{"as_of":"2026-08-17T17:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:372b5e7a275d8e97fdc5e3aa8e364bb2bb6a46066684baf5ca1ea021b13e562e","coverage":[{"denominator":163,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T16:44:07.826950Z","state":"measured"},{"denominator":103,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":103,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T18:54:48.738550Z","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":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":1,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.02546","snapshot_observed_at":"2026-08-02T18:54:48.738550Z","title":"R., Li, T","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.04508","last_updated":"2026-06-26T21:34:55Z","snapshot_observed_at":"2026-08-07T23:43:56.060663Z","submitted_at":"2026-03-04T19:00:20Z","title":"The dark fate of ultra-faint dwarfs: Gravothermal collapse in action","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-02T18:54:48.738550Z"},"links":{"cited_paper":"/paper/2509.02546","citing_paper":"/paper/2603.04508"},"observation_digest":"sha256:9a854ab78afbc8c5e2d215dc20f13eaa8b90d0271dd442f0f83759c466f74a0c","observation_id":"e2275479-0248-4c1a-946e-de2ba0fd7757","resolution":{"observed_at":"2026-08-02T18:54:48.738550Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"cited_work":{"arxiv_id":"2509.02546","doi":"10.48550/arxiv.2509.02546","metadata_source":"pith","pith_arxiv_id":"2509.02546","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","venue":"astro-ph.GA","work_id":"81aac547-7dc2-4be7-930f-cd31d3f90c7a","year":2025},"citing_paper":{"arxiv_id":"2607.22499","last_updated":"2026-07-24T17:11:47Z","snapshot_observed_at":"2026-08-14T13:31:11.922647Z","submitted_at":"2026-07-24T17:11:47Z","title":"Payne4GAIN: NLTE Corrections for Red Giants in Milky Way Mapper using H-Band Neural Network Emulators","version":1},"reference_index":243,"source":"arxiv_source","source_observed_at":"2026-08-01T04:40:27.505888Z"},"links":{"cited_paper":"/paper/2509.02546","citing_paper":"/paper/2607.22499"},"observation_digest":"sha256:f2353cf63a357779b1b405f1d93f4720cd9f5bb8899d038b170cc919736adb3c","observation_id":"f5c0ccec-9d41-4a00-8d27-bb1f56817d76","resolution":{"observed_at":"2026-08-01T04:43:33.333777Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-03T18:08:33.878862+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T18:08:33.878862+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.02546","snapshot_observed_at":"2026-08-01T09:44:43.721006Z","title":"R., Li, T","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.27316","last_updated":"2026-07-29T18:00:00Z","snapshot_observed_at":"2026-08-14T20:29:44.132452Z","submitted_at":"2026-07-29T18:00:00Z","title":"Semi-analytic Inference of Satellite Densities in the Cold Dark Matter Model Part I. Comparison to Ultra-faint Dwarf Kinematics","version":1},"reference_index":129,"source":"arxiv_source","source_observed_at":"2026-08-01T09:44:43.721006Z"},"links":{"cited_paper":"/paper/2509.02546","citing_paper":"/paper/2607.27316"},"observation_digest":"sha256:17282b47ca6ffc14bf91721b5c62c1766695279e44f68a1a4ddd4ee65573447b","observation_id":"66b31e0a-df26-4dab-a13d-36fed32ce214","resolution":{"observed_at":"2026-08-01T09:44:43.721006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2509.02546/citation-record","integrity":"/paper/2509.02546/integrity","json":"/paper/2509.02546/citation-record.json","paper":"/paper/2509.02546"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:44:07.313060Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.313060Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:9a7d0d7a7b321e46546b639adb9d101dc7041ffb6bc8a38450e5d47aaccb91d2","observation_id":"3185b741-0fa0-4bf5-b0a6-c63c2316030e","resolution":{"observed_at":"2026-08-15T16:44:07.313060Z","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":"10.1093/mnras/stad1312","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:48:30.845486Z","title":"K., Vincenzo, F., Ji, A","venue":null,"work_id":"81e82213-1457-46d6-be46-02e01651d086","year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.318808Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:8e843887da4e6ff5b792b57f92a1f548621054a554b91a83a85b0318690e7037","observation_id":"9ddce9e4-c6c6-4c53-82d1-e6a2a6b9f994","resolution":{"observed_at":"2026-08-15T16:48:30.881440Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T16:44:07.323950Z","title":"S., Erkal, D., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.323950Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:897318e9747a96c7e45b44809e74fc3dad0081948fbe31e0d9e1e37008940f58","observation_id":"102fbc5c-bba5-42a5-82a0-bd508c24332d","resolution":{"observed_at":"2026-08-15T16:44:07.323950Z","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":"10.1093/mnras/stad222","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:48:30.730019Z","title":"2023, Monthly Notices of the Royal Astronomical Society, 520, 1704, doi: 10.1093/mnras/stad222","venue":null,"work_id":"0bbff38a-e21d-4da2-9868-55ec520c784b","year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.329429Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:21e861f4225ca9317e31651e3abb1277f2b441b9a3dd4c060bc6b802a45e71d4","observation_id":"037892aa-adba-466c-9e32-02e52ed1bb73","resolution":{"observed_at":"2026-08-15T16:48:30.815156Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T16:44:07.334426Z","title":"2022, Nature Astronomy, 6, 659, doi: 10.1038/s41550-022-01638-7","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.334426Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:f7bffa9a69c804e06aff387d3b723dfb0e753a1751e15d42b153133777ad3d10","observation_id":"76d2a1bf-d1d7-4e92-98d5-98033e98cba4","resolution":{"observed_at":"2026-08-15T16:44:07.334426Z","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":"2026-08-15T16:44:07.339309Z","title":"F., & Fritz, T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.339309Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:c341bafb21ad5b96301837d0bc2c74fb145f330a6187bfc174e2163e479dff55","observation_id":"27859ef1-7c49-4c65-a8fc-56f717f2a962","resolution":{"observed_at":"2026-08-15T16:44:07.339309Z","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":"2026-08-15T16:44:07.344508Z","title":"2015, The