{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:VROVXAY4NWKNYAMLJYUNJEPH2M","short_pith_number":"pith:VROVXAY4","canonical_record":{"source":{"id":"1303.0024","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-28T21:39:11Z","cross_cats_sorted":[],"title_canon_sha256":"b6f736c56afdd901cd2aaf6267615ddf20ab1df1499412a5074bf486af9bcc36","abstract_canon_sha256":"bc69401558a99b661bd45e01096dd482323688b72ec4535dfa48855527b97a04"},"schema_version":"1.0"},"canonical_sha256":"ac5d5b831c6d94dc018b4e28d491e7d326ad3f0a35b48a45143a7d84c965c4d9","source":{"kind":"arxiv","id":"1303.0024","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1303.0024","created_at":"2026-05-18T01:51:25Z"},{"alias_kind":"arxiv_version","alias_value":"1303.0024v2","created_at":"2026-05-18T01:51:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.0024","created_at":"2026-05-18T01:51:25Z"},{"alias_kind":"pith_short_12","alias_value":"VROVXAY4NWKN","created_at":"2026-05-18T12:28:04Z"},{"alias_kind":"pith_short_16","alias_value":"VROVXAY4NWKNYAML","created_at":"2026-05-18T12:28:04Z"},{"alias_kind":"pith_short_8","alias_value":"VROVXAY4","created_at":"2026-05-18T12:28:04Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:VROVXAY4NWKNYAMLJYUNJEPH2M","target":"record","payload":{"canonical_record":{"source":{"id":"1303.0024","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-28T21:39:11Z","cross_cats_sorted":[],"title_canon_sha256":"b6f736c56afdd901cd2aaf6267615ddf20ab1df1499412a5074bf486af9bcc36","abstract_canon_sha256":"bc69401558a99b661bd45e01096dd482323688b72ec4535dfa48855527b97a04"},"schema_version":"1.0"},"canonical_sha256":"ac5d5b831c6d94dc018b4e28d491e7d326ad3f0a35b48a45143a7d84c965c4d9","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:25.743768Z","signature_b64":"153sNCwPdUAovzJ+nEbFElZVrmY23xV8LXa+cgGLDkVfXB/+DbMPr0G5vEiCVg+awvORpwQCz9a6RZAGtxyrDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ac5d5b831c6d94dc018b4e28d491e7d326ad3f0a35b48a45143a7d84c965c4d9","last_reissued_at":"2026-05-18T01:51:25.743013Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:25.743013Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1303.0024","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:51:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"uMaXZNpHVvPz4uYs1PPh7nnJHXQVbiHZIh9V9s/a9FTU9K1H8NM/1X5i/7LGcBQNw5hAQ3jx5pSj9DsxKghTAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T00:51:33.620517Z"},"content_sha256":"e49b11743605be4fa2ed938026309bc956ba053cd32532abede29541c8d9af37","schema_version":"1.0","event_id":"sha256:e49b11743605be4fa2ed938026309bc956ba053cd32532abede29541c8d9af37"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:VROVXAY4NWKNYAMLJYUNJEPH2M","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Physical Properties of Spectroscopically-Confirmed Galaxies at z >= 6. I. Basic Characteristics of the Rest-Frame UV Continuum and Lyman-alpha emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Eiichi Egami, Kazuhiro Shimasaku, Kristian Finlator, Linhua Jiang, Masami Ouchi, Matthew Mechtley, Nobunari Kashikawa, Rogier A. Windhorst, Romeel Dave, Seth H. Cohen, Xiaohui Fan","submitted_at":"2013-02-28T21:39:11Z","abstract_excerpt":"We present deep HST near-IR and Spitzer mid-IR observations of a large sample of spectroscopically-confirmed galaxies at z >= 6. The sample consists of 51 Lyman-alpha emitters (LAEs) at z ~ 5.7, 6.5, and 7.0, and 16 Lyman-break galaxies (LBGs) at 5.9 < z < 6.5. The near-IR images were mostly obtained with WFC3 in the F125W and F160W bands, and the mid-IR images were obtained with IRAC in the 3.6um and 4.5um bands. Our galaxies also have deep optical imaging data from Subaru Suprime-Cam. We utilize the multi-band data and secure redshifts to derive their rest-frame UV properties. These galaxies"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.0024","kind":"arxiv","version":2},"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":"2026-05-18T01:51:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"yf3JFlvq0pWRNs4WsIz51G9xICKchEhhdcVQRLpNnFoB1sau3uRY38UdgfSkA3tS9coGnufdRxPtA7KcVaWZDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T00:51:33.621092Z"},"content_sha256":"6c453a68d7b4f86827af021cb036ad3b1c3c3cc888269e5fd6b88742c721498e","schema_version":"1.0","event_id":"sha256:6c453a68d7b4f86827af021cb036ad3b1c3c3cc888269e5fd6b88742c721498e"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/VROVXAY4NWKNYAMLJYUNJEPH2M/bundle.json","state_url":"https://pith.science/pith/VROVXAY