{"as_of":"2026-08-17T01:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a7c5e522c4efeafce1bbe85a332ed6f9acb2095c0ef349a9a27d99d159b37888","coverage":[{"denominator":22,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":22,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T23:33:50.704834Z","state":"measured"},{"denominator":22,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":22,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2412.02426/citation-record","integrity":"/paper/2412.02426/integrity","json":"/paper/2412.02426/citation-record.json","paper":"/paper/2412.02426"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.31725/0367-7966-","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:33:50.744437Z","title":"Smirnov, A","venue":null,"work_id":"f8a17296-7df1-4444-8411-4075f6239602","year":2023},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.592780Z"},"links":{"citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:986ca2fc54f5f475d680be63e868ccf2c835bc7bdc43a8a8d68860ea28afd188","observation_id":"8a28801d-9978-47b2-97dd-fa036c1996d4","resolution":{"observed_at":"2026-08-11T23:33:50.750205Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.14789","last_updated":"2023-11-24T18:50:02Z","snapshot_observed_at":"2026-08-16T14:40:34.298546Z","submitted_at":"2023-11-24T18:50:02Z","title":"The Influence of the Bar on the Dynamics of Globular Clusters in the Central Region of the Milky Way. Frequency Analysis of Orbits According to Gaia EDR3 Data","version":1},"cited_work":{"arxiv_id":"2311.14789","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.14789","snapshot_observed_at":"2026-08-11T23:33:51.310980Z","title":"The Influence of the Bar on the Dynamics of Globular Clusters in the Central Region of the Milky Way. Frequency Analysis of Orbits According to Gaia EDR3 Data","venue":"astro-ph.GA","work_id":"551173e5-ee9f-4e20-8d7b-d31dfa7d7027","year":2023},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.598926Z"},"links":{"cited_paper":"/paper/2311.14789","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:ff2250b882aa711be25acf6cb87ff3db5f2db72570579d80d14af240f46bc088","observation_id":"c53c16be-778e-4980-8ee5-5178787bd291","resolution":{"observed_at":"2026-08-11T23:33:51.314606Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.18172","last_updated":"2024-01-04T09:31:18Z","snapshot_observed_at":"2026-08-16T14:48:15.581340Z","submitted_at":"2023-10-27T14:31:44Z","title":"Globular clusters and bar: captured or not captured?","version":2},"cited_work":{"arxiv_id":"2310.18172","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.18172","snapshot_observed_at":"2026-08-11T23:33:51.296400Z","title":"Globular clusters and bar: captured or not captured?","venue":"astro-ph.GA","work_id":"3b0e7e65-d9ff-4be9-b25b-4c4ff79f7986","year":2023},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.603888Z"},"links":{"cited_paper":"/paper/2310.18172","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:7b560b92cd903db04a8fd265fcc650aad961461e5c838ca9e1e056c9413f21a1","observation_id":"bce429f2-9e32-429c-b88d-b9fb38c8083e","resolution":{"observed_at":"2026-08-11T23:33:51.300425Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.15590","last_updated":"2024-06-21T18:44:37Z","snapshot_observed_at":"2026-08-16T13:40:37.994631Z","submitted_at":"2024-06-21T18:44:37Z","title":"Analysis of regularity/chaoticity of the globular clusters dynamics on the central region of the Milky Way","version":1},"cited_work":{"arxiv_id":"2406.15590","doi":null,"metadata_source":"pith","pith_arxiv_id":"2406.15590","snapshot_observed_at":"2026-08-11T23:33:51.281488Z","title":"Analysis of regularity/chaoticity of the globular clusters dynamics on the central region of the Milky Way","venue":"astro-ph.GA","work_id":"4508a934-1c07-412c-90e5-2c7e04ebd659","year":2024},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.610023Z"},"links":{"cited_paper":"/paper/2406.15590","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:9d23ff7990abd1c9e657d3a62bea21af6e75de0f8517798845a69cd15f13a619","observation_id":"d9cba94b-dfab-491e-b339-3126ebb58d33","resolution":{"observed_at":"2026-08-11T23:33:51.285193Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.09568","last_updated":"2021-07-12T18:58:54Z","snapshot_observed_at":"2026-08-16T18:44:35.612482Z","submitted_at":"2021-02-18T19:00:01Z","title":"Gaia EDR3 view on Galactic globular