{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2021:ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A","short_pith_number":"pith:ZKZOKCWG","canonical_record":{"source":{"id":"2105.13541","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2021-05-28T01:58:50Z","cross_cats_sorted":[],"title_canon_sha256":"a82ad38137903820a459501b267dcf824d80b149c1e4f83231904bbba59367eb","abstract_canon_sha256":"a97629e8af627be68abeec30defd5e777480d36436090a55d1b17e4a94ae301e"},"schema_version":"1.0"},"canonical_sha256":"cab2e50ac6ee6378b500b32d44eaf0d8003b0f1da9ea8fac7f4dca1d1548d469","source":{"kind":"arxiv","id":"2105.13541","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2105.13541","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"arxiv_version","alias_value":"2105.13541v2","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.13541","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"pith_short_12","alias_value":"ZKZOKCWG5ZRX","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"pith_short_16","alias_value":"ZKZOKCWG5ZRXRNIA","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"pith_short_8","alias_value":"ZKZOKCWG","created_at":"2026-07-05T04:21:46Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2021:ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A","target":"record","payload":{"canonical_record":{"source":{"id":"2105.13541","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2021-05-28T01:58:50Z","cross_cats_sorted":[],"title_canon_sha256":"a82ad38137903820a459501b267dcf824d80b149c1e4f83231904bbba59367eb","abstract_canon_sha256":"a97629e8af627be68abeec30defd5e777480d36436090a55d1b17e4a94ae301e"},"schema_version":"1.0"},"canonical_sha256":"cab2e50ac6ee6378b500b32d44eaf0d8003b0f1da9ea8fac7f4dca1d1548d469","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:21:46.460159Z","signature_b64":"zi/nohYgm8msAauwu894BzlBx9oTtAUgZ1eysKF6TIk6/POFHdQPVpC66nC9l3piq1NCEFLNwnVZxMlqnQtyDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cab2e50ac6ee6378b500b32d44eaf0d8003b0f1da9ea8fac7f4dca1d1548d469","last_reissued_at":"2026-07-05T04:21:46.459729Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:21:46.459729Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2105.13541","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":"2026-07-05T04:21:46Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"PKp+zLZamJki6Uu4gqq9lZoV0Z+h7myoL58j3h5Dd2HXuOW+klY0bac81ssPltivtbatj2XQg08FOh2dZK50AA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-05T11:06:41.446331Z"},"content_sha256":"3860fea68deeb15849379c8a7d97ce122f8d97c9ac0551afbb09e54d9c85f369","schema_version":"1.0","event_id":"sha256:3860fea68deeb15849379c8a7d97ce122f8d97c9ac0551afbb09e54d9c85f369"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2021:ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Alarcon, A. Amon, A. A. Plazas Malag\\'on, A. Campos, A. Carnero Rosell, A. Choi, A. Drlica-Wagner, A. E. Evrard, A. Farahi, A. Fert\\'e, A. J. Ross, A. Navarro-Alsina, A. Palmese, A. Porredon, A. R. Liddle, A. Roodman, A. Troja, B. Flaugher, B. Jain, B. Yanny, B. Yin, C. Chang, C. Conselice, C. Davis, C. Doux, C. J. Miller, C. S\\'anchez, C. To, D. Bacon, D. Brooks, D. Gruen, D. Huterer, D. J. James, D. L. Burke, D. L. Hollowood, D. Petravick, D. Thomas, D. W. Gerdes, E. Baxter, E. Gaztanaga, E. Krause, E. M. Huff, E. Sanchez, E. Sheldon, E. S. Rykoff, E. Suchyta, F. Andrade-Oliveira, F. Elsner, F. Menanteau, F. Paz-Chinch\\'on, G. Giannini, G. Gutierrez, G. M. Bernstein, G. Tarle, G. Zacharegkas, H. Camacho, H. Huang, H. Lin, H. T. Diehl, I. Ferrero, I. Harrison, I. Sevilla-Noarbe, I. Tutusaus, J. Annis, J. Blazek, J. Carretero, J. Cordero, J. DeRose, J. De Vicente, J. Elvin-Poole, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. Mohr, J. L. Marshall, J. McCullough, J. Muir, J. Myles, J. P. Dietrich, J. Prat, J. Sanchez, J. Weller (DES Collaboration), J. Zuntz, K. Bechtol, K. Eckert, K. Herner, K. Honscheid, K. Kuehn, L. F. Secco, L. N. da Costa, M. A. G. Maia, M. Aguena, M. A. Troxel, M. Carrasco Kind, M. Costanzi, M. Crocce, M. E. S. Pereira, M. Gatti, M. Jarvis, M. Raveri, M. R. Becker, M. Rodriguez-Monroy, M. Smith, M. Soares-Santos, N. Kuropatkin, N. MacCrann, N. Weaverdyck, O. Alves, O. Friedrich, O. Lahav, P. Doel, P.