{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:6IZLU3KW5SLYFQW6BN5R2Z2XEF","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":"a6bdfeff4f47e1647f113ff411403f18029b52f67b6ba98b47235f55e1e983ad","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-07-23T23:42:31Z","title_canon_sha256":"aa8976f21bdfcd3e3998fafc49356873ed1a276810ecff60125c8f2dc5abe28e"},"schema_version":"1.0","source":{"id":"1207.5564","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1207.5564","created_at":"2026-05-18T01:56:08Z"},{"alias_kind":"arxiv_version","alias_value":"1207.5564v1","created_at":"2026-05-18T01:56:08Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1207.5564","created_at":"2026-05-18T01:56:08Z"},{"alias_kind":"pith_short_12","alias_value":"6IZLU3KW5SLY","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_16","alias_value":"6IZLU3KW5SLYFQW6","created_at":"2026-05-18T12:26:56Z"},{"alias_kind":"pith_short_8","alias_value":"6IZLU3KW","created_at":"2026-05-18T12:26:56Z"}],"graph_snapshots":[{"event_id":"sha256:3d63b5db950089d0e34939e85c77c2bb5766a4c1b7bb9a3d173bb5b7928a7045","target":"graph","created_at":"2026-05-18T01:56:08Z","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 investigate the properties (e.g. star formation rate, dust attentuation, stellar mass and metallicity) of a sample of infrared luminous galaxies at z \\sim 1 via near-IR spectroscopy with Subaru-FMOS. Our sample consists of Herschel SPIRE and Spitzer MIPS selected sources in the COSMOS field with photometric redshifts in the range 0.7 < z-phot < 1.8, which have been targeted in 2 pointings (0.5 sq. deg.) with FMOS. We find a modest success rate for emission line detections, with candidate H{\\alpha} emission lines detected for 57 of 168 SPIRE sources (34 per cent). By stacking the near-IR spe","authors_text":"A. Bunker, A. Conley, A. Cooray, B. Schulz, C. Casey, D. Bonfield, D. Farrah, D. L. Clements, Douglas Scott, E. Chapin, E. Curtis-Lake, E. Ibar, E. Macaulay, F. Iwamuro, G. Dalton, G. Magdis, G. Marsden, I. G. Roseboom (Edinburgh), I. Lewis, J. Bock, J. S. Dunlop, K. Ohta, K. Yabe, L. Wang, M. Akiyama, M. J. Page, M. Kimura, M. Sumiyoshi, M. Symeonidis, M. Zemcov, N. Takato, N. Tamura, S. J. Ham, S. J. Oliver, T.Maihara, T. Mauch, T. Totani, V. Buat, Y. Moritani","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-07-23T23:42:31Z","title":"FMOS near-IR spectroscopy of Herschel selected galaxies: star formation rates, metallicity and dust attenuation at z~1"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.5564","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:d41b01193617d47a9582115de025213eb3ec0c81c4afe6c7d23223d9a5fd6e9b","target":"record","created_at":"2026-05-18T01:56:08Z","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":"a6bdfeff4f47e1647f113ff411403f18029b52f67b6ba98b47235f55e1e983ad","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-07-23T23:42:31Z","title_canon_sha256":"aa8976f21bdfcd3e3998fafc49356873ed1a276810ecff60125c8f2dc5abe28e"},"schema_version":"1.0","source":{"id":"1207.5564","kind":"arxiv","version":1}},"canonical_sha256":"f232ba6d56ec9782c2de0b7b1d6757216ea5986894931e29fdb9def1798bf488","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"f232ba6d56ec9782c2de0b7b1d6757216ea5986894931e29fdb9def1798bf488","first_computed_at":"2026-05-18T01:56:08.707691Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:56:08.707691Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"uMrBUOIFOPUSiTBuJ5p5rkZXYsZGse0M5yfsrJM14OtN7TMnsaV54V/xSZDnny/GCDWwbRz/atGGH9g0MdjwBw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:56:08.708428Z","signed_message":"canonical_sha256_bytes"},"source_id":"1207.5564","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:d41b01193617d47a9582115de025213eb3ec0c81c4afe6c7d23223d9a5fd6e9b","sha256:3d63b5db950089d0e34939e85c77c2bb5766a4c1b7bb9a3d173bb5b7928a7045"],"state_sha256":"192a27b18b5385cc41251a0a986862fac22bf83ae3c1d54610b60c5547b96ae6"}