{"as_of":"2026-08-19T09:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2fa0813fa70cfd9dea914d7e44803e52de008038fde92ff93446d2e72f2d5a0e","coverage":[{"denominator":139,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T10:37:48.426495Z","state":"measured"},{"denominator":102,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":102,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T19:41:21.778772Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-10T05:30:23.456663Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-10T05:30:23.456663Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"cited_work":{"arxiv_id":"2504.17853","doi":"10.48550/arxiv.2504.17853","metadata_source":"pith","pith_arxiv_id":"2504.17853","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","venue":"astro-ph.SR","work_id":"6790e40c-c580-42be-ae99-a0187a705e16","year":2025},"citing_paper":{"arxiv_id":"2506.05094","last_updated":"2025-06-05T14:39:37Z","snapshot_observed_at":"2026-08-13T14:01:34.195246Z","submitted_at":"2025-06-05T14:39:37Z","title":"Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly III: stellar evolution at different metallicities","version":1},"reference_index":115,"source":"arxiv_source","source_observed_at":"2026-08-07T10:32:43.685940Z"},"links":{"cited_paper":"/paper/2504.17853","citing_paper":"/paper/2506.05094"},"observation_digest":"sha256:5e43f385d743e6cfeca7e89011ccf36490d6641ebcd54bd66aba1e7b11b44080","observation_id":"8a235029-9605-4ec2-9b0f-0a120dc514bb","resolution":{"observed_at":"2026-08-07T10:32:45.130988Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"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":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.17853","snapshot_observed_at":"2026-08-15T19:41:21.778772Z","title":"S., et al., 2025, @doi [arXiv e-prints] 10.48550/arXiv.2504.17853 , https://ui.adsabs.harvard.edu/abs/2025arXiv250417853T p","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.15546","last_updated":"2025-06-24T12:22:12Z","snapshot_observed_at":"2026-08-18T22:38:04.766885Z","submitted_at":"2025-06-18T15:18:40Z","title":"Tracing the Milky Way: Calibrating chemical ages with high-precision Kepler data","version":2},"reference_index":124,"source":"arxiv_source","source_observed_at":"2026-08-15T19:41:21.778772Z"},"links":{"cited_paper":"/paper/2504.17853","citing_paper":"/paper/2506.15546"},"observation_digest":"sha256:9c5fc3b3c79b964b67e534a558bbdc67fabb6cf3a8185bafd053af356d883fb5","observation_id":"58d03894-44f4-41de-82c3-4d5d8a7ee708","resolution":{"observed_at":"2026-08-15T19:41:21.778772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2504.17853/citation-record","integrity":"/paper/2504.17853/integrity","json":"/paper/2504.17853/citation-record.json","paper":"/paper/2504.17853"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.114861Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.114861Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:5235dc45301b778a8bc238015e02ed59a9445fe7c43b8ee116474afadfb82ea0","observation_id":"790d9c33-a28b-4b17-925b-d1397088393b","resolution":{"observed_at":"2026-08-16T10:37:48.114861Z","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":"2026-08-16T10:37:48.118902Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.118902Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:04822ae28bc020a8870af8e566db20897f8c20188de3d89a39eb216454b597ae","observation_id":"632ae2ff-d14b-4d16-a152-de4108370bf7","resolution":{"observed_at":"2026-08-16T10:37:48.118902Z","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":"2026-08-16T10:37:48.122821Z","title":"2022, , 259, 35","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.122821Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:5c6154241c9a4bccf2d34ff98a169bcd92d47776229839543eece535ca71d06f","observation_id":"fbcbd849-8e69-4060-ac62-9f02ad233723","resolution":{"observed_at":"2026-08-16T10:37:48.122821Z","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":"2026-08-16T10:37:48.126198Z","title":"2023, , 678, A158","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.126198Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:d24a59ac4f32ae3c93d57b4ce967b62e029283610c66fa208dfcd6fcee272df8","observation_id":"792d3b07-10a4-4714-b330-819be240c78d","resolution":{"observed_at":"2026-08-16T10:37:48.126198Z","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":"2026-08-16T10:37:48.129507Z","title":"2017, , 838, 115","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.129507Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:5ec091427491edcb9a0a1e45c2ccdff9fd5def31f8fa2bd010617ee33c91ba2d","observation_id":"dd2ed11a-1b26-40b8-8590-6f506d9b8914","resolution":{"observed_at":"2026-08-16T10:37:48.129507Z","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":"2026-08-16T10:37:48.132656Z","title":"J., & Scott , P","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.132656Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:d89647e657711cb1bac622a1357e593f87f9a0c70591272fed42e1b8c9242247","observation_id":"1e611faf-deac-48fb-819f-bb52de3f295a","resolution":{"observed_at":"2026-08-16T10:37:48.132656Z","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":"2026-08-16T10:37:48.136107Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.136107Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:a11981bda71a880acaa59dc9e75e8e6e92c88371c1d1f5b4c98f647061b46a72","observation_id":"7013e6e8-61a8-40a0-b6d7-3a909801bf20","resolution":{"observed_at":"2026-08-16T10:37:48.136107Z","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":"2026-08-16T10:37:48.139322Z","title":"H., Chaplin , W","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.139322Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:44c723edca027ed4c35274ac0cb1c6ecb01384d37c0d52ef2cd3939e256abafc","observation_id":"4def0499-c715-4e13-a07c-bd3f775b620b","resolution":{"observed_at":"2026-08-16T10:37:48.139322Z","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":"2026-08-16T10:37:48.142685Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.142685Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:5cdc96754d789d98dad289b6eb21def8e1bd5400f3f273828ba06469c1d00b1f","observation_id":"5b454909-03cd-41d5-9447-221612edb972","resolution":{"observed_at":"2026-08-16T10:37:48.142685Z","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":"2026-08-16T10:37:48.145844Z","title":"A., Triaud , A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.145844Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:877b5f677a985779c5791e7ce25cd2aa88a4a86ec478b4329310800ead8c8f21","observation_id":"4e9387ed-f3bf-4aca-9d7e-15ad02794b2c","resolution":{"observed_at":"2026-08-16T10:37:48.145844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10812","last_updated":"2023-11-06T18:16:35Z","snapshot_observed_at":"2026-08-16T15:14:55.381794Z","submitted_at":"2023-07-19T17:46:20Z","title":"Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems -- A census of oscillating red-giants and main-sequence stars in Gaia DR3 binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10812","snapshot_observed_at":"2026-08-16T10:37:48.149027Z","title":"G., Grossmann , D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.149027Z"},"links":{"cited_paper":"/paper/2307.10812","citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:19216ef8fbc740a02bbbc491f29fd52639e9a2c259b59154d5704a2921c9539e","observation_id":"a8ccbb61-9f73-41a2-b0ee-980e23fc72c9","resolution":{"observed_at":"2026-08-16T10:37:48.149027Z","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":"2026-08-16T10:37:48.152638Z","title":"G., Grossmann , D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.152638Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:9bd5346a9efb3f4679f42de08c2fb4e1c7b410117be4582c93772fbc024bb711","observation_id":"638a66e9-e0c5-4ba9-951e-c61c5145ac3c","resolution":{"observed_at":"2026-08-16T10:37:48.152638Z","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":"2026-08-16T10:37:48.155750Z","title":"R., Mosser , B., Huber , D., et al","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.155750Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:306d7e7d452035e18ec8915d53b5f1743da5fbb3722c2eb3a6549bdda2354764","observation_id":"4b063f24-3b1b-4cb0-b9dd-6e708594b31c","resolution":{"observed_at":"2026-08-16T10:37:48.155750Z","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":"2026-08-16T10:37:48.158949Z","title":"& Kravtsov , A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.158949Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:39f5d853e6499bb205d5723e4d39a5a8743d9ffa5aa52c15080083e753baab45","observation_id":"092ccf5a-713b-4a32-ba7a-14ecb0628560","resolution":{"observed_at":"2026-08-16T10:37:48.158949Z","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":"2026-08-16T10:37:48.161964Z","title":"E., Shallis , M","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.161964Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:d6399a692c0a9dec91ef93f28166c850d82b22afa0cf8255e373fb6a57350484","observation_id":"3470c10a-01ea-4428-9c4d-c7d9020fe3de","resolution":{"observed_at":"2026-08-16T10:37:48.161964Z","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":"2026-08-16T10:37:48.165151Z","title":"C., Aguirre B rsen-Koch , V., Helmi , A., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.165151Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:bbb5bce805c815d8e41d82a345d43fcf7193f1486886335fe910de699f509366","observation_id":"3160a2c3-c3d4-48d6-b3c4-3502991f554c","resolution":{"observed_at":"2026-08-16T10:37:48.165151Z","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":"2026-08-16T10:37:48.168102Z","title":"J., Koch , D., Basri , G., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.168102Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:465ae17ebc144aca44304243be3a09ca99d94a8b680bed2ede9eb96cfe24c814","observation_id":"2c90ad66-b575-4b41-b685-8164d33112fa","resolution":{"observed_at":"2026-08-16T10:37:48.168102Z","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":"2026-08-16T10:37:48.171349Z","title":"2015, , 216, 29","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.171349Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:9c6f85f2b10aa91e7d6a08bb2e89b0c8477afe4085b43802c003361a207a8b14","observation_id":"cf14ea97-243c-4a13-975a-78ea6d8143f5","resolution":{"observed_at":"2026-08-16T10:37:48.171349Z","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":"2026-08-16T10:37:48.174703Z","title":"2023, , 679, A23","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.174703Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:6eb3779389387cc7c830989e5d6d48490dd46736e887d7541a7e076388dcdac1","observation_id":"06ac7e3e-3564-4570-b5fb-9b11d685d1ed","resolution":{"observed_at":"2026-08-16T10:37:48.174703Z","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":"2026-08-16T10:37:48.177587Z","title":"2022, , 668, A82","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.177587Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:b2802b02c47b806cff6ba0f9855796d055c4ec545ef0caf09d42756d089e1bd8","observation_id":"44ca8c76-2ea1-43b8-a88c-0464f6fff0a7","resolution":{"observed_at":"2026-08-16T10:37:48.177587Z","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":"2026-08-16T10:37:48.180886Z","title":"J., Miglio , A., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.180886Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:b7d334db75095b33051e02bbd9dc4abcc28697cbd4084dc9506408aad4d2c9ee","observation_id":"423b5a08-037a-4fb3-b80b-0fe9351dfc19","resolution":{"observed_at":"2026-08-16T10:37:48.180886Z","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":"2026-08-16T10:37:48.183877Z","title":"E., Willett , E., & Thomsen , J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.183877Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:e4916379a667ad63f3d7485ea48cfd148219bc22f249865de8734eed0e366099","observation_id":"bb17763c-c01e-4747-a883-65ffe9481b72","resolution":{"observed_at":"2026-08-16T10:37:48.183877Z","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":"2026-08-16T10:37:48.187042Z","title":"e , E., Grundahl , F., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.187042Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:60497eb047f57d782793fc2617e1b0ee6cf32135c6f870a1907693de7ef44380","observation_id":"117e2215-8eab-47d2-803e-02be79d57a4e","resolution":{"observed_at":"2026-08-16T10:37:48.187042Z","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":"2026-08-16T10:37:48.190264Z","title":"R., Quirion , P.-O., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.190264Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:b23049c14d1176f66b352b62481c1f9882bbbcfce67e0c0f881b67758e0e61d4","observation_id":"ebd44134-a6d9-444a-aac4-22edaedb9f7a","resolution":{"observed_at":"2026-08-16T10:37:48.190264Z","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":"2026-08-16T10:37:48.193376Z","title":"2019, , 482, 2305","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.193376Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:e4adf1ac67b4eff3d03e00be9eafa634bd281f9b9d292ed123942d1e0ec23596","observation_id":"89a0854f-6c81-40b3-85ce-e3790bb99279","resolution":{"observed_at":"2026-08-16T10:37:48.193376Z","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":"2026-08-16T10:37:48.196335Z","title":"2014, , 562, A10","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.196335Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:3433b25b35ce7ca3aefdfcbf8d56b6942de7ae6bf42378b04256fe10abe46d5b","observation_id":"6fdc911f-b662-4754-8081-b3da82e50da8","resolution":{"observed_at":"2026-08-16T10:37:48.196335Z","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":"2026-08-16T10:37:48.199651Z","title":"D., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.199651Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:92260a18be5a4d54f747ea953c263106a6d42839b491661123b12d86a768c881","observation_id":"f6768eee-4fd3-4c0f-b86e-f4e85acee48c","resolution":{"observed_at":"2026-08-16T10:37:48.199651Z","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":"2026-08-16T10:37:48.202640Z","title":"2006, , 373, 13","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.202640Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:c7ebc6f9483478f92bf155d9056309730325ec0a438544e67a1558a0ad5a59f7","observation_id":"6cf4c196-c33d-4cd9-8e20-4759c3f4b4e2","resolution":{"observed_at":"2026-08-16T10:37:48.202640Z","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":"2026-08-16T10:37:48.205732Z","title":"& VandenBerg , D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.205732Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:37e306f782327ed13a23f8a858097fe24de257bde2effab32c43abdb5601ff10","observation_id":"307ca41d-fc7b-46c6-a606-bebb20778887","resolution":{"observed_at":"2026-08-16T10:37:48.205732Z","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":"2026-08-16T10:37:48.208713Z","title":"& Kurucz , R","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.208713Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:8b2179b04d3acf5a91d71d8661170345a8e0af62e6f20cc4a2a86c1fa74eb1d0","observation_id":"dace46dd-ddc4-4b43-a618-83a74ed8ffdb","resolution":{"observed_at":"2026-08-16T10:37:48.208713Z","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":"2026-08-16T10:37:48.211853Z","title":"A., Rix , H.-W., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.211853Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:0cf75a10ed007f5033b9686f94eb697f94db2088a8b3eada13a59f24c67cfa0c","observation_id":"8db95397-0e88-4137-9616-76f83fa00a28","resolution":{"observed_at":"2026-08-16T10:37:48.211853Z","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":"2026-08-16T10:37:48.215115Z","title":"J., Serenelli , A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.215115Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:1fc91c2d7cd90eee16ba8f08ae3557bbf403bd97bd2e52f0dd31c583206535c0","observation_id":"beb176cb-8fc4-413e-b864-75a0e6280143","resolution":{"observed_at":"2026-08-16T10:37:48.215115Z","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":"2026-08-16T10:37:48.218067Z","title":"& Moresco , M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.218067Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:2a19240b6e9a4628e8b81587a0cc3f9ce57e82dfe9ce5e42b09b2c21faddc307","observation_id":"c5ce6925-ad6b-494c-b30e-0de017966edc","resolution":{"observed_at":"2026-08-16T10:37:48.218067Z","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":"2026-08-16T10:37:48.221147Z","title":"& Bloemen , S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.221147Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:3335c411e5cbaf47e0fbe442146b058ac65a74d3d763edbb0baef49f0d8fb1df","observation_id":"4f4d0f3d-83a7-4282-8b9a-089e6daccf37","resolution":{"observed_at":"2026-08-16T10:37:48.221147Z","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":"2026-08-16T10:37:48.224457Z","title":"& Southworth , J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.224457Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:cd8421cdf2559364300bc887bb9a523a8473a9f368a19aa0e0edcd4f25fe339c","observation_id":"acd9ba4e-f68c-4d1b-a7a0-a18977ed3d9a","resolution":{"observed_at":"2026-08-16T10:37:48.224457Z","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":"2026-08-16T10:37:48.227527Z","title":"& Southworth , J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.227527Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:3017f059f6d53635e108a6d0c95144b3ad32d955a70a231f6dd8cbb21895f9e8","observation_id":"1107131f-aae2-4416-b4ca-8c9bba4336d9","resolution":{"observed_at":"2026-08-16T10:37:48.227527Z","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":"2026-08-16T10:37:48.230575Z","title":"P., & Castilho , B","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.230575Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:289e573fa0d02a092b6d2c97063cef586f8563d3944a11007b24f2034598d5d8","observation_id":"b447ed55-b581-43e0-9456-3655304ba0d9","resolution":{"observed_at":"2026-08-16T10:37:48.230575Z","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":"2026-08-16T10:37:48.234668Z","title":"E., Kochoska , A., Hey , D., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.234668Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:7530f1bcaee83fe626613f1d7bb03778b8d028822548d2afbd25c3b63f0696d3","observation_id":"19d0c518-6379-46c9-8d67-c28d9120a64c","resolution":{"observed_at":"2026-08-16T10:37:48.234668Z","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":"2026-08-16T10:37:48.237673Z","title":"M., & Kuszlewicz , J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.237673Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:71ceab9f634c32a6da677e9a4a15daa14bd5c95b3ee4a1438a8c8d57af43e749","observation_id":"1866ae4d-faff-4276-9b2d-2b13e016403e","resolution":{"observed_at":"2026-08-16T10:37:48.237673Z","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":"2026-08-16T10:37:48.240681Z","title":null,"venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.240681Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:b0fbd2176c4be018044931c22c06bbafe62353fc87036082de63dbb0e963d153","observation_id":"9be9c47c-0aa4-4fbd-b825-1ccf17a4738f","resolution":{"observed_at":"2026-08-16T10:37:48.240681Z","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":"2026-08-16T10:37:48.243970Z","title":"2020, , 493, 5195","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.243970Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:84bfd77865c914aca9bf78a461955f6b888a070bb507377931af64f71c1fcad5","observation_id":"7f68f6f2-2400-4609-a1b9-49d84dda6271","resolution":{"observed_at":"2026-08-16T10:37:48.243970Z","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":"2026-08-16T10:37:48.246704Z","title":"R., Handberg , R., Miglio , A., et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.246704Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:c300360ab994284232c3062b166a32e8c7cd549add5ef7c8188c76584b0097a1","observation_id":"5f2ea385-8bda-4a3e-9fec-bc210bd4162f","resolution":{"observed_at":"2026-08-16T10:37:48.246704Z","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":"2026-08-16T10:37:48.249945Z","title":"2021, , 650, A115","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.249945Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:1c85327524e429a834282dd7666ec3c19131174e0c28dfdf203c43d6cba207c7","observation_id":"562ea90e-f20d-4f2e-8e6c-f6808a3caaac","resolution":{"observed_at":"2026-08-16T10:37:48.249945Z","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":"2026-08-16T10:37:48.252835Z","title":"A., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.252835Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:10f350c04b51c141263c085adf62c8d3c1875b8a03368961f46a435997aa209c","observation_id":"9b9e9f7c-1b0b-4e74-a92e-645f3dd5c098","resolution":{"observed_at":"2026-08-16T10:37:48.252835Z","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":"2026-08-16T10:37:48.256147Z","title":"P., Santos , N","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.256147Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:cc5be5f18e31ed555e165e941df8dded55f9f5c826c62b7e8f3c9b0f74e2f018","observation_id":"93d7fe76-9d8b-4c15-baf8-7d90e793da8d","resolution":{"observed_at":"2026-08-16T10:37:48.256147Z","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":"2026-08-16T10:37:48.259131Z","title":"J., Sazonova , E., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.259131Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:4921e9988789eeca23309422bcafabea30366c64570b109875496d3a1a5c9bd8","observation_id":"7ccbd5c9-4683-496e-9f81-67a5c9a520cb","resolution":{"observed_at":"2026-08-16T10:37:48.259131Z","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":"2026-08-16T10:37:48.262523Z","title":"W., Lang , D., & Goodman , J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.262523Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:2c6128ae686299760460876a3c5e34f245ed87ee18154ba5e26198392118ef71","observation_id":"c927a6e1-0593-47d6-a1f1-ff83e7cba813","resolution":{"observed_at":"2026-08-16T10:37:48.262523Z","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":"2026-08-16T10:37:48.265668Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.265668Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:866e2e01170e8d7d0182b90a312ad233a753ff0c27dfa46bf5b1c78dbe8a8878","observation_id":"cb984723-f2be-4bb0-89af-e2fe05736739","resolution":{"observed_at":"2026-08-16T10:37:48.265668Z","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":"2026-08-16T10:37:48.268737Z","title":"2023, , 674, A38","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.268737Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:c7c70186ee0f8cb39c2ad601f75f52461c55aa272b134c4cf9e7ee9dbbf289e8","observation_id":"bfaa9836-0d29-4315-a167-d3efadefc9d9","resolution":{"observed_at":"2026-08-16T10:37:48.268737Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.00211","last_updated":"2022-07-30T13:18:15Z","snapshot_observed_at":"2026-08-18T00:47:30.445982Z","submitted_at":"2022-07-30T13:18:15Z","title":"Gaia