{"as_of":"2026-08-11T16:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:1c9933f1ec6e345447a599925e729d96e270daa26a4137b3cceeaff945c9772f","coverage":[{"denominator":56,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":56,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T17:52:45.773640Z","state":"measured"},{"denominator":56,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":56,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2501.11882/citation-record","integrity":"/paper/2501.11882/integrity","json":"/paper/2501.11882/citation-record.json","paper":"/paper/2501.11882"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:52:47.811857Z","title":", year 1989","venue":null,"work_id":"134c8752-9d7f-493f-a693-9aa6a039c66a","year":1989},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.413126Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:d386f8c8188d4475161169fe559ea216f4c7e0e0a7c6f172c9e4034016dff632","observation_id":"e37bd79b-6fb6-49a7-923d-5f779c869c37","resolution":{"observed_at":"2026-08-10T17:52:47.817434Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0011493","last_updated":"2000-11-27T18:48:58Z","snapshot_observed_at":"2026-07-07T00:14:20.175442Z","submitted_at":"2000-11-27T18:48:58Z","title":"Stellar mass-to-light ratios and the Tully-Fisher relation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0011493","snapshot_observed_at":"2026-08-10T17:52:45.419676Z","title":", author de Jong , R.S","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.419676Z"},"links":{"cited_paper":"/paper/astro-ph/0011493","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:6010aeb7cbea8238a1d3a4a08f703bbf7bc50b0448336edae79acef27bd3074c","observation_id":"7f4a6a6d-9044-49e2-a101-55d46a5905cd","resolution":{"observed_at":"2026-08-10T17:52:45.419676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.00052","last_updated":"2017-06-29T22:59:56Z","snapshot_observed_at":"2026-08-07T01:13:58.694901Z","submitted_at":"2017-02-28T20:52:31Z","title":"Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.00052","snapshot_observed_at":"2026-08-10T17:52:45.426203Z","title":", author Bershady , M.A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.426203Z"},"links":{"cited_paper":"/paper/1703.00052","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:538795eb726ecd3e74df6896477fbfbf7c7ba4305e059396ef624757bb90670d","observation_id":"7a557ee0-0593-4c65-9910-6a91e1744f3d","resolution":{"observed_at":"2026-08-10T17:52:45.426203Z","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":"2026-08-10T17:52:45.432853Z","title":", author Charlot , S","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.432853Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:bb7eaa2ad870d9c8d9801dfbc7367dd3540b1d61c0beb2f1de9ef6d1db79d632","observation_id":"cf66036d-8e0d-4dc1-9d02-f75e2803dc34","resolution":{"observed_at":"2026-08-10T17:52:45.432853Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.1482","last_updated":"2014-12-03T21:00:27Z","snapshot_observed_at":"2026-07-06T04:02:33.136517Z","submitted_at":"2014-12-03T21:00:27Z","title":"Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.1482","snapshot_observed_at":"2026-08-10T17:52:45.439821Z","title":", author Bershady , M.A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.439821Z"},"links":{"cited_paper":"/paper/1412.1482","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:bc220c3228aa9f2355cb227814b320dfa7e0dfb95ada488abb04d543b9b49e32","observation_id":"dc99409c-6f3d-478a-98b2-c6acae080485","resolution":{"observed_at":"2026-08-10T17:52:45.439821Z","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":"2026-08-10T17:52:45.445791Z","title":", author Copin , Y","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.445791Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:202b4506e27566bbadb6a9d568014474f65c143e6791da9908350476404d2b23","observation_id":"735072f1-14d9-4a1d-a06a-38ead3f232d7","resolution":{"observed_at":"2026-08-10T17:52:45.445791Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.7095","last_updated":"2013-01-29T23:07:00Z","snapshot_observed_at":"2026-07-06T03:05:11.556832Z","submitted_at":"2013-01-29T23:07:00Z","title":"Modeling the Panchromatic Spectral Energy Distributions of Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.7095","snapshot_observed_at":"2026-08-10T17:52:45.453589Z","title":", year 2013","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.453589Z"},"links":{"cited_paper":"/paper/1301.7095","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:50e889c85fc364cdee8ca75438dbbc3b876b37f2754e33413ea8e7f4af66f99a","observation_id":"8a974eb5-c338-42fa-a1e6-77b275271a8c","resolution":{"observed_at":"2026-08-10T17:52:45.453589Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.2100","last_updated":"2008-10-14T07:33:25Z","snapshot_observed_at":"2026-08-08T05:43:20.065908Z","submitted_at":"2008-10-13T16:05:47Z","title":"High-Resolution