{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:KY5AEBRF5C3MWSR5SUDIGR6GVC","short_pith_number":"pith:KY5AEBRF","canonical_record":{"source":{"id":"1302.5655","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-22T17:30:50Z","cross_cats_sorted":[],"title_canon_sha256":"22105f2813607de7a21cd7fb36795a04aa6432fb474c13b4e552d8d41d61e25b","abstract_canon_sha256":"352e36e8a3e640e9ceaa197521ae93afe69ca0aebc4057315ba4aa805538ae50"},"schema_version":"1.0"},"canonical_sha256":"563a020625e8b6cb4a3d95068347c6a88e830040c6fb010b945e1017fc612700","source":{"kind":"arxiv","id":"1302.5655","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1302.5655","created_at":"2026-05-18T03:21:54Z"},{"alias_kind":"arxiv_version","alias_value":"1302.5655v2","created_at":"2026-05-18T03:21:54Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.5655","created_at":"2026-05-18T03:21:54Z"},{"alias_kind":"pith_short_12","alias_value":"KY5AEBRF5C3M","created_at":"2026-05-18T12:27:51Z"},{"alias_kind":"pith_short_16","alias_value":"KY5AEBRF5C3MWSR5","created_at":"2026-05-18T12:27:51Z"},{"alias_kind":"pith_short_8","alias_value":"KY5AEBRF","created_at":"2026-05-18T12:27:51Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:KY5AEBRF5C3MWSR5SUDIGR6GVC","target":"record","payload":{"canonical_record":{"source":{"id":"1302.5655","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-22T17:30:50Z","cross_cats_sorted":[],"title_canon_sha256":"22105f2813607de7a21cd7fb36795a04aa6432fb474c13b4e552d8d41d61e25b","abstract_canon_sha256":"352e36e8a3e640e9ceaa197521ae93afe69ca0aebc4057315ba4aa805538ae50"},"schema_version":"1.0"},"canonical_sha256":"563a020625e8b6cb4a3d95068347c6a88e830040c6fb010b945e1017fc612700","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:21:54.713874Z","signature_b64":"73ohnWp1CfJYHEKsnvE1bN28QvyTfy1Y56z4p/+GtYa3FBPAPouvcURegvkNONtDhqtMz/WakoYZz0UTbmWKCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"563a020625e8b6cb4a3d95068347c6a88e830040c6fb010b945e1017fc612700","last_reissued_at":"2026-05-18T03:21:54.713458Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:21:54.713458Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1302.5655","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":"2026-05-18T03:21:54Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"o9TA/qfkKQcZhd3GhgRFwLIU4TLHRL7WKI91h3kZHddiiVyu86BVxmYURT2owQk0njU+zx5CUSV+MmQYBbHfAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-23T01:25:34.021761Z"},"content_sha256":"6a59c0293b41eff1809950da9a89128ca55905a8346eb593c0adf0c73b11690f","schema_version":"1.0","event_id":"sha256:6a59c0293b41eff1809950da9a89128ca55905a8346eb593c0adf0c73b11690f"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:KY5AEBRF5C3MWSR5SUDIGR6GVC","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Ealet, Bruno Moraes, Carlo Schimd, Carlos H. Brandt, David J. Schlegel, Donald P. Schneider, Eric Jullo, Francisco Prada, Huanyuan Shan, Jean-Paul Kneib, Jeffrey A. Newman, Joel Brownstein, Johan Comparat, M. E. S. Pereira, Nick Mostek, Olivier Ilbert, S. Escoffier, Thomas Erben","submitted_at":"2013-02-22T17:30:50Z","abstract_excerpt":"The baryon acoustic oscillation (BAO) feature in the two-point correlation function of galaxies supplies a standard ruler to probe the expansion history of the Universe. We study here several galaxy selection schemes, aiming at building an emission-line galaxy (ELG) sample in the redshift range $0.6<z<1.7$, that would be suitable for future BAO studies, providing a highly biased galaxy sample. We analyse the angular galaxy clustering of galaxy selections at the redshifts 0.5, 0.7, 0.8, 1 and 1.2 and we combine this analysis with a halo occupation distribution (HOD) model to derive the properti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.5655","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":"2026-05-18T03:21:54Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"R2ZuTB6ZoT2x/wjRYxY13FMqIS+1GikGfhstaOjjGoIz23yoTuFsyDwAH91e9u/TECbyr0JsMRBVCYImA2sdBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-23T01:25:34.022424Z"},"content_sha256":"2b27debaf61c3ef397d7a6eaaed25275070025b72caf6a4f14a947e6df02c443","schema_version":"1.0","event_id":"sha256:2b27debaf61c3ef397d7a6eaaed25275070025b72caf6a4f14a947e6df02c443"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/KY5AEBRF5C3MWSR5SUDIGR6GVC/bundle.json","state_url":"https://pith.science/pith/KY5AEBRF5C3MWSR5SUDIGR6GVC/