-F. Leget, P. Fosalba, P. Lemos, P. Martini, P. Melchior, R. A. Gruendl, R. Cawthon, R. Chen, R. H. Wechsler, R. L. C. Ogando, R. Miquel, R. Morgan, R. P. Rollins, R. Rosenfeld, S. Allam, S. Bocquet, S. Desai, S. Dodelson, S. Everett, S. Pandey, S. R. Hinton, S. Serrano, T. F. Eifler, T. Giannantonio, T. M. C. Abbott, T. N. Varga, T. Shin, W. G. Hartley, X. Fang, Y. Park","submitted_at":"2021-05-28T01:58:50Z","abstract_excerpt":"We present and characterize the galaxy-galaxy lensing signal measured using the first three years of data from the Dark Energy Survey (DES Y3) covering 4132 deg$^2$. These galaxy-galaxy measurements are used in the DES Y3 3$\\times$2pt cosmological analysis, which combines weak lensing and galaxy clustering information. We use two lens samples: a magnitude-limited sample and the redMaGic sample, which span the redshift range $\\sim 0.2-1$ with 10.7 M and 2.6 M galaxies respectively. For the source catalog, we use the Metacalibration shape sample, consisting of $\\simeq$100 M galaxies separated in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.13541","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2105.13541/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2026-07-05T04:21:46Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"rPqNZ915EKzIyfFqO1ruAr/DI5hLbBTNFkA4mzIP6GT8VLRVF5sAYnv50MZsNVUvdaITR+q758T3XEEDtIENBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-05T11:06:41.446720Z"},"content_sha256":"4ce33b47aca3a7f3fed3aad1b8a44de5dde4bcd8c0ead59bb73cd6332295c60e","schema_version":"1.0","event_id":"sha256:4ce33b47aca3a7f3fed3aad1b8a44de5dde4bcd8c0ead59bb73cd6332295c60e"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A/bundle.json","state_url":"https://pith.science/pith/ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A/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":"2026-07-05T11:06:41Z","links":{"resolver":"https://pith.science/pith/ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A","bundle":"https://pith.science/pith/ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A/bundle.json","state":"https://pith.science/pith/ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2021:ZKZOKCWG5ZRXRNIAWMWUJ2XQ3A","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":"a97629e8af627be68abeec30defd5e777480d36436090a55d1b17e4a94ae301e","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2021-05-28T01:58:50Z","title_canon_sha256":"a82ad38137903820a459501b267dcf824d80b149c1e4f83231904bbba59367eb"},"schema_version":"1.0","source":{"id":"2105.13541","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2105.13541","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"arxiv_version","alias_value":"2105.13541v2","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.13541","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"pith_short_12","alias_value":"ZKZOKCWG5ZRX","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"pith_short_16","alias_value":"ZKZOKCWG5ZRXRNIA","created_at":"2026-07-05T04:21:46Z"},{"alias_kind":"pith_short_8","alias_value":"ZKZOKCWG","created_at":"2026-07-05T04:21:46Z"}],"graph_snapshots":[{"event_id":"sha256:4ce33b47aca3a7f3fed3aad1b8a44de5dde4bcd8c0ead59bb73cd6332295c60e","target":"graph","created_at":"2026-07-05T04:21:46Z","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"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/2105.13541/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We present and characterize the galaxy-galaxy lensing signal measured using the first three years of data from the Dark Energy Survey (DES Y3) covering 4132 deg$^2$. These galaxy-galaxy measurements are used in the DES Y3 3$\\times$2pt cosmological analysis, which combines weak lensing and galaxy clustering information. We