{"as_of":"2026-08-09T18:20:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4b4570afab311fdfe423506108724c7765d4e54b08c3bcdf5544057fd2f0cf35","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":15,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":15,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":15,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":15,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T05:30:21.079126Z","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":"2026-07-03T02:17:35.065778Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":"1908.00546","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-07-03T02:17:35.065778Z","title":"Smith, T.L","venue":null,"work_id":"2fcbe62a-d5e2-436a-b8fc-8d14f6fd947f","year":2019},"citing_paper":{"arxiv_id":"2002.04615","last_updated":"2021-01-20T08:21:53Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-02-11T19:00:01Z","title":"New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions","version":3},"reference_index":215,"source":"pdf_text","source_observed_at":"2026-05-23T22:35:49.730350Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2002.04615"},"observation_digest":"sha256:b6434ef62f7d26c83c9061aab666a676a4bfe4f26e3633b547d2ee097719b34a","observation_id":"a89f5169-a34e-4d4a-bc2a-6595c1b3a269","resolution":{"observed_at":"2026-05-23T22:35:50.563416Z","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":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":"1908.00546","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-07-03T02:17:35.065778Z","title":"Smith, T.L","venue":null,"work_id":"2fcbe62a-d5e2-436a-b8fc-8d14f6fd947f","year":2019},"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":120,"source":"pdf_text","source_observed_at":"2026-05-22T01:55:13.345095Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2505.16820"},"observation_digest":"sha256:fa29a19bfbe9b4b4df1b2ee3dbf055acd61604cf0e6bcc4b8ba950bbd5d063c0","observation_id":"21381778-2f39-4dd1-9c4d-e5918990ea80","resolution":{"observed_at":"2026-05-22T01:55:55.846896Z","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":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-08-07T05:30:21.079126Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.08193","last_updated":"2025-07-30T20:09:57Z","snapshot_observed_at":"2026-08-07T17:20:44.019468Z","submitted_at":"2025-06-09T20:08:22Z","title":"GW170817 Viable Einstein-Gauss-Bonnet Inflation Compatible with the Atacama Cosmology Telescope Data","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T05:30:21.079126Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2506.08193"},"observation_digest":"sha256:70509b194e51b0e952412f2d90396e5f2b4225fb94d29175b19ca36e2bef185b","observation_id":"56964f6d-e13e-4705-a550-4cbbddc95211","resolution":{"observed_at":"2026-08-07T05:30:21.079126Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-08-06T22:57:37.365225Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.20751","last_updated":"2025-06-25T18:24:57Z","snapshot_observed_at":"2026-08-09T17:48:13.197467Z","submitted_at":"2025-06-25T18:24:57Z","title":"The Persistence of Nonlinear Gravitational Wave Memory","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T22:57:37.365225Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2506.20751"},"observation_digest":"sha256:4f4aaf96b89f70f6b9b29956f9083b470013834b4f0121cb767962b884dccee6","observation_id":"e9bd8972-c101-4ec6-b23f-d915e648fabd","resolution":{"observed_at":"2026-08-06T22:57:37.365225Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-08-06T11:25:20.930060Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.22975","last_updated":"2026-06-03T21:46:18Z","snapshot_observed_at":"2026-08-06T11:25:12.896578Z","submitted_at":"2025-07-30T18:00:00Z","title":"Gamma-Rays and Gravitational Waves from Inelastic Higgs Portal Dark