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/KY5AEBRF5C3MWSR5SUDIGR6GVC/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":"2026-05-23T01:25:34Z","links":{"resolver":"https://pith.science/pith/KY5AEBRF5C3MWSR5SUDIGR6GVC","bundle":"https://pith.science/pith/KY5AEBRF5C3MWSR5SUDIGR6GVC/bundle.json","state":"https://pith.science/pith/KY5AEBRF5C3MWSR5SUDIGR6GVC/state.json","well_known_bundle":"https://pith.science/.well-known/pith/KY5AEBRF5C3MWSR5SUDIGR6GVC/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:KY5AEBRF5C3MWSR5SUDIGR6GVC","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":"352e36e8a3e640e9ceaa197521ae93afe69ca0aebc4057315ba4aa805538ae50","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-22T17:30:50Z","title_canon_sha256":"22105f2813607de7a21cd7fb36795a04aa6432fb474c13b4e552d8d41d61e25b"},"schema_version":"1.0","source":{"id":"1302.5655","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1302.5655","created_at":"2026-05-18T03:21:54Z"},{"alias_kind":"arxiv_version","alias_value":"1302.5655v2","created_at":"2026-05-18T03:21:54Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.5655","created_at":"2026-05-18T03:21:54Z"},{"alias_kind":"pith_short_12","alias_value":"KY5AEBRF5C3M","created_at":"2026-05-18T12:27:51Z"},{"alias_kind":"pith_short_16","alias_value":"KY5AEBRF5C3MWSR5","created_at":"2026-05-18T12:27:51Z"},{"alias_kind":"pith_short_8","alias_value":"KY5AEBRF","created_at":"2026-05-18T12:27:51Z"}],"graph_snapshots":[{"event_id":"sha256:2b27debaf61c3ef397d7a6eaaed25275070025b72caf6a4f14a947e6df02c443","target":"graph","created_at":"2026-05-18T03:21:54Z","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 baryon acoustic oscillation (BAO) feature in the two-point correlation function of galaxies supplies a standard ruler to probe the expansion history of the Universe. We study here several galaxy selection schemes, aiming at building an emission-line galaxy (ELG) sample in the redshift range $0.6<z<1.7$, that would be suitable for future BAO studies, providing a highly biased galaxy sample. We analyse the angular galaxy clustering of galaxy selections at the redshifts 0.5, 0.7, 0.8, 1 and 1.2 and we combine this analysis with a halo occupation distribution (HOD) model to derive the properti","authors_text":"A. Ealet, Bruno Moraes, Carlo Schimd, Carlos H. Brandt, David J. Schlegel, Donald P. Schneider, Eric Jullo, Francisco Prada, Huanyuan Shan, Jean-Paul Kneib, Jeffrey A. Newman, Joel Brownstein, Johan Comparat, M. E. S. Pereira, Nick Mostek, Olivier Ilbert, S. Escoffier, Thomas Erben","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-22T17:30:50Z","title":"Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.5655","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":"sha256:6a59c0293b41eff1809950da9a89128ca55905a8346eb593c0adf0c73b11690f","target":"record","created_at":"2026-05-18T03:21:54Z","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":"352e36e8a3e640e9ceaa197521ae93afe69ca0aebc4057315ba4aa805538ae50","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-22T17:30:50Z","title_canon_sha256":"22105f2813607de7a21cd7fb36795a04aa6432fb474c13b4e552d8d41d61e25b"},"schema_version":"1.0","source":{"id":"1302.5655","kind":"arxiv","version":2}},"canonical_sha256":"563a020625e8b6cb4a3d95068347c6a88e830040c6fb010b945e1017fc612700","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"563a020625e8b6cb4a3d95068347c6a88e830040c6fb010b945e1017fc612700","first_computed_at":"2026-05-18T03:21:54.713458Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:21:54.713458Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"73ohnWp1CfJYHEKsnvE1bN28QvyTfy1Y56z4p/+GtYa3FBPAPouvcURegvkNONtDhqtMz/WakoYZz0UTbmWKCw==","signature_status":"signed_v1","signed_at":"2026-05-18T03:21:54.713874Z","signed_message":"canonical_sha256_bytes"},"source_id":"1302.5655","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:6a59c0293b41eff1809950da9a89128ca55905a8346eb593c0adf0c73b11690f","sha256:2b27debaf61c3ef397d7a6eaaed25275070025b72caf6a4f14a947e6df02c443"],"state_sha256":"d3a2b89e638b0971e8b459b3424d1f84b391947004d03dce4a3c77db839082c5"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"+CU0farSl/nMfNxS79TygPMs8L4gf+BPm2KVlZHgz0Bq0xNWCOhPd9OF/bs/Q/R+I4uC6/1XEmqDcULV/P7yBg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-23T01:25:34.026089Z","bundle_sha256":"a1b78be1a727ee1ee76b73628ea1733292481cead2c44c9af49fcc69a4b9e89e"}}