Astrophysical Journal, 807, 50, doi: 10.1088/0004-637X/807/1/50","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.344508Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:ca4f3a50f1a0cd638fb14d4f18991962ada8b911cccb2d478dfa2e09cb74e6f8","observation_id":"4367c955-214f-4b85-8664-455df6fdabcc","resolution":{"observed_at":"2026-08-15T16:44:07.344508Z","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":"2026-08-15T16:44:07.349230Z","title":"B., Evans, N","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.349230Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:3b326eb3a17fbd50fbf6e8e6bef4b6172b26e976c8cb46c7e5c404b7d25ff4ba","observation_id":"1ff7e14f-206d-42e1-bb26-30bd8948243d","resolution":{"observed_at":"2026-08-15T16:44:07.349230Z","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":"2026-08-15T16:44:07.354726Z","title":"2008, Galactic Dynamics: Second Edition","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.354726Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:f3588207b1f055c48442a8f13fc3298a958f9a3d529f6ac05088f37c0e8d53fc","observation_id":"17b37584-d667-44a0-a6f7-ffbc56c9ff0f","resolution":{"observed_at":"2026-08-15T16:44:07.354726Z","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":"2026-08-15T16:44:07.360008Z","title":"2015, The Astrophysical Journal Supplement Series, 216, 29, doi: 10.1088/0067-0049/216/2/29","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.360008Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:e16b70bf35476c8220445f85226219b30f9387ff28030de9ae47f14f6cdc93ce","observation_id":"1568c80b-2385-49d5-8c21-7313c5dfb554","resolution":{"observed_at":"2026-08-15T16:44:07.360008Z","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":"2026-08-15T16:44:07.366486Z","title":"M., Tumlinson, J., Geha, M., et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.366486Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:5424a69f8a3cab4efb1816c50168f5ab5dd65b7b3d46b31169fadd1df5000b9e","observation_id":"8a7e2953-5a7a-4d15-a5ad-2c6041966f50","resolution":{"observed_at":"2026-08-15T16:44:07.366486Z","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":"2026-08-15T16:44:07.371762Z","title":"S., & Boylan-Kolchin, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.371762Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:96a5b596722c6a492d15bafde0ea95d25978486e2783ad47e39c76320d3baf6c","observation_id":"7da42144-f6ab-4084-a909-8fa225990242","resolution":{"observed_at":"2026-08-15T16:44:07.371762Z","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":"2026-08-15T16:44:07.376882Z","title":"G., Mateo, M., et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.376882Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:0f72f46e6a2788fc577d3c69db56f41b1cb1dfba9a80dc7c7b86b2dd9898d9bf","observation_id":"c822f5c8-1f87-4768-9bd7-ec6b3df9bf04","resolution":{"observed_at":"2026-08-15T16:44:07.376882Z","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":"2026-08-15T16:44:07.381904Z","title":"2008, Monthly Notices of the Royal Astronomical Society, 390, 71, doi: 10.1111/j.1365-2966.2008.13754.x","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.381904Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:340fe2fe37ee4e391982dbc39f0b0e2a2667aac69cda27a15e511413e06fb709","observation_id":"2c930021-2284-4299-89e5-61be6af022a6","resolution":{"observed_at":"2026-08-15T16:44:07.381904Z","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":"2026-08-15T16:44:07.387902Z","title":"E., Drlica-Wagner, A., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.387902Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:ec30f1f89c5c307cecf14e4bcf60483ef9a5a2ed0fbadf85daa01dd893445483","observation_id":"96798c71-f16c-411b-9a84-0d9d69807eab","resolution":{"observed_at":"2026-08-15T16:44:07.387902Z","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":"2026-08-15T16:44:07.392742Z","title":"J., & Necib, L","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.392742Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:08b86a7486c843d7005507d045b89bb60df7d2209bb740047d816c273a3e6e0c","observation_id":"e9ab0d0d-6957-4a9c-bd3c-95ab50faac7d","resolution":{"observed_at":"2026-08-15T16:44:07.392742Z","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":"2026-08-15T16:44:07.398848Z","title":"A., Leitherer, C., & Chen, Y","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.398848Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:6884c8f8097b5a67aa059982c0c36a53d611919f1ef5c5b6eef67e55e1253b8f","observation_id":"9b0dc85e-a317-4636-a39d-a53ad99e6800","resolution":{"observed_at":"2026-08-15T16:44:07.398848Z","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":"2026-08-15T16:44:07.404062Z","title":"D., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.404062Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:6b37ec0a49dec250594c3b42d9cca29144d740f759dcfaf610d850fddaef5bb8","observation_id":"3a1df4ac-8631-4c8c-b063-814cbddcf1e8","resolution":{"observed_at":"2026-08-15T16:44:07.404062Z","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":"2026-08-15T16:44:07.410771Z","title":"P., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.410771Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:e40b344e8c16cb00c57b5a2cc9556ed2d49a5a9fbc1e749240c2f057cc0b44d3","observation_id":"0491acc1-e066-4043-a31d-52d7e130f46c","resolution":{"observed_at":"2026-08-15T16:44:07.410771Z","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":"2026-08-15T16:44:07.415722Z","title":"2023, Astronomy &amp; Astrophysics, Volume 