{"as_of":"2026-08-05T23:51:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:afe6f63a20e326d65e7f8ae9a59c38f7e2bf73911ff1f88c9a2ae7099d0a5a3d","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":"2026-08-05T06:32:48.257954+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":"2026-08-02T00:50:14.890197Z","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":"2026-07-02T18:07:15.568388Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1606.02714","last_updated":"2017-05-24T16:06:04Z","snapshot_observed_at":"2026-07-06T04:59:17.326500Z","submitted_at":"2016-06-08T20:00:01Z","title":"Simulating the dust content of galaxies: successes and failures","version":2},"cited_work":{"arxiv_id":"1606.02714","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.02714","snapshot_observed_at":"2026-07-02T18:07:15.568388Z","title":"Simulating the dust content of galaxies: successes and failures","venue":"astro-ph.GA","work_id":"a9a193bd-9bd8-40d8-bcfe-2164d23ff5c7","year":2016},"citing_paper":{"arxiv_id":"2605.15310","last_updated":"2026-08-03T10:20:27Z","snapshot_observed_at":"2026-08-05T23:29:19.963660Z","submitted_at":"2026-05-14T18:23:08Z","title":"Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization","version":1},"reference_index":154,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1606.02714","citing_paper":"/paper/2605.15310"},"observation_digest":"sha256:eea74f04f15c6431e40381712ee4d390a61c51fd5d927e6ae5ccecf4f72f328f","observation_id":"83fc01d5-a2c6-46df-aebe-c49f7768860e","resolution":{"observed_at":"2026-05-19T16:17:39.038496Z","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":"1606.02714","last_updated":"2017-05-24T16:06:04Z","snapshot_observed_at":"2026-07-06T04:59:17.326500Z","submitted_at":"2016-06-08T20:00:01Z","title":"Simulating the dust content of galaxies: successes and failures","version":2},"cited_work":{"arxiv_id":"1606.02714","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.02714","snapshot_observed_at":"2026-07-02T18:07:15.568388Z","title":"Simulating the dust content of galaxies: successes and failures","venue":"astro-ph.GA","work_id":"a9a193bd-9bd8-40d8-bcfe-2164d23ff5c7","year":2016},"citing_paper":{"arxiv_id":"2605.19661","last_updated":"2026-05-20T11:06:21Z","snapshot_observed_at":"2026-07-06T23:30:21.283826Z","submitted_at":"2026-05-19T10:55:34Z","title":"COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12","version":1},"reference_index":111,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1606.02714","citing_paper":"/paper/2605.19661"},"observation_digest":"sha256:4e6a860c0af596a51d66fd52e60740ea2ca42df511f245467ee2bc22a0bc8c45","observation_id":"91e86716-b659-4bb8-a350-ee86d48c3ba4","resolution":{"observed_at":"2026-05-20T03:58:02.295263Z","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":"1606.02714","last_updated":"2017-05-24T16:06:04Z","snapshot_observed_at":"2026-07-06T04:59:17.326500Z","submitted_at":"2016-06-08T20:00:01Z","title":"Simulating the dust content of galaxies: successes and failures","version":2},"cited_work":{"arxiv_id":"1606.02714","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.02714","snapshot_observed_at":"2026-07-02T18:07:15.568388Z","title":"Simulating the dust content of galaxies: successes and failures","venue":"astro-ph.GA","work_id":"a9a193bd-9bd8-40d8-bcfe-2164d23ff5c7","year":2016},"citing_paper":{"arxiv_id":"2605.19661","last_updated":"2026-05-20T11:06:21Z","snapshot_observed_at":"2026-07-06T23:30:21.283826Z","submitted_at":"2026-05-19T10:55:34Z","title":"COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12","version":2},"reference_index":111,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1606.02714","citing_paper":"/paper/2605.19661"},"observation_digest":"sha256:8e139f425d20c610aa82758db0d22ba2e8aa3bdf0d5a8c8644f2dfe59e63e3c2","observation_id":"6e98f88d-c650-422b-9796-7a54ed8a38a1","resolution":{"observed_at":"2026-05-21T07:49:49.312094Z","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":"1606.02714","last_updated":"2017-05-24T16:06:04Z","snapshot_observed_at":"2026-07-06T04:59:17.326500Z","submitted_at":"2016-06-08T20:00:01Z","title":"Simulating the dust content of galaxies: successes and failures","version":2},"cited_work":{"arxiv_id":"1606.02714","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.02714","snapshot_observed_at":"2026-07-02T18:07:15.568388Z","title":"Simulating the dust content of