{"as_of":"2026-08-12T08:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:95172c34247fb9c8dc6567fa540986b93e400bb49b8e06e1b4fc856059ad73ed","coverage":[{"denominator":13,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T13:42:15.021061Z","state":"measured"},{"denominator":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:16:05.246042Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-07T15:16:09.131803Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"cited_work":{"arxiv_id":"2501.16192","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.16192","snapshot_observed_at":"2026-08-07T15:16:09.131803Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","venue":"astro-ph.GA","work_id":"da433497-a4bc-4e56-8b6d-5248738d2b31","year":2025},"citing_paper":{"arxiv_id":"2505.15910","last_updated":"2025-05-21T18:03:48Z","snapshot_observed_at":"2026-08-09T23:01:09.401904Z","submitted_at":"2025-05-21T18:03:48Z","title":"GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-07T15:16:05.246042Z"},"links":{"cited_paper":"/paper/2501.16192","citing_paper":"/paper/2505.15910"},"observation_digest":"sha256:4760ccde46c32299b9af9c89a8273d0527dc90a22278c931a6e09003e1e4e627","observation_id":"307a603f-8d88-47da-b01e-1539af5fe8f4","resolution":{"observed_at":"2026-08-07T15:16:09.214135Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2501.16192/citation-record","integrity":"/paper/2501.16192/integrity","json":"/paper/2501.16192/citation-record.json","paper":"/paper/2501.16192"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1710.03554","last_updated":"2017-10-10T13:03:12Z","snapshot_observed_at":"2026-07-06T06:03:31.798281Z","submitted_at":"2017-10-10T13:03:12Z","title":"MPDAF - A Python package for the analysis of VLT/MUSE data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.03554","snapshot_observed_at":"2026-08-10T13:42:14.967342Z","title":"Federico II","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:14.967342Z"},"links":{"cited_paper":"/paper/1710.03554","citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:f227a03e8c2b3b463bb1674e0e4e4ad60df73789aef281ffc08a4f28079169d1","observation_id":"2fd2ecc9-f7e6-4ba9-b995-653f943960f8","resolution":{"observed_at":"2026-08-10T13:42:14.967342Z","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":"2026-08-10T13:42:15.157774Z","title":"For conve- nience, the top axis shows the approximate distance to NGC 3314A","venue":null,"work_id":"f6bb38ed-c0b5-43d0-b6cc-e4848641cce4","year":2024},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:14.993151Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:4a173e819649631ce9ecafcae41c7c98060ccfe87833518274248fcb0acc46bb","observation_id":"523dd689-263d-4a9b-ab04-a178ed0cecf2","resolution":{"observed_at":"2026-08-10T13:42:15.161934Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.131963Z","title":"LEWIS_udg32_arxiv with narrower wavelength range (6200 ≤ λobs ≤ 7000 Å) and slightly higher SNR (≈ 3.5)","venue":null,"work_id":"4c63c3d4-f450-4249-917a-f538356167b5","year":2021},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:15.001582Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:220fa2ad2b7c5fbb610f065b03414d76fa99ed4916924439bb0954bda3cd1243","observation_id":"a8647fd0-296e-4ff0-ac2c-82da8d687a99","resolution":{"observed_at":"2026-08-10T13:42:15.136094Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.180603Z","title":"We follow the methodology in Iodice et al","venue":null,"work_id":"92c0366b-487c-44d9-81a3-d76b4c9256ae","year":2021},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:14.985395Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:ac2ca43e95b677c29b1174781c689697933c2bac62c691a408ab69f3be1c2bf6","observation_id":"33f8ff48-57b7-4856-ad56-fed3aa4317c2","resolution":{"observed_at":"2026-08-10T13:42:15.184490Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.144663Z","title":"wild bootstrapping","venue":null,"work_id":"c8254e7b-a63c-44bb-97bc-c9a2d2e8ea14","year":2018},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:14.996957Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:2c5e7d778c54e0e787f702110bd6fde1ed5a64c03c2a7db1644a60e192d88bd6","observation_id":"52e6f2f7-2775-4c72-809e-ae15efaf67e1","resolution":{"observed_at":"2026-08-10T13:42:15.149032Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.101436Z","title":"We fit the SSP models to background-subtracted spectra extracted from 8-pixel circular