clusters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.09568","snapshot_observed_at":"2026-08-11T23:33:50.615849Z","title":"Vasiliev, H","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.615849Z"},"links":{"cited_paper":"/paper/2102.09568","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:c03afc0daa92aa6b2c9a1282dd7742903394adb08d2c3a150e30c9595a1a7b1a","observation_id":"b4c100b4-3027-4678-adc3-639f24f20cc3","resolution":{"observed_at":"2026-08-11T23:33:50.615849Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.09526","last_updated":"2021-05-21T00:23:22Z","snapshot_observed_at":"2026-08-16T18:23:29.611415Z","submitted_at":"2021-05-20T05:36:05Z","title":"Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST and literature data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.09526","snapshot_observed_at":"2026-08-11T23:33:50.620928Z","title":"Baumgardt, E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.620928Z"},"links":{"cited_paper":"/paper/2105.09526","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:c13e697e20e34c5748687b192ee09650dd972d241d48d67c369def9c150d1ff5","observation_id":"bf27e5dc-1139-4cde-b8b0-18ded75de488","resolution":{"observed_at":"2026-08-11T23:33:50.620928Z","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":"2026-08-11T23:33:51.343961Z","title":"Palous, B","venue":null,"work_id":"498666e5-066f-4fe5-af9c-ec859ffdf2de","year":1993},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.626507Z"},"links":{"citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:0a40ae9bf2fc1548d4f1bd8bb0b786226b918682db4c61161e81025c5a829a9d","observation_id":"fa4a660b-87d4-4e2b-8add-7c9e8b216d6a","resolution":{"observed_at":"2026-08-11T23:33:51.348401Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.02008","last_updated":"2019-03-05T19:00:22Z","snapshot_observed_at":"2026-08-15T19:03:18.932214Z","submitted_at":"2019-03-05T19:00:22Z","title":"Transverse kinematics of the Galactic bar-bulge from VVV and Gaia","version":1},"cited_work":{"arxiv_id":"1903.02008","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.02008","snapshot_observed_at":"2026-08-11T23:33:51.242894Z","title":"Transverse kinematics of the Galactic bar-bulge from VVV and Gaia","venue":"astro-ph.GA","work_id":"925804fd-fdf6-486c-92a5-ef4f080d872d","year":2019},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.631111Z"},"links":{"cited_paper":"/paper/1903.02008","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:695e1267f2a9881a67b460784dd13aeedc38aa6d0f6b3c519910303684810a64","observation_id":"61599965-8076-4d3f-9f36-95ab1363b21a","resolution":{"observed_at":"2026-08-11T23:33:51.247303Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02294","last_updated":"2016-04-07T13:40:18Z","snapshot_observed_at":"2026-08-14T22:07:06.666038Z","submitted_at":"2016-03-07T21:09:41Z","title":"Chaotic motion and the evolution of morphological components in a time-dependent model of a barred galaxy within a dark matter halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02294","snapshot_observed_at":"2026-08-11T23:33:50.635399Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.635399Z"},"links":{"cited_paper":"/paper/1603.02294","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:37028cc39123898b953b4de07e8e871f307afdac584c148c83793a7558ad6341","observation_id":"a04edda4-6eac-4f11-ba4a-ef58fa368f81","resolution":{"observed_at":"2026-08-11T23:33:50.635399Z","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":"2026-08-11T23:33:51.334742Z","title":"Miyamoto, R","venue":null,"work_id":"dcdec939-02a4-4428-90f8-456bc6b28fd1","year":1975},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.641593Z"},"links":{"citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:caee6018024c45213eee488776efc8a3d84397822c78746deb86d6ec46d5e6cf","observation_id":"e6f6d527-52bc-4d7b-92d1-bfdec2595145","resolution":{"observed_at":"2026-08-11T23:33:51.337672Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"astr-ph/9611107","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:33:51.208191Z","title":null,"venue":null,"work_id":"3e4e2116-409d-48a9-ab12-459ab2fe37c6","year":1997},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.646455Z"},"links":{"citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:72adb2e24e16fb389e1f70ed4411b0f3dd0b93539414e0c2fc3b904ba0c33fbd","observation_id":"8305df8a-56e9-4666-8251-c162b188e7b3","resolution":{"observed_at":"2026-08-11T23:33:51.215173Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.08050","last_updated":"2023-05-24T08:54:06Z","snapshot_observed_at":"2026-08-14T21:46:36.699358Z","submitted_at":"2016-07-27T11:45:31Z","title":"Rotation Curve and Mass Distribution in the Galaxy from the Velocities of Objects at Distances up to 200 