galaxies: successes and failures","venue":"astro-ph.GA","work_id":"a9a193bd-9bd8-40d8-bcfe-2164d23ff5c7","year":2016},"citing_paper":{"arxiv_id":"2606.06108","last_updated":"2026-06-04T12:53:53Z","snapshot_observed_at":"2026-07-06T23:46:01.165261Z","submitted_at":"2026-06-04T12:53:53Z","title":"Grain-size evolution and rapid dust growth in high-redshift galaxies","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1606.02714","citing_paper":"/paper/2606.06108"},"observation_digest":"sha256:46aed6e1d8718c182224f80694260a771440b4f6a9c835ff3d532cc3a1e301a5","observation_id":"ce46e307-425c-481f-a627-dec43aa1cb26","resolution":{"observed_at":"2026-06-28T00:51:27.413586Z","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":"1606.02714","last_updated":"2017-05-24T16:06:04Z","snapshot_observed_at":"2026-07-06T04:59:17.326500Z","submitted_at":"2016-06-08T20:00:01Z","title":"Simulating the dust content of galaxies: successes and failures","version":2},"cited_work":{"arxiv_id":"1606.02714","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.02714","snapshot_observed_at":"2026-07-02T18:07:15.568388Z","title":"Simulating the dust content of galaxies: successes and failures","venue":"astro-ph.GA","work_id":"a9a193bd-9bd8-40d8-bcfe-2164d23ff5c7","year":2016},"citing_paper":{"arxiv_id":"2607.00165","last_updated":"2026-06-30T20:43:49Z","snapshot_observed_at":"2026-08-04T00:17:29.176666Z","submitted_at":"2026-06-30T20:43:49Z","title":"Far-infrared observations of dust in Ly$\\alpha$ emitters at z=2-6","version":1},"reference_index":171,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1606.02714","citing_paper":"/paper/2607.00165"},"observation_digest":"sha256:2a9ccdd39400b22ad16b3f21518e37b8ba9152c24d859e2b11a842c9d4e250f6","observation_id":"50916350-b69b-45df-8fa3-ab76f46057fd","resolution":{"observed_at":"2026-07-02T18:07:15.569651Z","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":"1606.02714","last_updated":"2017-05-24T16:06:04Z","snapshot_observed_at":"2026-07-06T04:59:17.326500Z","submitted_at":"2016-06-08T20:00:01Z","title":"Simulating the dust content of galaxies: successes and failures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.02714","snapshot_observed_at":"2026-07-14T05:32:07.775931Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11448","last_updated":"2026-07-13T11:59:50Z","snapshot_observed_at":"2026-07-16T23:19:47.905536Z","submitted_at":"2026-07-13T11:59:50Z","title":"Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster","version":1},"reference_index":112,"source":"arxiv_source","source_observed_at":"2026-07-14T05:32:07.775931Z"},"links":{"cited_paper":"/paper/1606.02714","citing_paper":"/paper/2607.11448"},"observation_digest":"sha256:683decf5f0f5d2f7bba7a12f533d0edbc09f39c04007822d8a01fada9eff1e6a","observation_id":"9195f06a-a367-48a6-81dc-4abb31a37c60","resolution":{"observed_at":"2026-07-14T05:32:07.775931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.02714","last_updated":"2017-05-24T16:06:04Z","snapshot_observed_at":"2026-07-06T04:59:17.326500Z","submitted_at":"2016-06-08T20:00:01Z","title":"Simulating the dust content of galaxies: successes and failures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.02714","snapshot_observed_at":"2026-08-02T00:50:14.890197Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14901","last_updated":"2026-07-16T12:17:52Z","snapshot_observed_at":"2026-08-04T23:31:36.964662Z","submitted_at":"2026-07-16T12:17:52Z","title":"The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-02T00:50:14.890197Z"},"links":{"cited_paper":"/paper/1606.02714","citing_paper":"/paper/2607.14901"},"observation_digest":"sha256:ab9a29e405bc33d78342496e2391eb7310e3490a4302ea61606b7db6bfaa6930","observation_id":"0f6f4679-29d6-4051-a2b1-4779ed0ab395","resolution":{"observed_at":"2026-08-02T00:50:14.890197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1606.02714/citation-record","integrity":"/paper/1606.02714/integrity","json":"/paper/1606.02714/citation-record.json","paper":"/paper/1606.02714"},"outbound":[],"paper":{"arxiv_id":"1606.02714","last_updated":"2017-05-24T16:06:04Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T04:59:17.326500Z","submitted_at":"2016-06-08T20:00:01Z","title":"Simulating the dust content of galaxies: successes and failures"},"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 7 inbound Pith citation observations for arXiv:1606.02714."}