{"as_of":"2026-08-07T21:21:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a8d866eddeb95b42610bd352fd5b3df2a745533bc07da86da738bf5c816bd127","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-14T07:24:53.781826Z","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":"2026-06-27T06:30:37.921066Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1801.07368","last_updated":"2018-01-23T01:50:34Z","snapshot_observed_at":"2026-07-06T06:19:46.086643Z","submitted_at":"2018-01-23T01:50:34Z","title":"Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem","version":1},"cited_work":{"arxiv_id":"1801.07368","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.07368","snapshot_observed_at":"2026-06-27T06:30:37.921066Z","title":"Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem","venue":"astro-ph.GA","work_id":"e0847413-aaea-49bf-ae21-64a3fba8cb81","year":2018},"citing_paper":{"arxiv_id":"2606.13393","last_updated":"2026-06-11T14:24:11Z","snapshot_observed_at":"2026-07-06T23:52:09.853158Z","submitted_at":"2026-06-11T14:24:11Z","title":"Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$","version":1},"reference_index":186,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1801.07368","citing_paper":"/paper/2606.13393"},"observation_digest":"sha256:1ea225c3f68672c7b19f77e3a9fe2739f63e661fb2ee77488397e112e09c4cfb","observation_id":"516ce5ea-2c20-4005-8db9-6a21a05a6560","resolution":{"observed_at":"2026-06-27T06:30:37.923106Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.07368","last_updated":"2018-01-23T01:50:34Z","snapshot_observed_at":"2026-07-06T06:19:46.086643Z","submitted_at":"2018-01-23T01:50:34Z","title":"Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem","version":1},"cited_work":{"arxiv_id":"1801.07368","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.07368","snapshot_observed_at":"2026-06-27T06:30:37.921066Z","title":"Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem","venue":"astro-ph.GA","work_id":"e0847413-aaea-49bf-ae21-64a3fba8cb81","year":2018},"citing_paper":{"arxiv_id":"2606.23790","last_updated":"2026-06-22T18:00:02Z","snapshot_observed_at":"2026-08-02T09:54:14.762872Z","submitted_at":"2026-06-22T18:00:02Z","title":"Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters","version":1},"reference_index":258,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1801.07368","citing_paper":"/paper/2606.23790"},"observation_digest":"sha256:847f282da13add65c6e93d2f5268dd54124090588a4c56fc7f9c60cca253fee2","observation_id":"79a8eb1b-f4f6-42e0-ac06-938f42aa33aa","resolution":{"observed_at":"2026-06-26T07:59:08.843347Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.07368","last_updated":"2018-01-23T01:50:34Z","snapshot_observed_at":"2026-07-06T06:19:46.086643Z","submitted_at":"2018-01-23T01:50:34Z","title":"Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.07368","snapshot_observed_at":"2026-07-11T06:23:06.110361Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05523","last_updated":"2026-07-06T18:01:40Z","snapshot_observed_at":"2026-08-03T16:38:10.592186Z","submitted_at":"2026-07-06T18:01:40Z","title":"BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\\simeq5.23$","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-07-11T06:23:06.110361Z"},"links":{"cited_paper":"/paper/1801.07368","citing_paper":"/paper/2607.05523"},"observation_digest":"sha256:db5de9c09cc4d8a3e1f3157bdcce10aafa37d2c1fcbd83772d9fc383b4672739","observation_id":"d3a16bda-ffee-45c7-aa6b-e4a3d1153275","resolution":{"observed_at":"2026-07-11T06:23:06.110361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.07368","last_updated":"2018-01-23T01:50:34Z","snapshot_observed_at":"2026-07-06T06:19:46.086643Z","submitted_at":"2018-01-23T01:50:34Z","title":"Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.07368","snapshot_observed_at":"2026-07-14T07:24:53.781826Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11049","last_updated":"2026-07-13T03:24:10Z","snapshot_observed_at":"2026-08-06T01:09:56.658799Z","submitted_at":"2026-07-13T03:24:10Z","title":"Gravitationally Lensed View of DSFG-1 in PLCK G165.7+67.0: Strong Dust Emission and Spatially Resolved Stellar Population Analysis with JWST and SMA","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-14T07:24:53.781826Z"},"links":{"cited_paper":"/paper/1801.07368","citing_paper":"/paper/2607.11049"},"observation_digest":"sha256:7c5767c343c012f6a958d87bb549c982f6912e39933ad7c5e9040f84238632d4","observation_id":"783923b9-3b0c-4e08-86fd-3b64a2bc0da2","resolution":{"observed_at":"2026-07-14T07:24:53.781826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1801.07368/citation-record","integrity":"/paper/1801.07368/integrity","json":"/paper/1801.07368/citation-record.json","paper":"/paper/1801.07368"},"outbound":[],"paper":{"arxiv_id":"1801.07368","last_updated":"2018-01-23T01:50:34Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T06:19:46.086643Z","submitted_at":"2018-01-23T01:50:34Z","title":"Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1801.07368."}