{"as_of":"2026-08-10T02:39:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0720b4454884abc0af9ac50a893b1c826c5cf5fa6097f7f5f32b68e746056480","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T22:50:00.656562Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-06-29T12:33:25.330455Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-08-08T22:50:00.656562Z","title":"Goldstein, O","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04434","last_updated":"2025-05-28T18:15:24Z","snapshot_observed_at":"2026-08-09T06:41:30.647303Z","submitted_at":"2025-02-06T19:00:00Z","title":"Searching for Inflationary Physics with the CMB Trispectrum: 1. Primordial Theory & Optimal Estimators","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-08T22:50:00.656562Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2502.04434"},"observation_digest":"sha256:3ca111191886e06ddf8976952428b0d7a7444b25ca18f1e2e114d8c505001913","observation_id":"e2ff6f55-b991-4e3b-a9ca-5a210a8be3c7","resolution":{"observed_at":"2026-08-08T22:50:00.656562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-08-08T14:22:19.949838Z","title":"Goldstein, O","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.06931","last_updated":"2025-05-28T18:18:25Z","snapshot_observed_at":"2026-08-08T18:55:41.963312Z","submitted_at":"2025-02-10T19:00:00Z","title":"Searching for Inflationary Physics with the CMB Trispectrum: 3. Constraints from Planck","version":3},"reference_index":153,"source":"pdf_text","source_observed_at":"2026-08-08T14:22:19.949838Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2502.06931"},"observation_digest":"sha256:cd65206a5a430d781cbb8a053b22e027543f0eb3b6f5239d24ddc51f98df4b86","observation_id":"15d47d41-2fbd-4dcf-b9f1-4a471f5b963a","resolution":{"observed_at":"2026-08-08T14:22:19.949838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-07-14T00:13:39.491869Z","title":"Goldstein, O","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.15729","last_updated":"2026-03-16T18:00:00Z","snapshot_observed_at":"2026-08-07T04:19:42.713539Z","submitted_at":"2026-03-16T18:00:00Z","title":"AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-07-14T00:13:39.491869Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2603.15729"},"observation_digest":"sha256:03b61aaf5cb62dce4dedd31fabcfc1aea099b0d28cb44f0eaab8e7602b0ed062","observation_id":"8813fefd-ed46-4542-9737-f9220cc60dff","resolution":{"observed_at":"2026-07-14T00:13:39.491869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":"2407.08731","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-06-29T12:33:25.330455Z","title":"Goldstein, O.H.E","venue":null,"work_id":"23cc7f40-df16-4e60-be59-b75629f0de1a","year":2024},"citing_paper":{"arxiv_id":"2604.07434","last_updated":"2026-04-08T18:00:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-08T18:00:00Z","title":"Scalars at the Cosmological Collider: Full Shapes of Tree Diagrams and Bispectrum Searches using Planck Data","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-10T17:48:05.613514Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2604.07434"},"observation_digest":"sha256:d06133f4b71962525593c89709bc6732867bb79a0724032f52c5a94c22da85d1","observation_id":"d960202e-58b0-45d2-965d-579f3752c9c8","resolution":{"observed_at":"2026-05-11T06:05:58.854894Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":"2407.08731","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-06-29T12:33:25.330455Z","title":"Goldstein, O.H.E","venue":null,"work_id":"23cc7f40-df16-4e60-be59-b75629f0de1a","year":2024},"citing_paper":{"arxiv_id":"2604.18581","last_updated":"2026-04-20T17:59:34Z","snapshot_observed_at":"2026-08-02T18:55:32.863776Z","submitted_at":"2026-04-20T17:59:34Z","title":"If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-10T03:22:25.185479Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2604.18581"},"observation_digest":"sha256:5e2cfbe113849d2a1cb994212a5a8c1737fdea303a98683ab67521ef5995cc5f","observation_id":"2f470497-5c60-410b-9bbf-127e6e237051","resolution":{"observed_at":"2026-05-11T12:31:06.904541Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":"2407.08731","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-06-29T12:33:25.330455Z","title":"Goldstein, O.H.E","venue":null,"work_id":"23cc7f40-df16-4e60-be59-b75629f0de1a","year":2024},"citing_paper":{"arxiv_id":"2605.20102","last_updated":"2026-05-19T16:54:35Z","snapshot_observed_at":"2026-08-01T20:40:21.899165Z","submitted_at":"2026-05-19T16:54:35Z","title":"Non-Relativistic