kpc","version":3},"cited_work":{"arxiv_id":"1607.08050","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.08050","snapshot_observed_at":"2026-08-11T23:33:51.071700Z","title":"Rotation Curve and Mass Distribution in the Galaxy from the Velocities of Objects at Distances up to 200 kpc","venue":"astro-ph.GA","work_id":"1491a909-2d46-403e-9aa4-fe09802b3450","year":2016},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.652639Z"},"links":{"cited_paper":"/paper/1607.08050","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:486c07a6f99cc88a43d0c266c47f47faa846b280831d7259941b8491b384fe50","observation_id":"3851df5f-daa7-47d5-846b-3f6d593a4001","resolution":{"observed_at":"2026-08-11T23:33:51.077093Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1310.2659","last_updated":"2014-02-26T10:54:04Z","snapshot_observed_at":"2026-08-14T23:59:32.089576Z","submitted_at":"2013-10-09T23:29:52Z","title":"Rotation Curve of the Milky Way out to $\\sim$ 200 kpc","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.2659","snapshot_observed_at":"2026-08-11T23:33:50.656105Z","title":"Bhattacharjee, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.656105Z"},"links":{"cited_paper":"/paper/1310.2659","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:cd66526f5a534bc952519fcd1d4c97d723ef8b06234bec1529bd3d0e0e471a3c","observation_id":"55efc844-7cb0-481f-aa47-263785b75c21","resolution":{"observed_at":"2026-08-11T23:33:50.656105Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.08875","last_updated":"2018-01-25T15:34:04Z","snapshot_observed_at":"2026-08-14T19:52:02.613160Z","submitted_at":"2018-01-25T15:34:04Z","title":"Refinement of Parameters of Six Selected Galactic Potential Models","version":1},"cited_work":{"arxiv_id":"1801.08875","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.08875","snapshot_observed_at":"2026-08-11T23:33:51.033807Z","title":"Refinement of Parameters of Six Selected Galactic Potential Models","venue":"astro-ph.GA","work_id":"5fb1f027-a92a-4b79-8fff-145869734026","year":2018},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.659942Z"},"links":{"cited_paper":"/paper/1801.08875","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:e1744fe6be2a62d418ef6f9ddaedaef63c362d3c514e644d1f75dfdbed61691f","observation_id":"1035a17e-92d5-4f01-89d6-e263ae2145ab","resolution":{"observed_at":"2026-08-11T23:33:51.039365Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0912.3693","last_updated":"2009-12-18T15:01:58Z","snapshot_observed_at":"2026-08-15T05:31:06.861209Z","submitted_at":"2009-12-18T15:01:58Z","title":"Local Kinematics and the Local Standard of Rest","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.3693","snapshot_observed_at":"2026-08-11T23:33:50.664644Z","title":"Sch¨ onrich, J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.664644Z"},"links":{"cited_paper":"/paper/0912.3693","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:b416d53a228d68fcc9ab2eea9b87b6b73250d54c718f1bd0a5821e5d7f616b75","observation_id":"72cc2b10-cfe8-4891-affc-b44854571652","resolution":{"observed_at":"2026-08-11T23:33:50.664644Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.08438","last_updated":"2016-07-01T15:11:42Z","snapshot_observed_at":"2026-08-14T22:21:10.954588Z","submitted_at":"2015-11-26T16:14:09Z","title":"Analysis of the Z Distribution of Young Objects in the Galactic Thin Disk","version":2},"cited_work":{"arxiv_id":"1511.08438","doi":null,"metadata_source":"pith","pith_arxiv_id":"1511.08438","snapshot_observed_at":"2026-08-11T23:33:50.866659Z","title":"Analysis of the Z Distribution of Young Objects in the Galactic Thin Disk","venue":"astro-ph.GA","work_id":"bc0bfe92-e70d-4d02-a5b5-360e9970673e","year":2015},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.673574Z"},"links":{"cited_paper":"/paper/1511.08438","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:529e24d364a9b1f9d0bb7d5763c1afb98829d934d35f9629926180b98b01d69f","observation_id":"4f4b902e-7412-4a85-8717-5e0485bea9d6","resolution":{"observed_at":"2026-08-11T23:33:50.871823Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.09775","last_updated":"2019-01-14T19:00:07Z","snapshot_observed_at":"2026-08-14T18:47:46.660069Z","submitted_at":"2018-07-25T18:00:01Z","title":"Proper motions and dynamics of the Milky Way globular cluster system from Gaia DR2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.09775","snapshot_observed_at":"2026-08-11T23:33:50.678505Z","title":"Vasiliev","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.678505Z"},"links":{"cited_paper":"/paper/1807.09775","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:ef53ece9dd78116302164c90aea114fee6c953b8b01d08a9ab8eceeebc737ae6","observation_id":"522b66cd-8c4b-48ff-a701-a28a82e5201e","resolution":{"observed_at":"2026-08-11T23:33:50.678505Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.08271","last_updated":"2019-09-10T10:31:31Z","snapshot_observed_at":"2026-08-14T16:13:10.534765Z","submitted_at":"2019-06-19T18:00:05Z","title":"Origin