Rotation Curves and Galaxy Mass Models from THINGS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.2100","snapshot_observed_at":"2026-08-10T17:52:45.460095Z","title":", author Walter , F","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.460095Z"},"links":{"cited_paper":"/paper/0810.2100","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:83beff009cb9c3f7339851f7ff6b9a9379edda3c6603101f4a38a89bd270f7fd","observation_id":"9bbbe767-09cd-496f-ab8c-13c1e2701fc9","resolution":{"observed_at":"2026-08-10T17:52:45.460095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.01183","snapshot_observed_at":"2026-08-10T17:52:45.466209Z","title":", author Mena , O","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.466209Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:b3fd0f01ad6a9c337727c686550758b01a43a8637348ba0cc8f14c12c4bf3a84","observation_id":"9327e5f5-d8a7-415e-8a85-40c6e3d91803","resolution":{"observed_at":"2026-08-10T17:52:45.466209Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.05744","last_updated":"2018-02-07T19:00:03Z","snapshot_observed_at":"2026-07-06T06:09:41.892391Z","submitted_at":"2017-11-15T19:00:03Z","title":"Improving galaxy morphologies for SDSS with Deep Learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.05744","snapshot_observed_at":"2026-08-10T17:52:45.472409Z","title":", author Huertas-Company , M","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.472409Z"},"links":{"cited_paper":"/paper/1711.05744","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:34ce1e61a3859eb4aca9491ffbaee73ae866abac3bbd331245ec20b70eeb5f0d","observation_id":"343f0112-90e2-48fd-b37e-8139b74c4ee3","resolution":{"observed_at":"2026-08-10T17:52:45.472409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10694","last_updated":"2021-10-20T18:00:01Z","snapshot_observed_at":"2026-07-31T01:09:37.144753Z","submitted_at":"2021-10-20T18:00:01Z","title":"SDSS-IV DR17: Final Release of MaNGA PyMorph Photometric and Deep Learning Morphological Catalogs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10694","snapshot_observed_at":"2026-08-10T17:52:45.483144Z","title":", author Margalef , B","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.483144Z"},"links":{"cited_paper":"/paper/2110.10694","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:77e9eca36b8d94c41b5c793c110bbd79643020d8daa266d2470e350fdb92b3fb","observation_id":"2cbf5def-a580-4a59-8257-0ed8a695b850","resolution":{"observed_at":"2026-08-10T17:52:45.483144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.3960","last_updated":"2012-05-20T13:25:08Z","snapshot_observed_at":"2026-07-06T02:39:33.682077Z","submitted_at":"2011-12-16T21:00:01Z","title":"Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.3960","snapshot_observed_at":"2026-08-10T17:52:45.488146Z","title":", author McGaugh , S.S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.488146Z"},"links":{"cited_paper":"/paper/1112.3960","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:c742ba481e64e7f9ade9bf88da99bd62261054d178bb6ee2046396d00ef10997","observation_id":"bacc7eda-aab0-41b7-841a-fda648f0babb","resolution":{"observed_at":"2026-08-10T17:52:45.488146Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.08213","last_updated":"2018-02-22T18:12:43Z","snapshot_observed_at":"2026-08-10T07:09:04.687942Z","submitted_at":"2018-02-22T18:12:43Z","title":"SDSS-IV MaNGA: Stellar angular momentum of about 2300 galaxies: unveiling the bimodality of massive galaxy properties","version":1},"cited_work":{"arxiv_id":"1802.08213","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.08213","snapshot_observed_at":"2026-08-10T17:52:47.312674Z","title":"SDSS-IV MaNGA: Stellar angular momentum of about 2300 galaxies: unveiling the bimodality of massive galaxy properties","venue":"astro-ph.GA","work_id":"42b01c66-ef21-48f3-8046-bb66d0c7bdd9","year":2018},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.493977Z"},"links":{"cited_paper":"/paper/1802.08213","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:d27a9b6072cbcb65b5dded290f322edd20c11e2e7b972c1defcf0c49262c5476","observation_id":"dc452bfd-bae5-413d-8820-7dbe53853a5d","resolution":{"observed_at":"2026-08-10T17:52:47.319350Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.11207","last_updated":"2023-10-25T23:32:02Z","snapshot_observed_at":"2026-08-07T09:30:53.206377Z","submitted_at":"2023-03-20T15:40:28Z","title":"Investigating Topological Order using Recurrent Neural Networks","version":3},"cited_work":{"arxiv_id":"2303.11207","doi":null,"metadata_source":"pith","pith_arxiv_id":"2303.11207","snapshot_observed_at":"2026-08-10T17:52:47.285620Z","title":"Investigating Topological Order using