449fab50d5702f5f44b9a5f7c254c4bda407","abstract_canon_sha256":"7cbbb3df49b06371cd7329555569a732049e565cd1f20217c4027f3926d249ea"},"schema_version":"1.0"},"canonical_sha256":"aa4c2d666fa19264163edac5033ccf318f6d1fa249327f8785602c53d1007833","source":{"kind":"arxiv","id":"1406.1176","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1406.1176","created_at":"2026-05-18T01:43:02Z"},{"alias_kind":"arxiv_version","alias_value":"1406.1176v1","created_at":"2026-05-18T01:43:02Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.1176","created_at":"2026-05-18T01:43:02Z"},{"alias_kind":"pith_short_12","alias_value":"VJGC2ZTPUGJG","created_at":"2026-05-18T12:28:54Z"},{"alias_kind":"pith_short_16","alias_value":"VJGC2ZTPUGJGIFR6","created_at":"2026-05-18T12:28:54Z"},{"alias_kind":"pith_short_8","alias_value":"VJGC2ZTP","created_at":"2026-05-18T12:28:54Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:VJGC2ZTPUGJGIFR63LCQGPGPGG","target":"record","payload":{"canonical_record":{"source":{"id":"1406.1176","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-04T20:00:04Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"4f6eccb5203eff50e730d4e5b686449fab50d5702f5f44b9a5f7c254c4bda407","abstract_canon_sha256":"7cbbb3df49b06371cd7329555569a732049e565cd1f20217c4027f3926d249ea"},"schema_version":"1.0"},"canonical_sha256":"aa4c2d666fa19264163edac5033ccf318f6d1fa249327f8785602c53d1007833","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:02.097335Z","signature_b64":"BNq3UhxavNZN+WHtFGAz7UoloDCLWVNG05uSyAVAJVSQ0cbVImiTOw7I4UfE2whXQUaJ+S9qNrAOy+CrZUP5Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aa4c2d666fa19264163edac5033ccf318f6d1fa249327f8785602c53d1007833","last_reissued_at":"2026-05-18T01:43:02.096829Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:02.096829Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1406.1176","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":"2026-05-18T01:43:02Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"un38qA13c7a8ORydzRD7NvDLAjU9CW2QPQli9KmGV6Cemj5T44ClbqpCKG7SWz5u1YLgZthILsEc0tBvEL7wCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T14:07:14.910895Z"},"content_sha256":"3cd4a6ea9fc5951d79d2e45d3f93e1b0b879af6e1e3acb348c13c553b6261d8a","schema_version":"1.0","event_id":"sha256:3cd4a6ea9fc5951d79d2e45d3f93e1b0b879af6e1e3acb348c13c553b6261d8a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:VJGC2ZTPUGJGIFR63LCQGPGPGG","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Molecular gas properties of UV-luminous star-forming galaxies at low redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Basu-Zych, D. C. Martin, L. P\\'erez, R. A. Overzier, T. S. Gon\\c{c}alves","submitted_at":"2014-06-04T20:00:04Z","abstract_excerpt":"Lyman break analogues (LBAs) are a population of star-forming galaxies at low redshift (z ~ 0.2) selected in the ultraviolet (UV). These objects present higher star formation rates and lower dust extinction than other galaxies with similar masses and luminosities in the local universe. In this work we present results from a survey with the Combined Array for Research in Millimetre-wave Astronomy (CARMA) to detect CO(1-0) emission in LBAs, in order to analyse the properties of the molecular gas in these galaxies. Our results show that LBAs follow the same Schmidt-Kennicutt law as local galaxies"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.1176","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":"2026-05-18T01:43:02Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"b2bI7RnocZZAjo7CfJftZV4ZeZBAGwZbSqp5udu4qeIz1pUxvWB0OqaE/hNlNfIQwS2sqKdOo+fQ/g865hhfCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T14:07:14.911608Z"},"content_sha256":"e2384580e252aaedb5f72bdb4180eda8f1c0a38f7fa36677104f7d24de5c02ea","schema_version":"1.0","event_id":"sha256:e2384580e252aaedb5f72bdb4180eda8f1c0a38f7fa36677104f7d24de5c02ea"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/VJGC2ZTPUGJGIFR63LCQGPGPGG/bundle.json","state_url":"https://pith.science/pith/VJGC2ZTPUGJGIFR63LCQGPGPGG/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/VJGC2ZTPUGJGIFR63LCQGPGPGG/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