674, id.A18, <NUMPAGES>42</NUMPAGES> pp., 674, A18, doi: 10.1051/0004-6361/202243964","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.415722Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:dd53d9f502a08da8b77ff4fa3c64e0c9c473def75068759f1c147306e2d38a6c","observation_id":"4cf937a4-d868-4427-b686-4f1c6bb1e69b","resolution":{"observed_at":"2026-08-15T16:44:07.415722Z","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":"2026-08-15T16:44:07.421729Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.421729Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:0215eadf26af33fbba9abba7b9a6c3db3bf4eceab889885971c8fa930123c555","observation_id":"dc7e65dd-31ab-4d3e-b65a-cbca3e86942c","resolution":{"observed_at":"2026-08-15T16:44:07.421729Z","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":"2026-08-15T16:44:07.426951Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.426951Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:84f0dc02faca8903f21c7eedcb28dcbaf7f86d7e55afa4aa731008016ccaeee9","observation_id":"e4a2c6cd-1344-4a52-aca7-8b8e89eda356","resolution":{"observed_at":"2026-08-15T16:44:07.426951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00036","snapshot_observed_at":"2026-08-15T16:44:07.432510Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.432510Z"},"links":{"cited_paper":"/paper/1611.00036","citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:854b33db03e37410a3589cb7a6132d48407275ca53da205416fdc03cf61f694d","observation_id":"ee9eb909-2a8a-4954-8f67-e961aaea5da0","resolution":{"observed_at":"2026-08-15T16:44:07.432510Z","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":"2026-08-15T16:44:07.438243Z","title":"J., Lang, D., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.438243Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:0c287566fe82dbaaf669a0b87b0afea50bf103431acec87c8a29dcbf2bb78b22","observation_id":"22cd4921-fd8a-44e3-a9ab-df735b4a854b","resolution":{"observed_at":"2026-08-15T16:44:07.438243Z","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":"2026-08-15T16:44:07.443318Z","title":"2016, The Astrophysical Journal Supplement Series, 222, 8, doi: 10.3847/0067-0049/222/1/8","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.443318Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:46cbd8df07d9dd65927952e30489bf68a494c10b206e850355574133d77cbfa2","observation_id":"eee45f44-e558-4d68-9db6-a563d1da3841","resolution":{"observed_at":"2026-08-15T16:44:07.443318Z","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":"2026-08-15T16:44:07.448654Z","title":"L., Nidever, D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.448654Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:fc589ac00d2ff55108d945721300012e85f0a6e8e560e0697d4523f0d49147ac","observation_id":"a7184660-c6fd-4e99-b6a8-8396a2546a45","resolution":{"observed_at":"2026-08-15T16:44:07.448654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18252","last_updated":"2025-08-29T18:01:42Z","snapshot_observed_at":"2026-08-14T14:18:36.553373Z","submitted_at":"2025-05-23T18:00:01Z","title":"The HST Legacy Archival Uniform Reduction of Local Group Imaging (LAURELIN). I. Photometry and Star Formation Histories for 36 Ultra-faint Dwarf Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18252","snapshot_observed_at":"2026-08-15T16:44:07.454784Z","title":"J., Choi, Y., Savino, A., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.454784Z"},"links":{"cited_paper":"/paper/2505.18252","citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:66672e5ab04e180aad16c59f6c0036550bcd6098fda0280c83601a39bee52e7b","observation_id":"40cb3c0e-4aa9-4384-a530-2f689012ccc5","resolution":{"observed_at":"2026-08-15T16:44:07.454784Z","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":"2026-08-15T16:44:07.460224Z","title":"A., & Macci` o, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.460224Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:b173fea1ac093774dadb7fbbff230c2c3eb3cee928bae894a20ffc76ddc3acad","observation_id":"07283485-b604-41de-aca3-cb6da1003c52","resolution":{"observed_at":"2026-08-15T16:44:07.460224Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.02245","last_updated":"2022-07-05T18:06:55Z","snapshot_observed_at":"2026-08-16T16:48:08.407667Z","submitted_at":"2022-07-05T18:06:55Z","title":"Blow-Away in the Extreme Low-Mass Starburst Galaxy Pox~186","version":1},"cited_work":{"arxiv_id":"2207.02245","doi":"10.48550/arxiv.2207.02245","metadata_source":"pith","pith_arxiv_id":"2207.02245","snapshot_observed_at":"2026-08-15T18:16:14.067578Z","title":"Blow-Away in the Extreme Low-Mass Starburst Galaxy Pox~186","venue":"astro-ph.GA","work_id":"b207efd7-092b-479e-b338-c82b1b12f475","year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.464807Z"},"links":{"cited_paper":"/paper/2207.02245","citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:d6d32006e24536bf8bb1aa000ba645fe3f4ad63a23900aa015dae4796be71eed","observation_id":"61ceea37-c981-4637-ae95-587c677ed2b9","resolution":{"observed_at":"2026-08-15T16:48:30.572808Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T16:44:07.470280Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.470280Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:fa37c84a5985f46f53eb12f2e24b014c0036e5ad197376051f1be61f5b7ea289","observation_id":"ec3129d1-030b-40c0-8e71-f3f94bb24cf2","resolution":{"observed_at":"2026-08-15T16:44:07.470280Z","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":"2026-08-15T16:44:07.475202Z","title":"N., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.475202Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:04d71c7423cc70c0dc8381a9bd64ec054fde68093fdaee47adb04af5cacbc46b","observation_id":"7dbcd692-ef58-4b0b-9407-fed541009c51","resolution":{"observed_at":"2026-08-15T16:44:07.475202Z","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":"2026-08-15T16:44:07.480510Z","title":"W., Thackeray, A","venue":null,"work_id":null,"year":1961},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