{"as_of":"2026-08-08T16:51:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:1ffa89b7d99f0814db12bc0935d41b099ff6afc084174134cb986b7b4392de3b","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":"2026-08-08T06:32:00.761636+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":"2026-08-07T13:10:28.284560Z","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":"2026-07-03T07:37:45.574232Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2310.08527","last_updated":"2025-01-30T15:21:04Z","snapshot_observed_at":"2026-07-06T16:32:07.186600Z","submitted_at":"2023-10-12T17:20:02Z","title":"Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data","version":2},"cited_work":{"arxiv_id":"2310.08527","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.08527","snapshot_observed_at":"2026-07-03T07:37:45.574232Z","title":"Tagliazucchi, M","venue":null,"work_id":"a39be32e-8cbb-4f85-b4a5-4aba433878fd","year":2025},"citing_paper":{"arxiv_id":"2505.16820","last_updated":"2026-04-13T03:10:33Z","snapshot_observed_at":"2026-07-06T21:28:38.694043Z","submitted_at":"2025-05-22T15:55:50Z","title":"Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order","version":3},"reference_index":290,"source":"pdf_text","source_observed_at":"2026-05-22T01:55:13.345095Z"},"links":{"cited_paper":"/paper/2310.08527","citing_paper":"/paper/2505.16820"},"observation_digest":"sha256:17e608f99dc848ff6d5f5046fe081b0cf5bdcc8bf7c45120a4d2bd92d1770350","observation_id":"08a02c48-05c8-4d2d-8cf3-066bf879660e","resolution":{"observed_at":"2026-05-22T01:55:55.012873Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.08527","last_updated":"2025-01-30T15:21:04Z","snapshot_observed_at":"2026-07-06T16:32:07.186600Z","submitted_at":"2023-10-12T17:20:02Z","title":"Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.08527","snapshot_observed_at":"2026-08-07T13:10:28.284560Z","title":"Tagliazucchi, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.22614","last_updated":"2025-08-25T16:37:04Z","snapshot_observed_at":"2026-08-08T08:39:50.666476Z","submitted_at":"2025-05-28T17:30:00Z","title":"Cosmological constraints on small-scale primordial non-Gaussianity","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-07T13:10:28.284560Z"},"links":{"cited_paper":"/paper/2310.08527","citing_paper":"/paper/2505.22614"},"observation_digest":"sha256:d08a5ef839d051385bc3aa25a6d97f6776c62947718a2362323ca76ac2f190cc","observation_id":"1989dc0c-7807-4522-ac9b-86a279a38b48","resolution":{"observed_at":"2026-08-07T13:10:28.284560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.08527","last_updated":"2025-01-30T15:21:04Z","snapshot_observed_at":"2026-07-06T16:32:07.186600Z","submitted_at":"2023-10-12T17:20:02Z","title":"Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data","version":2},"cited_work":{"arxiv_id":"2310.08527","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.08527","snapshot_observed_at":"2026-07-03T07:37:45.574232Z","title":"Tagliazucchi, M","venue":null,"work_id":"a39be32e-8cbb-4f85-b4a5-4aba433878fd","year":2025},"citing_paper":{"arxiv_id":"2507.09552","last_updated":"2026-04-28T09:13:42Z","snapshot_observed_at":"2026-07-06T21:56:19.049474Z","submitted_at":"2025-07-13T09:38:41Z","title":"Probing the scalar-induced gravitational waves with the Five-hundred-meter Aperture Spherical radio Telescope and the Square Kilometer Array","version":3},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-05-19T05:22:20.397762Z"},"links":{"cited_paper":"/paper/2310.08527","citing_paper":"/paper/2507.09552"},"observation_digest":"sha256:60919bfeffe0affac39ad936590e0a88f0e3ad4d121371c157b872656152fe23","observation_id":"02926761-4336-4cb3-8505-dec313f66212","resolution":{"observed_at":"2026-05-19T05:22:59.439185Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.08527","last_updated":"2025-01-30T15:21:04Z","snapshot_observed_at":"2026-07-06T16:32:07.186600Z","submitted_at":"2023-10-12T17:20:02Z","title":"Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.08527","snapshot_observed_at":"2026-08-06T11:33:42.775381Z","title":"Tagliazucchi, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.22688","last_updated":"2025-07-30T13:49:21Z","snapshot_observed_at":"2026-08-07T06:34:16.533257Z","submitted_at":"2025-07-30T13:49:21Z","title":"Tensor