{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:NNYIEZZCE4YD724ZC5YMYMN24Z","short_pith_number":"pith:NNYIEZZC","canonical_record":{"source":{"id":"1302.4477","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-18T22:46:23Z","cross_cats_sorted":[],"title_canon_sha256":"db56e064b3a964f397b6b78ff7e387d9b522d81e24a650ebd7118e3fe69ddd38","abstract_canon_sha256":"5abcd901084cb6a788be83609ec444313c233e400fc2cc5ca7b6ad8a12e753ec"},"schema_version":"1.0"},"canonical_sha256":"6b7082672227303feb991770cc31bae640de6ac74e3262bf1d912f90a8db0eb5","source":{"kind":"arxiv","id":"1302.4477","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1302.4477","created_at":"2026-05-18T01:51:35Z"},{"alias_kind":"arxiv_version","alias_value":"1302.4477v1","created_at":"2026-05-18T01:51:35Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.4477","created_at":"2026-05-18T01:51:35Z"},{"alias_kind":"pith_short_12","alias_value":"NNYIEZZCE4YD","created_at":"2026-05-18T12:27:52Z"},{"alias_kind":"pith_short_16","alias_value":"NNYIEZZCE4YD724Z","created_at":"2026-05-18T12:27:52Z"},{"alias_kind":"pith_short_8","alias_value":"NNYIEZZC","created_at":"2026-05-18T12:27:52Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:NNYIEZZCE4YD724ZC5YMYMN24Z","target":"record","payload":{"canonical_record":{"source":{"id":"1302.4477","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-18T22:46:23Z","cross_cats_sorted":[],"title_canon_sha256":"db56e064b3a964f397b6b78ff7e387d9b522d81e24a650ebd7118e3fe69ddd38","abstract_canon_sha256":"5abcd901084cb6a788be83609ec444313c233e400fc2cc5ca7b6ad8a12e753ec"},"schema_version":"1.0"},"canonical_sha256":"6b7082672227303feb991770cc31bae640de6ac74e3262bf1d912f90a8db0eb5","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:35.473058Z","signature_b64":"FkiXk6zdQyPGfZlDnGVUmn+fZhADojg2u31LaImqHT89wGmqkb4X547UR08bXHCJ4cchnuof9qzgiMoIksI+DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6b7082672227303feb991770cc31bae640de6ac74e3262bf1d912f90a8db0eb5","last_reissued_at":"2026-05-18T01:51:35.472662Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:35.472662Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1302.4477","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":"2026-05-18T01:51:35Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"inWsFAP4XTvDOco+75OpdXQFcVQAxva95HsVOZ3AcMi6NDcO1SrK91DZyErWyoRz/zKh+AYSx1ueholPUnF5Dg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T02:31:51.155462Z"},"content_sha256":"6daaafb2b7eee60eabb14311f659f96c2fc6842ef260034cd96368159f6fb67d","schema_version":"1.0","event_id":"sha256:6daaafb2b7eee60eabb14311f659f96c2fc6842ef260034cd96368159f6fb67d"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:NNYIEZZCE4YD724ZC5YMYMN24Z","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Mid-Infrared Properties of Nearby Luminous Infrared Galaxies I: Spitzer IRS Spectra for the GOALS Sample","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Evans, A.O. Petric, B. Chan, B.F. Madore, B. Schulz, C.R. Bridge, D. B. Sanders, D.C. Kim, D. Frayer, E.J. Murphy, E. Sturm, G. Bothun, H. Inami, H.W.W. Spoon, J.A. Rich, J.A. Surace, J.E. Melbourne, J. Howell, J. Marshall, J.M. Mazzarella, K. Iwasawa, K. Xu, L. Armus, L.J. Kewley, P. Appleton, S. Haan, S. Lord, S. Stierwalt, S. Veilleux, T. Diaz-Santos, T. Vavilkin, V. Charmandaris, V. U","submitted_at":"2013-02-18T22:46:23Z","abstract_excerpt":"The Great Observatories All-Sky LIRG Survey (GOALS) is a multiwavelength study of luminous infrared galaxies (LIRGs) in the local universe. Here we present low resolution Spitzer spectra covering 5-38um and provide a basic analysis of the mid-IR spectral properties for nearby LIRGs. In a companion paper, we discuss detailed fits to the spectra. The GOALS sample of 244 nuclei in 180 luminous and 22 ultraluminous IR galaxies represents a complete subset of the IRAS RBGS and covers a range of merger stages, morphologies and spectral types. The majority (>60%) of GOALS LIRGs have high 6.2um PAH