{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:HU3MOG3CZLIXBX2CQ45MSTESAF","short_pith_number":"pith:HU3MOG3C","canonical_record":{"source":{"id":"1807.09195","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-07-24T15:49:13Z","cross_cats_sorted":[],"title_canon_sha256":"2534b1f8ecd3ca7717e515e25535ef1d0a0c356d9bafcfc6cfe744dd23e673a1","abstract_canon_sha256":"ce3e4cd93b9dbd1258e9ad14a3245f26935444c773a4c0a30856ece807ca36b5"},"schema_version":"1.0"},"canonical_sha256":"3d36c71b62cad170df42873ac94c9201541cb037029ba1cc8b95f31c7ed0a6a5","source":{"kind":"arxiv","id":"1807.09195","version":4},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1807.09195","created_at":"2026-05-17T23:55:55Z"},{"alias_kind":"arxiv_version","alias_value":"1807.09195v4","created_at":"2026-05-17T23:55:55Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.09195","created_at":"2026-05-17T23:55:55Z"},{"alias_kind":"pith_short_12","alias_value":"HU3MOG3CZLIX","created_at":"2026-05-18T12:32:28Z"},{"alias_kind":"pith_short_16","alias_value":"HU3MOG3CZLIXBX2C","created_at":"2026-05-18T12:32:28Z"},{"alias_kind":"pith_short_8","alias_value":"HU3MOG3C","created_at":"2026-05-18T12:32:28Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:HU3MOG3CZLIXBX2CQ45MSTESAF","target":"record","payload":{"canonical_record":{"source":{"id":"1807.09195","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-07-24T15:49:13Z","cross_cats_sorted":[],"title_canon_sha256":"2534b1f8ecd3ca7717e515e25535ef1d0a0c356d9bafcfc6cfe744dd23e673a1","abstract_canon_sha256":"ce3e4cd93b9dbd1258e9ad14a3245f26935444c773a4c0a30856ece807ca36b5"},"schema_version":"1.0"},"canonical_sha256":"3d36c71b62cad170df42873ac94c9201541cb037029ba1cc8b95f31c7ed0a6a5","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:55:55.917059Z","signature_b64":"jiSZEzXhmXA70y4D7WYcIGunqkr2tXQHxep1qhMNNd0cxZomodoAdbbEya+ncod/yBGk7kvWWp8oGkHuwv8CDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3d36c71b62cad170df42873ac94c9201541cb037029ba1cc8b95f31c7ed0a6a5","last_reissued_at":"2026-05-17T23:55:55.916410Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:55:55.916410Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1807.09195","source_version":4,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-17T23:55:55Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"j7SZqHbBRZ4k7xswEZadONxBzXwp6S/RdDatP24+HhU95DkS97gzONy4K1lP7w71zD4vL9svNu7iDnhu58avBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-20T05:05:42.576331Z"},"content_sha256":"61c6ce9c60c0f475e091f08c08a80d9bebf0586fda4998744404b6104e787232","schema_version":"1.0","event_id":"sha256:61c6ce9c60c0f475e091f08c08a80d9bebf0586fda4998744404b6104e787232"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:HU3MOG3CZLIXBX2CQ45MSTESAF","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ami Choi, David Wittman, J. Anthony Tyson, Mijin Yoon, M. James Jee, Samuel Schmidt","submitted_at":"2018-07-24T15:49:13Z","abstract_excerpt":"We present cosmological parameter measurements from the Deep Lens Survey (DLS) using galaxy-mass and galaxy-galaxy power spectra in the multipole range $\\ell=250\\sim2000$. We measure galaxy-galaxy power spectra from two lens bins centered at $z\\sim0.27$ and $0.54$ and galaxy-mass power spectra by cross-correlating the positions of galaxies in these two lens bins with galaxy shapes in two source bins centered at $z\\sim0.64$ and $1.1$. We marginalize over a baryonic feedback process using a single-parameter representation and a sum of neutrino masses, as well as photometric redshift and shear ca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.09195","kind":"arxiv","version":4},"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":"2026-05-17T23:55:55Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ypJ+skTuuv+bMnlS/KKOMrWm8UFMk6yRIy9+oRxtzFk+F5hWcHWJ+AugYdjpU5fqGleE2+gAONJdxf3WMD3VBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-20T05:05:42.576686Z"},"content_sha256":"2d35459980aaeee456645fab00eb9ac0f5bb90cec3e0303af6b596bfdf276f77","schema_version":"1.0","event_id":"sha256:2d35459980aaeee456645fab00eb9ac0f5bb90cec3e0303af6b596bfdf276f77"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/HU3MOG3CZLIXBX2CQ45MSTESAF/bundle.json","state_url":"https://pith.science/pith/HU3MOG3CZLIXBX2CQ45MSTESAF/