":"2026-05-27T14:07:14Z","links":{"resolver":"https://pith.science/pith/VJGC2ZTPUGJGIFR63LCQGPGPGG","bundle":"https://pith.science/pith/VJGC2ZTPUGJGIFR63LCQGPGPGG/bundle.json","state":"https://pith.science/pith/VJGC2ZTPUGJGIFR63LCQGPGPGG/state.json","well_known_bundle":"https://pith.science/.well-known/pith/VJGC2ZTPUGJGIFR63LCQGPGPGG/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:VJGC2ZTPUGJGIFR63LCQGPGPGG","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":"7cbbb3df49b06371cd7329555569a732049e565cd1f20217c4027f3926d249ea","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-04T20:00:04Z","title_canon_sha256":"4f6eccb5203eff50e730d4e5b686449fab50d5702f5f44b9a5f7c254c4bda407"},"schema_version":"1.0","source":{"id":"1406.1176","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1406.1176","created_at":"2026-05-18T01:43:02Z"},{"alias_kind":"arxiv_version","alias_value":"1406.1176v1","created_at":"2026-05-18T01:43:02Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.1176","created_at":"2026-05-18T01:43:02Z"},{"alias_kind":"pith_short_12","alias_value":"VJGC2ZTPUGJG","created_at":"2026-05-18T12:28:54Z"},{"alias_kind":"pith_short_16","alias_value":"VJGC2ZTPUGJGIFR6","created_at":"2026-05-18T12:28:54Z"},{"alias_kind":"pith_short_8","alias_value":"VJGC2ZTP","created_at":"2026-05-18T12:28:54Z"}],"graph_snapshots":[{"event_id":"sha256:e2384580e252aaedb5f72bdb4180eda8f1c0a38f7fa36677104f7d24de5c02ea","target":"graph","created_at":"2026-05-18T01:43:02Z","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":"Lyman break analogues (LBAs) are a population of star-forming galaxies at low redshift (z ~ 0.2) selected in the ultraviolet (UV). These objects present higher star formation rates and lower dust extinction than other galaxies with similar masses and luminosities in the local universe. In this work we present results from a survey with the Combined Array for Research in Millimetre-wave Astronomy (CARMA) to detect CO(1-0) emission in LBAs, in order to analyse the properties of the molecular gas in these galaxies. Our results show that LBAs follow the same Schmidt-Kennicutt law as local galaxies","authors_text":"A. Basu-Zych, D. C. Martin, L. P\\'erez, R. A. Overzier, T. S. Gon\\c{c}alves","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-04T20:00:04Z","title":"Molecular gas properties of UV-luminous star-forming galaxies at low redshift"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.1176","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":"sha256:3cd4a6ea9fc5951d79d2e45d3f93e1b0b879af6e1e3acb348c13c553b6261d8a","target":"record","created_at":"2026-05-18T01:43:02Z","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":"7cbbb3df49b06371cd7329555569a732049e565cd1f20217c4027f3926d249ea","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-04T20:00:04Z","title_canon_sha256":"4f6eccb5203eff50e730d4e5b686449fab50d5702f5f44b9a5f7c254c4bda407"},"schema_version":"1.0","source":{"id":"1406.1176","kind":"arxiv","version":1}},"canonical_sha256":"aa4c2d666fa19264163edac5033ccf318f6d1fa249327f8785602c53d1007833","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"aa4c2d666fa19264163edac5033ccf318f6d1fa249327f8785602c53d1007833","first_computed_at":"2026-05-18T01:43:02.096829Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:43:02.096829Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"BNq3UhxavNZN+WHtFGAz7UoloDCLWVNG05uSyAVAJVSQ0cbVImiTOw7I4UfE2whXQUaJ+S9qNrAOy+CrZUP5Cg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:43:02.097335Z","signed_message":"canonical_sha256_bytes"},"source_id":"1406.1176","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3cd4a6ea9fc5951d79d2e45d3f93e1b0b879af6e1e3acb348c13c553b6261d8a","sha256:e2384580e252aaedb5f72bdb4180eda8f1c0a38f7fa36677104f7d24de5c02ea"],"state_sha256":"652551a5ccaf2af3fa57ca37be97302c905502e96457e8682785bce217b5e6c1"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"GNDaoNSd6UjuGhiFfQxogjZwGfPSavtAJNwkNbl6khJcoGQugLJj/iFsOFCrHX9clnAYVW8mCXMtXDn8mm5CDg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T14:07:14.916046Z","bundle_sha256":"81e30b5fa51e2fb309b737121133f2d92d8a3d83aa1781c8128c02290899d233"}}