{"as_of":"2026-08-07T12:40:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9ac060a9f1ac6ead1704ad061cd64f50bd1520ece6310edd7453f3299045f9d8","coverage":[{"denominator":84,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":84,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:02:36.047055Z","state":"measured"},{"denominator":88,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":88,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T20:53:24.842800Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"cited_work":{"arxiv_id":"2507.01377","doi":"10.48550/arxiv.2507.01377","metadata_source":"arxiv_reference","pith_arxiv_id":"2507.01377","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Zhang*, S","venue":"ArXiv.org","work_id":"ad6dbd46-c6fd-49c1-bd1b-3d17966efdd9","year":2025},"citing_paper":{"arxiv_id":"2511.18134","last_updated":"2026-06-24T07:42:32Z","snapshot_observed_at":"2026-08-03T20:53:20.327987Z","submitted_at":"2025-11-22T17:32:48Z","title":"Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-17T06:28:15.131726Z"},"links":{"cited_paper":"/paper/2507.01377","citing_paper":"/paper/2511.18134"},"observation_digest":"sha256:8e9ac926edf04a905d27f686f88a218dc2f587dbdfc24011696f89bbb183527e","observation_id":"884d0ee1-2e9a-4b12-a4ee-f7fa12996709","resolution":{"observed_at":"2026-05-17T06:29:10.092854Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.01377","snapshot_observed_at":"2026-08-03T20:53:24.842800Z","title":"Zhang*, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18134","last_updated":"2026-06-24T07:42:32Z","snapshot_observed_at":"2026-08-03T20:53:20.327987Z","submitted_at":"2025-11-22T17:32:48Z","title":"Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:24.842800Z"},"links":{"cited_paper":"/paper/2507.01377","citing_paper":"/paper/2511.18134"},"observation_digest":"sha256:2f25c5830fd7f15b3143a78a96f4675d35ad11ce26aad5fb19a035f71ca9a2f4","observation_id":"64c2ef86-6f54-4a9f-88d2-ba7de577d9a7","resolution":{"observed_at":"2026-08-03T20:53:24.842800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"cited_work":{"arxiv_id":"2507.01377","doi":"10.48550/arxiv.2507.01377","metadata_source":"arxiv_reference","pith_arxiv_id":"2507.01377","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Zhang*, S","venue":"ArXiv.org","work_id":"ad6dbd46-c6fd-49c1-bd1b-3d17966efdd9","year":2025},"citing_paper":{"arxiv_id":"2605.00818","last_updated":"2026-05-01T17:57:07Z","snapshot_observed_at":"2026-07-06T23:14:11.211164Z","submitted_at":"2026-05-01T17:57:07Z","title":"$4\\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-09T18:38:12.253954Z"},"links":{"cited_paper":"/paper/2507.01377","citing_paper":"/paper/2605.00818"},"observation_digest":"sha256:6eaa7bf8b157f9bb40f47df9882669f94e6530175f97b46e988bb101cb38e4c5","observation_id":"1e7ec497-71ab-4cf4-94d4-2364601217a3","resolution":{"observed_at":"2026-05-11T16:11:08.065507Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"cited_work":{"arxiv_id":"2507.01377","doi":"10.48550/arxiv.2507.01377","metadata_source":"arxiv_reference","pith_arxiv_id":"2507.01377","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Zhang*, S","venue":"ArXiv.org","work_id":"ad6dbd46-c6fd-49c1-bd1b-3d17966efdd9","year":2025},"citing_paper":{"arxiv_id":"2606.23651","last_updated":"2026-06-22T17:36:23Z","snapshot_observed_at":"2026-07-06T23:58:20.975630Z","submitted_at":"2026-06-22T17:36:23Z","title":"Revisiting the 'Lensing is Low' Problem with UNIONS","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-06-26T07:18:50.552454Z"},"links":{"cited_paper":"/paper/2507.01377","citing_paper":"/paper/2606.23651"},"observation_digest":"sha256:3f2991fb9b76a496127ca253de86106917717b5cb0ca441e2dca18ab11111dcb","observation_id":"dcc25253-1b2f-4099-a210-f68f452255e8","resolution":{"observed_at":"2026-06-26T07:19:07.151711Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.01377/citation-record","integrity":"/paper/2507.01377/integrity","json":"/paper/2507.01377/citation-record.json","paper":"/paper/2507.01377"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:28.217400Z","title":"The cosmological parameter space consists of five flatΛCDM pa- rameters:[Ω 𝑚,Ω𝑐ℎ2,Ω𝑏ℎ2,𝑛𝑠,log(10 10𝐴𝑠)]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.217400Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:874f9238dd0bd9464a05469a6a5e2db671013cf003d7459e337da8713926ff59","observation_id":"1670b8e8-f23f-4cfe-a18b-6124cedb3806","resolution":{"observed_at":"2026-08-06T21:02:28.217400Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:28.170334Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.170334Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:3d34d56159a56279e36edb656863fa7d3d0d7d852b00caa8b35be746ea09dba8","observation_id":"3bf88a46-7f77-42da-ae6a-6a50b9c5197b","resolution":{"observed_at":"2026-08-06T21:02:28.170334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:28.278541Z","title":"no photo-𝑧uncertainty","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.278541Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:9c0f31b4f1c199025f6f25c6bf5d1b802d4acd057d3a7ffbb864b55451d1b1db","observation_id":"7795f032-bc2d-4ba4-b186-22294846c705","resolution":{"observed_at":"2026-08-06T21:02:28.278541Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:28.372374Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.372374Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:8d5054e66138b55230b09cfc431a50cfe75b8123d9df6cf5eeeebb107df7d57e","observation_id":"9bb78ca2-ba8b-4ad8-92d0-f0ae9969bdc9","resolution":{"observed_at":"2026-08-06T21:02:28.372374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:39.013828Z","title":null,"venue":null,"work_id":"4b32e218-c909-449e-acd1-d6d066f490b4","year":null},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.463930Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:4c143a74507a52ceda548c6ca8c33ffcbaba021fdade6e52b89b9700a1c707fb","observation_id":"a5fc98eb-4b4f-46bb-8bb1-56e40859b808","resolution":{"observed_at":"2026-08-06T21:02:39.019422Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:39.000450Z","title":null,"venue":null,"work_id":"2329ec93-4c7c-46e8-b1a5-b22143ab694f","year":null},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.567948Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:9574deb0ae135a838dbcd930074669e00b902edf296198d2b49b9a062019d521","observation_id":"5f0ca038-4ac7-4f5f-8cbd-76c7d1ef5a28","resolution":{"observed_at":"2026-08-06T21:02:39.004344Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:29.198539Z","title":"Aghanim, Y","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.198539Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:1007dedeb53c8d9c1c2d408feaae83fcdc60b92ab20480dd57b9829a772ce666","observation_id":"91e930c0-fc27-4361-ba36-37e072040de1","resolution":{"observed_at":"2026-08-06T21:02:29.198539Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18307","last_updated":"2024-05-28T16:00:54Z","snapshot_observed_at":"2026-08-06T19:57:32.726415Z","submitted_at":"2024-05-28T16:00:54Z","title":"Status of the LambdaCDM theory: supporting evidence and