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/HU3MOG3CZLIXBX2CQ45MSTESAF/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":"2026-06-20T05:05:42Z","links":{"resolver":"https://pith.science/pith/HU3MOG3CZLIXBX2CQ45MSTESAF","bundle":"https://pith.science/pith/HU3MOG3CZLIXBX2CQ45MSTESAF/bundle.json","state":"https://pith.science/pith/HU3MOG3CZLIXBX2CQ45MSTESAF/state.json","well_known_bundle":"https://pith.science/.well-known/pith/HU3MOG3CZLIXBX2CQ45MSTESAF/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:HU3MOG3CZLIXBX2CQ45MSTESAF","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":"ce3e4cd93b9dbd1258e9ad14a3245f26935444c773a4c0a30856ece807ca36b5","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-07-24T15:49:13Z","title_canon_sha256":"2534b1f8ecd3ca7717e515e25535ef1d0a0c356d9bafcfc6cfe744dd23e673a1"},"schema_version":"1.0","source":{"id":"1807.09195","kind":"arxiv","version":4}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1807.09195","created_at":"2026-05-17T23:55:55Z"},{"alias_kind":"arxiv_version","alias_value":"1807.09195v4","created_at":"2026-05-17T23:55:55Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.09195","created_at":"2026-05-17T23:55:55Z"},{"alias_kind":"pith_short_12","alias_value":"HU3MOG3CZLIX","created_at":"2026-05-18T12:32:28Z"},{"alias_kind":"pith_short_16","alias_value":"HU3MOG3CZLIXBX2C","created_at":"2026-05-18T12:32:28Z"},{"alias_kind":"pith_short_8","alias_value":"HU3MOG3C","created_at":"2026-05-18T12:32:28Z"}],"graph_snapshots":[{"event_id":"sha256:2d35459980aaeee456645fab00eb9ac0f5bb90cec3e0303af6b596bfdf276f77","target":"graph","created_at":"2026-05-17T23:55:55Z","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 cosmological parameter measurements from the Deep Lens Survey (DLS) using galaxy-mass and galaxy-galaxy power spectra in the multipole range $\\ell=250\\sim2000$. We measure galaxy-galaxy power spectra from two lens bins centered at $z\\sim0.27$ and $0.54$ and galaxy-mass power spectra by cross-correlating the positions of galaxies in these two lens bins with galaxy shapes in two source bins centered at $z\\sim0.64$ and $1.1$. We marginalize over a baryonic feedback process using a single-parameter representation and a sum of neutrino masses, as well as photometric redshift and shear ca","authors_text":"Ami Choi, David Wittman, J. Anthony Tyson, Mijin Yoon, M. James Jee, Samuel Schmidt","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-07-24T15:49:13Z","title":"Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.09195","kind":"arxiv","version":4},"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":"sha256:61c6ce9c60c0f475e091f08c08a80d9bebf0586fda4998744404b6104e787232","target":"record","created_at":"2026-05-17T23:55:55Z","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":"ce3e4cd93b9dbd1258e9ad14a3245f26935444c773a4c0a30856ece807ca36b5","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-07-24T15:49:13Z","title_canon_sha256":"2534b1f8ecd3ca7717e515e25535ef1d0a0c356d9bafcfc6cfe744dd23e673a1"},"schema_version":"1.0","source":{"id":"1807.09195","kind":"arxiv","version":4}},"canonical_sha256":"3d36c71b62cad170df42873ac94c9201541cb037029ba1cc8b95f31c7ed0a6a5","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3d36c71b62cad170df42873ac94c9201541cb037029ba1cc8b95f31c7ed0a6a5","first_computed_at":"2026-05-17T23:55:55.916410Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:55:55.916410Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"jiSZEzXhmXA70y4D7WYcIGunqkr2tXQHxep1qhMNNd0cxZomodoAdbbEya+ncod/yBGk7kvWWp8oGkHuwv8CDg==","signature_status":"signed_v1","signed_at":"2026-05-17T23:55:55.917059Z","signed_message":"canonical_sha256_bytes"},"source_id":"1807.09195","source_kind":"arxiv","source_version":4}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:61c6ce9c60c0f475e091f08c08a80d9bebf0586fda4998744404b6104e787232","sha256:2d35459980aaeee456645fab00eb9ac0f5bb90cec3e0303af6b596bfdf276f77"],"state_sha256":"852611214dda0844b71ea467f9bf56d768729f07dc807720eca0e2f683532822"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Bk8vRtg+0Ns8cQmHMJqwhIfBNN9MLWYOrwaSwNmiTKLRdWHInnhoLUWzDi+Gw4hRrK/BJtck8ymjeLTk5nU4Cw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-20T05:05:42.578661Z","bundle_sha256":"555b858496f904033a74ed0179c276f5a5b349996c9e72c4e9eb1559eee994c0"}}