Recurrent Neural Networks","venue":"cond-mat.str-el","work_id":"f1ae2626-c38b-47c5-82d1-b9166e6acf05","year":2023},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.501459Z"},"links":{"cited_paper":"/paper/2303.11207","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:0e3a06c26bf1c401706ea8f71706345f519ff65a42dffcdac619ee22bb2538d4","observation_id":"5586e64e-5c73-4763-ac66-5de9779917dc","resolution":{"observed_at":"2026-08-10T17:52:47.295227Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.00065","last_updated":"2024-01-15T16:10:26Z","snapshot_observed_at":"2026-07-06T15:36:07.713593Z","submitted_at":"2023-05-31T18:00:03Z","title":"Distinguishing thermal histories of dark matter from structure formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.00065","snapshot_observed_at":"2026-08-10T17:52:45.506414Z","title":", author Li , Y.Z","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.506414Z"},"links":{"cited_paper":"/paper/2306.00065","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:57c22c29eb1c222cf6941dda130ec28dad33efd27a030c7e04ae0180ba1b4cf1","observation_id":"05dcff43-7a76-44ba-a8b8-1fe90e4f52b6","resolution":{"observed_at":"2026-08-10T17:52:45.506414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:52:47.794218Z","title":", year 1927","venue":null,"work_id":"4b5e90db-4278-475d-88ad-91db6df4b6a5","year":1927},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.511683Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:5bd325472e9f57d48db412357312164a2a8e5c7910341458499b497b7a6419a6","observation_id":"2b64914b-28e6-443d-ac3c-c415f1c66030","resolution":{"observed_at":"2026-08-10T17:52:47.798675Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.04158","last_updated":"2021-05-17T14:10:10Z","snapshot_observed_at":"2026-08-05T18:52:30.063395Z","submitted_at":"2020-10-08T17:59:05Z","title":"Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.04158","snapshot_observed_at":"2026-08-10T17:52:45.517137Z","title":", author Pogosian , L","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.517137Z"},"links":{"cited_paper":"/paper/2010.04158","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:c38ce94678c46d116f7f57ecc4f7fb144951c2e47b0bc010bb77779622b8b0ca","observation_id":"0d8e2edf-6763-4433-85a6-30016d9a2da8","resolution":{"observed_at":"2026-08-10T17:52:45.517137Z","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":"2026-08-10T17:52:45.528195Z","title":", year 1966","venue":null,"work_id":null,"year":1966},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.528195Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:4e078c17ece13618305a75009ff4f6622ff0368b0179d2a3cec93ce2890c9e85","observation_id":"9edd2159-d90f-4796-b23f-49c6abd67bfc","resolution":{"observed_at":"2026-08-10T17:52:45.528195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.09251","last_updated":"2016-06-29T20:00:02Z","snapshot_observed_at":"2026-07-06T05:01:49.181638Z","submitted_at":"2016-06-29T20:00:02Z","title":"SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.09251","snapshot_observed_at":"2026-08-10T17:52:45.534472Z","title":", author McGaugh , S.S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.534472Z"},"links":{"cited_paper":"/paper/1606.09251","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:61a35685949a30ed40bcb26713fbe1991426f5e2b6df15e4813a483ac4ee8c70","observation_id":"42f48942-fc95-401d-95d9-989a511ca1e6","resolution":{"observed_at":"2026-08-10T17:52:45.534472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.11712","last_updated":"2023-09-27T11:09:09Z","snapshot_observed_at":"2026-07-06T15:18:57.451425Z","submitted_at":"2023-04-23T18:00:37Z","title":"MaNGA DynPop -- II. Global stellar population, gradients, and star-formation histories from integral-field spectroscopy of 10K galaxies: link with galaxy rotation, shape, and total-density gradients","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.11712","snapshot_observed_at":"2026-08-10T17:52:45.539522Z","title":", author Zhu , K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.539522Z"},"links":{"cited_paper":"/paper/2304.11712","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:4063efbc4fa7b70166e0f28b55bdb4874494adb471d5cab227af491d8c3577d2","observation_id":"0fef1ee6-4162-4cb2-96bd-291bf90f4cf5","resolution":{"observed_at":"2026-08-10T17:52:45.539522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.12395","last_updated":"2024-04-23T12:28:20Z","snapshot_observed_at":"2026-07-06T16:22:01.657709Z","submitted_at":"2023-09-21T18:00:04Z","title":"MaNGA DynPop -- V. The dark-matter fraction versus stellar velocity dispersion relation and stellar initial mass function variations in galaxies: dynamical models and full spectrum fitting of integral-field