{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:CL364MA6EMNNRPZ3AQYUNAIOCS","short_pith_number":"pith:CL364MA6","canonical_record":{"source":{"id":"1706.04107","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-13T14:57:01Z","cross_cats_sorted":[],"title_canon_sha256":"5af399a94dd0dae54c5b893cecfb0adf06bab32a1a006218d515a8e4486acc90","abstract_canon_sha256":"d58ef66bcbfdf3b0596d19d77afe2c5f79b4ac15dc6a35880e17ebcd69cec280"},"schema_version":"1.0"},"canonical_sha256":"12f7ee301e231ad8bf3b043146810e14b539bf38b0709f56a593f47bd12b0a2f","source":{"kind":"arxiv","id":"1706.04107","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1706.04107","created_at":"2026-05-18T00:32:09Z"},{"alias_kind":"arxiv_version","alias_value":"1706.04107v1","created_at":"2026-05-18T00:32:09Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.04107","created_at":"2026-05-18T00:32:09Z"},{"alias_kind":"pith_short_12","alias_value":"CL364MA6EMNN","created_at":"2026-05-18T12:31:10Z"},{"alias_kind":"pith_short_16","alias_value":"CL364MA6EMNNRPZ3","created_at":"2026-05-18T12:31:10Z"},{"alias_kind":"pith_short_8","alias_value":"CL364MA6","created_at":"2026-05-18T12:31:10Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:CL364MA6EMNNRPZ3AQYUNAIOCS","target":"record","payload":{"canonical_record":{"source":{"id":"1706.04107","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-13T14:57:01Z","cross_cats_sorted":[],"title_canon_sha256":"5af399a94dd0dae54c5b893cecfb0adf06bab32a1a006218d515a8e4486acc90","abstract_canon_sha256":"d58ef66bcbfdf3b0596d19d77afe2c5f79b4ac15dc6a35880e17ebcd69cec280"},"schema_version":"1.0"},"canonical_sha256":"12f7ee301e231ad8bf3b043146810e14b539bf38b0709f56a593f47bd12b0a2f","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:32:09.554343Z","signature_b64":"etJ0zKAKYbEUCJ1PwRjD3dIbd79Z2sl1f/grUv7RoSfS+wWLglKkZi7tPMMe83nGO9PjYRfmjy+gMwepjkgsBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"12f7ee301e231ad8bf3b043146810e14b539bf38b0709f56a593f47bd12b0a2f","last_reissued_at":"2026-05-18T00:32:09.553723Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:32:09.553723Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1706.04107","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":"2026-05-18T00:32:09Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"m16CGPehoRhB/GyfUU87PDUUKppVdkT3lRk9x+cRZwZqRiRhVVhIMGEq274JCOogLZ7A2AlOBOdlQ9ggtuF6Dg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T11:55:51.105074Z"},"content_sha256":"9554c5e6712d5676d1bb5f966158220b9dbac07fac044ef7c5b662d63259745a","schema_version":"1.0","event_id":"sha256:9554c5e6712d5676d1bb5f966158220b9dbac07fac044ef7c5b662d63259745a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:CL364MA6EMNNRPZ3AQYUNAIOCS","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"ISM conditions in z~0.2 Lyman-Break Analogs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Contursi, A. Janssen, A.J. Baker, A. Poglitsch, A. Sternberg, A. Verma, B. Magnelli, D. Lutz, E. Sturm, J. Fischer, J. Gr\\'acia Carpio, L. J. Tacconi, M. Nielbock, R. Davies, R. Genzel, R. Herrera-Camus, S. Berta, S. Hailey-Dunsheath, S. Veilleux","submitted_at":"2017-06-13T14:57:01Z","abstract_excerpt":"We present an analysis of far--infrared (FIR) [CII] and [OI] fine structure line and continuum observations obtained with $Herschel$/PACS, and CO(1-0) observations obtained with the IRAM Plateau de Bure Interferometer, of Lyman Break Analogs (LBAs) at $z\\sim 0.2$. The principal aim of this work is to determine the typical ISM properties of $z\\sim 1-2$ Main Sequence (MS) galaxies, with stellar masses between $10^{9.5}$ and $10^{11}$ $M_{\\odot}$, which are currently not easily detectable in all these lines even with ALMA and NOEMA. We perform PDR modeling and apply different IR diagnostics to de"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.04107","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":"2026-05-18T00:32:09Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Cn8Z7cdcpBD9YXqPr74WoiaD9uqzhDUuCIcRecSPqns/oF90sQ0N8gdEpuG6WpApvQlKpBNOhQpTKOFl4iHvCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T11:55:51.105768Z"},"content_sha256":"43f79100d06b6e23c15be4d4d59938936c2fe95d5bba34a26dca631b0f91356e","schema_version":"1.0","event_id":"sha256:43f79100d06b6e23c15be4d4d59938936c2fe95d5bba34a26dca631b0f91356e"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/CL364MA6EMNNRPZ3AQYUNAIOCS/bundle.json","state_url":"https://pith.science/pith