{"as_of":"2026-08-18T09:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:650e980776db21e5fac644e2d8e678325156f98c987df4d8171ae00a58d65d24","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T20:02:01.670726Z","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":"2026-05-21T04:24:33.436980Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.20778","last_updated":"2025-03-26T17:56:38Z","snapshot_observed_at":"2026-08-17T12:49:32.512031Z","submitted_at":"2025-03-26T17:56:38Z","title":"Detectability of the chiral gravitational wave background from audible axions with the LISA-Taiji network","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.20778","snapshot_observed_at":"2026-08-07T04:45:38.644753Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.09744","last_updated":"2026-07-03T14:51:15Z","snapshot_observed_at":"2026-08-18T05:10:15.547249Z","submitted_at":"2025-06-11T13:48:57Z","title":"Distinguishing Monochromatic Signals in LISA and Taiji: Ultralight Dark Matter versus Gravitational Waves","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T04:45:38.644753Z"},"links":{"cited_paper":"/paper/2503.20778","citing_paper":"/paper/2506.09744"},"observation_digest":"sha256:0e47407712d162bea93de9eb7527f1a051f975919129ddbe589555bd4b059de9","observation_id":"14d7b419-321c-4512-8f6a-67befd86cf43","resolution":{"observed_at":"2026-08-07T04:45:38.644753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.20778","last_updated":"2025-03-26T17:56:38Z","snapshot_observed_at":"2026-08-17T12:49:32.512031Z","submitted_at":"2025-03-26T17:56:38Z","title":"Detectability of the chiral gravitational wave background from audible axions with the LISA-Taiji network","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.20778","snapshot_observed_at":"2026-08-05T22:27:25.545195Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.06987","last_updated":"2025-08-09T13:48:28Z","snapshot_observed_at":"2026-08-13T11:59:17.970025Z","submitted_at":"2025-08-09T13:48:28Z","title":"Fixed-Time Voltage Regulation for Boost Converters via Unit-Safe Saturating Functions","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-05T22:27:25.545195Z"},"links":{"cited_paper":"/paper/2503.20778","citing_paper":"/paper/2508.06987"},"observation_digest":"sha256:e87ba57f7a4c176ff98bbf7776b6efb98e5b6d1606ffe2574b56faf1e836cb35","observation_id":"b68926d4-f59e-4de0-972f-ce7469d8d975","resolution":{"observed_at":"2026-08-05T22:27:25.545195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.20778","last_updated":"2025-03-26T17:56:38Z","snapshot_observed_at":"2026-08-17T12:49:32.512031Z","submitted_at":"2025-03-26T17:56:38Z","title":"Detectability of the chiral gravitational wave background from audible axions with the LISA-Taiji network","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.20778","snapshot_observed_at":"2026-08-04T07:34:03.295005Z","title":"Detectability of the chiral gravitational wave background from audible axions with the LISA-Taiji network,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.25895","last_updated":"2026-07-06T10:34:35Z","snapshot_observed_at":"2026-08-12T13:39:04.145554Z","submitted_at":"2025-10-29T18:54:30Z","title":"Beyond general relativity: gravitational waves in non-minimally coupled theories","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-04T07:34:03.295005Z"},"links":{"cited_paper":"/paper/2503.20778","citing_paper":"/paper/2510.25895"},"observation_digest":"sha256:c65bfa974748c063092f563b4253c19b48cbc9d990a40d9ec37c7afef7e59674","observation_id":"5c57b474-1a48-43ec-b76e-84cc92411b51","resolution":{"observed_at":"2026-08-04T07:34:03.295005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.20778","last_updated":"2025-03-26T17:56:38Z","snapshot_observed_at":"2026-08-17T12:49:32.512031Z","submitted_at":"2025-03-26T17:56:38Z","title":"Detectability of the chiral gravitational wave background from audible axions with the LISA-Taiji network","version":1},"cited_work":{"arxiv_id":"2503.20778","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.20778","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"aeafc3e2-b5ee-4df2-a009-51aefa0ca946","year":2025},"citing_paper":{"arxiv_id":"2604.08141","last_updated":"2026-04-09T12:00:20Z","snapshot_observed_at":"2026-08-10T21:32:15.515348Z","submitted_at":"2026-04-09T12:00:20Z","title":"Detecting Chiral Gravitational Wave Background with a Dipole Pulsar Timing Array","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-10T17:24:16.394595Z"},"links":{"cited_paper":"/paper/2503.20778","citing_paper":"/paper/2604.08141"},"observation_digest":"sha256:d007e85381764db20bf732f7be12d3110ea2d08fae663abfe36ed6f427437b78","observation_id":"230abe78-d326-4fe8-82a7-abd4afebdf93","resolution":{"observed_at":"2026-05-11T06:51:51.361851Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.20778","last_updated":"2025-03-26T17:56:38Z","snapshot_observed_at":"2026-08-17T12:49:32.512031Z","submitted_at":"2025-03-26T17:56:38Z","title":"Detectability of the chiral gravitational wave background from audible axions with the LISA-Taiji network","version":1},"cited_work":{"arxiv_id":"2503.20778","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.20778","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"aeafc3e2-b5ee-4df2-a009-51aefa0ca946","year":2025},"citing_paper":{"arxiv_id":"2605.21092","last_updated":"2026-05-20T12:24:00Z","snapshot_observed_at":"2026-08-03T10:38:16.949612Z","submitted_at":"2026-05-20T12:24:00Z","title":"Audible Axion Magnetogenesis: Linking Intergalactic Magnetic Fields and Gravitational Waves","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-21T04:24:21.715932Z"},"links":{"cited_paper":"/paper/2503.20778","citing_paper":"/paper/2605.21092"},"observation_digest":"sha256:7ac9be9c2d546d4e520ffa3fb3a3e48365ecb462a069bd435519876e60b12f09","observation_id":"760e3886-1666-4460-8f15-ca137105db6c","resolution":{"observed_at":"2026-05-21T04:24:33.438380Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.20778","last_updated":"2025-03-26T17:56:38Z","snapshot_observed_at":"2026-08-17T12:49:32.512031Z","submitted_at":"2025-03-26T17:56:38Z","title":"Detectability of the chiral gravitational wave background from audible axions with the LISA-Taiji network","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.20778","snapshot_observed_at":"2026-08-11T20:02:01.670726Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.09299","last_updated":"2026-08-10T08:48:53Z","snapshot_observed_at":"2026-08-15T01:38:20.077434Z","submitted_at":"2026-08-10T08:48:53Z","title":"Correlated parity violation in gravity and electromagnetism from five-dimensional spacetime","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T20:02:01.670726Z"},"links":{"cited_paper":"/paper/2503.20778","citing_paper":"/paper/2608.09299"},"observation_digest":"sha256:bbc0d822733d1df0fc014633dce219c3a64dfd1c3d5e1986154b944316794980","observation_id":"98a73307-050b-425f-ad97-24adaf611bca","resolution":{"observed_at":"2026-08-11T20:02:01.670726Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.20778/citation-record","integrity":"/paper/2503.20778/integrity","json":"/paper/2503.20778/citation-record.json","paper":"/paper/2503.20778"},"outbound":[],"paper":{"arxiv_id":"2503.20778","last_updated":"2025-03-26T17:56:38Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T12:49:32.512031Z","submitted_at":"2025-03-26T17:56:38Z","title":"Detectability of the chiral gravitational wave background from audible axions with the LISA-Taiji network"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2503.20778."}