apertures","venue":null,"work_id":"c1adab38-3970-49ef-accb-0b6d3e1e5620","year":2023},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:15.012229Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:d8f4d16e94d593810bcfe041f5cfd21394263277b29c2478fcbe2dc10f5e37f4","observation_id":"65be3dbe-dc4e-4104-bd3c-309adfba0f71","resolution":{"observed_at":"2026-08-10T13:42:15.107199Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.069007Z","title":"The left panel of Fig","venue":null,"work_id":"dc41e11b-64c1-4c34-ba1a-e93c6b21b62d","year":2013},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:15.021061Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:92cde076b5f1162a0bc3c9ed5ad667640a208faf8ee9c6332c64660c22f49c0c","observation_id":"8849d572-e967-4c96-9940-b94026cddb66","resolution":{"observed_at":"2026-08-10T13:42:15.073863Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.220772Z","title":"45\" 43'00","venue":null,"work_id":"3a197489-d997-4762-9927-40f5f4120076","year":2021},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:14.973214Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:3914f6589ed0a9606ba481a1dd47c589f08789d9cc076e6b5e9a350b7af75677","observation_id":"45b92019-4898-47a1-8742-700b8c3006c1","resolution":{"observed_at":"2026-08-10T13:42:15.224962Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.083939Z","title":"We use the inbuilt exponentially declining star-formation history (SFH) parametrised byτ, the timescale for the SF decrease and T0, the time since the SF began","venue":null,"work_id":"3b409e55-04ae-4de5-9279-6bfef5a3fd93","year":2002},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":2003,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:15.016001Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:e4833bf7e3d719ee59dbd163a50cf53ed2aa061cad650f03de1e000b9fcd7779","observation_id":"5f162ff2-5776-4d1f-9793-104934f0798b","resolution":{"observed_at":"2026-08-10T13:42:15.089300Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.169136Z","title":"However, Iodice et al","venue":null,"work_id":"2dccb6c4-0f66-4ca6-bacb-a51d4111131f","year":2021},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":2007,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:14.989043Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:30612c770286b6f8d75ec9dddbb02aafe3ab3972f595ecbaa24337659d033801","observation_id":"20d9ab01-c556-4979-b99f-32852c2f9b91","resolution":{"observed_at":"2026-08-10T13:42:15.172966Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.193108Z","title":"These data (PI: R","venue":null,"work_id":"0ce6270a-4bac-43ff-9e68-bd868f227d94","year":2022},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":2015,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:14.981207Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:682db99e9e8894e59e67b8bd838d18cae1ad1061f4f0149e9d0a815dc33ee6a5","observation_id":"502dabcb-1763-4d4c-8d1c-ebf73d0ee3b3","resolution":{"observed_at":"2026-08-10T13:42:15.197187Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.115671Z","title":"(2020) and correcting for the contamination of foreground stars, back- ground stars, and the presence of intra-cluster GCs","venue":null,"work_id":"1024bd7b-b028-421e-881e-07c2b75e7dcc","year":2020},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":2020,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:15.006266Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:c293f6fa360c8cf06fc53e505516a9661da5609846af2397e8edb8e1d8251c3f","observation_id":"0dcc5116-c618-4540-898b-f495f6de052b","resolution":{"observed_at":"2026-08-10T13:42:15.121424Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:42:15.206948Z","title":null,"venue":null,"work_id":"0fa75644-077a-4e1e-b2a6-8a33da9897ff","year":2022},"citing_paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data","version":1},"reference_index":8000,"source":"pdf_text","source_observed_at":"2026-08-10T13:42:14.977349Z"},"links":{"citing_paper":"/paper/2501.16192"},"observation_digest":"sha256:8a26bd9a0b86fe99e1aa6b43586f869e813082db4df6e6e3861d85b3810a751e","observation_id":"bd107e84-6391-4859-9307-88979994b4ac","resolution":{"observed_at":"2026-08-10T13:42:15.210985Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2501.16192","last_updated":"2025-01-27T16:45:41Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-10T13:34:30.722303Z","submitted_at":"2025-01-27T16:45:41Z","title":"Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data"},"reference_resolution":{"displayed":13,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":2,"verified_exact":0,"verified_fuzzy":10},"total_outbound_references":13},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 13 of 13 outbound references and 1 inbound Pith citation observation for arXiv:2501.16192."}