anomalies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.18307","snapshot_observed_at":"2026-08-06T21:02:28.744967Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.744967Z"},"links":{"cited_paper":"/paper/2405.18307","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:bada75de7e88ea212d49bfaff2a3686a73e142ae79e58b819ac9d5db6bc21e82","observation_id":"58e946a5-6b92-40e9-bf9c-72b1397daf17","resolution":{"observed_at":"2026-08-06T21:02:28.744967Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13549","last_updated":"2022-03-21T13:57:33Z","snapshot_observed_at":"2026-08-02T14:00:01.779912Z","submitted_at":"2021-05-28T01:58:58Z","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13549","snapshot_observed_at":"2026-08-06T21:02:28.866253Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.866253Z"},"links":{"cited_paper":"/paper/2105.13549","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:c41c8c997f9d9d249106a42a372f452e9809d13c7be2b71acc114a74a080c75a","observation_id":"99030594-9204-4b1c-a0d4-ab5136417dbc","resolution":{"observed_at":"2026-08-06T21:02:28.866253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00705","last_updated":"2023-12-28T04:58:17Z","snapshot_observed_at":"2026-08-06T03:09:33.589104Z","submitted_at":"2023-04-03T03:37:05Z","title":"Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.00705","snapshot_observed_at":"2026-08-06T21:02:28.953775Z","title":"Sugiyama, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.953775Z"},"links":{"cited_paper":"/paper/2304.00705","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:a9867d7ee3189f003a8f9bb379ad79f30fef010f64a77fc3f092bf05f981d105","observation_id":"413daf0e-6e2b-45c2-9578-72ff9d0ec0ee","resolution":{"observed_at":"2026-08-06T21:02:28.953775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19441","last_updated":"2025-10-21T16:24:56Z","snapshot_observed_at":"2026-07-06T20:58:14.950470Z","submitted_at":"2025-03-25T08:30:40Z","title":"KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19441","snapshot_observed_at":"2026-08-06T21:02:28.974897Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.974897Z"},"links":{"cited_paper":"/paper/2503.19441","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:50e80cc98cac0739538cfd0d20333f8096f89354d8572e123d2a12e4b64ec769","observation_id":"78cd7f06-74b8-402e-a5c8-00f1a8502e62","resolution":{"observed_at":"2026-08-06T21:02:28.974897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07603","last_updated":"2019-03-27T15:38:08Z","snapshot_observed_at":"2026-08-03T04:46:01.318400Z","submitted_at":"2019-03-18T17:50:59Z","title":"Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.07603","snapshot_observed_at":"2026-08-06T21:02:29.030699Z","title":"J.876, 85 (2019), arXiv:1903.07603 [astro-ph.CO]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.030699Z"},"links":{"cited_paper":"/paper/1903.07603","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:6e64e900493448031b4809536cbd45e507e267f6bcd9f1ca74b031b973961f98","observation_id":"c002fa34-8968-4e10-ac8a-61878d9fa1c8","resolution":{"observed_at":"2026-08-06T21:02:29.030699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.00845","last_updated":"2018-03-26T02:21:13Z","snapshot_observed_at":"2026-08-06T18:39:18.180076Z","submitted_at":"2017-10-02T18:03:12Z","title":"The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.00845","snapshot_observed_at":"2026-08-06T21:02:29.114753Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.114753Z"},"links":{"cited_paper":"/paper/1710.00845","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:f9ce187896bda9e40f0db990bc0e754c545eb610de7265c68d542358d6a76a2c","observation_id":"c603d266-6014-4fa9-a10a-bdf9258a5500","resolution":{"observed_at":"2026-08-06T21:02:29.114753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02419","last_updated":"2021-11-29T15:17:33Z","snapshot_observed_at":"2026-08-03T21:37:50.796376Z","submitted_at":"2021-11-03T18:00:01Z","title":"Cosmological inference from the emulator based halo model II: Joint analysis of galaxy-galaxy weak lensing and galaxy clustering from HSC-Y1 and SDSS","version":2},"cited_work":{"arxiv_id":"2111.02419","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.02419","snapshot_observed_at":"2026-08-06T21:02:38.390643Z","title":"Cosmological inference from the emulator based halo model II: Joint analysis of galaxy-galaxy weak lensing and galaxy clustering from HSC-Y1 and SDSS","venue":"astro-ph.CO","work_id":"95af214f-f7a7-46a2-8921-ae653444a7c8","year":2021},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.973421Z"},"links":{"cited_paper":"/paper/2111.02419","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:1420d0f584cafa7c2fe12099b92d9a3f9c10a361fcddac2742a5a78da31a9304","observation_id":"e137957b-aeb9-41c5-84bd-88d5ded5c5d2","resolution":{"observed_at":"2026-08-06T21:02:38.469422Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.05709","last_updated":"2023-02-11T14:51:33Z","snapshot_observed_at":"2026-08-07T08:09:37.398585Z","submitted_at":"2023-02-11T14:51:33Z","title":"Hubble Tension: The Evidence of New Physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.05709","snapshot_observed_at":"2026-08-06T21:02:29.290491Z","title":"Hu and F.-Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.290491Z"},"links":{"cited_paper":"/paper/2302.05709","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:ab6bf7b2ecc30a945a8e1c851fbaf4714a4d3e36b82d71db1eff08b322e96198","observation_id":"77b1b18d-617b-463e-87fa-b5b91f49be98","resolution":{"observed_at":"2026-08-06T21:02:29.290491Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11285","last_updated":"2020-10-13T11:11:55Z","snapshot_observed_at":"2026-08-04T06:53:16.719529Z","submitted_at":"2020-08-25T21:41:42Z","title":"Cosmology Intertwined III: $f \\sigma_8$ and $S_8$","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.11285","snapshot_observed_at":"2026-08-06T21:02:29.375524Z","title":"Di Valentino, L","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.375524Z"},"links":{"cited_paper":"/paper/2008.11285","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:098bd3d62fb565df4a00987200faf7efffca32172b6b88ca421507e6c4358810","observation_id":"e3b80231-91a3-4f0e-9972-4d5712d2b568","resolution":{"observed_at":"2026-08-06T21:02:29.375524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:38.971507Z","title":"Dodelson and F","venue":null,"work_id":"5dbfec88-4662-4153-8a8b-b64fb57aa84e","year":2020},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.521864Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:411e9ceebfeb36f3e511e638f13f7f972eaa7e5f52380456dfc3ec90f351c671","observation_id":"38a49631-d4f9-4625-ae69-294df31b38f2","resolution":{"observed_at":"2026-08-06T21:02:38.975576Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:29.631710Z","title":"Cooray and R","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.631710Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:80a61e2b2a40b2a0062f01634be539adcd3391bbb2a617d547c3b5ef8e7fe6ca","observation_id":"b060ddbd-3196-4760-a012-2d365fd788b1","resolution":{"observed_at":"2026-08-06T21:02:29.631710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12021","last_updated":"2025-11-24T12:55:36Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-11-18T20:03:34Z","title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12021","snapshot_observed_at":"2026-08-06T21:02:29.796745Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.796745Z"},"links":{"cited_paper":"/paper/2411.12021","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:141dca6a1bd5eb415caef59a4ee5135e14dc1b76625c8b7343618b7cbc7e199d","observation_id":"3aa87e22-956f-4448-81c9-010c2da8e76d","resolution":{"observed_at":"2026-08-06T21:02:29.796745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13540","last_updated":"2021-05-28T01:58:49Z","snapshot_observed_at":"2026-07-06T11:13:32.596343Z","submitted_at":"2021-05-28T01:58:49Z","title":"Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13540","snapshot_observed_at":"2026-08-06T21:02:29.893570Z","title":"Rodríguez-Monroy, N","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:29.893570Z"},"links":{"cited_paper":"/paper/2105.13540","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:55493fdc7864fa8a367e4cfb992acc3dcb71471f32a0f9e3c01228d6d960c737","observation_id":"2eac95dc-d857-40f2-9a68-acfe55353acc","resolution":{"observed_at":"2026-08-06T21:02:29.893570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00703","last_updated":"2023-11-16T16:21:04Z","snapshot_observed_at":"2026-07-06T15:11:07.800604Z","submitted_at":"2023-04-03T03:37:03Z","title":"Hyper