Cosmological Collider Signals","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-20T04:09:09.627969Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2605.20102"},"observation_digest":"sha256:800d0eb24fd22f6e300e1d2fb89fda44303f03afab26e402a1ff59bff0a409a1","observation_id":"6e9f958c-a8fe-4368-8b06-102ed3b35b6f","resolution":{"observed_at":"2026-05-20T04:13:01.400028Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":"2407.08731","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-06-29T12:33:25.330455Z","title":"Goldstein, O.H.E","venue":null,"work_id":"23cc7f40-df16-4e60-be59-b75629f0de1a","year":2024},"citing_paper":{"arxiv_id":"2605.28054","last_updated":"2026-05-27T06:59:43Z","snapshot_observed_at":"2026-07-06T23:37:40.695655Z","submitted_at":"2026-05-27T06:59:43Z","title":"Fermionic Bubble Loop in Cosmological Collider Revisited: Exact signals from spectral and Mellin-Barnes methods","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-06-29T11:29:32.957501Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2605.28054"},"observation_digest":"sha256:8f76c521a72539526676caf12c9c8724aa8b4e0f0bd6a5fddf455768432e0acd","observation_id":"cdf25cda-c86f-46ce-b6b5-374135a518ae","resolution":{"observed_at":"2026-06-29T12:33:25.331845Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-07-12T07:57:37.399343Z","title":"Goldstein, O","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.02651","last_updated":"2026-07-02T18:00:00Z","snapshot_observed_at":"2026-07-12T23:17:38.009212Z","submitted_at":"2026-07-02T18:00:00Z","title":"First Search for Kaluza-Klein Gravitons and Radion Using Planck Data","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-12T07:57:37.399343Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2607.02651"},"observation_digest":"sha256:b4ab93051ab0d7affc6691d2db5229b0207babb24b8ddad4b4d29b181369bb89","observation_id":"9491b5e2-188b-4d9f-9f27-ab7c0ca726e5","resolution":{"observed_at":"2026-07-12T07:57:37.399343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08731","snapshot_observed_at":"2026-07-31T05:29:30.379243Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.24939","last_updated":"2026-07-27T18:00:24Z","snapshot_observed_at":"2026-08-09T00:26:01.543160Z","submitted_at":"2026-07-27T18:00:24Z","title":"Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models","version":1},"reference_index":207,"source":"arxiv_source","source_observed_at":"2026-07-31T05:29:30.379243Z"},"links":{"cited_paper":"/paper/2407.08731","citing_paper":"/paper/2607.24939"},"observation_digest":"sha256:160eb7e5f6628de7f407bfbf79e6371c344a9ff833f391dbc532bd37e3577ec6","observation_id":"adb82c14-85ec-4d72-a597-e659753c1f0a","resolution":{"observed_at":"2026-07-31T05:29:30.379243Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2407.08731/citation-record","integrity":"/paper/2407.08731/integrity","json":"/paper/2407.08731/citation-record.json","paper":"/paper/2407.08731"},"outbound":[],"paper":{"arxiv_id":"2407.08731","last_updated":"2024-07-11T17:58:15Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T18:45:01.801741Z","submitted_at":"2024-07-11T17:58:15Z","title":"Massive-ish Particles from Small-ish Scales: Non-Perturbative Techniques for Cosmological Collider Physics from Large-Scale Structure Surveys"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2407.08731."}