/CL364MA6EMNNRPZ3AQYUNAIOCS/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/CL364MA6EMNNRPZ3AQYUNAIOCS/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":"2026-05-27T11:55:51Z","links":{"resolver":"https://pith.science/pith/CL364MA6EMNNRPZ3AQYUNAIOCS","bundle":"https://pith.science/pith/CL364MA6EMNNRPZ3AQYUNAIOCS/bundle.json","state":"https://pith.science/pith/CL364MA6EMNNRPZ3AQYUNAIOCS/state.json","well_known_bundle":"https://pith.science/.well-known/pith/CL364MA6EMNNRPZ3AQYUNAIOCS/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:CL364MA6EMNNRPZ3AQYUNAIOCS","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":"d58ef66bcbfdf3b0596d19d77afe2c5f79b4ac15dc6a35880e17ebcd69cec280","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-13T14:57:01Z","title_canon_sha256":"5af399a94dd0dae54c5b893cecfb0adf06bab32a1a006218d515a8e4486acc90"},"schema_version":"1.0","source":{"id":"1706.04107","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1706.04107","created_at":"2026-05-18T00:32:09Z"},{"alias_kind":"arxiv_version","alias_value":"1706.04107v1","created_at":"2026-05-18T00:32:09Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.04107","created_at":"2026-05-18T00:32:09Z"},{"alias_kind":"pith_short_12","alias_value":"CL364MA6EMNN","created_at":"2026-05-18T12:31:10Z"},{"alias_kind":"pith_short_16","alias_value":"CL364MA6EMNNRPZ3","created_at":"2026-05-18T12:31:10Z"},{"alias_kind":"pith_short_8","alias_value":"CL364MA6","created_at":"2026-05-18T12:31:10Z"}],"graph_snapshots":[{"event_id":"sha256:43f79100d06b6e23c15be4d4d59938936c2fe95d5bba34a26dca631b0f91356e","target":"graph","created_at":"2026-05-18T00:32:09Z","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 an analysis of far--infrared (FIR) [CII] and [OI] fine structure line and continuum observations obtained with $Herschel$/PACS, and CO(1-0) observations obtained with the IRAM Plateau de Bure Interferometer, of Lyman Break Analogs (LBAs) at $z\\sim 0.2$. The principal aim of this work is to determine the typical ISM properties of $z\\sim 1-2$ Main Sequence (MS) galaxies, with stellar masses between $10^{9.5}$ and $10^{11}$ $M_{\\odot}$, which are currently not easily detectable in all these lines even with ALMA and NOEMA. We perform PDR modeling and apply different IR diagnostics to de","authors_text":"A. Contursi, A. Janssen, A.J. Baker, A. Poglitsch, A. Sternberg, A. Verma, B. Magnelli, D. Lutz, E. Sturm, J. Fischer, J. Gr\\'acia Carpio, L. J. Tacconi, M. Nielbock, R. Davies, R. Genzel, R. Herrera-Camus, S. Berta, S. Hailey-Dunsheath, S. Veilleux","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-13T14:57:01Z","title":"ISM conditions in z~0.2 Lyman-Break Analogs"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.04107","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":"sha256:9554c5e6712d5676d1bb5f966158220b9dbac07fac044ef7c5b662d63259745a","target":"record","created_at":"2026-05-18T00:32:09Z","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":"d58ef66bcbfdf3b0596d19d77afe2c5f79b4ac15dc6a35880e17ebcd69cec280","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-13T14:57:01Z","title_canon_sha256":"5af399a94dd0dae54c5b893cecfb0adf06bab32a1a006218d515a8e4486acc90"},"schema_version":"1.0","source":{"id":"1706.04107","kind":"arxiv","version":1}},"canonical_sha256":"12f7ee301e231ad8bf3b043146810e14b539bf38b0709f56a593f47bd12b0a2f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"12f7ee301e231ad8bf3b043146810e14b539bf38b0709f56a593f47bd12b0a2f","first_computed_at":"2026-05-18T00:32:09.553723Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:32:09.553723Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"etJ0zKAKYbEUCJ1PwRjD3dIbd79Z2sl1f/grUv7RoSfS+wWLglKkZi7tPMMe83nGO9PjYRfmjy+gMwepjkgsBw==","signature_status":"signed_v1","signed_at":"2026-05-18T00:32:09.554343Z","signed_message":"canonical_sha256_bytes"},"source_id":"1706.04107","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:9554c5e6712d5676d1bb5f966158220b9dbac07fac044ef7c5b662d63259745a","sha256:43f79100d06b6e23c15be4d4d59938936c2fe95d5bba34a26dca631b0f91356e"],"state_sha256":"ee1f7f8169f63d34533aafceac22925b45215fb9c3e9bbe69211bbf81fb244a0"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"d2gXq+CdK7zwjfPis52h2LLPoiLUhPM/GW+NxohvCCHiYcE9SvUcXS1wgBVgxaQVtxhmFNdmKFxkjliTiInRBg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T11:55:51.109283Z","bundle_sha256":"e937d52648ee4f746b4e0e2e669a7f6dd149fc2bbf591a4be68d3231a82d96d4"}}