Data Release 3: Summary of the content and survey properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.00211","snapshot_observed_at":"2026-08-16T10:37:48.271580Z","title":"2022, arXiv e-prints, arXiv:2208.00211","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.271580Z"},"links":{"cited_paper":"/paper/2208.00211","citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:94531751649beff1ab602d4f5013ab78eb9718ddda41ea9db8deb3db26e321ab","observation_id":"174e1194-c326-42f8-949e-0f75653d2576","resolution":{"observed_at":"2026-08-16T10:37:48.271580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.09399","last_updated":"2024-02-14T18:55:10Z","snapshot_observed_at":"2026-08-16T14:18:32.166617Z","submitted_at":"2024-02-14T18:55:10Z","title":"Chronology of our Galaxy from Gaia Colour-Magnitude Diagram-fitting (ChronoGal). I. The formation and evolution of the thin disk from the Gaia Catalogue of Nearby Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.09399","snapshot_observed_at":"2026-08-16T10:37:48.275521Z","title":"2024, arXiv e-prints, arXiv:2402.09399","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.275521Z"},"links":{"cited_paper":"/paper/2402.09399","citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:9b6b3e39708f4f01fe259540a4f2c150062d02cf8e60dd43df8aac495d6a5e2d","observation_id":"7239e8e7-04df-4e3c-a61d-714fed674ee8","resolution":{"observed_at":"2026-08-16T10:37:48.275521Z","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":"2026-08-16T10:37:48.278924Z","title":"2016, , 832, 121","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.278924Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:b23d076a018b736a50e834baabce15a288792d22bbc006fd58f26ed59530646d","observation_id":"5eaa4db5-04de-4c3a-882e-82caf0b9cab3","resolution":{"observed_at":"2026-08-16T10:37:48.278924Z","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":"2026-08-16T10:37:48.282177Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.282177Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:8e631e5afb41cd8110269d70d74d9dd110af70607cb5eca59464a661ecf39b1a","observation_id":"25626239-1402-458d-a9b2-0110b1a7ff2c","resolution":{"observed_at":"2026-08-16T10:37:48.282177Z","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":"2026-08-16T10:37:48.285597Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.285597Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:d43aa06bfcc8caa30c29d7ab54eade28c7ece6e758651ef8fb09fe641cf89408","observation_id":"4bfc873c-a935-4a40-beb1-c5a956179225","resolution":{"observed_at":"2026-08-16T10:37:48.285597Z","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":"2026-08-16T10:37:48.288851Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.288851Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:4fb9730acfcc175ac2d3f56853671db8617a054aafc54930367adf0b7d7329f1","observation_id":"561a3bf2-13b1-4728-80c7-0a6f1aeeef3b","resolution":{"observed_at":"2026-08-16T10:37:48.288851Z","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":"2026-08-16T10:37:48.292018Z","title":"M., Schlafly , E., Zucker , C., Speagle , J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.292018Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:a88fdcb8fb21bf66723f79fe10182ab696fe196efd41addf254471e16dd8e844","observation_id":"b257dfbd-69b1-4ccd-8267-ef4152dd0498","resolution":{"observed_at":"2026-08-16T10:37:48.292018Z","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":"2026-08-16T10:37:48.295091Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.295091Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:301520c3978a4757b705337e013aac57c916896e994546190dd476f0cb1f659e","observation_id":"c93aea96-6a83-4dc2-a961-19cf72b9c78d","resolution":{"observed_at":"2026-08-16T10:37:48.295091Z","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":"2026-08-16T10:37:48.298129Z","title":"2008, , 486, 951","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.298129Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:1b9492a769081e53d5fecc25cdc7a17ecf79aaf655b7744fe7a455f66b456744","observation_id":"8b1d6fd8-a1d7-49c9-ab5b-f2c4839343eb","resolution":{"observed_at":"2026-08-16T10:37:48.298129Z","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":"2026-08-16T10:37:48.301563Z","title":"2017, , 472, 979","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.301563Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:6534505689a6ef5096555ceba0383823da7e6a1a0c10887cf13a6a5bdcbd3249","observation_id":"247250a9-4720-4711-b5cd-23c6c1239389","resolution":{"observed_at":"2026-08-16T10:37:48.301563Z","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":"2026-08-16T10:37:48.304675Z","title":"& Lund , M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.304675Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:02f74bdc80a28a9bc2b15ee8ffe05db7bbf05420da2ef3419b26a2bdbd960712","observation_id":"7d584086-c047-4c64-9c79-4fd998854817","resolution":{"observed_at":"2026-08-16T10:37:48.304675Z","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":"2026-08-16T10:37:48.307673Z","title":"M., Chaplin , W","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.307673Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:a08c26ce54d24f372338677de4c08f66359e6437de3bd600d3738344e8b8a03e","observation_id":"2aa29bd3-c1a3-40a7-a77a-d9110812a09e","resolution":{"observed_at":"2026-08-16T10:37:48.307673Z","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":"2026-08-16T10:37:48.310714Z","title":"2020, , 58, 205","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.310714Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:05fd3000cd85c90024aac6d67d11be728be9b03a80aa482d53db876b26d86483","observation_id":"92f8c9c9-5f5f-4c55-a11b-ad01359512d6","resolution":{"observed_at":"2026-08-16T10:37:48.310714Z","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":"2026-08-16T10:37:49.143052Z","title":"W., Stello , D., & De Silva , G","venue":null,"work_id":"0be39dbe-630a-472a-b005-47fb6c0a8c76","year":2024},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.313789Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:27fb68cb6ee5e050a5fba38f6a424c3de4e2085e06896c07c9891fc3839a05ab","observation_id":"b713afad-6e1b-4bf9-8764-e828245d2fe5","resolution":{"observed_at":"2026-08-16T10:37:49.146274Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.316815Z","title":"R., et al","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.316815Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:6718c37696822b2a19499deee94cee1d2f4255716d39d97cf5aec2aabc584193","observation_id":"4ea513d3-4458-4dae-bb46-45dc53740b2e","resolution":{"observed_at":"2026-08-16T10:37:48.316815Z","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":"2026-08-16T10:37:48.319755Z","title":"O., Wende-von Berg , S., Dreizler , S., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.319755Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:780d36aef458f254fe2fdb627144de8bea68b02459470f34d6c3d15e4164b3df","observation_id":"701ef1a6-3e2d-493c-b8de-a8dd02280d4c","resolution":{"observed_at":"2026-08-16T10:37:48.319755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.09428","last_updated":"2019-06-22T10:38:07Z","snapshot_observed_at":"2026-07-06T08:02:08.270581Z","submitted_at":"2019-06-22T10:38:07Z","title":"Release note: Massive peak bagging of red giants in the Kepler field","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.09428","snapshot_observed_at":"2026-08-16T10:37:48.322791Z","title":"2019, arXiv e-prints, arXiv:1906.09428","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.322791Z"},"links":{"cited_paper":"/paper/1906.09428","citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:71afc81c1d0845cb9fc669d2888461ea58303150cdf3358f5e0ebe785c3102e8","observation_id":"ee55f637-d69b-4649-95f6-9bd057103b34","resolution":{"observed_at":"2026-08-16T10:37:48.322791Z","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":"2026-08-16T10:37:49.122680Z","title":"2010, , 522, A1","venue":null,"work_id":"925b0ce1-1f50-41ff-8572-b4196a3db54d","year":2010},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.326548Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:eb58b4d81e4a4214ed6942c2faf3620e4f94955ef2bab8c6ff96f8200fac4794","observation_id":"636bf95f-90cc-4af8-b952-4802e89fc7a9","resolution":{"observed_at":"2026-08-16T10:37:49.125880Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:49.113311Z","title":"1996, The College Mathematics Journal, 27, 2","venue":null,"work_id":"ac22b75c-18cb-48f3-90a2-b6b32df3a286","year":1996},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.329610Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:790fef043143ad1c2baf6e22231114ce088eb729f12aeedacaefa9b8adb4bcbc","observation_id":"2bdcd629-524a-4bb7-a664-d32b00585a41","resolution":{"observed_at":"2026-08-16T10:37:49.116620Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.332696Z","title":"& Wright , J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.332696Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:d22c514a45bd489368f1855ede79d7ef47acc728dc8fe8074679878ab08d8671","observation_id":"548b2f59-dd7f-4ee3-bde2-33b53b761499","resolution":{"observed_at":"2026-08-16T10:37:48.332696Z","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":"2026-08-16T10:37:49.098346Z","title":"2023, , 677, A21","venue":null,"work_id":"ebf01294-6b62-47d3-939a-6060cd459da4","year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.335763Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:58f401cbef07f5609e6f77e2fc907358fdab649798c48b82bf52d19047963133","observation_id":"d26cef51-32b3-42b8-b8f6-d54d814d484d","resolution":{"observed_at":"2026-08-16T10:37:49.101600Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.338869Z","title":"2013, Stellar Structure and Evolution","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.338869Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:c81781284ba7c5862a6f2ab5cf05b760ac53a98cd8c3116501f22e6ec063e509","observation_id":"a8d19e59-7d02-4722-aeca-094cbd2e2241","resolution":{"observed_at":"2026-08-16T10:37:48.338869Z","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":"2026-08-16T10:37:48.341818Z","title":null,"venue":null,"work_id":null,"year":1966},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.341818Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:22349507b602d9f8942e6f37cb62e68ca44921c86f4467ea05a185a2410e2955","observation_id":"3e49ed31-14a4-479d-b614-bb63b148eafa","resolution":{"observed_at":"2026-08-16T10:37:48.341818Z","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":"2026-08-16T10:37:48.344655Z","title":"L., Babusiaux , C., & Cox , N","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.344655Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:7e78a4ce37395b7d57111a27b7d540bd115a11c644ed13ab599d709b22f18547","observation_id":"0ec63b52-411f-41db-98a2-49fdf5b61679","resolution":{"observed_at":"2026-08-16T10:37:48.344655Z","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":"2026-08-16T10:37:49.074406Z","title":null,"venue":null,"work_id":"b7c6a4c8-2484-4bfa-a1ce-5fbf5aa2f8cb","year":2019},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.347677Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:f06a967a08ba0f27a19fe58c04617f465a67583bad75398306399759d5116b41","observation_id":"077279e3-29d0-4535-a2a3-ac578608330b","resolution":{"observed_at":"2026-08-16T10:37:49.077371Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:49.064743Z","title":null,"venue":null,"work_id":"69db1ae8-e507-43cc-bee3-16c79c671080","year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.350593Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:be484e69e1b84a98e020cc318832d85158aaca17a385c280928c001e5a738a0d","observation_id":"8f58c27a-9f67-42b1-bf75-6272b8bbbeae","resolution":{"observed_at":"2026-08-16T10:37:49.067994Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:49.055315Z","title":null,"venue":null,"work_id":"2675f59a-0b6b-4f85-aaa7-258bede16478","year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.353469Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:29d27810f34c4307a9fb68bae78dfd3e385d422701a03f778d98352435690464","observation_id":"d74c5f0a-54d7-40a4-bea4-8ea23b4511e1","resolution":{"observed_at":"2026-08-16T10:37:49.058630Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.356336Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.356336Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:31f87a2153f416520d76abf54c68e607fed3cfb4233d8d3be671dcefe3b90f17","observation_id":"fe2299bd-0c5a-4abc-bdfd-003b5b27a39c","resolution":{"observed_at":"2026-08-16T10:37:48.356336Z","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":"2026-08-16T10:37:49.039146Z","title":"2013, , 558, A38","venue":null,"work_id":"31599c1b-5080-43d7-9b26-41e4967829fd","year":2013},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.359176Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:81b3d004e4ab985db71d4eef5b9adf933a452af654b4161857ce95210dcc3dae","observation_id":"98af6faf-c84c-4c45-9503-4d37a18748f5","resolution":{"observed_at":"2026-08-16T10:37:49.042575Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.361968Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.361968Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:2371d72b22efc1088f80582427be888841029daa944ede9a2f332741ab8ff9dc","observation_id":"e71b9d05-6c8f-4fe5-b518-5f858a0d673b","resolution":{"observed_at":"2026-08-16T10:37:48.361968Z","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":"2026-08-16T10:37:48.364894Z","title":"& Greggio , L","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.364894Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:f01dce6ecec633c72c34cc90467674b95e6a233dcbfde625fa5f82818809b242","observation_id":"5e1368cc-d003-4880-be98-33bcd1d5b1ad","resolution":{"observed_at":"2026-08-16T10:37:48.364894Z","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":"2026-08-16T10:37:48.367766Z","title":"2023, , 671, A53","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.367766Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:8f3d2cd0a4da5af6b6e1057b2197b4719b0c8ca42e9fa862b17873824dedc58d","observation_id":"e675829a-b595-4db4-b6de-9b39c47bcc37","resolution":{"observed_at":"2026-08-16T10:37:48.367766Z","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":"2026-08-16T10:37:48.370737Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.370737Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:aa493e37d8c52bda3b2c15eef64f64f631e00500e9e4f724a42f5a5705946524","observation_id":"d601a68f-6917-4a1d-9259-bfd3cb4866d4","resolution":{"observed_at":"2026-08-16T10:37:48.370737Z","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":"2026-08-16T10:37:49.007785Z","title":null,"venue":null,"work_id":"5255819e-3f90-4753-94ac-867976111fe6","year":2023},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.373769Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:f54012637c3a8a0d595e08ef8ef99784a7e9f12fef2bab4f0e83a644fa947721","observation_id":"486bae76-8b0d-4ac2-92ff-f0a5537eaff1","resolution":{"observed_at":"2026-08-16T10:37:49.010976Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.376855Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.376855Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:4e36381053b52a35530c48741fb47f53f6115af85b748229b3f390a338766036","observation_id":"4d45f807-c65c-4ae1-a936-40e73553d018","resolution":{"observed_at":"2026-08-16T10:37:48.376855Z","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":"2026-08-16T10:37:48.992667Z","title":"T., et al","venue":null,"work_id":"c99e74b1-083d-4ebc-9ae9-d7a9cce5aab1","year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.379764Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:d6bca985337fe56d13f7b05f3c48c420679059e595df86a109c00d3b65d508c8","observation_id":"a39036e2-fbc3-4ea5-ae4a-d6efeba626f1","resolution":{"observed_at":"2026-08-16T10:37:48.995930Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.982823Z","title":"2017, Astronomische Nachrichten, 338, 644","venue":null,"work_id":"2e1fbaa9-23ba-4383-bbf6-f33ef3789088","year":2017},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.382731Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:21f7ecacf3f06c1cb47026c9e497df51ff5c74310a2afc299b254b2963d2bc8d","observation_id":"c39e3df4-e08b-4d67-a232-f05eef525981","resolution":{"observed_at":"2026-08-16T10:37:48.986050Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.973496Z","title":"2021 b , Experimental Astronomy, 51, 963","venue":null,"work_id":"c0ad9196-84b1-493c-b05f-c94d003c3983","year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.385917Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:2cd4bd11e20427e50f22175cf72671836d3d373cfa092f4b983e74de90db7a93","observation_id":"f8e070e4-e24c-4073-90fb-d35cde0b8b6d","resolution":{"observed_at":"2026-08-16T10:37:48.976858Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.963424Z","title":"T., Miglio , A., et al","venue":null,"work_id":"4e4ba1f9-91fd-4815-90a1-32684f9a9a45","year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.388919Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:3265524a374c845a4cd3814977a7048a5c43351c54d4784111a89177bc106bb7","observation_id":"c355ae63-cdd7-4575-afcb-9daf25c231c2","resolution":{"observed_at":"2026-08-16T10:37:48.966876Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.392042Z","title":"& Appourchaux , T","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.392042Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:e7bc74092cfe8121d1f2a52edfa226bd337679e6b8ecfe2d1cc0343a7c4ed527","observation_id":"871394d2-8ed7-4e3a-88b9-04174f758a80","resolution":{"observed_at":"2026-08-16T10:37:48.392042Z","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":"2026-08-16T10:37:48.395095Z","title":"2014, , 572, L5","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.395095Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:af3778a58b7010c0c44f26ca17e76cd3a5d79f0e4149969a8d7061d188c72110","observation_id":"9957b2ae-b425-4606-a188-551ea183cd1a","resolution":{"observed_at":"2026-08-16T10:37:48.395095Z","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":"2026-08-16T10:37:48.399385Z","title":"J., Belkacem , K., et al","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.399385Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:7830210b53220f57a975b8497d66164c001a415261d32cfe6e6ca14764fdcecf","observation_id":"4a6e9cd5-71a8-4dd0-a6d2-8d9585634b8c","resolution":{"observed_at":"2026-08-16T10:37:48.399385Z","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":"2026-08-16T10:37:48.937297Z","title":"B., Davies , G","venue":null,"work_id":"3642e918-978d-4a9c-84ba-9bec63eaf3b5","year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.402655Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:1e180e4c4722c04e839937d394687ed14a0492939932b129d948e2fa075bc56c","observation_id":"d9fc1813-7ab4-45a7-83e0-3193757ed981","resolution":{"observed_at":"2026-08-16T10:37:48.940550Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.405765Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.405765Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:8775eb7df94d9f574d474e656549a2a6cfd88cdf28c4a9e7f9c02e2cdb95cdf3","observation_id":"13fd04c4-2101-4979-9c94-6202fc10abb1","resolution":{"observed_at":"2026-08-16T10:37:48.405765Z","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":"2026-08-16T10:37:48.408499Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.408499Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:3d50997752cfce42ab321e1e303be82ca00f1ded6a4a717bce48abef4089929d","observation_id":"b3cfa7b9-5f05-4218-8ddc-948b85562c34","resolution":{"observed_at":"2026-08-16T10:37:48.408499Z","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":"2026-08-16T10:37:48.916562Z","title":null,"venue":null,"work_id":"e922186a-fa44-431e-bcb9-20f55f5b10ea","year":2019},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.411424Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:94bdf08b6e5765cb9079b655ce98abc50e5abc3f02ea6b34174989f59bc4b214","observation_id":"00f2c939-1ba9-47b1-a56d-bbcde7898845","resolution":{"observed_at":"2026-08-16T10:37:48.920085Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T10:37:48.414306Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.414306Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:e6bcf550b1f87b8aa20e0817ac960375c747706b8525f34828f2ddd138ee161f","observation_id":"186bbe70-89a3-4aa9-adcf-2b6ed9fc4550","resolution":{"observed_at":"2026-08-16T10:37:48.414306Z","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":"2026-08-16T10:37:48.417321Z","title":"2021, , 645, A96","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.417321Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:f76ee9d62ad59142c9e77b169d29ace05be05c384ceddbe7af89668a3d3c3162","observation_id":"43ee9516-6e43-4531-ab3a-5ba72b269266","resolution":{"observed_at":"2026-08-16T10:37:48.417321Z","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":"2026-08-16T10:37:48.420302Z","title":"H., Elsworth , Y","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.420302Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:d129f28520c62ae37b94d17bfc130236266871cbe72542c022134cf9dc1ff3a8","observation_id":"76f6819a-128f-43a1-ba92-18069af4a31f","resolution":{"observed_at":"2026-08-16T10:37:48.420302Z","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":"2026-08-16T10:37:48.423482Z","title":"A., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.423482Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:78d9e4d303114540adce12e9e9d482d22b5e39e4b45090dc9918cd8416fa7529","observation_id":"c8d8cf04-c077-48b0-8630-52bce20ab97f","resolution":{"observed_at":"2026-08-16T10:37:48.423482Z","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":"2026-08-16T10:37:48.883315Z","title":"2018, Modeling and Analysis of Eclipsing Binary Stars; The theory and design principles of PHOEBE (IOP Publishing, Bristol, UK)","venue":null,"work_id":"24eec238-36da-493b-aae8-0bfc831ca9c6","year":2018},"citing_paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-16T10:37:48.426495Z"},"links":{"citing_paper":"/paper/2504.17853"},"observation_digest":"sha256:01fec94ec39de296a7b5655af2df76d7ae65180fe40a2f81544e80f766863d5a","observation_id":"9e8eb592-c2a4-4146-94d9-9b02f531120e","resolution":{"observed_at":"2026-08-16T10:37:48.886864Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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"}}],"paper":{"arxiv_id":"2504.17853","last_updated":"2025-04-24T18:00:39Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-19T06:03:44.753660Z","submitted_at":"2025-04-24T18:00:39Z","title":"Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":89,"verified_exact":0,"verified_fuzzy":11},"total_outbound_references":139},"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 19 August 2026, this Paper Citation Record lists 100 of 139 outbound references and 2 inbound Pith citation observations for arXiv:2504.17853."}