{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:O5EEKQDIL4RFWSWIINGZZLCAIF","short_pith_number":"pith:O5EEKQDI","canonical_record":{"source":{"id":"1703.05764","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-03-16T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"7d3ec5e83109b86dbc091c433ec422f52518b9ce036b9afb61e4d24f541efad2","abstract_canon_sha256":"46abb22abe3656b117ff03f44cf1ab0357a38ced1291a52b3d8cb8e9dbd42401"},"schema_version":"1.0"},"canonical_sha256":"77484540685f225b4ac8434d9cac40414575844213eead69af50cf6668f9c671","source":{"kind":"arxiv","id":"1703.05764","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1703.05764","created_at":"2026-05-18T00:43:53Z"},{"alias_kind":"arxiv_version","alias_value":"1703.05764v1","created_at":"2026-05-18T00:43:53Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.05764","created_at":"2026-05-18T00:43:53Z"},{"alias_kind":"pith_short_12","alias_value":"O5EEKQDIL4RF","created_at":"2026-05-18T12:31:34Z"},{"alias_kind":"pith_short_16","alias_value":"O5EEKQDIL4RFWSWI","created_at":"2026-05-18T12:31:34Z"},{"alias_kind":"pith_short_8","alias_value":"O5EEKQDI","created_at":"2026-05-18T12:31:34Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:O5EEKQDIL4RFWSWIINGZZLCAIF","target":"record","payload":{"canonical_record":{"source":{"id":"1703.05764","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-03-16T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"7d3ec5e83109b86dbc091c433ec422f52518b9ce036b9afb61e4d24f541efad2","abstract_canon_sha256":"46abb22abe3656b117ff03f44cf1ab0357a38ced1291a52b3d8cb8e9dbd42401"},"schema_version":"1.0"},"canonical_sha256":"77484540685f225b4ac8434d9cac40414575844213eead69af50cf6668f9c671","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:43:53.517864Z","signature_b64":"dcHX8rpsubJ+R9ePgBFcJFcVPogPm6TDWhT8GzXm+ayG1SGHpNKkQedGiolfMHi0DOstqNFxvARzjthifI+mCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"77484540685f225b4ac8434d9cac40414575844213eead69af50cf6668f9c671","last_reissued_at":"2026-05-18T00:43:53.517226Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:43:53.517226Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1703.05764","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":"2026-05-18T00:43:53Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"i9ZXJ6Aqt4jhMI4POD+LVFXkAFa0XsODOQHEO7EOaCPdrq8laGsK5D72WZOaREoH0rHVIE4/fQzyrvqQWtHwAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T13:27:31.435807Z"},"content_sha256":"575ce12a09b8d0fbe1c8e8f989cf7c95b9d2d51f08086068ecee9b11abe76a61","schema_version":"1.0","event_id":"sha256:575ce12a09b8d0fbe1c8e8f989cf7c95b9d2d51f08086068ecee9b11abe76a61"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:O5EEKQDIL4RFWSWIINGZZLCAIF","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using [CI] and CO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Allison W. S. Man, Bitten Gullberg, Carlos De Breuck, Eelco van Kampen, Erica J. Nelson, Gerg\\\"o Popping, Marco Spaans, Matthieu B\\'ethermin, Pieter G. van Dokkum, Roberto Decarli, Scott C. Trager, Vincenzo Mainieri","submitted_at":"2017-03-16T18:00:01Z","abstract_excerpt":"We present ALMA detections of the [CI] 1-0, CO J=3-2, and CO J=4-3 emission lines, as well as the ALMA band 4 continuum for a compact star-forming galaxy (cSFG) at z=2.225, 3D-HST GS30274. As is typical for cSFGs, this galaxy has a stellar mass of $1.89 \\pm 0.47\\,\\times 10^{11}\\,\\rm{M}_\\odot$, with a star formation rate of $214\\pm44\\,\\rm{M}_\\odot\\,\\rm{yr}^{-1}$ putting it on the star-forming `main-sequence', but with an H-band effective radius of 2.5 kpc, making it much smaller than the bulk of `main-sequence' star-forming galaxies. The intensity ratio of the line detections yield an ISM densi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.05764","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":"2026-05-18T00:43:53Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"GHEqO+Xz0TVRQXH5aLPAS0hepoY1hjcj8BcmLZ6QzUIebYlIGvzajZiRv2XGL9M6i4H1UfC61m0wm8fmnRffCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T13:27:31.436500Z"},"content_sha256":"382d1cf277c6f33b782a439a80d9d2679c35ceff31420b983fdddf4ceb1ac9b2","schema_version":"1.0","event_id":"sha256:382d1cf277c6f33b782a439a80d9d2679c35ceff31420b983fdddf4ceb1ac9b2"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/O5EEKQDIL4RFWSWIINGZZLCAIF/bundle.json","state_url":"https://pith.science/pith/O5EEKQDIL4RFWSWIINGZZLCAIF/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/O5EEKQDIL4RFWSWIINGZZLCAIF/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":"2026-05-26T13:27:31Z","links":{"resolver":"https://pith.science/pith/O5EEKQDIL4RFWSWIINGZZLCAIF","bundle":"https://pith.science/pith/O5EEKQDIL4RFWSWIINGZZLCAIF/bundle.json","state":"https://pith.science/pith/O5EEKQDIL4RFWSWIINGZZLCAIF/state.json","well_known_bundle":"https://pith.science/.well-known/pith/O5EEKQDIL4RFWSWIINGZZLCAIF/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:O5EEKQDIL4RFWSWIINGZZLCAIF","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":"46abb22abe3656b117ff03f44cf1ab0357a38ced1291a52b3d8cb8e9dbd42401","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-03-16T18:00:01Z","title_canon_sha256":"7d3ec5e83109b86dbc091c433ec422f52518b9ce036b9afb61e4d24f541efad2"},"schema_version":"1.0","source":{"id":"1703.05764","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1703.05764","created_at":"2026-05-18T00:43:53Z"},{"alias_kind":"arxiv_version","alias_value":"1703.05764v1","created_at":"2026-05-18T00:43:53Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.05764","created_at":"2026-05-18T00:43:53Z"},{"alias_kind":"pith_short_12","alias_value":"O5EEKQDIL4RF","created_at":"2026-05-18T12:31:34Z"},{"alias_kind":"pith_short_16","alias_value":"O5EEKQDIL4RFWSWI","created_at":"2026-05-18T12:31:34Z"},{"alias_kind":"pith_short_8","alias_value":"O5EEKQDI","created_at":"2026-05-18T12:31:34Z"}],"graph_snapshots":[{"event_id":"sha256:382d1cf277c6f33b782a439a80d9d2679c35ceff31420b983fdddf4ceb1ac9b2","target":"graph","created_at":"2026-05-18T00:43:53Z","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 ALMA detections of the [CI] 1-0, CO J=3-2, and CO J=4-3 emission lines, as well as the ALMA band 4 continuum for a compact star-forming galaxy (cSFG) at z=2.225, 3D-HST GS30274. As is typical for cSFGs, this galaxy has a stellar mass of $1.89 \\pm 0.47\\,\\times 10^{11}\\,\\rm{M}_\\odot$, with a star formation rate of $214\\pm44\\,\\rm{M}_\\odot\\,\\rm{yr}^{-1}$ putting it on the star-forming `main-sequence', but with an H-band effective radius of 2.5 kpc, making it much smaller than the bulk of `main-sequence' star-forming galaxies. The intensity ratio of the line detections yield an ISM densi","authors_text":"Allison W. S. Man, Bitten Gullberg, Carlos De Breuck, Eelco van Kampen, Erica J. Nelson, Gerg\\\"o Popping, Marco Spaans, Matthieu B\\'ethermin, Pieter G. van Dokkum, Roberto Decarli, Scott C. Trager, Vincenzo Mainieri","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-03-16T18:00:01Z","title":"ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using [CI] and CO"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.05764","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":"sha256:575ce12a09b8d0fbe1c8e8f989cf7c95b9d2d51f08086068ecee9b11abe76a61","target":"record","created_at":"2026-05-18T00:43:53Z","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":"46abb22abe3656b117ff03f44cf1ab0357a38ced1291a52b3d8cb8e9dbd42401","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-03-16T18:00:01Z","title_canon_sha256":"7d3ec5e83109b86dbc091c433ec422f52518b9ce036b9afb61e4d24f541efad2"},"schema_version":"1.0","source":{"id":"1703.05764","kind":"arxiv","version":1}},"canonical_sha256":"77484540685f225b4ac8434d9cac40414575844213eead69af50cf6668f9c671","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"77484540685f225b4ac8434d9cac40414575844213eead69af50cf6668f9c671","first_computed_at":"2026-05-18T00:43:53.517226Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:43:53.517226Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"dcHX8rpsubJ+R9ePgBFcJFcVPogPm6TDWhT8GzXm+ayG1SGHpNKkQedGiolfMHi0DOstqNFxvARzjthifI+mCA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:43:53.517864Z","signed_message":"canonical_sha256_bytes"},"source_id":"1703.05764","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:575ce12a09b8d0fbe1c8e8f989cf7c95b9d2d51f08086068ecee9b11abe76a61","sha256:382d1cf277c6f33b782a439a80d9d2679c35ceff31420b983fdddf4ceb1ac9b2"],"state_sha256":"b67382ab556cf958af3ba5e2572c76cee1186b90831dc4f93cd6e0707e724eb1"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"BArug6KrkAkntTfyeySVZS1XCz//rLj72rvR7QGl8xJSDei4BHF69pTVKiDcZ3j75Fv244kF3xYr+Z9O5PBIBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T13:27:31.440002Z","bundle_sha256":"b741c8eabd369db4af6ccb6f3dc9ff1936f30d7503df4383259ceafa1ffd6567"}}