{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2006:5EWVOUDVFR2HJ6LDNOSWUFUGUV","short_pith_number":"pith:5EWVOUDV","canonical_record":{"source":{"id":"astro-ph/0612199","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-07T22:43:19Z","cross_cats_sorted":[],"title_canon_sha256":"979adcc536954558a0516c5c4210446229159615d92ea836aa83763158d9e921","abstract_canon_sha256":"0a99d2fbb856c7fc6815db6a78eaf3c9ae3bf02dc46efc07c4b5d5f271b09c1f"},"schema_version":"1.0"},"canonical_sha256":"e92d5750752c7474f9636ba56a1686a56e927957c8b4335538f0e49df3086dd4","source":{"kind":"arxiv","id":"astro-ph/0612199","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0612199","created_at":"2026-05-18T04:37:01Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0612199v1","created_at":"2026-05-18T04:37:01Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0612199","created_at":"2026-05-18T04:37:01Z"},{"alias_kind":"pith_short_12","alias_value":"5EWVOUDVFR2H","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_16","alias_value":"5EWVOUDVFR2HJ6LD","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_8","alias_value":"5EWVOUDV","created_at":"2026-05-18T12:25:53Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2006:5EWVOUDVFR2HJ6LDNOSWUFUGUV","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0612199","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-07T22:43:19Z","cross_cats_sorted":[],"title_canon_sha256":"979adcc536954558a0516c5c4210446229159615d92ea836aa83763158d9e921","abstract_canon_sha256":"0a99d2fbb856c7fc6815db6a78eaf3c9ae3bf02dc46efc07c4b5d5f271b09c1f"},"schema_version":"1.0"},"canonical_sha256":"e92d5750752c7474f9636ba56a1686a56e927957c8b4335538f0e49df3086dd4","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:37:01.329740Z","signature_b64":"IxWaubaE6a2Z8owBV8KWrY2w3oAt/zNXQhIHuVT2fk1MKNLZgU9NbdNC+kUARRGhrNXZeEZ48+EX+ryV5/F2Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e92d5750752c7474f9636ba56a1686a56e927957c8b4335538f0e49df3086dd4","last_reissued_at":"2026-05-18T04:37:01.329062Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:37:01.329062Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0612199","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":"2026-05-18T04:37:01Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"eT3evZhQDcZWfnn29UfEQuYStQ9qh0TzNVN8d/9L2/F62WfNBOxzht9ALDzEGyR6m4gXeidL7l8OiiRI0DCHCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T01:38:25.679618Z"},"content_sha256":"81fbe073edb17ec8bccef996ca1dd7b367c3c88b97818688ec3cecac60786a0b","schema_version":"1.0","event_id":"sha256:81fbe073edb17ec8bccef996ca1dd7b367c3c88b97818688ec3cecac60786a0b"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2006:5EWVOUDVFR2HJ6LDNOSWUFUGUV","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Integral Field Spectroscopy of a Candidate Disk Galaxy at z~1.5 using Laser Guide Star Adaptive Optics","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A.Krabbe, A. Quirrenbach, C.C. Steidel, C. Iserlohe, D.K. Erb, D.R. Law, J.E. Larkin, J. Weiss, M.Barczys, M.W. McElwain, S.A. Wright","submitted_at":"2006-12-07T22:43:19Z","abstract_excerpt":"We present 0.1\" resolution near-infrared integral field spectroscopy of Halpha in a z=1.4781 star forming galaxy, Q2343-BM133. These observations were obtained with OSIRIS (OH Suppressing Infra-Red Imaging Spectrograph) using the W.M. Keck Observatory Laser Guide Star Adaptive Optics system. Halpha emission is resolved over a 0.8\" (6.8 kpc) x 0.5\" (4.3 kpc) region with a 0.1\" spatial resolution. We find a global flux of 4.2+/-0.6x10^{-16} ergs s^{-1} cm^{-2}, and detect a spatially resolved velocity gradient of ~134 km s^{-1} across the galaxy and a global velocity dispersion of 73+/-9 km s^{-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612199","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":"2026-05-18T04:37:01Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ixMDF/Sw2DKs6ubp4oPXmVzBInj4hC7cmIJT7kHwRUW1i1/grCBvyoUYamTgqOhQUYa+PFJVuVE/hFAIgrNYDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T01:38:25.680277Z"},"content_sha256":"3dcc3a287e9806e1bfd02ecddb2d879ed09d2ce554105525345354643d1430f0","schema_version":"1.0","event_id":"sha256:3dcc3a287e9806e1bfd02ecddb2d879ed09d2ce554105525345354643d1430f0"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/5EWVOUDVFR2HJ6LDNOSWUFUGUV/bundle.json","state_url":"https://pith.science/pith/5EWVOUDVFR2HJ6LDNOSWUFUGUV/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/5EWVOUDVFR2HJ6LDNOSWUFUGUV/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":"2026-06-05T01:38:25Z","links":{"resolver":"https://pith.science/pith/5EWVOUDVFR2HJ6LDNOSWUFUGUV","bundle":"https://pith.science/pith/5EWVOUDVFR2HJ6LDNOSWUFUGUV/bundle.json","state":"https://pith.science/pith/5EWVOUDVFR2HJ6LDNOSWUFUGUV/state.json","well_known_bundle":"https://pith.science/.well-known/pith/5EWVOUDVFR2HJ6LDNOSWUFUGUV/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2006:5EWVOUDVFR2HJ6LDNOSWUFUGUV","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":"0a99d2fbb856c7fc6815db6a78eaf3c9ae3bf02dc46efc07c4b5d5f271b09c1f","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-07T22:43:19Z","title_canon_sha256":"979adcc536954558a0516c5c4210446229159615d92ea836aa83763158d9e921"},"schema_version":"1.0","source":{"id":"astro-ph/0612199","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0612199","created_at":"2026-05-18T04:37:01Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0612199v1","created_at":"2026-05-18T04:37:01Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0612199","created_at":"2026-05-18T04:37:01Z"},{"alias_kind":"pith_short_12","alias_value":"5EWVOUDVFR2H","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_16","alias_value":"5EWVOUDVFR2HJ6LD","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_8","alias_value":"5EWVOUDV","created_at":"2026-05-18T12:25:53Z"}],"graph_snapshots":[{"event_id":"sha256:3dcc3a287e9806e1bfd02ecddb2d879ed09d2ce554105525345354643d1430f0","target":"graph","created_at":"2026-05-18T04:37:01Z","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 0.1\" resolution near-infrared integral field spectroscopy of Halpha in a z=1.4781 star forming galaxy, Q2343-BM133. These observations were obtained with OSIRIS (OH Suppressing Infra-Red Imaging Spectrograph) using the W.M. Keck Observatory Laser Guide Star Adaptive Optics system. Halpha emission is resolved over a 0.8\" (6.8 kpc) x 0.5\" (4.3 kpc) region with a 0.1\" spatial resolution. We find a global flux of 4.2+/-0.6x10^{-16} ergs s^{-1} cm^{-2}, and detect a spatially resolved velocity gradient of ~134 km s^{-1} across the galaxy and a global velocity dispersion of 73+/-9 km s^{-","authors_text":"A.Krabbe, A. Quirrenbach, C.C. Steidel, C. Iserlohe, D.K. Erb, D.R. Law, J.E. Larkin, J. Weiss, M.Barczys, M.W. McElwain, S.A. Wright","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2006-12-07T22:43:19Z","title":"Integral Field Spectroscopy of a Candidate Disk Galaxy at z~1.5 using Laser Guide Star Adaptive Optics"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612199","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":"sha256:81fbe073edb17ec8bccef996ca1dd7b367c3c88b97818688ec3cecac60786a0b","target":"record","created_at":"2026-05-18T04:37:01Z","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":"0a99d2fbb856c7fc6815db6a78eaf3c9ae3bf02dc46efc07c4b5d5f271b09c1f","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-07T22:43:19Z","title_canon_sha256":"979adcc536954558a0516c5c4210446229159615d92ea836aa83763158d9e921"},"schema_version":"1.0","source":{"id":"astro-ph/0612199","kind":"arxiv","version":1}},"canonical_sha256":"e92d5750752c7474f9636ba56a1686a56e927957c8b4335538f0e49df3086dd4","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"e92d5750752c7474f9636ba56a1686a56e927957c8b4335538f0e49df3086dd4","first_computed_at":"2026-05-18T04:37:01.329062Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:37:01.329062Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"IxWaubaE6a2Z8owBV8KWrY2w3oAt/zNXQhIHuVT2fk1MKNLZgU9NbdNC+kUARRGhrNXZeEZ48+EX+ryV5/F2Ag==","signature_status":"signed_v1","signed_at":"2026-05-18T04:37:01.329740Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0612199","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:81fbe073edb17ec8bccef996ca1dd7b367c3c88b97818688ec3cecac60786a0b","sha256:3dcc3a287e9806e1bfd02ecddb2d879ed09d2ce554105525345354643d1430f0"],"state_sha256":"c92de8f2dcab4526cfe61cca900bf12799880bc202c553b74ec57ee8412a2bf5"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ssR2wVRShQ4qGE9BaVxGvg+abnAhLMUzOw+VcFc7erq05NVi+O2v6DUocgt2rmSB/c+QWst3vpnMAXZ6Nv6DBg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-05T01:38:25.683349Z","bundle_sha256":"b0aefef19a02d4b04d990c040f1120665e7958bc09b5a47c57c9cd10fe709ba4"}}