.480510Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:66ac1e7f5c506056d6c9ebcbd043e1d0ee47a05afbd3d9b494b53a71d91ce75e","observation_id":"4bebc949-af84-49ff-9484-492993e0afb2","resolution":{"observed_at":"2026-08-15T16:44:07.480510Z","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":"2026-08-15T16:44:07.485175Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.485175Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:cc3f1ce9847c82b00c7cc9af73a2069f56d29b948b537a73989543354566298b","observation_id":"22c9761f-9bd6-44b4-ab91-07b4c2ca50d3","resolution":{"observed_at":"2026-08-15T16:44:07.485175Z","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":"2026-08-15T16:44:07.489816Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.489816Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:f76fdf36e2fac0b53e22c78c7e3931fd7a287aa4ce6dcccb0cfd72fd8dcd4dd3","observation_id":"0594d639-70e3-471a-9485-79cb7e6ac2fc","resolution":{"observed_at":"2026-08-15T16:44:07.489816Z","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":"2026-08-15T16:44:07.494427Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.494427Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:51b8f10347996c9944d8debaa55bd0a53086239d374f249ed0275417459bb3a4","observation_id":"7237012e-1423-4ca8-b8be-926fd8e9a736","resolution":{"observed_at":"2026-08-15T16:44:07.494427Z","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":"2026-08-15T16:44:07.498939Z","title":"2016, Journal of Open Source Software, 1, 24, doi: 10.21105/joss.00024","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.498939Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:7ebd306c479b6640e159ca01f98c190b249391defd9854d44b9a625b84eeffe8","observation_id":"34a0c616-0e37-4373-8f70-0253c6bb6c15","resolution":{"observed_at":"2026-08-15T16:44:07.498939Z","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":"2026-08-15T16:44:07.504439Z","title":"W., Lang, D., & Goodman, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.504439Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:471441d5688732c952a661ea545df6932d41218e8a607df4e52806244d97fb6f","observation_id":"343597c7-4d06-4525-99f8-222470b7c0d2","resolution":{"observed_at":"2026-08-15T16:44:07.504439Z","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":"2026-08-15T16:44:07.508933Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.508933Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:249057f2424f32a482fd245d7bca919cf61a2b5ff627454f1292768f1e6613b3","observation_id":"61d699f9-64e6-4ab5-a8f5-5406bd8702b6","resolution":{"observed_at":"2026-08-15T16:44:07.508933Z","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":"2026-08-15T16:44:07.513377Z","title":"E., Gilmore, G., & Wyse, R","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.513377Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:22a992455a5f1476cae86f38b452465487e991116da5f14006c23a27b74d0a1b","observation_id":"877643c4-127b-4ecd-bde2-269dab62afe0","resolution":{"observed_at":"2026-08-15T16:44:07.513377Z","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":"2026-08-15T16:44:07.518558Z","title":"D., Geha, M., & Willman, B","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.518558Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:0c0590e0df4b329b0eeb8c53e548c9a2275b538aa9a056f40fae5484554b680d","observation_id":"cb3cccb2-11c7-4b1b-9562-b19b43d98122","resolution":{"observed_at":"2026-08-15T16:44:07.518558Z","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":"2026-08-15T16:44:07.523562Z","title":"W., Weisz, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.523562Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:9d1ae9a77fec28988b8a4235f30cacfae6f4dced9eeb5eb3f1e4c135534a0db3","observation_id":"0a5290b2-905f-4c76-aa71-b0e1c3f97e55","resolution":{"observed_at":"2026-08-15T16:44:07.523562Z","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":"2026-08-15T16:44:07.528288Z","title":"I., Frenk, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.528288Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:8c5bdcc67e28553089dc6ed49d1952297c77c0af5eef6a9a8dcc9d00e79ad2d2","observation_id":"4efd129f-87da-4f8a-94b5-402fa230e179","resolution":{"observed_at":"2026-08-15T16:44:07.528288Z","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":"2026-08-15T16:44:07.533098Z","title":"M., & Walker, M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.533098Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:b87b4aae398da71a9ac0761c05207afa5aa4ccbb56dc0ebcd3bd326375db0659","observation_id":"498a16f8-d651-4505-a796-19d3c37b9a5e","resolution":{"observed_at":"2026-08-15T16:44:07.533098Z","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":"2026-08-15T16:44:07.537612Z","title":"E., Monaco, L., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.537612Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:487dcb803c1ec5a2120ceecf320435264b68a96c727461513ac6337715d1b521","observation_id":"238f5f76-c296-4988-aba2-293941e61682","resolution":{"observed_at":"2026-08-15T16:44:07.537612Z","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":"2026-08-15T16:44:07.543080Z","title":"M., Brasseur, C","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.543080Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:bca8335ca772eef8f484115d4ce1e8ae9cc9f8e8f787b402cbafbf0c78d12225","observation_id":"383b0b0a-2cef-4eda-b27f-89adcfde1852","resolution":{"observed_at":"2026-08-15T16:44:07.543080Z","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":"2026-08-15T16:44:07.548060Z","title":"J., Sukhbold, T., Weinberg, D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.548060Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:8a649d628729bca057a4b148d03238e6ba567ffcbd15ceab68f8077edfe560b7","observation_id":"6d139b88-6117-476f-ac49-72cf80cfa8ba","resolution":{"observed_at":"2026-08-15T16:44:07.548060Z","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