induced gravitational waves","version":1},"reference_index":105,"source":"pdf_text","source_observed_at":"2026-08-06T11:33:42.775381Z"},"links":{"cited_paper":"/paper/2310.08527","citing_paper":"/paper/2507.22688"},"observation_digest":"sha256:73d20cafd5384726ea900604dec577cdb7fdc765351044dac334c368ec47fc06","observation_id":"163f9164-a527-45a9-8ac7-e0bdf4e26451","resolution":{"observed_at":"2026-08-06T11:33:42.775381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.08527","last_updated":"2025-01-30T15:21:04Z","snapshot_observed_at":"2026-07-06T16:32:07.186600Z","submitted_at":"2023-10-12T17:20:02Z","title":"Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.08527","snapshot_observed_at":"2026-08-05T15:54:08.342655Z","title":"Tagliazucchi, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.19328","last_updated":"2026-06-02T10:21:11Z","snapshot_observed_at":"2026-08-06T11:12:02.586056Z","submitted_at":"2025-08-26T18:00:00Z","title":"Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-05T15:54:08.342655Z"},"links":{"cited_paper":"/paper/2310.08527","citing_paper":"/paper/2508.19328"},"observation_digest":"sha256:9758c57215fda88f789ed4b6b3d6806bec0cdd525a9e668bd4dd37f36ca4629a","observation_id":"96b73e62-4e9a-470e-aeba-a8268b75039b","resolution":{"observed_at":"2026-08-05T15:54:08.342655Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.08527","last_updated":"2025-01-30T15:21:04Z","snapshot_observed_at":"2026-07-06T16:32:07.186600Z","submitted_at":"2023-10-12T17:20:02Z","title":"Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data","version":2},"cited_work":{"arxiv_id":"2310.08527","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.08527","snapshot_observed_at":"2026-07-03T07:37:45.574232Z","title":"Tagliazucchi, M","venue":null,"work_id":"a39be32e-8cbb-4f85-b4a5-4aba433878fd","year":2025},"citing_paper":{"arxiv_id":"2606.11312","last_updated":"2026-06-11T15:15:07Z","snapshot_observed_at":"2026-08-03T04:41:01.909999Z","submitted_at":"2026-06-09T18:01:00Z","title":"CMB Constraints on Pre-Inflationary Axion Dark Matter Isocurvature","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-06-27T11:56:00.320652Z"},"links":{"cited_paper":"/paper/2310.08527","citing_paper":"/paper/2606.11312"},"observation_digest":"sha256:bfe31bf939eb79baf6916567d40cc17b8851e2921e2f627531f8e00cb52afea7","observation_id":"bae7adde-d2a3-4014-9a30-d9f376c40fb2","resolution":{"observed_at":"2026-07-03T07:37:45.575441Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.08527","last_updated":"2025-01-30T15:21:04Z","snapshot_observed_at":"2026-07-06T16:32:07.186600Z","submitted_at":"2023-10-12T17:20:02Z","title":"Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.08527","snapshot_observed_at":"2026-07-14T09:40:09.826288Z","title":"Tagliazucchi, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.10730","last_updated":"2026-07-12T12:29:42Z","snapshot_observed_at":"2026-08-02T19:13:11.745940Z","submitted_at":"2026-07-12T12:29:42Z","title":"Scalar-induced gravitational waves from a box-shaped curvature power spectrum","version":1},"reference_index":118,"source":"pdf_text","source_observed_at":"2026-07-14T09:40:09.826288Z"},"links":{"cited_paper":"/paper/2310.08527","citing_paper":"/paper/2607.10730"},"observation_digest":"sha256:5088b14d938f17c418f1a5aa5a4e523a1c0356281596e314916b5ea55c0b9222","observation_id":"7455b07d-deb7-404e-bc02-33418875d014","resolution":{"observed_at":"2026-07-14T09:40:09.826288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2310.08527/citation-record","integrity":"/paper/2310.08527/integrity","json":"/paper/2310.08527/citation-record.json","paper":"/paper/2310.08527"},"outbound":[],"paper":{"arxiv_id":"2310.08527","last_updated":"2025-01-30T15:21:04Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T16:32:07.186600Z","submitted_at":"2023-10-12T17:20:02Z","title":"Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2310.08527."}