4NWKNYAMLJYUNJEPH2M/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/VROVXAY4NWKNYAMLJYUNJEPH2M/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":"2026-05-26T00:51:33Z","links":{"resolver":"https://pith.science/pith/VROVXAY4NWKNYAMLJYUNJEPH2M","bundle":"https://pith.science/pith/VROVXAY4NWKNYAMLJYUNJEPH2M/bundle.json","state":"https://pith.science/pith/VROVXAY4NWKNYAMLJYUNJEPH2M/state.json","well_known_bundle":"https://pith.science/.well-known/pith/VROVXAY4NWKNYAMLJYUNJEPH2M/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:VROVXAY4NWKNYAMLJYUNJEPH2M","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":"bc69401558a99b661bd45e01096dd482323688b72ec4535dfa48855527b97a04","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-28T21:39:11Z","title_canon_sha256":"b6f736c56afdd901cd2aaf6267615ddf20ab1df1499412a5074bf486af9bcc36"},"schema_version":"1.0","source":{"id":"1303.0024","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1303.0024","created_at":"2026-05-18T01:51:25Z"},{"alias_kind":"arxiv_version","alias_value":"1303.0024v2","created_at":"2026-05-18T01:51:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.0024","created_at":"2026-05-18T01:51:25Z"},{"alias_kind":"pith_short_12","alias_value":"VROVXAY4NWKN","created_at":"2026-05-18T12:28:04Z"},{"alias_kind":"pith_short_16","alias_value":"VROVXAY4NWKNYAML","created_at":"2026-05-18T12:28:04Z"},{"alias_kind":"pith_short_8","alias_value":"VROVXAY4","created_at":"2026-05-18T12:28:04Z"}],"graph_snapshots":[{"event_id":"sha256:6c453a68d7b4f86827af021cb036ad3b1c3c3cc888269e5fd6b88742c721498e","target":"graph","created_at":"2026-05-18T01:51:25Z","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 deep HST near-IR and Spitzer mid-IR observations of a large sample of spectroscopically-confirmed galaxies at z >= 6. The sample consists of 51 Lyman-alpha emitters (LAEs) at z ~ 5.7, 6.5, and 7.0, and 16 Lyman-break galaxies (LBGs) at 5.9 < z < 6.5. The near-IR images were mostly obtained with WFC3 in the F125W and F160W bands, and the mid-IR images were obtained with IRAC in the 3.6um and 4.5um bands. Our galaxies also have deep optical imaging data from Subaru Suprime-Cam. We utilize the multi-band data and secure redshifts to derive their rest-frame UV properties. These galaxies","authors_text":"Eiichi Egami, Kazuhiro Shimasaku, Kristian Finlator, Linhua Jiang, Masami Ouchi, Matthew Mechtley, Nobunari Kashikawa, Rogier A. Windhorst, Romeel Dave, Seth H. Cohen, Xiaohui Fan","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-28T21:39:11Z","title":"Physical Properties of Spectroscopically-Confirmed Galaxies at z >= 6. I. Basic Characteristics of the Rest-Frame UV Continuum and Lyman-alpha emission"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.0024","kind":"arxiv","version":2},"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:e49b11743605be4fa2ed938026309bc956ba053cd32532abede29541c8d9af37","target":"record","created_at":"2026-05-18T01:51:25Z","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":"bc69401558a99b661bd45e01096dd482323688b72ec4535dfa48855527b97a04","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-28T21:39:11Z","title_canon_sha256":"b6f736c56afdd901cd2aaf6267615ddf20ab1df1499412a5074bf486af9bcc36"},"schema_version":"1.0","source":{"id":"1303.0024","kind":"arxiv","version":2}},"canonical_sha256":"ac5d5b831c6d94dc018b4e28d491e7d326ad3f0a35b48a45143a7d84c965c4d9","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"ac5d5b831c6d94dc018b4e28d491e7d326ad3f0a35b48a45143a7d84c965c4d9","first_computed_at":"2026-05-18T01:51:25.743013Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:51:25.743013Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"153sNCwPdUAovzJ+nEbFElZVrmY23xV8LXa+cgGLDkVfXB/+DbMPr0G5vEiCVg+awvORpwQCz9a6RZAGtxyrDA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:51:25.743768Z","signed_message":"canonical_sha256_bytes"},"source_id":"1303.0024","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:e49b11743605be4fa2ed938026309bc956ba053cd32532abede29541c8d9af37","sha256:6c453a68d7b4f86827af021cb036ad3b1c3c3cc888269e5fd6b88742c721498e"],"state_sha256":"0d794814edb7cb145fcbccd5d20fb9e8345ccb116280770ba6b23a965f7e06e1"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"VLfFrGPvyv7xoglpAFjcNzZDFUr119RoXbsj3FRdLJbjf2jxcPRhkqpa+rbnTv+WWrt7ZAIk7yMgxkThMk1cBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T00:51:33.624680Z","bundle_sha256":"c1e01372636c350eb7229a1491c7540bd386c3af820d930dcc1ec672dda6e4a2"}}