Suprime-Cam Year 3 Results: Measurements of Clustering of SDSS-BOSS Galaxies, Galaxy-Galaxy Lensing and Cosmic Shear","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.00703","snapshot_observed_at":"2026-08-06T21:02:30.594300Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.594300Z"},"links":{"cited_paper":"/paper/2304.00703","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:6bf87d183d8214fbb5dcff36f2c8ff57d7fe686566d2494e1e174a44aaf1cb19","observation_id":"2874d9b0-93cc-4143-b625-19d6b808f7b5","resolution":{"observed_at":"2026-08-06T21:02:30.594300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.05858","last_updated":"2018-03-15T06:15:14Z","snapshot_observed_at":"2026-07-06T05:38:27.260025Z","submitted_at":"2017-04-19T18:00:51Z","title":"The Hyper Suprime-Cam SSP Survey: Overview and Survey Design","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.05858","snapshot_observed_at":"2026-08-06T21:02:30.032451Z","title":"Aihara, N","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.032451Z"},"links":{"cited_paper":"/paper/1704.05858","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:c1d4c155cb76fa91f72161fc6c222e1eef7226d4cad73957e8a4045f9d2159df","observation_id":"9b68cb14-1946-408e-a4f6-073a619334a3","resolution":{"observed_at":"2026-08-06T21:02:30.032451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:38.956431Z","title":"Miyazaki, Y","venue":null,"work_id":"03a26b2a-2200-4afd-abe0-b92be13a64f4","year":2018},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.128425Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:54f06ae1ad81adaa5c34ac67ef1fc6b74ddda6f8f5848eb1a6874db345e93e82","observation_id":"b4e00235-89c9-41c0-b55c-f9d323793c86","resolution":{"observed_at":"2026-08-06T21:02:38.961350Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2107.00136","last_updated":"2022-02-02T02:36:43Z","snapshot_observed_at":"2026-07-06T11:24:49.784288Z","submitted_at":"2021-06-30T22:46:20Z","title":"The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.00136","snapshot_observed_at":"2026-08-06T21:02:30.250411Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.250411Z"},"links":{"cited_paper":"/paper/2107.00136","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:35278a72f15eb89cd51c6279b5341c2014671f4bd484d8ded0de55cf6e54d747","observation_id":"dd336647-2a74-4d57-819a-b96a3341d3ec","resolution":{"observed_at":"2026-08-06T21:02:30.250411Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.00963","last_updated":"2015-05-21T19:10:12Z","snapshot_observed_at":"2026-08-06T05:47:44.936450Z","submitted_at":"2015-01-05T20:23:21Z","title":"The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.00963","snapshot_observed_at":"2026-08-06T21:02:30.314964Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.314964Z"},"links":{"cited_paper":"/paper/1501.00963","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:78d7144e7e13abeb5667de2ae3783966047e8c46264ca545ca259a616d39d603","observation_id":"1e870795-ded2-4ddb-83e6-e3e31d130fff","resolution":{"observed_at":"2026-08-06T21:02:30.314964Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00702","last_updated":"2023-11-30T23:20:07Z","snapshot_observed_at":"2026-08-06T08:21:34.190523Z","submitted_at":"2023-04-03T03:37:02Z","title":"Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.00702","snapshot_observed_at":"2026-08-06T21:02:30.392865Z","title":"Takada, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.392865Z"},"links":{"cited_paper":"/paper/2304.00702","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:c8d924df38c6ccd75a94caff144d37d4f6ec8192acd9c900de9c3a1b13f578b1","observation_id":"c9b70237-8544-448b-8c33-643fe51fc0b9","resolution":{"observed_at":"2026-08-06T21:02:30.392865Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00701","last_updated":"2023-04-04T17:22:14Z","snapshot_observed_at":"2026-08-05T13:53:35.348801Z","submitted_at":"2023-04-03T03:37:01Z","title":"Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.00701","snapshot_observed_at":"2026-08-06T21:02:30.479271Z","title":"Zhang, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.479271Z"},"links":{"cited_paper":"/paper/2304.00701","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:3a29704462edf774d0e83d69c7ca517b95a40ca3aa49e713e5be4517272b8c9a","observation_id":"11659c60-0a96-46d3-8e38-c284ced4882c","resolution":{"observed_at":"2026-08-06T21:02:30.479271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.10966","last_updated":"2021-11-22T03:10:08Z","snapshot_observed_at":"2026-07-06T12:10:42.498280Z","submitted_at":"2021-11-22T03:10:08Z","title":"HSC Year 1 cosmology results with the minimal bias method: HSC$\\times$BOSS galaxy-galaxy weak lensing and BOSS galaxy clustering","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.10966","snapshot_observed_at":"2026-08-06T21:02:31.112642Z","title":"Sugiyama, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.112642Z"},"links":{"cited_paper":"/paper/2111.10966","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:3880cf1504eb55e85eba1920f1282cb356dcf2f9492cb83428b0274171ba2a02","observation_id":"588ad967-53dc-41e8-a00e-1307cbfd69aa","resolution":{"observed_at":"2026-08-06T21:02:31.112642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00704","last_updated":"2023-04-06T15:04:24Z","snapshot_observed_at":"2026-08-06T04:34:20.742819Z","submitted_at":"2023-04-03T03:37:04Z","title":"Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo Model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.00704","snapshot_observed_at":"2026-08-06T21:02:30.690511Z","title":"Miyatake, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.690511Z"},"links":{"cited_paper":"/paper/2304.00704","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:b4584fec76e6ecfd93a9569311265deee7c2ac93775960aebc550286ffa47f79","observation_id":"69d1e344-f81b-4515-8605-09f2ce24bf21","resolution":{"observed_at":"2026-08-06T21:02:30.690511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.0744","last_updated":"2010-12-20T08:03:18Z","snapshot_observed_at":"2026-07-06T02:16:15.421430Z","submitted_at":"2010-10-05T01:05:31Z","title":"Combining cluster observables and stacked weak lensing to probe dark energy: Self-calibration of systematic uncertainties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.0744","snapshot_observed_at":"2026-08-06T21:02:30.761292Z","title":"Oguri and M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.761292Z"},"links":{"cited_paper":"/paper/1010.0744","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:f06df86e123405e90f1fd4178627e4709adadfd0c4d17931d03a2ff4e8a63caa","observation_id":"98e4fc5a-6b55-4009-81f3-e7ce7b9640d6","resolution":{"observed_at":"2026-08-06T21:02:30.761292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.16516","last_updated":"2023-11-20T20:00:05Z","snapshot_observed_at":"2026-07-06T14:24:45.757232Z","submitted_at":"2022-11-29T19:00:00Z","title":"Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.16516","snapshot_observed_at":"2026-08-06T21:02:30.847406Z","title":"Mandelbaum, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.847406Z"},"links":{"cited_paper":"/paper/2211.16516","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:148c7ae0b9adbedb081812103d26e8f1afa0ba1ea80a530f520b2aa1aad9d506","observation_id":"ec3e9bc1-3825-4d72-a71d-eb245c934cbf","resolution":{"observed_at":"2026-08-06T21:02:30.847406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.01537","last_updated":"2018-09-04T13:58:22Z","snapshot_observed_at":"2026-07-06T05:54:07.143205Z","submitted_at":"2017-08-04T14:52:34Z","title":"Dark