Matter","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T11:25:20.930060Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2507.22975"},"observation_digest":"sha256:dfcb1a9a2708e272a161f35ef6222796dfe0ef62bbae094d974160a022a75c73","observation_id":"8ee7b311-a355-49bc-9ab4-a01f3c340e12","resolution":{"observed_at":"2026-08-06T11:25:20.930060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-08-04T07:36:36.567916Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.25353","last_updated":"2026-06-03T13:30:58Z","snapshot_observed_at":"2026-08-09T04:22:49.787736Z","submitted_at":"2025-10-29T10:14:08Z","title":"Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-04T07:36:36.567916Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2510.25353"},"observation_digest":"sha256:dabd711e71b95d151add4cb7a54595f6ba7f49bd1fd20d5c25777ef9c3e7966c","observation_id":"48188199-6486-4471-a0fe-554d434e6082","resolution":{"observed_at":"2026-08-04T07:36:36.567916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":"1908.00546","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-07-03T02:17:35.065778Z","title":"Smith, T.L","venue":null,"work_id":"2fcbe62a-d5e2-436a-b8fc-8d14f6fd947f","year":2019},"citing_paper":{"arxiv_id":"2511.00996","last_updated":"2026-07-22T01:08:05Z","snapshot_observed_at":"2026-08-04T00:32:09.189736Z","submitted_at":"2025-11-02T16:07:09Z","title":"Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings","version":4},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-21T19:14:16.875074Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2511.00996"},"observation_digest":"sha256:ad22d3a3553fe90311603eeb1539e2e3bd78b88b45fa70ba746b3e396df436e8","observation_id":"44e47412-5d91-470d-8c82-67294f94ac38","resolution":{"observed_at":"2026-05-21T19:14:19.291566Z","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":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-08-04T00:32:12.976237Z","title":"Smith, T.L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.00996","last_updated":"2026-07-22T01:08:05Z","snapshot_observed_at":"2026-08-04T00:32:09.189736Z","submitted_at":"2025-11-02T16:07:09Z","title":"Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings","version":5},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:12.976237Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2511.00996"},"observation_digest":"sha256:314c32e471916e5b7c1235c654a9bfc1c836a451b20bfa2acc389ec233aca97a","observation_id":"7b4d2d13-ab76-4d92-85b8-60eec5ab8b7e","resolution":{"observed_at":"2026-08-04T00:32:12.976237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":"1908.00546","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-07-03T02:17:35.065778Z","title":"Smith, T.L","venue":null,"work_id":"2fcbe62a-d5e2-436a-b8fc-8d14f6fd947f","year":2019},"citing_paper":{"arxiv_id":"2511.21488","last_updated":"2026-07-22T01:34:09Z","snapshot_observed_at":"2026-08-03T20:05:41.053409Z","submitted_at":"2025-11-26T15:21:11Z","title":"Bayesian analysis of the complex singlet model with phase transition gravitational waves","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-21T17:52:39.351449Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2511.21488"},"observation_digest":"sha256:00d792169b113f72e21146821ddfab1f13d2df8526652c44a84632f3285ea2a5","observation_id":"92c7240b-1750-4d09-bd88-74ffb44643f6","resolution":{"observed_at":"2026-05-21T17:54:18.485998Z","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":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-08-03T20:05:43.660492Z","title":"Smith, T.L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.21488","last_updated":"2026-07-22T01:34:09Z","snapshot_observed_at":"2026-08-03T20:05:41.053409Z","submitted_at":"2025-11-26T15:21:11Z","title":"Bayesian analysis of the complex singlet model with phase transition gravitational waves","version":4},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-03T20:05:43.660492Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2511.21488"},"observation_digest":"sha256:3d8c8a1c1a0968ef081790b39568da3a2a562c52d6526b1a41482e3c6d1ec820","observation_id":"134413b3-fe7a-43ee-ac09-0680986e60a2","resolution":{"observed_at":"2026-08-03T20:05:43.660492Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-08-02T17:45:19.412677Z","title":"Smith, T.L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.21762","last_updated":"2026-07-22T02:46:22Z","snapshot_observed_at":"2026-08-07T04:03:13.217115Z","submitted_at":"2026-03-23T09:56:39