spectroscopy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.12395","snapshot_observed_at":"2026-08-10T17:52:45.544810Z","title":", author Zhu , K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.544810Z"},"links":{"cited_paper":"/paper/2309.12395","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:edb36601335ee061f572b6df88043537abcd222e6500ee2e1f0cd53b196541f0","observation_id":"96200878-92b4-44d2-b2d7-cf82830a52af","resolution":{"observed_at":"2026-08-10T17:52:45.544810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.0007","last_updated":"2014-06-13T01:11:59Z","snapshot_observed_at":"2026-08-04T05:19:08.451508Z","submitted_at":"2014-02-28T21:00:32Z","title":"Cosmic Star Formation History","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.0007","snapshot_observed_at":"2026-08-10T17:52:45.551949Z","title":", author Dickinson , M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.551949Z"},"links":{"cited_paper":"/paper/1403.0007","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:72b899318b677721ec4499e0ab9b0579dbc0dd2d580415e7e447d79b8f30899b","observation_id":"f3bcf2f8-d3c6-443e-9097-711b8e52c107","resolution":{"observed_at":"2026-08-10T17:52:45.551949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.00385","last_updated":"2021-07-01T11:53:18Z","snapshot_observed_at":"2026-07-06T11:25:00.076469Z","submitted_at":"2021-07-01T11:53:18Z","title":"Morphological classification of compact and extended radio galaxies using convolutional neural networks and data augmentation techniques","version":1},"cited_work":{"arxiv_id":"2107.00385","doi":null,"metadata_source":"pith","pith_arxiv_id":"2107.00385","snapshot_observed_at":"2026-08-10T17:52:47.122203Z","title":"Morphological classification of compact and extended radio galaxies using convolutional neural networks and data augmentation techniques","venue":"astro-ph.GA","work_id":"0528e9d0-3a67-4e65-9dc9-bd20af12ad1c","year":2021},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.558612Z"},"links":{"cited_paper":"/paper/2107.00385","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:bea68a99377537a6821249bf9b09cc0db982b59e7ff80341bfb7387cd0cd1914","observation_id":"66761273-2290-44e4-b5c2-8a276661c120","resolution":{"observed_at":"2026-08-10T17:52:47.127040Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1107.2934","last_updated":"2011-12-07T21:12:12Z","snapshot_observed_at":"2026-07-06T02:30:54.440299Z","submitted_at":"2011-07-14T20:01:18Z","title":"The Baryonic Tully-Fisher Relation of Gas Rich Galaxies as a Test of LCDM and MOND","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.2934","snapshot_observed_at":"2026-08-10T17:52:45.564486Z","title":", year 2012","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.564486Z"},"links":{"cited_paper":"/paper/1107.2934","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:7055c035fff1086a501d07929b7048aa8fd85b5672864db5cd06e6389a8ac36a","observation_id":"a7ee847e-ca1a-48ab-83c5-06c269d7ea70","resolution":{"observed_at":"2026-08-10T17:52:45.564486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.05917","last_updated":"2016-09-19T20:02:10Z","snapshot_observed_at":"2026-08-10T10:13:35.764019Z","submitted_at":"2016-09-19T20:02:10Z","title":"The Radial Acceleration Relation in Rotationally Supported Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.05917","snapshot_observed_at":"2026-08-10T17:52:45.570378Z","title":", author Lelli , F","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.570378Z"},"links":{"cited_paper":"/paper/1609.05917","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:cd5a3a1b83a74d5f9f6475ae1484473a40cd2115f6c494ba3ea9911cebdb23d3","observation_id":"29714b5b-ca8e-4721-b804-001a8819d110","resolution":{"observed_at":"2026-08-10T17:52:45.570378Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0003001","last_updated":"2000-03-01T00:20:58Z","snapshot_observed_at":"2026-07-07T00:10:15.760445Z","submitted_at":"2000-03-01T00:20:58Z","title":"The Baryonic Tully-Fisher Relation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0003001","snapshot_observed_at":"2026-08-10T17:52:45.577480Z","title":", author Schombert , J.M","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.577480Z"},"links":{"cited_paper":"/paper/astro-ph/0003001","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:caf84ec217b8147047b3778fefebe0ebc41e7642c47b0f7eac353ae43b0106b3","observation_id":"63a9dbef-98e4-47fe-8f4f-ff95126c8132","resolution":{"observed_at":"2026-08-10T17:52:45.577480Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.11007","last_updated":"2023-08-21T19:46:48Z","snapshot_observed_at":"2026-07-06T16:08:45.401095Z","submitted_at":"2023-08-21T19:46:48Z","title":"Mitigating Bias in Deep Learning: Training Unbiased Models on Biased Data for the Morphological Classification of