Energy Survey Year 1 Results: Galaxy-Galaxy Lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.01537","snapshot_observed_at":"2026-08-06T21:02:30.912374Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.912374Z"},"links":{"cited_paper":"/paper/1708.01537","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:25411ee4a00a547a17f6aa670b2540a3dc13b8c2b761bc4f6766871fcd83eb4e","observation_id":"909084df-3465-427a-8211-01b14581a8d0","resolution":{"observed_at":"2026-08-06T21:02:30.912374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.4973","last_updated":"2010-07-23T11:15:55Z","snapshot_observed_at":"2026-07-06T02:00:42.877269Z","submitted_at":"2009-11-26T00:04:53Z","title":"An algorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.4973","snapshot_observed_at":"2026-08-06T21:02:30.981587Z","title":"Baldauf, R","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:30.981587Z"},"links":{"cited_paper":"/paper/0911.4973","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:fd50a7a9608716acca6ae20aaf84e198447f8447b47f331d631748eb85b27521","observation_id":"fbd14ac3-cde3-48b7-98e2-70f8e5b61b68","resolution":{"observed_at":"2026-08-06T21:02:30.981587Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.1120","last_updated":"2013-03-10T02:26:17Z","snapshot_observed_at":"2026-07-06T02:51:15.592134Z","submitted_at":"2012-07-04T20:35:56Z","title":"Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.1120","snapshot_observed_at":"2026-08-06T21:02:31.059679Z","title":"Nakajima, R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.059679Z"},"links":{"cited_paper":"/paper/1207.1120","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:9d9a8dffe462d8eedc9ae4be79acdff0ca74523a1c3d56f96c7f37603ec52e92","observation_id":"2a4821e8-b2d5-4191-af66-8bdea316f2ec","resolution":{"observed_at":"2026-08-06T21:02:31.059679Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:38.941062Z","title":"Lupton, S","venue":null,"work_id":"b2ee9c67-8aa4-4867-a6f1-14ed870295aa","year":2018},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.666232Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:273a6db39ef7f6bb318bb4468bd17e6e25b19164fa77b2848dee67ac67e23431","observation_id":"f6992a4c-4c02-471a-be08-29ef4742d968","resolution":{"observed_at":"2026-08-06T21:02:38.945873Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.09504","last_updated":"2019-07-26T13:32:16Z","snapshot_observed_at":"2026-07-06T07:16:36.095212Z","submitted_at":"2018-11-23T14:59:14Z","title":"Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.09504","snapshot_observed_at":"2026-08-06T21:02:31.210440Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.210440Z"},"links":{"cited_paper":"/paper/1811.09504","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:7830a046bb0ecfffba05f7eb95a1bc92b00ce0cacd617aa3a0350e98baa632d5","observation_id":"569b63bf-2218-4201-8fbd-5ec238693390","resolution":{"observed_at":"2026-08-06T21:02:31.210440Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.0022","last_updated":"2012-11-07T22:32:13Z","snapshot_observed_at":"2026-07-06T02:52:54.937210Z","submitted_at":"2012-07-31T20:05:09Z","title":"The Baryon Oscillation Spectroscopic Survey of SDSS-III","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.0022","snapshot_observed_at":"2026-08-06T21:02:31.267630Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.267630Z"},"links":{"cited_paper":"/paper/1208.0022","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:0d965db82302819198ed77f797f4acd1c34dad015e86764e55a5c242857345fc","observation_id":"1c5e9052-c177-429a-a0e9-8baa77a9b634","resolution":{"observed_at":"2026-08-06T21:02:31.267630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.06873","last_updated":"2020-08-16T10:25:36Z","snapshot_observed_at":"2026-07-31T11:33:20.703143Z","submitted_at":"2020-08-16T10:25:36Z","title":"Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.06873","snapshot_observed_at":"2026-08-06T21:02:31.352730Z","title":"Sugiyama, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.352730Z"},"links":{"cited_paper":"/paper/2008.06873","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:2c70b8c95171e1f2e5bdcfc3666b5dd3f259f678e2aa7c949328e4d31faae91c","observation_id":"257b9e72-df60-4bac-8854-216cb323eb97","resolution":{"observed_at":"2026-08-06T21:02:31.352730Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.0649","last_updated":"2009-03-17T13:15:00Z","snapshot_observed_at":"2026-07-06T01:46:51.846123Z","submitted_at":"2008-12-03T04:38:54Z","title":"The Seventh Data Release of the Sloan Digital Sky Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.0649","snapshot_observed_at":"2026-08-06T21:02:31.443064Z","title":"Allam,C.AllendePrieto,D.An,K.S.J.Anderson,S.F.Ander- son, J.Annis, N.A.Bahcall, C.A.L.Bailer-Jones, J.C.Baren- tine, B","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.443064Z"},"links":{"cited_paper":"/paper/0812.0649","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:cf0a7b059671b3aab7a7337f2cbc95fc686187065cdc4c51da15e4faeb2f779a","observation_id":"a11beb62-7bd6-4e81-9e56-2ac4a622af4c","resolution":{"observed_at":"2026-08-06T21:02:31.443064Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0602326","last_updated":"2006-02-15T02:50:35Z","snapshot_observed_at":"2026-07-30T22:06:41.814247Z","submitted_at":"2006-02-15T02:50:35Z","title":"The 2.5 m Telescope of the Sloan Digital Sky Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0602326","snapshot_observed_at":"2026-08-06T21:02:31.529801Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.529801Z"},"links":{"cited_paper":"/paper/astro-ph/0602326","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:0dba3e2610143495936cbb7fdd8e4e9b9b652b250ed3dcf70c86b8ccb4d8a35e","observation_id":"b1559873-22fd-4f1d-b35a-524657ff2728","resolution":{"observed_at":"2026-08-06T21:02:31.529801Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.02501","last_updated":"2024-11-06T11:09:38Z","snapshot_observed_at":"2026-07-06T19:10:12.721500Z","submitted_at":"2024-09-04T07:57:20Z","title":"Impact of survey spatial variability on galaxy redshift distributions and the cosmological $3\\times2$-point statistics for the Rubin Legacy Survey of Space and Time (LSST)","version":2},"cited_work":{"arxiv_id":"2409.02501","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.02501","snapshot_observed_at":"2026-08-06T21:02:37.923010Z","title":"Impact of survey spatial variability on galaxy redshift distributions and the cosmological $3\\times2$-point statistics for the Rubin Legacy Survey of Space and Time (LSST)","venue":"astro-ph.CO","work_id":"30e15622-d1c4-4a62-8f80-c9902d41c490","year":2024},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.576009Z"},"links":{"cited_paper":"/paper/2409.02501","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:32bfc2b4a68de837b2a6a27eef75fccfca3dfb74c4d5973a56f6d59c26489343","observation_id":"0f868b9b-aac3-4bbe-822f-c1cb54db3ffb","resolution":{"observed_at":"2026-08-06T21:02:38.005195Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1407.7676","last_updated":"2015-02-15T12:13:45Z","snapshot_observed_at":"2026-07-06T03:50:19.678861Z","submitted_at":"2014-07-29T09:36:05Z","title":"GalSim: The modular galaxy image simulation