":"2026-08-15T16:44:07.552894Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.552894Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:ffa85dc8819218b406f4c9469b2ff9f7007ce6292d5000462978927599207ade","observation_id":"14dd4de5-b968-42a1-8867-ed8a777c2085","resolution":{"observed_at":"2026-08-15T16:44:07.552894Z","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":"2026-08-15T16:44:07.557559Z","title":"R., Millman, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.557559Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:758aea33b722cb8fc46e99a8212212986503d97f434ac1e5ff5bc8411decd218","observation_id":"cb66188c-3637-43a1-89cf-5a5de59891df","resolution":{"observed_at":"2026-08-15T16:44:07.557559Z","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":"2026-08-15T16:44:07.562126Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.562126Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:8895451f3d0566d43b70ae21c79c09c9cb2b72e5a0b2eda0e84e9ae74d9779b9","observation_id":"e0f6b30e-e4c1-40c2-9c0d-df0329c9e71d","resolution":{"observed_at":"2026-08-15T16:44:07.562126Z","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":"2026-08-15T16:44:07.566887Z","title":"2012, The Astrophysical Journal, 755, 145, doi: 10.1088/0004-637X/755/2/145 —","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.566887Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:2d0c9104bc023f47a52c9a87c7eee2e68afa5b1063710036869189af2811f1ef","observation_id":"567e3a15-5918-4d0b-a48b-2d890b888145","resolution":{"observed_at":"2026-08-15T16:44:07.566887Z","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":"2026-08-15T16:44:07.572042Z","title":"2020, The Astrophysical Journal, 904, 45, doi: 10.3847/1538-4357/abbe0a","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.572042Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:4237d4dae1cc2e2963f21c143beb26db7741944bbf6d61c4f60841a13a8df987","observation_id":"3a6ae5b6-7ab7-4fa1-a696-844111fe4484","resolution":{"observed_at":"2026-08-15T16:44:07.572042Z","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":"2026-08-15T16:44:07.576965Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.576965Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:779144c8f117dc21f710338a2f65cfc0cf8c3475e01060c83c1d2f6ae19188ac","observation_id":"8c572fb9-0f47-4bc2-b6b0-7dbb10194be3","resolution":{"observed_at":"2026-08-15T16:44:07.576965Z","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":"2026-08-15T16:44:07.581769Z","title":"2023, The Astrophysical Journal, 953, 185, doi: 10.3847/1538-4357/ace33e","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.581769Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:452d4d43d60232d2747142117c4b656d69d7031bfab5fda37ec556e439fea291","observation_id":"f9344b53-ba6a-47b7-a539-45606e8b6eee","resolution":{"observed_at":"2026-08-15T16:44:07.581769Z","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":"10.1103/physrevd.103.023017","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:48:30.373298Z","title":"2021b, Physical Review D, 103, 023017, doi: 10.1103/PhysRevD.103.023017","venue":null,"work_id":"82ce5fdb-bed3-44b7-8d33-fad3f6c0789f","year":null},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.586512Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:447e78f178ed40ea3f4348ceb0bc8d06dce0529425d6e88ef432d32815d113eb","observation_id":"92eca991-6c6f-47b4-af8e-089e18ed900e","resolution":{"observed_at":"2026-08-15T16:48:30.379652Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T16:44:07.591554Z","title":"2015, The Astrophysical Journal, 809, 147, doi: 10.1088/0004-637X/809/2/147","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.591554Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:f7c0e059c8b30b2273952a0e346dc4c71772ed16688bc0b55434d018364a2fd8","observation_id":"fb073e3d-741f-4bc8-af20-a84b604aafaf","resolution":{"observed_at":"2026-08-15T16:44:07.591554Z","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":"2026-08-15T16:44:07.596133Z","title":"1990, The Astrophysical Journal, 356, 359, doi: 10.1086/168845","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.596133Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:9743625343f6a264e6b3f9243d9cdb2f5502996043400c461bb054bceb920d5b","observation_id":"68d29992-4584-4ebe-8e75-d3736d3b02ff","resolution":{"observed_at":"2026-08-15T16:44:07.596133Z","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":"2026-08-15T16:44:07.601003Z","title":"R., et al","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.601003Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:ded56573a56a7b11244105374a593732077cbd9a76ae75191e95a8348b79ebe5","observation_id":"29f5330c-57cc-40d4-97b6-efa9e7ea6c7b","resolution":{"observed_at":"2026-08-15T16:44:07.601003Z","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":"2026-08-15T16:44:07.605883Z","title":"F., Wetzel, A., Kereˇ s, D., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.605883Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:083968661b40c83d055e88f3ab78e9b046f8ca25efb920094e4f13ab172622f4","observation_id":"6052e982-a703-4e32-adda-da248fe11f08","resolution":{"observed_at":"2026-08-15T16:44:07.605883Z","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":"2026-08-15T16:44:07.610799Z","title":"2023, Physical Review D, 108, 083530, doi: 