of the system of globular clusters in the Milky Way","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.08271","snapshot_observed_at":"2026-08-11T23:33:50.682882Z","title":"Massari, H","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.682882Z"},"links":{"cited_paper":"/paper/1906.08271","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:3e4b0cf54a4638b0480a65edbee47cf62ac83fce41676e44685a024459b09bc4","observation_id":"860b777e-ec1f-4fbc-9aa2-a4923272a494","resolution":{"observed_at":"2026-08-11T23:33:50.682882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.13597","last_updated":"2020-04-28T15:34:54Z","snapshot_observed_at":"2026-08-13T22:53:07.384870Z","submitted_at":"2020-04-28T15:34:54Z","title":"Milky Way Subsystems from Globular Clusters Kinematics Using Gaia DR2 and HST Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.13597","snapshot_observed_at":"2026-08-11T23:33:50.687402Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.687402Z"},"links":{"cited_paper":"/paper/2004.13597","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:17db6cabf093e7c83affebe4bf0696f0365d45e5a83a6e8c2fbec5170d8d803a","observation_id":"29201fe2-2118-4937-807c-b617c184f7f2","resolution":{"observed_at":"2026-08-11T23:33:50.687402Z","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":"2026-08-11T23:33:51.321925Z","title":"Morbidelli","venue":null,"work_id":"38aabac3-ab7b-45df-a952-b5bb95a45b30","year":2014},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.695172Z"},"links":{"citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:7edf3279222b30419fe05a09bb1d2b4899e972c8b0f437eaa59ca8fc4f743d21","observation_id":"267eaaf2-6b01-479a-945e-fcd0118d9405","resolution":{"observed_at":"2026-08-11T23:33:51.325223Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.00761","last_updated":"2024-03-01T18:59:01Z","snapshot_observed_at":"2026-08-16T14:13:38.805623Z","submitted_at":"2024-03-01T18:59:01Z","title":"Orbital analysis of stars in the nuclear stellar disc of the Milky Way","version":1},"cited_work":{"arxiv_id":"2403.00761","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.00761","snapshot_observed_at":"2026-08-11T23:33:50.784721Z","title":"Orbital analysis of stars in the nuclear stellar disc of the Milky Way","venue":"astro-ph.GA","work_id":"4146efac-1c82-492a-869e-dcbc84e73f57","year":2024},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.699292Z"},"links":{"cited_paper":"/paper/2403.00761","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:9e13bd7c827590263c23890dd60be991a857b3537d5007031110b8ccc3fc1273","observation_id":"2a4c7f79-1dc1-4b4d-bd50-fe07206cfadf","resolution":{"observed_at":"2026-08-11T23:33:50.790133Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0906.4784","last_updated":"2010-02-02T21:27:35Z","snapshot_observed_at":"2026-08-15T05:45:06.794361Z","submitted_at":"2009-06-25T20:24:53Z","title":"The Orbital Evolution Induced by Baryonic Condensation in Triaxial Halos","version":2},"cited_work":{"arxiv_id":"0906.4784","doi":null,"metadata_source":"pith","pith_arxiv_id":"0906.4784","snapshot_observed_at":"2026-08-11T23:33:50.765716Z","title":"The Orbital Evolution Induced by Baryonic Condensation in Triaxial Halos","venue":"astro-ph.CO","work_id":"2544b95e-2982-4631-aeaf-a5fac17a5ee6","year":2009},"citing_paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T23:33:50.704834Z"},"links":{"cited_paper":"/paper/0906.4784","citing_paper":"/paper/2412.02426"},"observation_digest":"sha256:00f829722757171c34a02710407f5f1208111e63fc60544b07c9d3f3d025cd83","observation_id":"352daee5-05e0-4af2-a381-31952395cd85","resolution":{"observed_at":"2026-08-11T23:33:50.770168Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2412.02426","last_updated":"2024-12-03T12:45:35Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-15T19:03:01.151550Z","submitted_at":"2024-12-03T12:45:35Z","title":"The influence of the bar on the chaotic dynamics of globular clusters in the central region of the Galaxy"},"reference_resolution":{"displayed":22,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":8,"verified_exact":10,"verified_fuzzy":3},"total_outbound_references":22},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 22 of 22 outbound references and 0 inbound Pith citation observations for arXiv:2412.02426."}