toolkit","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.7676","snapshot_observed_at":"2026-08-06T21:02:32.126356Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.126356Z"},"links":{"cited_paper":"/paper/1407.7676","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:43fb73b788b29df88c9800b314f779b22b329e94ac3fb652a3c3f6fce0f71ee8","observation_id":"56ea5fcb-ecc6-4582-8a9a-59aebf36587b","resolution":{"observed_at":"2026-08-06T21:02:32.126356Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.13045","last_updated":"2021-08-30T08:10:14Z","snapshot_observed_at":"2026-08-05T11:50:30.862426Z","submitted_at":"2021-08-30T08:10:14Z","title":"Third Data Release of the Hyper Suprime-Cam Subaru Strategic Program","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.13045","snapshot_observed_at":"2026-08-06T21:02:31.723720Z","title":"Aihara, Y","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.723720Z"},"links":{"cited_paper":"/paper/2108.13045","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:462b680f7eb0b82de1a57f3aa9a9d54d8674b477ac75eeb826ac0a8caf00f94c","observation_id":"4dab924b-8f1b-4751-891a-f409c2a14ecc","resolution":{"observed_at":"2026-08-06T21:02:31.723720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12221","last_updated":"2019-08-22T08:15:21Z","snapshot_observed_at":"2026-07-06T07:56:19.842919Z","submitted_at":"2019-05-29T05:23:25Z","title":"Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12221","snapshot_observed_at":"2026-08-06T21:02:31.789495Z","title":"Aihara, Y","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.789495Z"},"links":{"cited_paper":"/paper/1905.12221","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:8c3ca265cf49bacc0f25d84c12da23784b4d1cf4b92db266f22fcea76e415c8c","observation_id":"d17d0315-e6de-4ac7-81e7-aea4afad981f","resolution":{"observed_at":"2026-08-06T21:02:31.789495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.01511","last_updated":"2020-03-16T05:22:50Z","snapshot_observed_at":"2026-08-03T18:53:40.778565Z","submitted_at":"2020-02-29T08:03:19Z","title":"Photometric Redshifts for the Hyper Suprime-Cam Subaru Strategic Program Data Release 2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.01511","snapshot_observed_at":"2026-08-06T21:02:31.849247Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.849247Z"},"links":{"cited_paper":"/paper/2003.01511","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:16c42c184288c29f54c2dcf104ba0aaa5af04312d33733d6e483d046573ee6a1","observation_id":"2705c7e0-05f3-4727-a9fe-0478c52bfc5f","resolution":{"observed_at":"2026-08-06T21:02:31.849247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.06766","last_updated":"2017-05-18T18:55:40Z","snapshot_observed_at":"2026-07-06T05:43:17.830485Z","submitted_at":"2017-05-18T18:55:40Z","title":"The Hyper Suprime-Cam Software Pipeline","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.06766","snapshot_observed_at":"2026-08-06T21:02:31.911344Z","title":"Bosch, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.911344Z"},"links":{"cited_paper":"/paper/1705.06766","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:df1b234c628397e76d1e93aba4f1d524ffd81388f0bbe1970840ffd1bc71cdb5","observation_id":"0513c7aa-b576-4b27-99e8-b63b97345238","resolution":{"observed_at":"2026-08-06T21:02:31.911344Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0301054","last_updated":"2003-04-04T19:14:45Z","snapshot_observed_at":"2026-07-07T00:30:33.951336Z","submitted_at":"2003-01-04T17:37:16Z","title":"Shear calibration biases in weak lensing surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0301054","snapshot_observed_at":"2026-08-06T21:02:31.984694Z","title":"Hirata and U","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:31.984694Z"},"links":{"cited_paper":"/paper/astro-ph/0301054","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:d6db1b49787e79597a0ed827fe1c9e831e878da56c836e20b1317768c352e649","observation_id":"0c4fec03-8376-4cb7-a1af-34306fa2c799","resolution":{"observed_at":"2026-08-06T21:02:31.984694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:32.047257Z","title":"Mandelbaum, C","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.047257Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:aae06bcd1666e5e61c445d3b0b1f64ca88455269fc66ebd891db603f43f5a878","observation_id":"25ee1a28-6245-4b8c-8a47-b96110d51b3b","resolution":{"observed_at":"2026-08-06T21:02:32.047257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9611107","last_updated":"1997-10-21T23:14:37Z","snapshot_observed_at":"2026-07-07T01:15:03.940917Z","submitted_at":"1996-11-13T22:59:55Z","title":"A Universal Density Profile from Hierarchical Clustering","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9611107","snapshot_observed_at":"2026-08-06T21:02:32.783275Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.783275Z"},"links":{"cited_paper":"/paper/astro-ph/9611107","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:5b455bae9996bccec1118cb1a7bcd1015592a5b4e72d0f8025592b2a6adee13b","observation_id":"89ef1cbe-5673-4aab-87c5-b183f7af2e7e","resolution":{"observed_at":"2026-08-06T21:02:32.783275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.4693","last_updated":"2014-08-04T22:45:52Z","snapshot_observed_at":"2026-07-06T03:49:19.093285Z","submitted_at":"2014-07-17T14:59:53Z","title":"A cluster finding algorithm based on the multiband identification of red sequence galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.4693","snapshot_observed_at":"2026-08-06T21:02:32.223761Z","title":"Oguri, Mon","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.223761Z"},"links":{"cited_paper":"/paper/1407.4693","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:4f3f08d22cc5b74a0dc8fcec6a6128a4b6ab8b4fee8a178f439d64e9b6ad4761","observation_id":"0da09d7e-690a-45b0-8e11-7e776293e573","resolution":{"observed_at":"2026-08-06T21:02:32.223761Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.06792","last_updated":"2017-06-30T02:40:28Z","snapshot_observed_at":"2026-08-03T19:49:36.260781Z","submitted_at":"2017-05-18T20:34:49Z","title":"Two- and three-dimensional wide-field weak lensing mass maps from the Hyper Suprime-Cam Subaru Strategic Program S16A data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.06792","snapshot_observed_at":"2026-08-06T21:02:32.309777Z","title":"Oguri, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.309777Z"},"links":{"cited_paper":"/paper/1705.06792","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:5fa0612f774864e3eba38b5b22f191036e500002efe0f4b8f76d8ef1119c3742","observation_id":"c6ef82d7-9e8f-4cf0-81c4-33b7ac0400dc","resolution":{"observed_at":"2026-08-06T21:02:32.309777Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00752","last_updated":"2017-08-23T23:07:01Z","snapshot_observed_at":"2026-07-06T05:17:08.626715Z","submitted_at":"2016-11-02T19:50:06Z","title":"Galaxy-galaxy lensing estimators and their covariance properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00752","snapshot_observed_at":"2026-08-06T21:02:32.400131Z","title":"Singh, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.400131Z"},"links":{"cited_paper":"/paper/1611.00752","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:f4fc4893889994b113fdc49d938e90a64dc43704cb78646be0130eb22ffe13e3","observation_id":"1a73cb31-7d1a-4934-ba79-5be3462c1fc8","resolution":{"observed_at":"2026-08-06T21:02:32.400131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.01472","last_updated":"2017-11-24T10:51:49Z","snapshot_observed_at":"2026-08-02T11:42:32.391535Z","submitted_at":"2017-06-05T18:00:15Z","title":"Full-sky Gravitational Lensing Simulation for Large-area Galaxy Surveys and Cosmic Microwave Background