{"as_of":"2026-08-05T06:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f28b74d26008e0c3b4078dd52005b4aef10feeefc410583b755ff2a006101bbc","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T00:45:31.648844Z","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":"2026-06-26T17:19:35.759227Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-08-02T18:02:44.161768Z","title":"XL VIII,Planck intermediate results","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.17799","last_updated":"2026-07-21T06:40:21Z","snapshot_observed_at":"2026-08-04T20:20:28.931349Z","submitted_at":"2026-03-18T14:55:13Z","title":"Enhanced foreground mitigation in thermal SZ Compton-$y$ maps via polarization and deprojection","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-02T18:02:44.161768Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2603.17799"},"observation_digest":"sha256:51b30f6e53fba4058f6ae7c2d6e04e79bcc2dea0fa16d15ac0c009f07986a476","observation_id":"d717fbc9-2f26-41aa-9d4e-a2fa8476c0a2","resolution":{"observed_at":"2026-08-02T18:02:44.161768Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":"1605.09387","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-06-26T17:19:35.759227Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","venue":"astro-ph.CO","work_id":"a6f21e54-d7d1-490a-a570-aaffe4630552","year":2016},"citing_paper":{"arxiv_id":"2604.14088","last_updated":"2026-04-20T14:26:52Z","snapshot_observed_at":"2026-07-06T23:01:55.698452Z","submitted_at":"2026-04-15T17:04:26Z","title":"BROOM: a python package for model-independent analysis of microwave astronomical data","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-10T12:30:31.484944Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2604.14088"},"observation_digest":"sha256:95285e5fc03ac86cac3a73b48e3bc949ca6c9c34bb2046071bd7157c97f4cf6a","observation_id":"ee3db1e3-d5ea-4cbb-9080-c062d75dcaf0","resolution":{"observed_at":"2026-05-11T11:51:02.397969Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":"1605.09387","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-06-26T17:19:35.759227Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","venue":"astro-ph.CO","work_id":"a6f21e54-d7d1-490a-a570-aaffe4630552","year":2016},"citing_paper":{"arxiv_id":"2605.03783","last_updated":"2026-05-05T14:09:38Z","snapshot_observed_at":"2026-07-06T23:16:40.201701Z","submitted_at":"2026-05-05T14:09:38Z","title":"New constraints on primordial non-Gaussianity from large-scale cross-correlations of CMB lensing and the cosmic infrared background","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-05-07T13:37:14.763193Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2605.03783"},"observation_digest":"sha256:8180c057b1d6975b739133581cc4b095144e536721989bd912e2263dc3d16601","observation_id":"f4bf4537-65d4-4b27-87c5-951bc1041008","resolution":{"observed_at":"2026-05-12T08:51:25.041299Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":"1605.09387","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-06-26T17:19:35.759227Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","venue":"astro-ph.CO","work_id":"a6f21e54-d7d1-490a-a570-aaffe4630552","year":2016},"citing_paper":{"arxiv_id":"2605.18938","last_updated":"2026-05-18T17:59:32Z","snapshot_observed_at":"2026-07-06T23:29:42.583875Z","submitted_at":"2026-05-18T17:59:32Z","title":"First detection of the moving lens effect with ACT and DESI LS","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-20T08:46:08.699588Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2605.18938"},"observation_digest":"sha256:94e3c620b7a3ea3d117d71aca7ce4ff0ec9b6abf2e79c85137d7043485c1689b","observation_id":"7b8872ff-7dfa-4944-8714-2c21d176dc80","resolution":{"observed_at":"2026-05-20T08:48:09.179719Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":"1605.09387","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-06-26T17:19:35.759227Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","venue":"astro-ph.CO","work_id":"a6f21e54-d7d1-490a-a570-aaffe4630552","year":2016},"citing_paper":{"arxiv_id":"2606.19694","last_updated":"2026-06-18T01:46:44Z","snapshot_observed_at":"2026-08-03T08:44:53.896326Z","submitted_at":"2026-06-18T01:46:44Z","title":"PMO Polaris CO survey. II. Where is the