{"as_of":"2026-08-15T07:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e272d81e958adc9269d27280a87b207fd9d7bec508cd056976b3f6c498ebc298","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T00:16:22.364747Z","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":"2026-07-10T13:17:05.178189Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2006.08638","last_updated":"2020-06-15T18:00:06Z","snapshot_observed_at":"2026-08-14T00:42:24.134949Z","submitted_at":"2020-06-15T18:00:06Z","title":"The Data Processing Pipeline for the MUSE Instrument","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.08638","snapshot_observed_at":"2026-08-06T16:20:15.074944Z","title":", author Palsa , R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.13979","last_updated":"2025-07-18T14:43:04Z","snapshot_observed_at":"2026-08-13T11:55:29.353457Z","submitted_at":"2025-07-18T14:43:04Z","title":"Recent Chemo-morphological Coma Evolution of Comet 67P/Churyumov-Gerasimenko","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-06T16:20:15.074944Z"},"links":{"cited_paper":"/paper/2006.08638","citing_paper":"/paper/2507.13979"},"observation_digest":"sha256:0b67a5ab9213aa604b1101d33a0323728ac5447aff37f2743223a512e56c981b","observation_id":"f36e1e67-944e-4590-92ee-e56b904ba1d0","resolution":{"observed_at":"2026-08-06T16:20:15.074944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.08638","last_updated":"2020-06-15T18:00:06Z","snapshot_observed_at":"2026-08-14T00:42:24.134949Z","submitted_at":"2020-06-15T18:00:06Z","title":"The Data Processing Pipeline for the MUSE Instrument","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.08638","snapshot_observed_at":"2026-08-06T14:34:10.682503Z","title":"M., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.18347","last_updated":"2025-07-24T12:19:38Z","snapshot_observed_at":"2026-08-13T17:45:19.476003Z","submitted_at":"2025-07-24T12:19:38Z","title":"The PyKOALA python library: a multi-instrument package for IFS data reduction","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-06T14:34:10.682503Z"},"links":{"cited_paper":"/paper/2006.08638","citing_paper":"/paper/2507.18347"},"observation_digest":"sha256:9ed39515b134de0e5c27d458dc997863615eb0d460d625516d1f8087a5df14a2","observation_id":"d24fb9a4-d6ae-4ba5-a151-001812e62c15","resolution":{"observed_at":"2026-08-06T14:34:10.682503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.08638","last_updated":"2020-06-15T18:00:06Z","snapshot_observed_at":"2026-08-14T00:42:24.134949Z","submitted_at":"2020-06-15T18:00:06Z","title":"The Data Processing Pipeline for the MUSE Instrument","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.08638","snapshot_observed_at":"2026-07-12T09:34:56.798673Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.00408","last_updated":"2026-07-08T15:04:19Z","snapshot_observed_at":"2026-08-13T06:10:57.772187Z","submitted_at":"2026-07-01T04:05:56Z","title":"Exploring the synergies of $[\\mathrm{O\\,II}]\\lambda 3727$ with MUSE spectroscopy in PHANGS H II regions","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-12T09:34:56.798673Z"},"links":{"cited_paper":"/paper/2006.08638","citing_paper":"/paper/2607.00408"},"observation_digest":"sha256:9601c0fddc362e61eb26360c40925ef04b9ae5921c609f41b5304a5dbaea8d25","observation_id":"bfcc6287-168c-4b25-a62e-3326dd545b46","resolution":{"observed_at":"2026-07-12T09:34:56.798673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.08638","last_updated":"2020-06-15T18:00:06Z","snapshot_observed_at":"2026-08-14T00:42:24.134949Z","submitted_at":"2020-06-15T18:00:06Z","title":"The Data Processing Pipeline for the MUSE Instrument","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.08638","snapshot_observed_at":"2026-07-11T09:01:37.245115Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.05087","last_updated":"2026-07-06T13:49:22Z","snapshot_observed_at":"2026-08-13T23:08:39.564087Z","submitted_at":"2026-07-06T13:49:22Z","title":"Lyman-alpha