{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:6IZLU3KW5SLYFQW6BN5R2Z2XEF","short_pith_number":"pith:6IZLU3KW","canonical_record":{"source":{"id":"1207.5564","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-07-23T23:42:31Z","cross_cats_sorted":[],"title_canon_sha256":"aa8976f21bdfcd3e3998fafc49356873ed1a276810ecff60125c8f2dc5abe28e","abstract_canon_sha256":"a6bdfeff4f47e1647f113ff411403f18029b52f67b6ba98b47235f55e1e983ad"},"schema_version":"1.0"},"canonical_sha256":"f232ba6d56ec9782c2de0b7b1d6757216ea5986894931e29fdb9def1798bf488","source":{"kind":"arxiv","id":"1207.5564","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"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:6IZLU3KW5SLYFQW6BN5R2Z2XEF","target":"record","payload":{"canonical_record":{"source":{"id":"1207.5564","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-07-23T23:42:31Z","cross_cats_sorted":[],"title_canon_sha256":"aa8976f21bdfcd3e3998fafc49356873ed1a276810ecff60125c8f2dc5abe28e","abstract_canon_sha256":"a6bdfeff4f47e1647f113ff411403f18029b52f67b6ba98b47235f55e1e983ad"},"schema_version":"1.0"},"canonical_sha256":"f232ba6d56ec9782c2de0b7b1d6757216ea5986894931e29fdb9def1798bf488","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:08.708428Z","signature_b64":"uMrBUOIFOPUSiTBuJ5p5rkZXYsZGse0M5yfsrJM14OtN7TMnsaV54V/xSZDnny/GCDWwbRz/atGGH9g0MdjwBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f232ba6d56ec9782c2de0b7b1d6757216ea5986894931e29fdb9def1798bf488","last_reissued_at":"2026-05-18T01:56:08.707691Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:08.707691Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1207.5564","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":"2026-05-18T01:56:08Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"CFeeNU4Bwd9C7iSL1Cb3PDHgaJcwKBC0D33teVZyPIxi1tWQgOy16jQVQZd/xEftNN3cS98XJOqgrTMHjcoPDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T15:08:54.834882Z"},"content_sha256":"d41b01193617d47a9582115de025213eb3ec0c81c4afe6c7d23223d9a5fd6e9b","schema_version":"1.0","event_id":"sha256:d41b01193617d47a9582115de025213eb3ec0c81c4afe6c7d23223d9a5fd6e9b"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:6IZLU3KW5SLYFQW6BN5R2Z2XEF","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"FMOS near-IR spectroscopy of Herschel selected galaxies: star formation rates, metallicity and dust attenuation at z~1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","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","submitted_at":"2012-07-23T23:42:31Z","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"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.5564","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":"2026-05-18T01:56:08Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"rp1a7imVvurleEWry2cAI7qbfj9e2Rjhri/wyHaHfmf+B1g/slButam2HXnkss0PDoEidAJMptMbXV7MHFqZBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T15:08:54.835592Z"},"content_sha256":"3d63b5db950089d0e34939e85c77c2bb5766a4c1b7bb9a3d173bb5b7928a7045","schema_version":"1.0","event_id":"sha256:3d63b5db950089d0e34939e85c77c2bb5766a4c1b7bb9a3d173bb5b7928a7045"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/6IZLU3KW5SLYFQW6BN5R2Z2XEF/bundle.json","state_url":"https://pith.science/pith/6IZLU3KW5SLYFQW6BN5R2Z2XEF/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/6IZLU3KW5SLYFQW6BN5R2Z2XEF/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":"2026-05-25T15:08:54Z","links":{"resolver":"https://pith.science/pith/6IZLU3KW5SLYFQW6BN5R2Z2XEF","bundle":"https://pith.science/pith/6IZLU3KW5SLYFQW6BN5R2Z2XEF/bundle.json","state":"https://pith.science/pith/6IZLU3KW5SLYFQW6BN5R2Z2XEF/state.json","well_known_bundle":"https://pith.science/.well-known/pith/6IZLU3KW5SLYFQW6BN5R2Z2XEF/bundle.json"},"state":{"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"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"IdJWCVxIFzqDquyeCQ//gUHb5SwBJNbCKDVJeZlw9D9u1/bKRcht/ethUzauFcZ9Qq4WfDb+NcuojRsn9GLlBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T15:08:54.838693Z","bundle_sha256":"04684e7bdad9a04cd72084c0eba0bfd643e6c66ce0e716d8e117cfa1cbbb7e00"}}