eq"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.4477","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":"2026-05-18T01:51:35Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"UJjqQat9FknEiVW0AIgza192BzRgIMvkZMMEsbzLi9920Cw4QQQ0PIGdlFg0EhMiTIbj5zwMpsG4G2ShCYbMBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T02:31:51.156027Z"},"content_sha256":"856c441edd5447772d02df3ba35a9cf60d5762c8a297cb478ece7aa7e07bff5c","schema_version":"1.0","event_id":"sha256:856c441edd5447772d02df3ba35a9cf60d5762c8a297cb478ece7aa7e07bff5c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/NNYIEZZCE4YD724ZC5YMYMN24Z/bundle.json","state_url":"https://pith.science/pith/NNYIEZZCE4YD724ZC5YMYMN24Z/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/NNYIEZZCE4YD724ZC5YMYMN24Z/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":"2026-06-05T02:31:51Z","links":{"resolver":"https://pith.science/pith/NNYIEZZCE4YD724ZC5YMYMN24Z","bundle":"https://pith.science/pith/NNYIEZZCE4YD724ZC5YMYMN24Z/bundle.json","state":"https://pith.science/pith/NNYIEZZCE4YD724ZC5YMYMN24Z/state.json","well_known_bundle":"https://pith.science/.well-known/pith/NNYIEZZCE4YD724ZC5YMYMN24Z/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:NNYIEZZCE4YD724ZC5YMYMN24Z","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":"5abcd901084cb6a788be83609ec444313c233e400fc2cc5ca7b6ad8a12e753ec","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-18T22:46:23Z","title_canon_sha256":"db56e064b3a964f397b6b78ff7e387d9b522d81e24a650ebd7118e3fe69ddd38"},"schema_version":"1.0","source":{"id":"1302.4477","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1302.4477","created_at":"2026-05-18T01:51:35Z"},{"alias_kind":"arxiv_version","alias_value":"1302.4477v1","created_at":"2026-05-18T01:51:35Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.4477","created_at":"2026-05-18T01:51:35Z"},{"alias_kind":"pith_short_12","alias_value":"NNYIEZZCE4YD","created_at":"2026-05-18T12:27:52Z"},{"alias_kind":"pith_short_16","alias_value":"NNYIEZZCE4YD724Z","created_at":"2026-05-18T12:27:52Z"},{"alias_kind":"pith_short_8","alias_value":"NNYIEZZC","created_at":"2026-05-18T12:27:52Z"}],"graph_snapshots":[{"event_id":"sha256:856c441edd5447772d02df3ba35a9cf60d5762c8a297cb478ece7aa7e07bff5c","target":"graph","created_at":"2026-05-18T01:51:35Z","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":"The Great Observatories All-Sky LIRG Survey (GOALS) is a multiwavelength study of luminous infrared galaxies (LIRGs) in the local universe. Here we present low resolution Spitzer spectra covering 5-38um and provide a basic analysis of the mid-IR spectral properties for nearby LIRGs. In a companion paper, we discuss detailed fits to the spectra. The GOALS sample of 244 nuclei in 180 luminous and 22 ultraluminous IR galaxies represents a complete subset of the IRAS RBGS and covers a range of merger stages, morphologies and spectral types. The majority (>60%) of GOALS LIRGs have high 6.2um PAH eq","authors_text":"A. Evans, A.O. Petric, B. Chan, B.F. Madore, B. Schulz, C.R. Bridge, D. B. Sanders, D.C. Kim, D. Frayer, E.J. Murphy, E. Sturm, G. Bothun, H. Inami, H.W.W. Spoon, J.A. Rich, J.A. Surace, J.E. Melbourne, J. Howell, J. Marshall, J.M. Mazzarella, K. Iwasawa, K. Xu, L. Armus, L.J. Kewley, P. Appleton, S. Haan, S. Lord, S. Stierwalt, S. Veilleux, T. Diaz-Santos, T. Vavilkin, V. Charmandaris, V. U","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-18T22:46:23Z","title":"Mid-Infrared Properties of Nearby Luminous Infrared Galaxies I: Spitzer IRS Spectra for the GOALS Sample"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.4477","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":"sha256:6daaafb2b7eee60eabb14311f659f96c2fc6842ef260034cd96368159f6fb67d","target":"record","created_at":"2026-05-18T01:51:35Z","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":"5abcd901084cb6a788be83609ec444313c233e400fc2cc5ca7b6ad8a12e753ec","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-18T22:46:23Z","title_canon_sha256":"db56e064b3a964f397b6b78ff7e387d9b522d81e24a650ebd7118e3fe69ddd38"},"schema_version":"1.0","source":{"id":"1302.4477","kind":"arxiv","version":1}},"canonical_sha256":"6b7082672227303feb991770cc31bae640de6ac74e3262bf1d912f90a8db0eb5","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"6b7082672227303feb991770cc31bae640de6ac74e3262bf1d912f90a8db0eb5","first_computed_at":"2026-05-18T01:51:35.472662Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:51:35.472662Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"FkiXk6zdQyPGfZlDnGVUmn+fZhADojg2u31LaImqHT89wGmqkb4X547UR08bXHCJ4cchnuof9qzgiMoIksI+DA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:51:35.473058Z","signed_message":"canonical_sha256_bytes"},"source_id":"1302.4477","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:6daaafb2b7eee60eabb14311f659f96c2fc6842ef260034cd96368159f6fb67d","sha256:856c441edd5447772d02df3ba35a9cf60d5762c8a297cb478ece7aa7e07bff5c"],"state_sha256":"5cd035f30e50a992bc757eed04e816225a9d2e01d12e7534e6eea9e647245503"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"lQoVOtaku4EaoRNXYkOGNMc4ijPzSNS/D3NyJ6sJnme0NBPYTLEwssKKdukkj8PPdgEuauGOY7inm5oI2IxFDA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-05T02:31:51.158914Z","bundle_sha256":"1b1489ca6023bd3dc7f145666ebb2fa4b22813c4cd55fb8a1b14b375508e1bfd"}}