haloes in the aftermath of reionisation","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-11T09:01:37.245115Z"},"links":{"cited_paper":"/paper/2006.08638","citing_paper":"/paper/2607.05087"},"observation_digest":"sha256:730db34f9c795267a112fc4d9b0fb072034c5adebd6d2847c2217f438d86bb8f","observation_id":"4b675d64-bb66-4e8c-a1fc-b8ba11b01216","resolution":{"observed_at":"2026-07-11T09:01:37.245115Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.08638","last_updated":"2020-06-15T18:00:06Z","snapshot_observed_at":"2026-08-14T00:42:24.134949Z","submitted_at":"2020-06-15T18:00:06Z","title":"The Data Processing Pipeline for the MUSE Instrument","version":1},"cited_work":{"arxiv_id":"2006.08638","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.08638","snapshot_observed_at":"2026-07-10T13:17:05.178189Z","title":"The Data Processing Pipeline for the MUSE Instrument","venue":"astro-ph.IM","work_id":"0d8dae11-2401-4853-bf77-53594318216c","year":2020},"citing_paper":{"arxiv_id":"2607.08090","last_updated":"2026-07-09T03:55:45Z","snapshot_observed_at":"2026-08-02T13:57:46.281635Z","submitted_at":"2026-07-09T03:55:45Z","title":"Multi-wavelength Constraints on the Transient EP250905a","version":1},"reference_index":186,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2006.08638","citing_paper":"/paper/2607.08090"},"observation_digest":"sha256:2ffe74dadad7308b2354ef2c327a953be00fe4d49821f285ebab662ac55ba67b","observation_id":"26fef3bf-5b17-40d2-bbb5-b4b7a49b875a","resolution":{"observed_at":"2026-07-10T13:17:05.179894Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.08638","last_updated":"2020-06-15T18:00:06Z","snapshot_observed_at":"2026-08-14T00:42:24.134949Z","submitted_at":"2020-06-15T18:00:06Z","title":"The Data Processing Pipeline for the MUSE Instrument","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.08638","snapshot_observed_at":"2026-08-01T12:43:57.838526Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":192,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.838526Z"},"links":{"cited_paper":"/paper/2006.08638","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:115da9598c5c7ed7df9b6292cd3ebd173d88bd27b34698683f8c32c5ce833422","observation_id":"58576ec7-98c4-438b-b19d-64725ae37d62","resolution":{"observed_at":"2026-08-01T12:43:57.838526Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.08638","last_updated":"2020-06-15T18:00:06Z","snapshot_observed_at":"2026-08-14T00:42:24.134949Z","submitted_at":"2020-06-15T18:00:06Z","title":"The Data Processing Pipeline for the MUSE Instrument","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.08638","snapshot_observed_at":"2026-08-12T00:16:22.364747Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.08275","last_updated":"2026-08-08T18:10:02Z","snapshot_observed_at":"2026-08-15T06:54:21.448694Z","submitted_at":"2026-08-08T18:10:02Z","title":"The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-12T00:16:22.364747Z"},"links":{"cited_paper":"/paper/2006.08638","citing_paper":"/paper/2608.08275"},"observation_digest":"sha256:e848132fad1d17dd90712fb98c1c9aa3596ec28682ad58b21614233f2ebe8980","observation_id":"27ced7d6-f2c8-43fe-8a22-398b23ead92c","resolution":{"observed_at":"2026-08-12T00:16:22.364747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2006.08638/citation-record","integrity":"/paper/2006.08638/integrity","json":"/paper/2006.08638/citation-record.json","paper":"/paper/2006.08638"},"outbound":[],"paper":{"arxiv_id":"2006.08638","last_updated":"2020-06-15T18:00:06Z","latest_version":1,"primary_category":"astro-ph.IM","snapshot_observed_at":"2026-08-14T00:42:24.134949Z","submitted_at":"2020-06-15T18:00:06Z","title":"The Data Processing Pipeline for the MUSE Instrument"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2006.08638."}