Experiments","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.01472","snapshot_observed_at":"2026-08-06T21:02:32.511850Z","title":"Takahashi, T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.511850Z"},"links":{"cited_paper":"/paper/1706.01472","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:91a502be5c961e4092acca2649c68ed76f7bed0d7cd4a5f1a01b7263ed6add34","observation_id":"ffdaaf02-c006-4a27-a08e-77b8a0a5c5a8","resolution":{"observed_at":"2026-08-06T21:02:32.511850Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:38.925484Z","title":"Hinshaw, D","venue":null,"work_id":"2eabd296-a398-4a97-95ee-85ca46b2ef79","year":2013},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.591312Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:e908342f730c4a882be07e7719736d39a503a8d0a5165919feaae210fc3e7e55","observation_id":"e1ce3b80-7ad1-499e-b8a1-6e4c2f7ec7a8","resolution":{"observed_at":"2026-08-06T21:02:38.930904Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.09488","last_updated":"2019-03-17T02:24:58Z","snapshot_observed_at":"2026-07-06T07:29:20.308370Z","submitted_at":"2019-01-28T02:37:15Z","title":"Mock galaxy shape catalogs in the Subaru Hyper Suprime-Cam Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.09488","snapshot_observed_at":"2026-08-06T21:02:32.677552Z","title":"Shirasaki, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.677552Z"},"links":{"cited_paper":"/paper/1901.09488","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:4789245bc3f4fdd01c623a481c01c10bd479ab19c781c9be3fb9de06b6fa1d9f","observation_id":"b95316d5-d568-42c0-a5f6-3b12b8895292","resolution":{"observed_at":"2026-08-06T21:02:32.677552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.1153","last_updated":"2008-02-27T20:30:31Z","snapshot_observed_at":"2026-07-06T01:29:48.173337Z","submitted_at":"2007-09-07T20:18:02Z","title":"Cross-correlation Weak Lensing of SDSS Galaxy Clusters I: Measurements","version":2},"cited_work":{"arxiv_id":"0709.1153","doi":null,"metadata_source":"pith","pith_arxiv_id":"0709.1153","snapshot_observed_at":"2026-08-06T21:02:36.910895Z","title":"Cross-correlation Weak Lensing of SDSS Galaxy Clusters I: Measurements","venue":"astro-ph","work_id":"0a32c605-17ca-45ca-98f2-26e704e6f414","year":2007},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.458798Z"},"links":{"cited_paper":"/paper/0709.1153","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:f40cf4647958ca4883a87fde7f2ce46e098b2d6ce09ea0a6fd7416df414ed63c","observation_id":"164b4c38-b926-486d-ae0e-fcda2683cfa6","resolution":{"observed_at":"2026-08-06T21:02:37.031446Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1110.4372","last_updated":"2013-01-12T02:16:53Z","snapshot_observed_at":"2026-07-06T02:36:06.035370Z","submitted_at":"2011-10-19T20:00:04Z","title":"The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.4372","snapshot_observed_at":"2026-08-06T21:02:32.869055Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.869055Z"},"links":{"cited_paper":"/paper/1110.4372","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:4d6cf6e2a0bee4920d07d700adf8a64f87f2189c28e455ff14f2d75e965d114a","observation_id":"62a7adba-339c-4889-bd43-5fb110d2bf25","resolution":{"observed_at":"2026-08-06T21:02:32.869055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:32.978504Z","title":"Zehavi, Z","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:32.978504Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:74a5cfe442678180c0fa4e431b4924fefe08e5209a8f274d6c5e73ced999e938","observation_id":"03eef9cc-29b5-4409-ab80-6fb7591b6f73","resolution":{"observed_at":"2026-08-06T21:02:32.978504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.1856","last_updated":"2015-03-22T09:33:54Z","snapshot_observed_at":"2026-07-06T03:48:17.300160Z","submitted_at":"2014-07-07T20:08:23Z","title":"The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.1856","snapshot_observed_at":"2026-08-06T21:02:33.076230Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.076230Z"},"links":{"cited_paper":"/paper/1407.1856","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:39adca80dd6272536ef4cf55004500f306ce5d24f4f8eb34ea1001c5ebd835a2","observation_id":"74ab5bc6-8de8-4a20-b12a-1f81e603c84a","resolution":{"observed_at":"2026-08-06T21:02:33.076230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9912508","last_updated":"1999-12-23T23:20:38Z","snapshot_observed_at":"2026-08-05T12:09:14.357181Z","submitted_at":"1999-12-23T23:20:38Z","title":"Weak Gravitational Lensing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9912508","snapshot_observed_at":"2026-08-06T21:02:33.176325Z","title":"Bartelmann and P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.176325Z"},"links":{"cited_paper":"/paper/astro-ph/9912508","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:90f80ed3caefe10421c5932deae8ef905e1b1ec9fb68952785c475f14dca8995","observation_id":"7e17c3f0-fa20-4106-8512-5fd68fc3e0a7","resolution":{"observed_at":"2026-08-06T21:02:33.176325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0312036","last_updated":"2004-01-28T00:11:35Z","snapshot_observed_at":"2026-07-07T00:38:42.432535Z","submitted_at":"2003-12-01T20:50:46Z","title":"The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0312036","snapshot_observed_at":"2026-08-06T21:02:33.248322Z","title":"McKay, A","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.248322Z"},"links":{"cited_paper":"/paper/astro-ph/0312036","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:f74ed5e4346bc326c1279898fc61c5275e868d8190dd8c5c150609ece61a3a9e","observation_id":"da0fde36-0615-4bb4-8873-6fde181b0a12","resolution":{"observed_at":"2026-08-06T21:02:33.248322Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0210604","last_updated":"2002-12-02T20:51:01Z","snapshot_observed_at":"2026-07-07T00:29:21.493197Z","submitted_at":"2002-10-28T19:59:26Z","title":"Weak Lensing Results from the 75 Square Degree CTIO Survey","version":2},"cited_work":{"arxiv_id":"astro-ph/0210604","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0210604","snapshot_observed_at":"2026-08-06T21:02:37.195003Z","title":"Weak Lensing Results from the 75 Square Degree CTIO Survey","venue":"astro-ph","work_id":"4280e9d5-4712-4aa5-bc87-a9ccf356410a","year":2002},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.363256Z"},"links":{"cited_paper":"/paper/astro-ph/0210604","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:b0286284e64a3ec4cffe209bd96995b1f1cee531feb7c3d7d558d85f218f5e8b","observation_id":"67e7d242-d947-42a8-871e-27ce49c7b03d","resolution":{"observed_at":"2026-08-06T21:02:37.319027Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1206.6890","last_updated":"2012-06-28T20:00:39Z","snapshot_observed_at":"2026-07-06T02:50:54.653474Z","submitted_at":"2012-06-28T20:00:39Z","title":"Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- I. Theoretical Framework","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.6890","snapshot_observed_at":"2026-08-06T21:02:33.997048Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.997048Z"},"links":{"cited_paper":"/paper/1206.6890","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:9e97b1f5df4a693a9e5d042fc295bd2340271be4fe1331aeeffe6407a0ee4ca8","observation_id":"19d2ae36-679b-49f6-b019-0f41c9fc821b","resolution":{"observed_at":"2026-08-06T21:02:33.997048Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.1480","last_updated":"2015-03-21T02:31:46Z","snapshot_observed_at":"2026-07-06T03:27:32.821538Z","submitted_at":"2013-11-06T19:37:05Z","title":"The Weak Lensing Signal and the Clustering of BOSS Galaxies I: Measurements","version":2},"cited_work":{"arxiv_id":"1311.1480","doi":null,"metadata_source":"pith","pith_arxiv_id":"1311.1480","snapshot_observed_at":"2026-08-06T21:02:36.604045Z","title":"The Weak Lensing Signal and the Clustering of BOSS Galaxies I: Measurements","venue":"astro-ph.CO","work_id":"1c3ce9ce-43f3-4a08-a430-9606e7a87a9f","year":2013},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.557535Z"},"links":{"cited_paper":"/paper/1311.1480","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:fd3e7702ead9a7855da8bd840d4bd67c4a812ef2773a310f214bc181f399533f","observation_id":"3f23d984-33c6-4a2f-9057-48e884822a68","resolution":{"observed_at":"2026-08-06T21:02:36.725470Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0705.0166","last_updated":"2008-04-18T18:10:33Z","snapshot_observed_at":"2026-07-06T01:27:02.768950Z","submitted_at":"2007-05-01T21:25:39Z","title":"Dark energy constraints from cosmic shear power spectra: impact of intrinsic alignments on photometric redshift requirements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.0166","snapshot_observed_at":"2026-08-06T21:02:33.645073Z","title":"Bridle and L","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.645073Z"},"links":{"cited_paper":"/paper/0705.0166","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:f0c97374c6f3f700dd1102b9f6d9af9509b976e1255780227cb5b607a1b6e51c","observation_id":"d4e3f7ae-db8f-46d1-9d32-3984bdc3c0b2","resolution":{"observed_at":"2026-08-06T21:02:33.645073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.1808","last_updated":"2013-03-07T20:42:16Z","snapshot_observed_at":"2026-08-03T17:52:15.648305Z","submitted_at":"2013-03-07T20:42:16Z","title":"CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.1808","snapshot_observed_at":"2026-08-06T21:02:33.739074Z","title":"Heymans, E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.739074Z"},"links":{"cited_paper":"/paper/1303.1808","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:e62823252435ac22a95c90a92ca59aae9d7c9be4ea3150be88935a4a172f4863","observation_id":"329d052f-73f5-40c2-ae58-f02c6f213e39","resolution":{"observed_at":"2026-08-06T21:02:33.739074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9911177","last_updated":"2000-06-01T12:13:06Z","snapshot_observed_at":"2026-07-07T01:29:40.678750Z","submitted_at":"1999-11-10T17:57:36Z","title":"Efficient Computation of CMB anisotropies in closed FRW models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9911177","snapshot_observed_at":"2026-08-06T21:02:33.789577Z","title":"Lewis, A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.789577Z"},"links":{"cited_paper":"/paper/astro-ph/9911177","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:b10a927f1a9d18eb698a357728df4b37681fd8c68c6de2fad1bb827348f33186","observation_id":"fcd7ab35-d550-42c7-92d9-e4012b8259a4","resolution":{"observed_at":"2026-08-06T21:02:33.789577Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.2701","last_updated":"2012-11-05T02:47:22Z","snapshot_observed_at":"2026-07-06T02:53:40.801090Z","submitted_at":"2012-08-13T20:11:04Z","title":"Revising the Halofit Model for the Nonlinear Matter Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.2701","snapshot_observed_at":"2026-08-06T21:02:33.864390Z","title":"J.761, 152 (2012), arXiv:1208.2701 [astro-ph.CO]","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.864390Z"},"links":{"cited_paper":"/paper/1208.2701","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:e2b057d2dc030fa28b270b342eaf38f0c7389e944de20aaa3c93660b912a7dd6","observation_id":"5a54acee-4942-455e-bd50-0cfd8e2e467f","resolution":{"observed_at":"2026-08-06T21:02:33.864390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.01146","last_updated":"2019-08-20T17:10:49Z","snapshot_observed_at":"2026-07-06T06:59:10.619185Z","submitted_at":"2018-09-04T18:00:01Z","title":"Modeling baryonic physics in future weak lensing surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.01146","snapshot_observed_at":"2026-08-06T21:02:33.912268Z","title":"Huang, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:33.912268Z"},"links":{"cited_paper":"/paper/1809.01146","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:a426fd4f33d6cee5b403fd3073faddad3be3aa3bad1d7a8c4aeeebb643459a50","observation_id":"fb13aea6-5a76-4075-8768-d278c0efd174","resolution":{"observed_at":"2026-08-06T21:02:33.912268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.08233","last_updated":"2022-02-16T18:24:56Z","snapshot_observed_at":"2026-07-06T12:38:30.234691Z","submitted_at":"2022-02-16T18:24:56Z","title":"Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey","version":1},"cited_work":{"arxiv_id":"2202.08233","doi":null,"metadata_source":"pith","pith_arxiv_id":"2202.08233","snapshot_observed_at":"2026-08-06T21:02:36.281886Z","title":"Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey","venue":"astro-ph.CO","work_id":"75b6877d-dc4b-4809-9100-cfa99bec1b7f","year":2022},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:34.885497Z"},"links":{"cited_paper":"/paper/2202.08233","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:fef84c34bd7f576827143ae2b6a5635aca6c526e1cdd5e33c0adb774ac36f8f4","observation_id":"1954ce2b-5460-462f-80c2-8766a591c412","resolution":{"observed_at":"2026-08-06T21:02:36.342767Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13541","last_updated":"2022-04-05T19:46:23Z","snapshot_observed_at":"2026-07-06T11:13:32.596343Z","submitted_at":"2021-05-28T01:58:50Z","title":"Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13541","snapshot_observed_at":"2026-08-06T21:02:34.106938Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:34.106938Z"},"links":{"cited_paper":"/paper/2105.13541","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:5c571a337a599ed81ec226a1a8778cde09eb7b4cbd13b7164c1a2508003fc631","observation_id":"1706e2e9-6ca2-46ce-813e-8fe158b2c18c","resolution":{"observed_at":"2026-08-06T21:02:34.106938Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0406275","last_updated":"2010-08-24T18:31:06Z","snapshot_observed_at":"2026-08-05T15:00:32.709238Z","submitted_at":"2004-06-10T20:21:55Z","title":"Intrinsic alignment-lensing interference as a contaminant of cosmic shear","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0406275","snapshot_observed_at":"2026-08-06T21:02:34.332635Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:34.332635Z"},"links":{"cited_paper":"/paper/astro-ph/0406275","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:5c3db9a30979d357a04fbc80392f5395a8a0ddeb7e466b45d89e73cd62747109","observation_id":"d257702f-d006-446b-9dcd-d9baf4bb39be","resolution":{"observed_at":"2026-08-06T21:02:34.332635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.1755","last_updated":"2015-04-08T16:28:29Z","snapshot_observed_at":"2026-07-06T03:59:48.655454Z","submitted_at":"2014-11-06T21:00:02Z","title":"Intrinsic alignments of SDSS-III BOSS LOWZ sample galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.1755","snapshot_observed_at":"2026-08-06T21:02:34.434366Z","title":"Singh, R","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:34.434366Z"},"links":{"cited_paper":"/paper/1411.1755","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:b91bbddba0b7cf1e57e71587ec35bfb044fc5d6b925102ba3e15896bf080904c","observation_id":"39ab77f1-8213-40b8-8c7a-b08a3cefeada","resolution":{"observed_at":"2026-08-06T21:02:34.434366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.12675","last_updated":"2024-06-18T14:49:09Z","snapshot_observed_at":"2026-07-06T18:33:02.286642Z","submitted_at":"2024-06-18T14:49:09Z","title":"Dark Energy Survey Year 3 Results: Cosmology from galaxy clustering and galaxy-galaxy lensing in harmonic