10.1103/PhysRevD.108.083530","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.610799Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:c80322f84ec3e3d0fc7d4d294fa42a395c8f9be31bab7481b038ba2df67e0e16","observation_id":"43f7557b-20b1-4b83-8c7a-fe9f7261b924","resolution":{"observed_at":"2026-08-15T16:44:07.610799Z","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":"2026-08-15T16:44:07.615433Z","title":null,"venue":null,"work_id":null,"year":1926},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.615433Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:17328a328f359022bc714106ef63b59b9c1944948a5e203698d2debec6aa90da","observation_id":"5e17bb00-20e8-4d4d-9332-6ad00294bac0","resolution":{"observed_at":"2026-08-15T16:44:07.615433Z","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":"2026-08-15T16:44:07.621196Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.621196Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:3aa3b7be6d449617c32fe156eb28a305ed96dc31c6bcf48a901da1ccf85ae9ae","observation_id":"cb0260a4-c923-4bd5-b046-a8919eef70a6","resolution":{"observed_at":"2026-08-15T16:44:07.621196Z","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":"2026-08-15T16:44:07.626018Z","title":"O., Wende-von Berg, S., Dreizler, S., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.626018Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:fccf5e31e2dea578000fbddd7fdeebfae0295d6d04e55d1d31b09541c952a688","observation_id":"a7050b7f-cb15-4977-96d0-73454c26a6de","resolution":{"observed_at":"2026-08-15T16:44:07.626018Z","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":"2026-08-15T16:44:07.630670Z","title":"A., McConnachie, A., Cuillandre, J.-C., et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.630670Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:d93fd5cfe2b264d1c06361e20e554b05330b47691ac3980f751fbc38a321afb6","observation_id":"a83a6e7a-5e54-4872-8f38-7e5df51adc30","resolution":{"observed_at":"2026-08-15T16:44:07.630670Z","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":"2026-08-15T16:44:07.635325Z","title":"N., Aoki, W., Arimoto, N., & Okamoto, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.635325Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:7346bb00819673983ac6241b486b4587e837b1dae9b2fe5952bf7acc10e149b8","observation_id":"12dfa3cc-be9c-4f7c-820e-bf29685d1209","resolution":{"observed_at":"2026-08-15T16:44:07.635325Z","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":"2026-08-15T16:44:07.639978Z","title":"A., Li, T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.639978Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:4237aaa5e0ee576cd30c8a8b55be4b0a38642da96ea474f97a9e49e67a99741c","observation_id":"0d5f29cf-3fab-4349-8efc-a714a512b312","resolution":{"observed_at":"2026-08-15T16:44:07.639978Z","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":"2026-08-15T16:44:07.644782Z","title":"R., Sestito, F., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.644782Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:33b775aa9af83bf5f97c2baf827cfcb15be45be717095fe1769df909c06a87cf","observation_id":"8dabd1ac-4f90-4317-9106-718262308ff7","resolution":{"observed_at":"2026-08-15T16:44:07.644782Z","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":"2026-08-15T16:44:07.650376Z","title":"2016, Monthly Notices of the Royal Astronomical Society, 461, 2212, doi: 10.1093/mnras/stw1343","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.650376Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:9e98ea61f91d331be715d13bf51414cf3627fbe3a04d362d3fb46b994dc84b4b","observation_id":"fa421872-3480-4f6a-ad98-5afde5cb33d5","resolution":{"observed_at":"2026-08-15T16:44:07.650376Z","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":"2026-08-15T16:44:07.655601Z","title":"P., Koposov, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.655601Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:fa30b40c8c41bb07db9f4f7b5db7cfbe5a59132bb7ddebd48f7fba86382c43c3","observation_id":"6f9d4abe-6142-4887-a16d-109e8cb91854","resolution":{"observed_at":"2026-08-15T16:44:07.655601Z","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":"2026-08-15T16:44:07.660464Z","title":"W., Conroy, C., Johnson, B","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.660464Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:f82054b68e718377ffc242dcd7e321e5b262cce6de6efc72213ecba9095491d0","observation_id":"339f6952-b68e-4a57-9ba6-71883160a8df","resolution":{"observed_at":"2026-08-15T16:44:07.660464Z","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":"2026-08-15T16:44:07.664994Z","title":"2017, Monthly Notices of the Royal Astronomical Society, 466, 2006, doi: 10.1093/mnras/stw3188","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.664994Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:839a56d6fae05c0fe26d9f86d458f49e87853783be45e2749e9c6d0325be1d19","observation_id":"869bd3b2-3b01-42b7-b6e3-f12500bb8c18","resolution":{"observed_at":"2026-08-15T16:44:07.664994Z","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":"2026-08-15T16:44:07.669549Z","title":"2024, The Astrophysical Journal, 966, 129, doi: 10.3847/1538-4357/ad3042","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.669549Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:0c74c8ea758855d2ccf8dea791922b529f0df46c69232203e7889b66c75a619e","observation_id":"b241e8dd-f9db-40c0-b102-bece460dfe5e","resolution":{"observed_at":"2026-08-15T16:44:07.669549Z","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":"2026-08-15T16:44:07.674261Z","title":"P., Besla, G., Anderson, J., & Alcock, C","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.674261Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:578eaf6823d4407f6a331170c7bb7db5205e8429c5ddc4bee87d7326f8916b13","observation_id":"17e34162-a1af-4231-b176-d264884d3b11","resolution":{"observed_at":"2026-08-15T16:44:07.674261Z","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":"2026-08-15T16:44:07.679246Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.679246Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:ac33226141890a729df5066bb11a5ed9c2ecf0f38a66ed3e59ddc1a50bcf6ee8","observation_id":"28c0d1f4-003f-42e1-9553-770370d71f36","resolution":{"observed_at":"2026-08-15T16:44:07.679246Z","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":"2026-08-15T16:44:07.685899Z","title":"A., Nabergoj, D., & Seljak, U","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.685899Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:04ad6d038a2825443ca4d80d82ccd4de9d987c224dba2e4125e9e227d5aebe76","observation_id":"c90d4d90-2543-412f-af52-27145d6f6825","resolution":{"observed_at":"2026-08-15T16:44:07.685899Z","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":"2026-08-15T16:44:07.691106Z","title":"2022b, The