Galaxies","version":1},"cited_work":{"arxiv_id":"2308.11007","doi":null,"metadata_source":"pith","pith_arxiv_id":"2308.11007","snapshot_observed_at":"2026-08-10T17:52:47.051654Z","title":"Mitigating Bias in Deep Learning: Training Unbiased Models on Biased Data for the Morphological Classification of Galaxies","venue":"astro-ph.GA","work_id":"3f6ea7e5-0de4-4080-92b7-275057a0ceed","year":2023},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.583421Z"},"links":{"cited_paper":"/paper/2308.11007","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:4a18e9035c163970948977623157a6bc0b4ec1033839c7e4b6eb479f246da50f","observation_id":"7450c282-032a-4829-83e5-e9abd0055f84","resolution":{"observed_at":"2026-08-10T17:52:47.055955Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T17:52:45.590333Z","title":", year 1983","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.590333Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:4a158e5bec3c84726a7f02cd244f25c89eda7b46c2335609ae22fc7117cb8d48","observation_id":"82a08315-1504-4b91-bf11-6faf008ba28b","resolution":{"observed_at":"2026-08-10T17:52:45.590333Z","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":"2026-08-10T17:52:45.598505Z","title":", author Williams , L.L.R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.598505Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:3910081d5e55b74f8e4deec1ff70fc2bd6da8e341816240f4995f6e1f492d0d9","observation_id":"c70896e9-c976-4193-837d-7294aebbb86f","resolution":{"observed_at":"2026-08-10T17:52:45.598505Z","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":"2026-08-10T17:52:45.604059Z","title":", author Grobler , T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.604059Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:1d9da228c867b22bbfdba12f3a379e0d14a038ca61741cdb922ef1f21350fb51","observation_id":"15fb2819-cdf2-4207-acae-1e6760db7300","resolution":{"observed_at":"2026-08-10T17:52:45.604059Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.12199","last_updated":"2022-09-25T11:30:23Z","snapshot_observed_at":"2026-08-07T21:24:54.780968Z","submitted_at":"2022-09-25T11:30:23Z","title":"RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic Scales","version":1},"cited_work":{"arxiv_id":"2209.12199","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.12199","snapshot_observed_at":"2026-08-10T17:52:46.838800Z","title":"RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic Scales","venue":"astro-ph.GA","work_id":"f1f326cd-4b12-413c-ad94-f62ddfdb9d73","year":2022},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.611133Z"},"links":{"cited_paper":"/paper/2209.12199","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:3a7e93e5cecd2f84d10a8ec02c49892edd8a7b0adc758f4579fd7d1428b0df58","observation_id":"475b444b-7fee-43c4-b988-7e3790a35d59","resolution":{"observed_at":"2026-08-10T17:52:46.843923Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.02049","last_updated":"2017-09-07T02:31:51Z","snapshot_observed_at":"2026-07-06T05:58:26.432050Z","submitted_at":"2017-09-07T02:31:51Z","title":"2D Bayesian automated tilted-ring fitting of disk galaxies in large HI galaxy surveys: 2DBAT","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.02049","snapshot_observed_at":"2026-08-10T17:52:45.616213Z","title":", author Staveley-Smith , L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.616213Z"},"links":{"cited_paper":"/paper/1709.02049","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:e508f561b6247fc62c200e5d8698b7c4587f793b3bcc1e3f3e34f0f904b0a73e","observation_id":"671fdc27-7079-43a0-8036-2bdb5a27fa52","resolution":{"observed_at":"2026-08-10T17:52:45.616213Z","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":"2026-08-10T17:52:45.622202Z","title":", author Skara , F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.622202Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:b1394d004eba4ca0b5c8e69b3cddc40b79738132e3a36f06ae1a366b0c122046","observation_id":"36eee7ff-3728-4a18-b87a-79a86d91c666","resolution":{"observed_at":"2026-08-10T17:52:45.622202Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.11001","last_updated":"2019-01-30T18:52:20Z","snapshot_observed_at":"2026-08-09T07:43:36.257558Z","submitted_at":"2019-01-30T18:52:20Z","title":"Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies","version":1},"cited_work":{"arxiv_id":"1901.11001","doi":null,"metadata_source":"pith","pith_arxiv_id":"1901.11001","snapshot_observed_at":"2026-08-10T17:52:46.691311Z","title":"Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies","venue":"astro-ph.GA","work_id":"757c35c2-9d8e-4522-a59e-47b881c1ec2e","year":2019},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.629272Z"},"links":{"cited_paper":"/paper/1901.11001","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:a77ae38aba24e6188f24f9165dc5aa01597fd755245f37618908bb396464c10f","observation_id":"1214089e-f393-4d69-84d4-c23d7a4ef444","resolution":{"observed_at":"2026-08-10T17:52:46.700030Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03233","last_updated":"2019-12-06T17:15:26Z","snapshot_observed_at":"2026-08-02T16:32:24.782527Z","submitted_at":"2019-12-06T17:15:26Z","title":"Properties