space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.12675","snapshot_observed_at":"2026-08-06T21:02:34.548022Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:34.548022Z"},"links":{"cited_paper":"/paper/2406.12675","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:34487afcfb819cdb91621ec096aea86ecaafc12147dc77cfd1c9bc13f7b3984f","observation_id":"a9f4ce5e-e53e-4875-a7bb-9fad39640f1a","resolution":{"observed_at":"2026-08-06T21:02:34.548022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.10169","last_updated":"2023-04-18T19:03:14Z","snapshot_observed_at":"2026-07-06T13:22:57.607155Z","submitted_at":"2022-06-21T08:02:25Z","title":"Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.10169","snapshot_observed_at":"2026-08-06T21:02:34.724245Z","title":"Zhang, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:34.724245Z"},"links":{"cited_paper":"/paper/2206.10169","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:bdd5a79882e55efea37a6378d77ff4f41742c439f888dcf4efd8c7bbb70673c7","observation_id":"047ed741-6020-4838-84b2-b4563acab862","resolution":{"observed_at":"2026-08-06T21:02:34.724245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:38.986158Z","title":null,"venue":null,"work_id":"76e64c71-3166-44e2-b955-48f64a9dee35","year":null},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:28.651171Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:d753aa0291fdf59055d03e611c1fbc23735f6c7e73859614a5512a699945c320","observation_id":"6f33b379-93de-4d24-a143-9fc6dc39be3f","resolution":{"observed_at":"2026-08-06T21:02:38.990193Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.11594","last_updated":"2019-08-08T12:38:48Z","snapshot_observed_at":"2026-07-06T08:10:28.700449Z","submitted_at":"2019-07-26T14:31:58Z","title":"The BAO+BBN take on the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.11594","snapshot_observed_at":"2026-08-06T21:02:35.016090Z","title":"Schöneberg, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:35.016090Z"},"links":{"cited_paper":"/paper/1907.11594","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:5663b5e3c98cf0cf5da197eb8d989ae19d3760107477c5c6f29a67a1520ff9b5","observation_id":"53355ae9-8691-4ea1-8b86-2f9867bf1a4d","resolution":{"observed_at":"2026-08-06T21:02:35.016090Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608064","last_updated":"2006-12-05T12:58:45Z","snapshot_observed_at":"2026-08-06T21:02:04.532561Z","submitted_at":"2006-08-02T15:21:52Z","title":"Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0608064","snapshot_observed_at":"2026-08-06T21:02:35.174416Z","title":"Hartlap, P","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:35.174416Z"},"links":{"cited_paper":"/paper/astro-ph/0608064","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:e5b3fc958a556e7c45eb5a74651cd6028b3b74ff8d75c5e935240585bfc98c3b","observation_id":"d421d4f0-41da-40df-ac68-c4249c625ecf","resolution":{"observed_at":"2026-08-06T21:02:35.174416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.3409","last_updated":"2018-04-03T13:50:52Z","snapshot_observed_at":"2026-08-04T19:52:15.282208Z","submitted_at":"2014-09-11T12:20:37Z","title":"CosmoSIS: modular cosmological parameter estimation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.3409","snapshot_observed_at":"2026-08-06T21:02:35.311879Z","title":"Bridle, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:35.311879Z"},"links":{"cited_paper":"/paper/1409.3409","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:7956688628ef6a51b7b5a4df981daf1c1d51f01ba23232bf9e79b92ec0fdd623","observation_id":"01f4dfc5-1d35-4706-8c98-faa05258d82e","resolution":{"observed_at":"2026-08-06T21:02:35.311879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.00113","last_updated":"2020-12-31T23:58:13Z","snapshot_observed_at":"2026-07-06T10:29:15.513689Z","submitted_at":"2020-12-31T23:58:13Z","title":"Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.00113","snapshot_observed_at":"2026-08-06T21:02:35.437237Z","title":"Miyatake, Y","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:35.437237Z"},"links":{"cited_paper":"/paper/2101.00113","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:924593a882a33a142f0a63e77b144254e05a3ff235b40238203d121c967affed","observation_id":"7af30726-950d-48aa-acd1-fbde08a5649e","resolution":{"observed_at":"2026-08-06T21:02:35.437237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.04649","last_updated":"2018-06-12T17:15:27Z","snapshot_observed_at":"2026-07-06T06:44:25.518684Z","submitted_at":"2018-06-12T17:15:27Z","title":"Concordance and Discordance in Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.04649","snapshot_observed_at":"2026-08-06T21:02:35.610681Z","title":"Raveri and W","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:35.610681Z"},"links":{"cited_paper":"/paper/1806.04649","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:c8c8ee0129f610fc1e799311455e7049e8fc59cf85490a504104ab8cd5968e64","observation_id":"933166a0-cc67-4613-936d-1c15973e427c","resolution":{"observed_at":"2026-08-06T21:02:35.610681Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0910.3786","last_updated":"2010-08-17T18:46:40Z","snapshot_observed_at":"2026-07-06T02:01:57.305966Z","submitted_at":"2009-10-20T18:47:23Z","title":"Weak lensing power spectra for precision cosmology: Multiple-deflection, reduced shear and lensing bias corrections","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0910.3786","snapshot_observed_at":"2026-08-06T21:02:35.746340Z","title":"Krause and C","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:35.746340Z"},"links":{"cited_paper":"/paper/0910.3786","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:0d4b933ad80f78dd928a4d47907c2e28ad2279cd66a3cd39ee61b5cbb4bd4181","observation_id":"d33a34b2-5dc5-4cc0-b8bb-b697efb81ead","resolution":{"observed_at":"2026-08-06T21:02:35.746340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:02:38.910434Z","title":"Zhang and X","venue":null,"work_id":"da4fb5f0-e0e4-4c74-9c67-1a855040fc86","year":2025},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:35.907519Z"},"links":{"citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:9410ea5d4bc8244d73fbd491fbe488cec032d3f66dff2ee3aa7f42bc00ddf7b8","observation_id":"6ff516a6-5934-47b1-a8f5-a9d088623a01","resolution":{"observed_at":"2026-08-06T21:02:38.914715Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9911102","last_updated":"2000-05-23T10:29:36Z","snapshot_observed_at":"2026-07-07T01:29:33.471797Z","submitted_at":"1999-11-06T01:01:09Z","title":"Massive Lossless Data Compression and Multiple Parameter Estimation from Galaxy Spectra","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9911102","snapshot_observed_at":"2026-08-06T21:02:36.047055Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:36.047055Z"},"links":{"cited_paper":"/paper/astro-ph/9911102","citing_paper":"/paper/2507.01377"},"observation_digest":"sha256:1b620c966a9f96dd9abe4b36dfd212f955bdf7ab32d12ff25f2a784f6021b1ff","observation_id":"bccd9b1b-ac15-43d2-849a-9ab80f618211","resolution":{"observed_at":"2026-08-06T21:02:36.047055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.01377","last_updated":"2025-07-24T21:06:23Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-06T21:11:11.620150Z","submitted_at":"2025-07-02T05:37:36Z","title":"Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration"},"reference_resolution":{"displayed":84,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":72,"verified_exact":6,"verified_fuzzy":5},"total_outbound_references":84},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 84 of 84 outbound references and 4 inbound Pith citation observations for arXiv:2507.01377."}