Journal of Open Source Software, 7, 4634, doi: 10.21105/joss.04634","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.691106Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:9890e76c5af1c89f68a9e1c98632dbda71e5ebebde68a53582630b4930cc84ce","observation_id":"d4d71edf-5b9f-45a8-ac6b-7aae1a1e0046","resolution":{"observed_at":"2026-08-15T16:44:07.691106Z","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":"2026-08-15T16:44:07.696013Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.696013Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:5f5ae3dc5b30a46cb67a708fea1da97c31f9eb57767513f464be8af98a33fd6d","observation_id":"b63c3da3-2e7d-41d1-aa32-27b573e5d5be","resolution":{"observed_at":"2026-08-15T16:44:07.696013Z","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":"2026-08-15T16:44:07.701333Z","title":"1962, The Astronomical Journal, 67, 471, doi: 10.1086/108756","venue":null,"work_id":null,"year":1962},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.701333Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:cf27e9f571deb76271f4f7f3268fbd9730dad7cfc23c732378330bfb1c9986bd","observation_id":"265dae6a-a486-4a91-bdfe-c9545fcca3d6","resolution":{"observed_at":"2026-08-15T16:44:07.701333Z","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":"2026-08-15T16:44:07.706357Z","title":"N., Cohen, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.706357Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:487700c7162235acf5a4ad406013ee7055714a9f57ad534143ae7d76b603f36d","observation_id":"ecc60560-0d15-4684-85fb-34fda6c5bc45","resolution":{"observed_at":"2026-08-15T16:44:07.706357Z","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":"2026-08-15T16:44:07.711469Z","title":"N., Lanfranchi, G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.711469Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:95081ce419f2e74d6de1f454eef0ad80dd4609d8f52b685aa27e3130b61d685d","observation_id":"bd404667-b938-4797-bd57-1addf8118e48","resolution":{"observed_at":"2026-08-15T16:44:07.711469Z","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":"2026-08-15T16:44:07.716364Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.716364Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:4986735e9247cc649428ce8f7a27a5f3c36fd05ebf8b7ced8e8ea3bd596da9e8","observation_id":"924a5f39-f214-4738-8b6a-7ff474dcc0da","resolution":{"observed_at":"2026-08-15T16:44:07.716364Z","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":"2026-08-15T16:44:07.722192Z","title":"E., Gilmore, G., Walker, M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.722192Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:faab13e2a83d78e47c9800deaacf1222261ee5a72ea6c1e0a9680bbbc62f677f","observation_id":"bb6f2311-b7c3-4118-a9ab-bbc17b9c0146","resolution":{"observed_at":"2026-08-15T16:44:07.722192Z","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":"2026-08-15T16:44:07.727134Z","title":"E., Walker, M","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.727134Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:09d5d53d7b5c88ae7adb713973391850cf51e7a10f9becadb6fca59846ad9b46","observation_id":"473f9fca-31a0-41bf-b00e-133115f41ace","resolution":{"observed_at":"2026-08-15T16:44:07.727134Z","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":"2026-08-15T16:44:07.732064Z","title":"E., Erkal, D., Li, T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.732064Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:646a5593d352074d808bcff9364394a9166ae8312b08c68268bfce64b076f57b","observation_id":"667cbeec-dea5-4220-8aca-9227992b2cf1","resolution":{"observed_at":"2026-08-15T16:44:07.732064Z","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":"2026-08-15T16:44:07.736758Z","title":"2001, Monthly Notices of the Royal Astronomical Society, 322, 231, doi: 10.1046/j.1365-8711.2001.04022.x K¨ upper, A","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.736758Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:d18a6d7357f0c13cf34ee1253619eaec0742a4480566d83095968bda702f06f3","observation_id":"44937fee-6af8-459a-8176-ea5754472b76","resolution":{"observed_at":"2026-08-15T16:44:07.736758Z","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":"2026-08-15T16:44:07.741673Z","title":"2020, Monthly Notices of the Royal Astronomical Society, 495, 3276, doi: 10.1093/mnras/staa585","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.741673Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:0b5a79adb59dca8747750c90ad5086f536aae5c5d36c49f67ef36013f52e17ed","observation_id":"89253497-3d73-46e7-917b-3cc833a359fb","resolution":{"observed_at":"2026-08-15T16:44:07.741673Z","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":"2026-08-15T16:44:07.746387Z","title":"K., Lee, Y","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.746387Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:bcb9d9a0322f84525790a9cd2963cec772badd4be6e463555be56bb71091ea7a","observation_id":"3d476298-b5cd-41cc-8ca8-5b595d46f3da","resolution":{"observed_at":"2026-08-15T16:44:07.746387Z","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":"10.1051/0004-6361:20054627","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T16:44:09.075215Z","title":"A., Matteucci, F., & Cescutti, G","venue":null,"work_id":"c8a6144b-d1e9-45bd-b26f-82c9e5543e60","year":2006},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.755891Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:026762be04692bb233e27155cf00bfec31024fb0a0b3a17c0c4597e588e4bad1","observation_id":"91f2ab09-6c16-4fc4-83ab-d3578412670d","resolution":{"observed_at":"2026-08-15T16:44:09.080726Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T16:44:07.765311Z","title":"2021, The Astrophysical Journal, 916, 8, doi: 