of galaxies with an offset between the position angles of the major kinematic and photometric axes","version":1},"cited_work":{"arxiv_id":"1912.03233","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.03233","snapshot_observed_at":"2026-08-10T17:52:46.642966Z","title":"Properties of galaxies with an offset between the position angles of the major kinematic and photometric axes","venue":"astro-ph.GA","work_id":"23afcd28-f982-4372-a26f-2ffe23670c2a","year":2019},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.634563Z"},"links":{"cited_paper":"/paper/1912.03233","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:0c8217309011ddf74dc0597c1b0df7a38b6c22c3828f08a4e8966600a1c5dc8e","observation_id":"beb1335a-fca6-4f5a-8127-c967eed033bf","resolution":{"observed_at":"2026-08-10T17:52:46.651233Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04510","last_updated":"2022-07-18T20:33:57Z","snapshot_observed_at":"2026-07-06T12:16:41.817858Z","submitted_at":"2021-12-08T19:00:02Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04510","snapshot_observed_at":"2026-08-10T17:52:45.642084Z","title":", author Yuan , W","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.642084Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:ecd0dfed533105b55d63434b6de3598d06cbd08d816775fbf6e180e932b2f730","observation_id":"0bd06382-c11e-4dfe-af2d-448e0cb90b6a","resolution":{"observed_at":"2026-08-10T17:52:45.642084Z","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":"2026-08-10T17:52:45.648480Z","title":", author Ford , W","venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.648480Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:0d182ca9821bd0185628f3e65c41f8fb675b02c25bee9c10f4d81de3078f70e5","observation_id":"2d42327e-a24b-459f-b117-023644ba49e8","resolution":{"observed_at":"2026-08-10T17:52:45.648480Z","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":"2026-08-10T17:52:45.662246Z","title":", year 1955","venue":null,"work_id":null,"year":1955},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.662246Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:bff092f24e2a4d14d8a369a148209c6714deec450b4bebea784f8017eb370765","observation_id":"0f10a6df-85f5-45e8-998c-e5d1ff8b8446","resolution":{"observed_at":"2026-08-10T17:52:45.662246Z","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":"2026-08-10T17:52:45.670527Z","title":", author McGaugh , S.S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.670527Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:9483bdebcc12c48bb0163cf7defccc5dd568614512a9c23a12f58c42e130fea2","observation_id":"1a189520-5e21-4d22-8b7d-5a3728ff7e08","resolution":{"observed_at":"2026-08-10T17:52:45.670527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:52:47.774252Z","title":", year 1915","venue":null,"work_id":"34a4d478-aede-4bd5-89c0-236c977545f4","year":1915},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.677512Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:7ce2a311a5ed2e0dc15e693c5e7901e240342a19a3ea06d845e7022f0050d071","observation_id":"0959ec78-bfd9-4f33-b024-c7390491bb0c","resolution":{"observed_at":"2026-08-10T17:52:47.781273Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07034","last_updated":"2021-04-14T18:00:00Z","snapshot_observed_at":"2026-07-06T10:59:39.139457Z","submitted_at":"2021-04-14T18:00:00Z","title":"The Intrinsic Scatter of Galaxy Scaling Relations","version":1},"cited_work":{"arxiv_id":"2104.07034","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.07034","snapshot_observed_at":"2026-08-10T17:52:46.506545Z","title":"The Intrinsic Scatter of Galaxy Scaling Relations","venue":"astro-ph.GA","work_id":"d058307c-b348-499d-a253-c7912407561f","year":2021},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.685848Z"},"links":{"cited_paper":"/paper/2104.07034","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:2b4851322768de10a663fbd27ce13697f0a82a6e6e8fdb5000f234ec6cc368af","observation_id":"a7b7e99a-b1bb-4f36-8975-ae272230cb54","resolution":{"observed_at":"2026-08-10T17:52:46.514684Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.10034","last_updated":"2023-10-25T13:40:13Z","snapshot_observed_at":"2026-08-08T05:26:56.117764Z","submitted_at":"2023-09-18T18:00:02Z","title":"Cosmological parameters derived from the final (PR4) Planck data release","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.10034","snapshot_observed_at":"2026-08-10T17:52:45.691747Z","title":", author Banday , A.J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.691747Z"},"links":{"cited_paper":"/paper/2309.10034","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:633fdf87091b842deec8ef85eed7f40a6608c2a4e9fdaea468ffeb0a23c6095b","observation_id":"c59ad4b3-301f-41c3-b036-27a5bb3d21bc","resolution":{"observed_at":"2026-08-10T17:52:45.691747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:52:47.758027Z","title":", author Fisher , J.R","venue":null,"work_id":"bb4d2119-d47a-409e-8b51-fb19d4b9d3d1","year":1977},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.698012Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:341c4fcaff0ed87375cbc53960905600b254f3126dee1a53ace1795f5a52c518","observation_id":"955c9eef-c070-46a3-b2ed-1cd2ca393bb6","resolution":{"observed_at":"2026-08-10T17:52:47.762954Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T17:52:45.704582Z","title":", year 2017 a","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.704582Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:b45720cc46a4732d6e37946948a889749978974ea45c103e07e6bbb9e92733dd","observation_id":"0c474ca1-d5bb-4e8b-862f-64642826273e","resolution":{"observed_at":"2026-08-10T17:52:45.704582Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.05944","last_updated":"2017-09-13T07:13:43Z","snapshot_observed_at":"2026-07-06T06:00:08.350506Z","submitted_at":"2017-09-13T07:13:43Z","title":"Evidence for galaxy dynamics tracing background cosmology below the de Sitter scale of acceleration","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.05944","snapshot_observed_at":"2026-08-10T17:52:45.710240Z","title":", year 2017 b","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.710240Z"},"links":{"cited_paper":"/paper/1709.05944","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:ce87fcc4b60d741df2c77d07ba39cf4fd2b771b2f7e66e77465a5b96f194e00b","observation_id":"d332cef2-f16c-4a20-965a-b7b7cd5899f8","resolution":{"observed_at":"2026-08-10T17:52:45.710240Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.06212","last_updated":"2022-11-26T03:05:12Z","snapshot_observed_at":"2026-07-06T06:33:52.149780Z","submitted_at":"2018-04-17T13:04:18Z","title":"Self-similar galaxy dynamics below the de Sitter scale of acceleration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.06212","snapshot_observed_at":"2026-08-10T17:52:45.715516Z","title":", year 2018","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.715516Z"},"links":{"cited_paper":"/paper/1804.06212","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:d731cb468bc02bcf004fa02b058e13542e35ab99cdd360a31508d13b70ea57e2","observation_id":"9a4b2536-42ed-4ac0-88aa-6e8feb50c202","resolution":{"observed_at":"2026-08-10T17:52:45.715516Z","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":"2026-08-10T17:52:45.720871Z","title":", year 2021","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.720871Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:71483863638ddcbfa992afa2da3ac3aa21a7842f477f094617d13369cc978be5","observation_id":"57d66c2d-93be-4d1c-b63f-1f17656509ba","resolution":{"observed_at":"2026-08-10T17:52:45.720871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.06399","last_updated":"2024-08-12T09:06:35Z","snapshot_observed_at":"2026-07-06T18:59:47.901397Z","submitted_at":"2024-08-12T09:06:35Z","title":"Galaxy dynamics tracing quantum cosmology beyond $\\Lambda$CDM below the de Sitter scale of acceleration","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.06399","snapshot_observed_at":"2026-08-10T17:52:45.726164Z","title":", year 2024 a","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.726164Z"},"links":{"cited_paper":"/paper/2408.06399","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:dd1c7c8b36d09affc43253f103e8617c0b6f2836ed0246b2fa991ad3fd7989a6","observation_id":"2ad82213-b841-47b8-ba16-d136118f99e4","resolution":{"observed_at":"2026-08-10T17:52:45.726164Z","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":"2026-08-10T17:52:45.731536Z","title":", year 2024 b","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.731536Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:8bba49a4849200e20ef0bb83444a1c49047ac9c8827dc5397915fd1bf8995d69","observation_id":"29c25d05-b469-4f9a-95ee-6331f62525a2","resolution":{"observed_at":"2026-08-10T17:52:45.731536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.10865","last_updated":"2024-12-12T09:24:21Z","snapshot_observed_at":"2026-08-11T15:06:43.175501Z","submitted_at":"2024-03-16T09:18:36Z","title":"On the Hubble expansion in a Big Bang quantum cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.10865","snapshot_observed_at":"2026-08-10T17:52:45.736965Z","title":", year 