Z","title":"Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-02T17:45:19.412677Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2603.21762"},"observation_digest":"sha256:4bfbfa264b95c6e51d0a28aed782ab83933638cae57aa85dc0f73a0a64e9c18d","observation_id":"a721cf67-eef8-4572-b136-c86194c76dc4","resolution":{"observed_at":"2026-08-02T17:45:19.412677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":"1908.00546","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-07-03T02:17:35.065778Z","title":"Smith, T.L","venue":null,"work_id":"2fcbe62a-d5e2-436a-b8fc-8d14f6fd947f","year":2019},"citing_paper":{"arxiv_id":"2606.09713","last_updated":"2026-06-08T16:38:36Z","snapshot_observed_at":"2026-08-05T16:32:17.465260Z","submitted_at":"2026-06-08T16:38:36Z","title":"PTA-Compatible Domain Walls at LISA and Taiji: Bayesian Reconstruction and Multiband Inference","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-06-27T16:00:44.904807Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2606.09713"},"observation_digest":"sha256:c7647b73e7de0633f5dc4cb302578559b8ea494d20063586e26bfc99edaeff08","observation_id":"8b3a55af-9c87-4b76-b6e6-47aa8a56bf54","resolution":{"observed_at":"2026-07-03T02:17:35.067200Z","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":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":"1908.00546","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-07-03T02:17:35.065778Z","title":"Smith, T.L","venue":null,"work_id":"2fcbe62a-d5e2-436a-b8fc-8d14f6fd947f","year":2019},"citing_paper":{"arxiv_id":"2606.28071","last_updated":"2026-06-26T13:36:03Z","snapshot_observed_at":"2026-08-08T07:53:47.070449Z","submitted_at":"2026-06-26T13:36:03Z","title":"Construction of Sensitivity Curves for Dynamic LISA and Taiji","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-06-29T03:29:40.165686Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2606.28071"},"observation_digest":"sha256:e22cc7faa0bbf5d1be0ba86b7ee92a9d55e26d3011cb2aeeeb66745cd93df449","observation_id":"480e7f3c-aea4-4283-8d19-14104049d331","resolution":{"observed_at":"2026-07-01T17:35:51.886119Z","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":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-07-31T02:53:21.819893Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28592","last_updated":"2026-07-30T17:45:00Z","snapshot_observed_at":"2026-08-08T00:26:56.278957Z","submitted_at":"2026-07-30T17:45:00Z","title":"LISA Reconstruction Landscape for Metastable Cosmic Strings","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-07-31T02:53:21.819893Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2607.28592"},"observation_digest":"sha256:9ff280c8b8a4346c8432c3cace8ad89eab4f75b94ad8be07e51c5f4027bb1257","observation_id":"2362fe0d-e54e-4016-bbd8-672d1dea5482","resolution":{"observed_at":"2026-07-31T02:53:21.819893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00546","snapshot_observed_at":"2026-08-06T00:31:00.535646Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.01165","last_updated":"2026-08-02T11:36:42Z","snapshot_observed_at":"2026-08-09T12:09:47.530524Z","submitted_at":"2026-08-02T11:36:42Z","title":"From Quantum Correlations to Inflationary Tracking Scalar Field Evolution","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T00:31:00.535646Z"},"links":{"cited_paper":"/paper/1908.00546","citing_paper":"/paper/2608.01165"},"observation_digest":"sha256:53ad7c91d0f68398ac64c27903f043c6d2267b0105976d974aa18e02264617f2","observation_id":"ae67b8e1-705a-40ce-9311-44ada1a58290","resolution":{"observed_at":"2026-08-06T00:31:00.535646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1908.00546/citation-record","integrity":"/paper/1908.00546/integrity","json":"/paper/1908.00546/citation-record.json","paper":"/paper/1908.00546"},"outbound":[],"paper":{"arxiv_id":"1908.00546","last_updated":"2019-12-06T14:20:19Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-09T11:04:44.511669Z","submitted_at":"2019-08-01T18:00:01Z","title":"LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources"},"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 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:1908.00546."}