dust?","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2606.19694"},"observation_digest":"sha256:bad52c8a07f58494608346f960542f4d6bd004fe69c395580e512511fe77a36d","observation_id":"7bcde8be-0e35-46d3-ad84-df78d3b18483","resolution":{"observed_at":"2026-06-26T17:19:35.761813Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":"1605.09387","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-06-26T17:19:35.759227Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","venue":"astro-ph.CO","work_id":"a6f21e54-d7d1-490a-a570-aaffe4630552","year":2016},"citing_paper":{"arxiv_id":"2606.26576","last_updated":"2026-06-25T03:52:30Z","snapshot_observed_at":"2026-07-07T00:00:56.276365Z","submitted_at":"2026-06-25T03:52:30Z","title":"Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor","version":1},"reference_index":225,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2606.26576"},"observation_digest":"sha256:f1d9ef49fe2dfea8f2cba85fb3916cde3c9ef16c1b7ac1de784eaa7900f0d1b6","observation_id":"94a79dd8-572b-485a-b6f2-7168a63d4a7e","resolution":{"observed_at":"2026-06-26T04:28:58.871166Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":"1605.09387","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-06-26T17:19:35.759227Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","venue":"astro-ph.CO","work_id":"a6f21e54-d7d1-490a-a570-aaffe4630552","year":2016},"citing_paper":{"arxiv_id":"2606.27244","last_updated":"2026-06-25T16:31:55Z","snapshot_observed_at":"2026-07-07T00:01:29.987067Z","submitted_at":"2026-06-25T16:31:55Z","title":"Methodological Frontiers in 21-cm Intensity Mapping: the Treatment of Systematics and Foreground Contamination","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2606.27244"},"observation_digest":"sha256:c018e163f77d5f42ba1d12880d7195005dfc5c2c75f00a267a8c6d840071ad24","observation_id":"31fc387a-4684-42c3-8f30-3efb139c8590","resolution":{"observed_at":"2026-06-26T03:48:57.324091Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-07-12T04:17:05.392304Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03185","last_updated":"2026-07-03T10:43:50Z","snapshot_observed_at":"2026-07-12T04:17:02.531167Z","submitted_at":"2026-07-03T10:43:50Z","title":"DHARA: Data Handling and Automated Reduction pipeline for AIMPOL","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-12T04:17:05.392304Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2607.03185"},"observation_digest":"sha256:1c094d39ad383bdc4d8de32775f6c4cdca213d684666cc2dda5d9926ac66e4c8","observation_id":"8c92e9fe-de35-4c47-8011-94f432eec45a","resolution":{"observed_at":"2026-07-12T04:17:05.392304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-07-14T04:54:13.013192Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11539","last_updated":"2026-07-13T13:23:31Z","snapshot_observed_at":"2026-08-04T04:21:20.548931Z","submitted_at":"2026-07-13T13:23:31Z","title":"Two Earliest Optical-UV Tidal Disruption Events Hidden in the SDSS DR7 Catalog Unveiled by the Transformer-Based Spectrum Classifier","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-07-14T04:54:13.013192Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2607.11539"},"observation_digest":"sha256:cfa9062a7f4218d6be667b9ec3e8ca191c7744696df40f161b99747e5c61a6ef","observation_id":"5ef8d1a5-e02c-4305-97e9-e47695a3a47e","resolution":{"observed_at":"2026-07-14T04:54:13.013192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.09387","snapshot_observed_at":"2026-08-03T00:45:31.648844Z","title":"Aghanim, M","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.28712","last_updated":"2026-07-30T17:59:02Z","snapshot_observed_at":"2026-08-05T06:14:07.864718Z","submitted_at":"2026-07-30T17:59:02Z","title":"Single Frequency CMB Foreground Removal with Inter-scale Machine Learning","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-03T00:45:31.648844Z"},"links":{"cited_paper":"/paper/1605.09387","citing_paper":"/paper/2607.28712"},"observation_digest":"sha256:2771d2cd72554485c14bb51c23767626b0c0e40bb0a0623cdee31c3ecabe4229","observation_id":"6bcd7193-a644-486a-88bf-2e8c36d15eef","resolution":{"observed_at":"2026-08-03T00:45:31.648844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1605.09387/citation-record","integrity":"/paper/1605.09387/integrity","json":"/paper/1605.09387/citation-record.json","paper":"/paper/1605.09387"},"outbound":[],"paper":{"arxiv_id":"1605.09387","last_updated":"2016-08-09T18:55:34Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-31T04:22:46.026188Z","submitted_at":"2016-05-30T20:00:03Z","title":"Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:1605.09387."}