2025","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.736965Z"},"links":{"cited_paper":"/paper/2403.10865","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:58fbdfed546aaed8e882817175172dd58f14e1023b3ab7084512f2d788270407","observation_id":"5ebb2505-2334-40cc-9b26-5654b95d847b","resolution":{"observed_at":"2026-08-10T17:52:45.736965Z","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":"2026-08-10T17:52:45.742822Z","title":", author Wright , M.C.H","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.742822Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:eb7674f3c88f516d7018d1619d4a23a367bfbde8442941e30c0d674bf2811ed5","observation_id":"12e51da3-353b-400d-8971-303fef10de2f","resolution":{"observed_at":"2026-08-10T17:52:45.742822Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.00856","last_updated":"2019-11-04T16:36:34Z","snapshot_observed_at":"2026-08-07T22:17:13.167958Z","submitted_at":"2019-01-03T18:59:59Z","title":"The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Overview","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.00856","snapshot_observed_at":"2026-08-10T17:52:45.749102Z","title":", author Cappellari , M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.749102Z"},"links":{"cited_paper":"/paper/1901.00856","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:48eb75af0681d713b0666367409684e7a8b3072ab82ce5900936c1d61f35aed5","observation_id":"f74c9155-be3c-4e65-99ef-fbd3e7c08fea","resolution":{"observed_at":"2026-08-10T17:52:45.749102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.02745","last_updated":"2019-11-18T00:46:16Z","snapshot_observed_at":"2026-07-06T07:19:40.564502Z","submitted_at":"2018-12-06T19:00:00Z","title":"SDSS-IV MaStar -- A Large and Comprehensive Empirical Stellar Spectral Library: First Release","version":2},"cited_work":{"arxiv_id":"1812.02745","doi":null,"metadata_source":"pith","pith_arxiv_id":"1812.02745","snapshot_observed_at":"2026-08-10T17:52:46.112987Z","title":"SDSS-IV MaStar -- A Large and Comprehensive Empirical Stellar Spectral Library: First Release","venue":"astro-ph.IM","work_id":"d5b97697-77b4-441e-bb4a-616495f0243e","year":2018},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.755671Z"},"links":{"cited_paper":"/paper/1812.02745","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:789f4d438f02c7f478ccc2dcc358972acd676e530f63473177db9a9338430437","observation_id":"6e588d03-5c7f-4800-8e94-f0e6021b66d6","resolution":{"observed_at":"2026-08-10T17:52:46.120420Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.00671","last_updated":"2023-09-01T18:00:00Z","snapshot_observed_at":"2026-07-06T16:13:23.343694Z","submitted_at":"2023-09-01T18:00:00Z","title":"Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5","version":1},"cited_work":{"arxiv_id":"2309.00671","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.00671","snapshot_observed_at":"2026-08-10T17:52:46.082348Z","title":"Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5","venue":"astro-ph.GA","work_id":"8a3ab70d-e81a-443f-898f-265bc8e658b5","year":2023},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.762314Z"},"links":{"cited_paper":"/paper/2309.00671","citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:d7cb2618e7fc6f483953c94bd5f6f36ffaf7adc7787f6ea0c6b2ada8d77f9c84","observation_id":"a7cceaaa-7d9b-447c-9962-eade8b1fcfe3","resolution":{"observed_at":"2026-08-10T17:52:46.090576Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T17:52:45.767369Z","title":", author Charlot , S","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.767369Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:30f03fb39dace3ae6e8dec18681e4db30ec87c3b960f28e677ca7bbe86b82130","observation_id":"68214336-19cc-48dd-a912-029584dfca0f","resolution":{"observed_at":"2026-08-10T17:52:45.767369Z","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":"2026-08-10T17:52:45.773640Z","title":", year 1937","venue":null,"work_id":null,"year":1937},"citing_paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-10T17:52:45.773640Z"},"links":{"citing_paper":"/paper/2501.11882"},"observation_digest":"sha256:55153360eeaee80a503127d5c193216d6221bb82495c03b5dfcbfab70807b23f","observation_id":"a3ec0ad3-feef-4645-a070-1bf3c953570c","resolution":{"observed_at":"2026-08-10T17:52:45.773640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2501.11882","last_updated":"2025-01-21T04:30:54Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-11T05:25:28.516599Z","submitted_at":"2025-01-21T04:30:54Z","title":"Prospects for high-resolution probes of galaxy dynamics tracing background cosmology in MaNGA"},"reference_resolution":{"displayed":56,"state_counts":{"malformed_identifier":0,"metadata_mismatch":9,"parse_uncertain":0,"unresolved":42,"verified_exact":1,"verified_fuzzy":4},"total_outbound_references":56},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 56 of 56 outbound references and 0 inbound Pith citation observations for arXiv:2501.11882."}