10.3847/1538-4357/ac0436","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.765311Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:c5d91b55b7aebb1aaf15c7b66c7f635e32e32c5a7ae4bca7db41884f42d79117","observation_id":"e934fb67-c1f3-4d60-bacd-23d0b1dc1829","resolution":{"observed_at":"2026-08-15T16:44:07.765311Z","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":"2026-08-15T16:44:07.770320Z","title":"S., Koposov, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.770320Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:2e4cba05c66200121602392e544f38670ebf3bd805671d2511a31ede31a0dd58","observation_id":"5c5a286e-bfed-4945-b4be-6a6e86731bd3","resolution":{"observed_at":"2026-08-15T16:44:07.770320Z","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":"2026-08-15T16:44:07.775435Z","title":"S., Ji, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.775435Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:685d3b52698bdb33f4c6d4ed3a8cc722054bd6b7d258ce1bd3a36035ba8852af","observation_id":"27914f90-8fea-491b-8051-4a4440fb8d03","resolution":{"observed_at":"2026-08-15T16:44:07.775435Z","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":"2026-08-15T16:44:07.780163Z","title":"O., P´ erez-Villegas, A., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.780163Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:b930a821cc3a6d26a2abd3885aebabb07053b15cf671c131252b2cccd7937cfb","observation_id":"72d9ab4e-7a82-4549-a635-a4323943a9c5","resolution":{"observed_at":"2026-08-15T16:44:07.780163Z","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":"2026-08-15T16:44:07.784625Z","title":"2022, Monthly Notices of the Royal Astronomical Society, 516, 2348, doi: 10.1093/mnras/stac1827","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.784625Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:e1119519aa4c4c2c63463b23f534c50ceba8ee3d3e8a64f8b18a1a801c23fca3","observation_id":"7f96ba25-1783-4a6b-a166-775e32cca32c","resolution":{"observed_at":"2026-08-15T16:44:07.784625Z","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":"2026-08-15T16:44:07.794005Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.794005Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:f9034b2c17e045d3e6b76f3c76ce3ebdeda67103ee57f370470e0b178290c211","observation_id":"3e0b91b5-d0c5-45d0-8e9e-fa129986c8fc","resolution":{"observed_at":"2026-08-15T16:44:07.794005Z","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":"2026-08-15T16:44:07.798843Z","title":"F., & Jin, S","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.798843Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:fe8f77d960ef2b76647f6fe5f3f2adc673c2cbe8c49e66098366cad195d68580","observation_id":"22cf11e0-c4dd-425e-b00e-9b5c61c28c14","resolution":{"observed_at":"2026-08-15T16:44:07.798843Z","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":"2026-08-15T16:44:07.803424Z","title":"D., Minor, Q","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.803424Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:1f49870f905a93bdcdce5f0ddb5b6128cb46c6c7e357fa6c5a0412e67729db7e","observation_id":"e0e6ec0d-e71d-4723-aa17-7b917e72a392","resolution":{"observed_at":"2026-08-15T16:44:07.803424Z","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":"2026-08-15T16:44:07.808272Z","title":"P., & Watkins, L","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.808272Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:b2055be898dd44db42b68d46347f8a380ac49616216815b818bdef83ed25d2d8","observation_id":"d6605c36-59eb-4ad6-abf1-b82b67fb8948","resolution":{"observed_at":"2026-08-15T16:44:07.808272Z","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":"2026-08-15T16:44:07.812903Z","title":"2001, The Astrophysical Journal, 559, 754, doi: 10.1086/322356","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.812903Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:56dcec42ba0cd1d761211f4d86a8e066e4898b690592ba72fd459a77fbf6f29a","observation_id":"bcfb2b27-7917-4dd7-8169-cd88e0e829b0","resolution":{"observed_at":"2026-08-15T16:44:07.812903Z","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":"2026-08-15T16:44:07.817633Z","title":"W., & Venn, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.817633Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:5cd68b6da5df49b2c9260cfdc3c6e5afdb3be612a25b5fd72b4c7c6ed6968eb5","observation_id":"569810aa-bc0a-4568-b1d0-f3e992bd91c9","resolution":{"observed_at":"2026-08-15T16:44:07.817633Z","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":"2026-08-15T16:44:07.822383Z","title":"2010, in Proceedings of the 9th Python in Science Conference, ed","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.822383Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:01dda29e8d914c4e7fc5449a1b0de55ccfa0635932b9e94ad6207e4b3fae97af","observation_id":"b428eae0-cdf5-4509-a518-a0871544b3de","resolution":{"observed_at":"2026-08-15T16:44:07.822383Z","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":"2026-08-15T16:44:07.826950Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints","version":1},"reference_index":103,"source":"pdf_text","source_observed_at":"2026-08-15T16:44:07.826950Z"},"links":{"citing_paper":"/paper/2509.02546"},"observation_digest":"sha256:9de7a3428e851cdd1b660bbbb8fa55ca22a5920b90a328e678824aba077cd02d","observation_id":"d26564ef-67fa-4f28-928b-f12ad023174f","resolution":{"observed_at":"2026-08-15T16:44:07.826950Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2509.02546","last_updated":"2025-09-02T17:45:11Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-15T16:34:30.939770Z","submitted_at":"2025-09-02T17:45:11Z","title":"Chemodynamics of Bo\\\"otesI with $S^{5}$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":95,"verified_exact":4,"verified_fuzzy":0},"total_outbound_references":163},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 100 of 163 outbound references and 3 inbound Pith citation observations for arXiv:2509.02546."}