use two lens samples: a magnitude-limited sample and the redMaGic sample, which span the redshift range $\\sim 0.2-1$ with 10.7 M and 2.6 M galaxies respectively. For the source catalog, we use the Metacalibration shape sample, consisting of $\\simeq$100 M galaxies separated in","authors_text":"A. Alarcon, A. Amon, A. A. Plazas Malag\\'on, A. Campos, A. Carnero Rosell, A. Choi, A. Drlica-Wagner, A. E. Evrard, A. Farahi, A. Fert\\'e, A. J. Ross, A. Navarro-Alsina, A. Palmese, A. Porredon, A. R. Liddle, A. Roodman, A. Troja, B. Flaugher, B. Jain, B. Yanny, B. Yin, C. Chang, C. Conselice, C. Davis, C. Doux, C. J. Miller, C. S\\'anchez, C. To, D. Bacon, D. Brooks, D. Gruen, D. Huterer, D. J. James, D. L. Burke, D. L. Hollowood, D. Petravick, D. Thomas, D. W. Gerdes, E. Baxter, E. Gaztanaga, E. Krause, E. M. Huff, E. Sanchez, E. Sheldon, E. S. Rykoff, E. Suchyta, F. Andrade-Oliveira, F. Elsner, F. Menanteau, F. Paz-Chinch\\'on, G. Giannini, G. Gutierrez, G. M. Bernstein, G. Tarle, G. Zacharegkas, H. Camacho, H. Huang, H. Lin, H. T. Diehl, I. Ferrero, I. Harrison, I. Sevilla-Noarbe, I. Tutusaus, J. Annis, J. Blazek, J. Carretero, J. Cordero, J. DeRose, J. De Vicente, J. Elvin-Poole, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. Mohr, J. L. Marshall, J. McCullough, J. Muir, J. Myles, J. P. Dietrich, J. Prat, J. Sanchez, J. Weller (DES Collaboration), J. Zuntz, K. Bechtol, K. Eckert, K. Herner, K. Honscheid, K. Kuehn, L. F. Secco, L. N. da Costa, M. A. G. Maia, M. Aguena, M. A. Troxel, M. Carrasco Kind, M. Costanzi, M. Crocce, M. E. S. Pereira, M. Gatti, M. Jarvis, M. Raveri, M. R. Becker, M. Rodriguez-Monroy, M. Smith, M. Soares-Santos, N. Kuropatkin, N. MacCrann, N. Weaverdyck, O. Alves, O. Friedrich, O. Lahav, P. Doel, P.-F. Leget, P. Fosalba, P. Lemos, P. Martini, P. Melchior, R. A. Gruendl, R. Cawthon, R. Chen, R. H. Wechsler, R. L. C. Ogando, R. Miquel, R. Morgan, R. P. Rollins, R. Rosenfeld, S. Allam, S. Bocquet, S. Desai, S. Dodelson, S. Everett, S. Pandey, S. R. Hinton, S. Serrano, T. F. Eifler, T. Giannantonio, T. M. C. Abbott, T. N. Varga, T. Shin, W. G. Hartley, X. Fang, Y. Park","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2021-05-28T01:58:50Z","title":"Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.13541","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":"sha256:3860fea68deeb15849379c8a7d97ce122f8d97c9ac0551afbb09e54d9c85f369","target":"record","created_at":"2026-07-05T04:21:46Z","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":"a97629e8af627be68abeec30defd5e777480d36436090a55d1b17e4a94ae301e","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2021-05-28T01:58:50Z","title_canon_sha256":"a82ad38137903820a459501b267dcf824d80b149c1e4f83231904bbba59367eb"},"schema_version":"1.0","source":{"id":"2105.13541","kind":"arxiv","version":2}},"canonical_sha256":"cab2e50ac6ee6378b500b32d44eaf0d8003b0f1da9ea8fac7f4dca1d1548d469","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"cab2e50ac6ee6378b500b32d44eaf0d8003b0f1da9ea8fac7f4dca1d1548d469","first_computed_at":"2026-07-05T04:21:46.459729Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-05T04:21:46.459729Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"zi/nohYgm8msAauwu894BzlBx9oTtAUgZ1eysKF6TIk6/POFHdQPVpC66nC9l3piq1NCEFLNwnVZxMlqnQtyDw==","signature_status":"signed_v1","signed_at":"2026-07-05T04:21:46.460159Z","signed_message":"canonical_sha256_bytes"},"source_id":"2105.13541","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3860fea68deeb15849379c8a7d97ce122f8d97c9ac0551afbb09e54d9c85f369","sha256:4ce33b47aca3a7f3fed3aad1b8a44de5dde4bcd8c0ead59bb73cd6332295c60e"],"state_sha256":"be48dd38c0aa4f677e5b76b846fa6077ff8af6233963b39aad631beccc984fbd"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"fEBPr0W0EEqyIQRGTI5L8+n/YzrIM6AaPZh1vM+GZQJPfaCYv/GgKZeIo7q+hFK0aLsMkI8p8Pl2mRBt8L3tBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-07-05T11:06:41.448748Z","bundle_sha256":"04ac18f7e819b706bec32e3c81cea592f593fac5988188d2641c703962a1b4d0"}}