{"as_of":"2026-08-08T01:21:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:879f06e182d4e9a3ded96baebb8d17440e84aae220394b0c30549219d57ccf1d","coverage":[{"denominator":12,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T12:51:51.466124Z","state":"measured"},{"denominator":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.23521/citation-record","integrity":"/paper/2505.23521/integrity","json":"/paper/2505.23521/citation-record.json","paper":"/paper/2505.23521"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:53.695352Z","title":null,"venue":null,"work_id":"6cd3b62c-5955-4d86-98c1-f52535bed6cc","year":1975},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:50.261294Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:40fa5a7f363ef591d7410305ff0acefe0bc99b9fe8d7bb8e31f386dfb1d411b1","observation_id":"2bfb3fd8-4e48-4276-b3aa-fa253fe4811c","resolution":{"observed_at":"2026-08-07T12:51:53.800480Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:53.456366Z","title":"General relativistic dynamics of irrotational dust: Cosmological implications","venue":null,"work_id":"4fed6b38-4a5a-4307-932d-a14f029c4874","year":1994},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:50.376810Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:da6082ee0846d800869dcb32badfd6cd048777bd6cc81d2dd68325b273cfa035","observation_id":"31079cb0-d4f2-4a89-9717-ac64a347ffb9","resolution":{"observed_at":"2026-08-07T12:51:53.547198Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:53.193083Z","title":"Scalar Induced Gravitational Waves Review","venue":null,"work_id":"d27c4018-5ea7-434a-be7b-e039830bae0f","year":2021},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:50.503488Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:2bee195d5da2dc47c514375ba03ecf48d196ea5ee0130c695aeeff00dbe14fe1","observation_id":"027546c0-9ab9-426e-899f-5851d1bbd6ec","resolution":{"observed_at":"2026-08-07T12:51:53.356984Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:52.971432Z","title":"The NANOGrav 15 yr Data Set: Evidence for a Gravitational-wave Background","venue":null,"work_id":"e3198c03-fe67-4d50-8c2f-52d2df7dd686","year":2023},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:50.580121Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:c32e9a0229df3c07400c0c0943f7116028d6272a6d74f02a8d774222d4114f31","observation_id":"ee7dbb95-2d40-4be2-ab50-325b9649f292","resolution":{"observed_at":"2026-08-07T12:51:53.084685Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:52.794931Z","title":"and others","venue":null,"work_id":"5c7627e2-f942-4962-b5de-e01e308fad87","year":2023},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:50.672361Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:60753316959afa678086589d81a45c519c9c4d427c89d0bb0ed0311b639a8ff2","observation_id":"b932d8fd-f7ef-451b-9748-1dade1f45731","resolution":{"observed_at":"2026-08-07T12:51:52.860924Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:52.582115Z","title":"The NANOGrav 15 yr Data Set: Search for Signals from New Physics","venue":null,"work_id":"d384610d-c732-4825-9340-e5c1a8f664e6","year":2023},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:50.757578Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:210334efd347ab00b6576fe4b5d7a1e3f5129d6094e745a1640aa5ee715657c8","observation_id":"418dafa3-de6f-4115-9e2f-e6cd4333ebb3","resolution":{"observed_at":"2026-08-07T12:51:52.690030Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:50.841097Z","title":"Laser Interferometer Space Antenna","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:50.841097Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:35fa3930368cf34ac7db56bc5df1cf60ae08d70199a4ee7ca8179af43e449c0a","observation_id":"0a10a776-5dd6-4d97-baba-eef573c6c1c5","resolution":{"observed_at":"2026-08-07T12:51:50.841097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:52.396670Z","title":"Reconstructing Primordial Curvature Perturbations via Scalar- Induced Gravitational Waves with LISA","venue":null,"work_id":"a3ed56f9-00fd-49b4-b37e-7dd73aa9a62e","year":2025},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:50.927669Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:fc17989163e68533e47d1b3b4570d229e494ec83591cbf1bab68656eb2479d25","observation_id":"afb90fdb-6470-4e70-b668-327c9b2bde43","resolution":{"observed_at":"2026-08-07T12:51:52.486492Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:52.177627Z","title":"Gravitational Waves Induced by Scalar Perturbations with a Lognormal Peak","venue":null,"work_id":"24aee1f7-5c64-43aa-b5f4-d688c70826c3","year":2020},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:51.055859Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:5e439f1bcada5530efb1af9948ac7c69be1b9ea69168b1776b6411f0ce64048f","observation_id":"2c2b3a19-d24b-4070-8c42-81a5c69da856","resolution":{"observed_at":"2026-08-07T12:51:52.284545Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:51.952240Z","title":"Gravitational wave astronomy with the SKA","venue":null,"work_id":"930d142b-d1f2-47b4-9d65-86deb0424ab8","year":2015},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:51.166500Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:89980d54ab0e7ca56fca435aace3f9acda7439385b50d81831fdec183b5ad55b","observation_id":"c96056e6-ef59-4739-8622-a65169a43a23","resolution":{"observed_at":"2026-08-07T12:51:52.067986Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:51.771727Z","title":"Prospects for Scalar-Induced Gravitational Waves detection with SKA","venue":null,"work_id":"36021aac-97b3-4cc7-b7fb-2b34d9fdae1b","year":2025},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:51.299832Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:e1a2404d736c37673f2c44d53752f4c3f8e050fa6ac617129136d62c0ef6f219","observation_id":"cb56ab80-3fa7-4950-bb3f-331ee1e4559a","resolution":{"observed_at":"2026-08-07T12:51:51.839424Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:51:51.583306Z","title":"Forecasting the sensitivity of pulsar timing arrays to gravitational wave backgrounds","venue":null,"work_id":"bc7b3c0f-0bdb-432d-88d8-746b46ffe7ad","year":2024},"citing_paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T12:51:51.466124Z"},"links":{"citing_paper":"/paper/2505.23521"},"observation_digest":"sha256:57525b5637e2c10224128b86a1d42f1ff99d176b495e36f53a1566cc5ef867b5","observation_id":"cb58407e-3f32-43ae-873d-df2369f660aa","resolution":{"observed_at":"2026-08-07T12:51:51.655421Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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"}}],"paper":{"arxiv_id":"2505.23521","last_updated":"2025-05-29T15:01:27Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T12:42:03.154025Z","submitted_at":"2025-05-29T15:01:27Z","title":"Constraining primordial curvature perturbations with present and future GW detectors"},"reference_resolution":{"displayed":12,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":2,"verified_exact":0,"verified_fuzzy":10},"total_outbound_references":12},"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 8 August 2026, this Paper Citation Record lists 12 of 12 outbound references and 0 inbound Pith citation observations for arXiv:2505.23521."}