{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:JK6ZOAVZYWRXCM2B6ZURNN7XER","short_pith_number":"pith:JK6ZOAVZ","canonical_record":{"source":{"id":"1811.06577","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-11-15T20:06:17Z","cross_cats_sorted":[],"title_canon_sha256":"a99e3984daa8ee43152095ce1b2bfd789db2b4a4dd27a434a773bb4d2ecddf7f","abstract_canon_sha256":"684aba0c4b9013082da9a7886d061c50c8596d4e7e4794701f23e003021f875b"},"schema_version":"1.0"},"canonical_sha256":"4abd9702b9c5a3713341f66916b7f724549d4ce83512f4b3b873d89c5e4bb136","source":{"kind":"arxiv","id":"1811.06577","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1811.06577","created_at":"2026-05-17T23:58:36Z"},{"alias_kind":"arxiv_version","alias_value":"1811.06577v1","created_at":"2026-05-17T23:58:36Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.06577","created_at":"2026-05-17T23:58:36Z"},{"alias_kind":"pith_short_12","alias_value":"JK6ZOAVZYWRX","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_16","alias_value":"JK6ZOAVZYWRXCM2B","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_8","alias_value":"JK6ZOAVZ","created_at":"2026-05-18T12:32:31Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:JK6ZOAVZYWRXCM2B6ZURNN7XER","target":"record","payload":{"canonical_record":{"source":{"id":"1811.06577","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-11-15T20:06:17Z","cross_cats_sorted":[],"title_canon_sha256":"a99e3984daa8ee43152095ce1b2bfd789db2b4a4dd27a434a773bb4d2ecddf7f","abstract_canon_sha256":"684aba0c4b9013082da9a7886d061c50c8596d4e7e4794701f23e003021f875b"},"schema_version":"1.0"},"canonical_sha256":"4abd9702b9c5a3713341f66916b7f724549d4ce83512f4b3b873d89c5e4bb136","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:58:36.424021Z","signature_b64":"AbzWj52AZUcL8LgslNu4KS/H7Qwh++1NqwHruC8l11fxgjUuh5OtykZ5AhT0rLvBzR5JLHkcY6nrZq0AYKGGAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4abd9702b9c5a3713341f66916b7f724549d4ce83512f4b3b873d89c5e4bb136","last_reissued_at":"2026-05-17T23:58:36.423451Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:58:36.423451Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1811.06577","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":"2026-05-17T23:58:36Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"HIvzXp3oEQhKSx+nFKXMJFGw/2OVfkE4fYG3NorqiGbo5mbyJv5cZtWckuqq3bpMDQU4X5iZuYvxoXBexGuwAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T23:23:35.576773Z"},"content_sha256":"d9d3a1e21b5a0b817edbf1ba8d78b42f93d833781eb1fbaacf1572911b57f6ba","schema_version":"1.0","event_id":"sha256:d9d3a1e21b5a0b817edbf1ba8d78b42f93d833781eb1fbaacf1572911b57f6ba"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:JK6ZOAVZYWRXCM2B6ZURNN7XER","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Global Correlations Between the Radio Continuum, Infrared and CO Emission in Dwarf Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bruce Elmegreen, Casiana Munoz-Tunon, Fatemeh S. Tabatabaei, Jorge Sanchez Almeida, Mercedes E. Filho","submitted_at":"2018-11-15T20:06:17Z","abstract_excerpt":"Correlations between the radio continuum, infrared and CO emission are known to exist for several types of galaxies and across several orders of magnitude. However, the low-mass, low-luminosity and low-metallicity regime of these correlations is not well known. A sample of metal-rich and metal-poor dwarf galaxies from the literature has been assembled to explore this extreme regime. The results demonstrate that the properties of dwarf galaxies are not simple extensions of those of more massive galaxies; the different correlations reflect different star-forming conditions and different coupling"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.06577","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":"2026-05-17T23:58:36Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"SEzn5xYleiow4SJ/HQFnCiAkaGNnFIfxHQs9qMgcwETCZ3UFaf/30gRGD5Kvv12ivjOK2To/4NBVq6sLiUyVBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T23:23:35.577378Z"},"content_sha256":"edad13345a5d0fa9e94d10468af9cbcf44ffed49288ed1a67ba094024761c363","schema_version":"1.0","event_id":"sha256:edad13345a5d0fa9e94d10468af9cbcf44ffed49288ed1a67ba094024761c363"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/JK6ZOAVZYWRXCM2B6ZURNN7XER/bundle.json","state_url":"https://pith.science/pith/JK6ZOAVZYWRXCM2B6ZURNN7XER/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/JK6ZOAVZYWRXCM2B6ZURNN7XER/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":"2026-06-04T23:23:35Z","links":{"resolver":"https://pith.science/pith/JK6ZOAVZYWRXCM2B6ZURNN7XER","bundle":"https://pith.science/pith/JK6ZOAVZYWRXCM2B6ZURNN7XER/bundle.json","state":"https://pith.science/pith/JK6ZOAVZYWRXCM2B6ZURNN7XER/state.json","well_known_bundle":"https://pith.science/.well-known/pith/JK6ZOAVZYWRXCM2B6ZURNN7XER/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:JK6ZOAVZYWRXCM2B6ZURNN7XER","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":"684aba0c4b9013082da9a7886d061c50c8596d4e7e4794701f23e003021f875b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-11-15T20:06:17Z","title_canon_sha256":"a99e3984daa8ee43152095ce1b2bfd789db2b4a4dd27a434a773bb4d2ecddf7f"},"schema_version":"1.0","source":{"id":"1811.06577","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1811.06577","created_at":"2026-05-17T23:58:36Z"},{"alias_kind":"arxiv_version","alias_value":"1811.06577v1","created_at":"2026-05-17T23:58:36Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.06577","created_at":"2026-05-17T23:58:36Z"},{"alias_kind":"pith_short_12","alias_value":"JK6ZOAVZYWRX","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_16","alias_value":"JK6ZOAVZYWRXCM2B","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_8","alias_value":"JK6ZOAVZ","created_at":"2026-05-18T12:32:31Z"}],"graph_snapshots":[{"event_id":"sha256:edad13345a5d0fa9e94d10468af9cbcf44ffed49288ed1a67ba094024761c363","target":"graph","created_at":"2026-05-17T23:58:36Z","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":"Correlations between the radio continuum, infrared and CO emission are known to exist for several types of galaxies and across several orders of magnitude. However, the low-mass, low-luminosity and low-metallicity regime of these correlations is not well known. A sample of metal-rich and metal-poor dwarf galaxies from the literature has been assembled to explore this extreme regime. The results demonstrate that the properties of dwarf galaxies are not simple extensions of those of more massive galaxies; the different correlations reflect different star-forming conditions and different coupling","authors_text":"Bruce Elmegreen, Casiana Munoz-Tunon, Fatemeh S. Tabatabaei, Jorge Sanchez Almeida, Mercedes E. Filho","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-11-15T20:06:17Z","title":"Global Correlations Between the Radio Continuum, Infrared and CO Emission in Dwarf Galaxies"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.06577","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:d9d3a1e21b5a0b817edbf1ba8d78b42f93d833781eb1fbaacf1572911b57f6ba","target":"record","created_at":"2026-05-17T23:58:36Z","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":"684aba0c4b9013082da9a7886d061c50c8596d4e7e4794701f23e003021f875b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-11-15T20:06:17Z","title_canon_sha256":"a99e3984daa8ee43152095ce1b2bfd789db2b4a4dd27a434a773bb4d2ecddf7f"},"schema_version":"1.0","source":{"id":"1811.06577","kind":"arxiv","version":1}},"canonical_sha256":"4abd9702b9c5a3713341f66916b7f724549d4ce83512f4b3b873d89c5e4bb136","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"4abd9702b9c5a3713341f66916b7f724549d4ce83512f4b3b873d89c5e4bb136","first_computed_at":"2026-05-17T23:58:36.423451Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:58:36.423451Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"AbzWj52AZUcL8LgslNu4KS/H7Qwh++1NqwHruC8l11fxgjUuh5OtykZ5AhT0rLvBzR5JLHkcY6nrZq0AYKGGAw==","signature_status":"signed_v1","signed_at":"2026-05-17T23:58:36.424021Z","signed_message":"canonical_sha256_bytes"},"source_id":"1811.06577","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:d9d3a1e21b5a0b817edbf1ba8d78b42f93d833781eb1fbaacf1572911b57f6ba","sha256:edad13345a5d0fa9e94d10468af9cbcf44ffed49288ed1a67ba094024761c363"],"state_sha256":"7ab3530d09b92d3f4e1982ac54aa9c938c2514176744c0eb925d6650eaa03fd3"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"teWxBK7n1btu69ZNvKyzQUpbNyD9MzTHeC+TD3jBKg0zVEzwpPRuXXnYu083x1gQrkbmnhjnq+P+9tgNkByWDQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T23:23:35.579636Z","bundle_sha256":"a25d19ce367760128112dab3bfd5c92748145025ff3481a4e0c9dce51aef72aa"}}