{"as_of":"2026-08-19T04:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7a24ff17e2144ebd573363a61ec3975daf241cd7b2b803a1d71d2292d3e5da8e","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:56:25.735923Z","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":"2026-08-11T10:24:25.380661Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1611.07961","last_updated":"2017-04-25T06:58:49Z","snapshot_observed_at":"2026-08-14T21:28:54.675612Z","submitted_at":"2016-11-23T20:12:41Z","title":"Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07961","snapshot_observed_at":"2026-08-14T04:57:51.556489Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.02614","last_updated":"2019-09-05T19:46:18Z","snapshot_observed_at":"2026-08-17T01:49:06.509134Z","submitted_at":"2019-09-05T19:46:18Z","title":"Fate of scalar dark matter solitons around supermassive galactic black holes","version":1},"reference_index":117,"source":"pdf_text","source_observed_at":"2026-08-14T04:57:51.556489Z"},"links":{"cited_paper":"/paper/1611.07961","citing_paper":"/paper/1909.02614"},"observation_digest":"sha256:7954265d3ab28ac2cfc2c8f469cac97df8a2a8b5c8d4f577415e3c2dd01fe6cc","observation_id":"4a27fd49-40f0-425b-9e74-d4cc7eb6f1f5","resolution":{"observed_at":"2026-08-14T04:57:51.556489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07961","last_updated":"2017-04-25T06:58:49Z","snapshot_observed_at":"2026-08-14T21:28:54.675612Z","submitted_at":"2016-11-23T20:12:41Z","title":"Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07961","snapshot_observed_at":"2026-08-15T21:56:25.735923Z","title":"Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08786","last_updated":"2025-08-26T12:59:02Z","snapshot_observed_at":"2026-08-18T00:28:06.981968Z","submitted_at":"2025-05-13T17:59:01Z","title":"Kination-like Era Driven by the Effective Inflaton/Higgs Potential","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T21:56:25.735923Z"},"links":{"cited_paper":"/paper/1611.07961","citing_paper":"/paper/2505.08786"},"observation_digest":"sha256:a5853fdccc3162f844d20d00c58e606518a9cd770fd8418c39b278bdd0ea5de6","observation_id":"1d1b6322-24fc-49cd-a253-f63e3ce49212","resolution":{"observed_at":"2026-08-15T21:56:25.735923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07961","last_updated":"2017-04-25T06:58:49Z","snapshot_observed_at":"2026-08-14T21:28:54.675612Z","submitted_at":"2016-11-23T20:12:41Z","title":"Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07961","snapshot_observed_at":"2026-08-05T23:25:27.106250Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.05395","last_updated":"2026-06-24T22:07:40Z","snapshot_observed_at":"2026-08-19T01:29:10.135006Z","submitted_at":"2025-08-07T13:48:53Z","title":"Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-05T23:25:27.106250Z"},"links":{"cited_paper":"/paper/1611.07961","citing_paper":"/paper/2508.05395"},"observation_digest":"sha256:f5dce132a2bb76f508f91849e461bbcb0867ddbaf6a9ff25dcf4ca08362595a1","observation_id":"981a9e3f-6cfe-4a82-930b-1743cba0b512","resolution":{"observed_at":"2026-08-05T23:25:27.106250Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07961","last_updated":"2017-04-25T06:58:49Z","snapshot_observed_at":"2026-08-14T21:28:54.675612Z","submitted_at":"2016-11-23T20:12:41Z","title":"Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07961","snapshot_observed_at":"2026-08-01T23:55:11.387425Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.15219","last_updated":"2026-08-11T17:30:53Z","snapshot_observed_at":"2026-08-18T20:59:35.784455Z","submitted_at":"2026-07-16T17:21:20Z","title":"Cosmic string gravitational wave backgrounds at LISA: II. Reconstruction of conventional signals over astrophysical foregrounds","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-01T23:55:11.387425Z"},"links":{"cited_paper":"/paper/1611.07961","citing_paper":"/paper/2607.15219"},"observation_digest":"sha256:50a78f474820ad275da0094e88fb181d55e26cd45cadc7281f11151dce70531b","observation_id":"d1e92d89-4c0d-471a-a32f-aaa002b168d8","resolution":{"observed_at":"2026-08-01T23:55:11.387425Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07961","last_updated":"2017-04-25T06:58:49Z","snapshot_observed_at":"2026-08-14T21:28:54.675612Z","submitted_at":"2016-11-23T20:12:41Z","title":"Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO","version":2},"cited_work":{"arxiv_id":"1611.07961","doi":null,"metadata_source":"pith","pith_arxiv_id":"1611.07961","snapshot_observed_at":"2026-08-11T10:24:25.380661Z","title":"Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO","venue":"astro-ph.CO","work_id":"2287c9b9-191b-4c83-889c-00e1e651a5be","year":2016},"citing_paper":{"arxiv_id":"2608.09814","last_updated":"2026-08-10T16:33:52Z","snapshot_observed_at":"2026-08-15T07:20:19.913013Z","submitted_at":"2026-08-10T16:33:52Z","title":"Leptogenesis in Brane-modified cosmology: Signatures in primordial gravitational waves","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T10:24:24.674607Z"},"links":{"cited_paper":"/paper/1611.07961","citing_paper":"/paper/2608.09814"},"observation_digest":"sha256:9f4f3282844dc5766a069ba82929b38dc232186f9c2c660bed2f63c19698dfbf","observation_id":"13d535db-6082-4fdd-bbd5-4ab27c856810","resolution":{"observed_at":"2026-08-11T10:24:25.385544Z","resolver_source":"local_arxiv","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"}}],"links":{"evidence":"/evidence","html":"/paper/1611.07961/citation-record","integrity":"/paper/1611.07961/integrity","json":"/paper/1611.07961/citation-record.json","paper":"/paper/1611.07961"},"outbound":[],"paper":{"arxiv_id":"1611.07961","last_updated":"2017-04-25T06:58:49Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T21:28:54.675612Z","submitted_at":"2016-11-23T20:12:41Z","title":"Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO"},"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 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1611.07961."}