{"as_of":"2026-08-07T18:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e671ce875265712831db9d73d5a9a19a33954e02b047f784f03d043bf8003bec","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T14:43:16.869771Z","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":"2026-05-14T18:47:36.776410Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1708.07750","last_updated":"2017-08-24T05:33:03Z","snapshot_observed_at":"2026-07-06T05:56:41.814255Z","submitted_at":"2017-08-24T05:33:03Z","title":"Improved constraints on the dark energy equation of state using Gaussian processes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.07750","snapshot_observed_at":"2026-08-05T14:43:16.869771Z","title":"Wang and X.-H","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.20971","last_updated":"2026-06-14T15:39:47Z","snapshot_observed_at":"2026-08-07T16:00:32.224666Z","submitted_at":"2025-08-28T16:25:22Z","title":"Cosmo-Learn: code for learning cosmology using different methods and mock data","version":2},"reference_index":134,"source":"pdf_text","source_observed_at":"2026-08-05T14:43:16.869771Z"},"links":{"cited_paper":"/paper/1708.07750","citing_paper":"/paper/2508.20971"},"observation_digest":"sha256:dcf439920f3a059a39e7b703bbdeeaa67ce6878787d0d221bf58dd92488c9e40","observation_id":"36b5480b-1b36-493c-bd73-642075775a06","resolution":{"observed_at":"2026-08-05T14:43:16.869771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.07750","last_updated":"2017-08-24T05:33:03Z","snapshot_observed_at":"2026-07-06T05:56:41.814255Z","submitted_at":"2017-08-24T05:33:03Z","title":"Improved constraints on the dark energy equation of state using Gaussian processes","version":1},"cited_work":{"arxiv_id":"1708.07750","doi":null,"metadata_source":"pith","pith_arxiv_id":"1708.07750","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Improved constraints on the dark energy equation of state using Gaussian processes","venue":"astro-ph.CO","work_id":"af967200-409c-4d9a-9d33-c27e00100451","year":2017},"citing_paper":{"arxiv_id":"2605.13427","last_updated":"2026-05-13T12:22:36Z","snapshot_observed_at":"2026-08-02T04:56:01.889215Z","submitted_at":"2026-05-13T12:22:36Z","title":"Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational \\(H(z)\\) Data","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-14T18:44:05.693005Z"},"links":{"cited_paper":"/paper/1708.07750","citing_paper":"/paper/2605.13427"},"observation_digest":"sha256:e6cdddcaf62fe2b89dd7ca26965b5773f7a8003b8e8081180f199e92f1cbab44","observation_id":"f1204465-951b-4873-bf78-8d0d631d2d95","resolution":{"observed_at":"2026-05-14T18:47:36.779209Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/1708.07750/citation-record","integrity":"/paper/1708.07750/integrity","json":"/paper/1708.07750/citation-record.json","paper":"/paper/1708.07750"},"outbound":[],"paper":{"arxiv_id":"1708.07750","last_updated":"2017-08-24T05:33:03Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T05:56:41.814255Z","submitted_at":"2017-08-24T05:33:03Z","title":"Improved constraints on the dark energy equation of state using Gaussian processes"},"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 2 inbound Pith citation observations for arXiv:1708.07750."}