{"as_of":"2026-08-20T05:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b4cf2839a6144621bb470865d6892221251e3d8866ec0a240268ec6975d71ab7","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T21:59:30.875058Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-11T06:37:51.907076Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2009.10726","last_updated":"2021-02-18T19:00:03Z","snapshot_observed_at":"2026-08-18T22:52:30.315143Z","submitted_at":"2020-09-22T18:00:00Z","title":"Tango for three: Sagittarius, LMC, and the Milky Way","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10726","snapshot_observed_at":"2026-08-10T21:59:30.875058Z","title":"Vasiliev, V","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.03409","last_updated":"2025-05-22T15:36:21Z","snapshot_observed_at":"2026-08-17T22:59:56.601397Z","submitted_at":"2025-01-06T22:11:28Z","title":"Empirical Modeling of Magnetic Braking in Millisecond Pulsars to Measure the Local Dark Matter Density and Effects of Orbiting Satellite Galaxies","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T21:59:30.875058Z"},"links":{"cited_paper":"/paper/2009.10726","citing_paper":"/paper/2501.03409"},"observation_digest":"sha256:7a8cace815df3532038b5fb3659c031ce6c6edd20e2c8b905489afe44c975f8a","observation_id":"44c1ea4b-259b-4637-80e1-d4c9ecab29e2","resolution":{"observed_at":"2026-08-10T21:59:30.875058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10726","last_updated":"2021-02-18T19:00:03Z","snapshot_observed_at":"2026-08-18T22:52:30.315143Z","submitted_at":"2020-09-22T18:00:00Z","title":"Tango for three: Sagittarius, LMC, and the Milky Way","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10726","snapshot_observed_at":"2026-08-07T00:51:07.984449Z","title":"Tango for three: Sagittarius, LMC, and the Milky Way.Mon","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.13813","last_updated":"2025-06-14T18:04:22Z","snapshot_observed_at":"2026-08-17T13:41:00.279996Z","submitted_at":"2025-06-14T18:04:22Z","title":"Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T00:51:07.984449Z"},"links":{"cited_paper":"/paper/2009.10726","citing_paper":"/paper/2506.13813"},"observation_digest":"sha256:824ebf35faf1da88cba6c7f6acfb05c1a93583d11b079aca67baafa55e2ab191","observation_id":"2f20edef-29a1-4e2d-a975-49d6016c3406","resolution":{"observed_at":"2026-08-07T00:51:07.984449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10726","last_updated":"2021-02-18T19:00:03Z","snapshot_observed_at":"2026-08-18T22:52:30.315143Z","submitted_at":"2020-09-22T18:00:00Z","title":"Tango for three: Sagittarius, LMC, and the Milky Way","version":2},"cited_work":{"arxiv_id":"2009.10726","doi":null,"metadata_source":"pith","pith_arxiv_id":"2009.10726","snapshot_observed_at":"2026-07-11T06:37:51.907076Z","title":"Tango for three: Sagittarius, LMC, and the Milky Way","venue":"astro-ph.GA","work_id":"8f5ed0aa-1390-4b0a-8c66-acf29d812bfb","year":2020},"citing_paper":{"arxiv_id":"2607.05510","last_updated":"2026-07-06T18:00:04Z","snapshot_observed_at":"2026-08-06T10:32:42.332283Z","submitted_at":"2026-07-06T18:00:04Z","title":"Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-07-11T06:35:48.157333Z"},"links":{"cited_paper":"/paper/2009.10726","citing_paper":"/paper/2607.05510"},"observation_digest":"sha256:a019050a0f49fc62b1c91debcaf822e033cdbdbc909e23596e29d822a2d6808c","observation_id":"060c2e07-0e2d-4242-bc0e-b18827148561","resolution":{"observed_at":"2026-07-11T06:37:51.909782Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10726","last_updated":"2021-02-18T19:00:03Z","snapshot_observed_at":"2026-08-18T22:52:30.315143Z","submitted_at":"2020-09-22T18:00:00Z","title":"Tango for three: Sagittarius, LMC, and the Milky Way","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10726","snapshot_observed_at":"2026-08-01T11:10:05.887102Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.20006","last_updated":"2026-07-22T10:44:47Z","snapshot_observed_at":"2026-08-04T11:41:55.980209Z","submitted_at":"2026-07-22T10:44:47Z","title":"LMC-induced Perturbations in the Milky Way Halo II: Bridging Field-level Inference and Summary-level Simulation-Based Inference","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-01T11:10:05.887102Z"},"links":{"cited_paper":"/paper/2009.10726","citing_paper":"/paper/2607.20006"},"observation_digest":"sha256:7631249efe53addb6cab98eba9e069d5a1d1c48fd8ee583b5b162d53d36d6916","observation_id":"6ee91836-26be-44fa-abfe-4081cbb566c3","resolution":{"observed_at":"2026-08-01T11:10:05.887102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10726","last_updated":"2021-02-18T19:00:03Z","snapshot_observed_at":"2026-08-18T22:52:30.315143Z","submitted_at":"2020-09-22T18:00:00Z","title":"Tango for three: Sagittarius, LMC, and the Milky Way","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10726","snapshot_observed_at":"2026-07-30T11:06:41.395964Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.23829","last_updated":"2026-07-26T20:33:59Z","snapshot_observed_at":"2026-08-16T09:50:33.877798Z","submitted_at":"2026-07-26T20:33:59Z","title":"Neighbors, Not Kin: Kinematic evidence for tidal tails from NGC 7492 along the Sagittarius stream","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-07-30T11:06:41.395964Z"},"links":{"cited_paper":"/paper/2009.10726","citing_paper":"/paper/2607.23829"},"observation_digest":"sha256:3bdd3e5a7322bffb44b97b835c4bd7dfd846f4dada6797b00d458d0d2a8e01e3","observation_id":"e0e8d6f3-b52c-491c-96c3-b060cd167a12","resolution":{"observed_at":"2026-07-30T11:06:41.395964Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2009.10726/citation-record","integrity":"/paper/2009.10726/integrity","json":"/paper/2009.10726/citation-record.json","paper":"/paper/2009.10726"},"outbound":[],"paper":{"arxiv_id":"2009.10726","last_updated":"2021-02-18T19:00:03Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-18T22:52:30.315143Z","submitted_at":"2020-09-22T18:00:00Z","title":"Tango for three: Sagittarius, LMC, and the Milky Way"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2009.10726."}