{"as_of":"2026-08-08T22:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:dec0a02db80d30ebd2d110bad1f1b18c7d430409f9bb6a1c12125d3052168faa","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":16,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":16,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":16,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":16,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:00:28.612042Z","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":"2026-05-20T03:48:02.874035Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":"1906.01593","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Belgacemet al.(LISA Cosmology Working Group), J","venue":null,"work_id":"36ce1202-ac50-4a17-8333-cfc7d91c3382","year":2019},"citing_paper":{"arxiv_id":"1912.02622","last_updated":"2020-03-24T17:57:53Z","snapshot_observed_at":"2026-08-02T17:41:15.064781Z","submitted_at":"2019-12-05T14:57:00Z","title":"Science Case for the Einstein Telescope","version":4},"reference_index":205,"source":"pdf_text","source_observed_at":"2026-05-16T00:13:18.137293Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/1912.02622"},"observation_digest":"sha256:20922b0f13c83807c4ec8d36c3f23947b83237dd94dc89d5fd82127a737f0a27","observation_id":"b73a4fae-962b-469a-942e-616cfd8031be","resolution":{"observed_at":"2026-05-16T00:13:18.660758Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":"1906.01593","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Belgacemet al.(LISA Cosmology Working Group), J","venue":null,"work_id":"36ce1202-ac50-4a17-8333-cfc7d91c3382","year":2019},"citing_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-05-14T19:42:39.936694Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2203.06142"},"observation_digest":"sha256:fdecfdfadf7eee9d7c65dc2a7bf3f89e3f1ba838c7a548a2fd037aebd0fb3b0b","observation_id":"5b9c7cb7-aab5-4554-aa0e-d4f7fbfa9c7f","resolution":{"observed_at":"2026-05-14T19:42:40.921160Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-07T15:00:28.612042Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.16883","last_updated":"2025-05-29T16:46:47Z","snapshot_observed_at":"2026-08-07T16:30:52.556811Z","submitted_at":"2025-05-22T16:36:53Z","title":"Test-Field vs Physical Quasi-Normal Modes in Scalar-Tensor Theories","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T15:00:28.612042Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2505.16883"},"observation_digest":"sha256:c9204e2715d9e9fe26bae8ae556da6b373cb184ba5a57a6f110b0c1c6b29ee48","observation_id":"1343e52b-594b-444f-a91e-a0b0e5ca6dd4","resolution":{"observed_at":"2026-08-07T15:00:28.612042Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-07T12:29:22.087721Z","title":"Belgacem et al., Testing modified gravity at cosmological distances with LISA standard sirens , JCAP 07 (2019) 024, [ arXiv:1906.01593]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.24620","last_updated":"2025-05-30T14:11:50Z","snapshot_observed_at":"2026-08-07T12:15:01.990223Z","submitted_at":"2025-05-30T14:11:50Z","title":"Covariant diffusion and drift of the stochastic GW background with LISA","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T12:29:22.087721Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2505.24620"},"observation_digest":"sha256:5edf06fcb08ebd9044018b36e0583175951b2339b8d52d5976fed2da23f36285","observation_id":"110db766-3412-4cd1-9b1c-00a278be64e1","resolution":{"observed_at":"2026-08-07T12:29:22.087721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-07T11:20:51.276132Z","title":"Belgacemet al.(LISA Cosmology Working Group), JCAP07, 024, arXiv:1906.01593 [astro-ph.CO]","venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2506.02909","last_updated":"2025-06-03T14:15:25Z","snapshot_observed_at":"2026-08-08T20:47:21.600712Z","submitted_at":"2025-06-03T14:15:25Z","title":"Test Gravitational-Wave Polarizations with Space-Based Detectors","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T11:20:51.276132Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2506.02909"},"observation_digest":"sha256:d29e3c0bfe0d4a5fd126b47861e651aefe33fa94e43332e4f1060622f8abc8b2","observation_id":"19c711d9-9775-40db-ba30-39143a916bd4","resolution":{"observed_at":"2026-08-07T11:20:51.276132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-07T10:33:12.790550Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.05180","last_updated":"2025-06-09T15:14:05Z","snapshot_observed_at":"2026-08-08T09:25:11.125753Z","submitted_at":"2025-06-05T15:52:40Z","title":"Viscosity in Isotropic Cosmological Backgrounds in General Relativity and Starobinsky Gravity","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T10:33:12.790550Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2506.05180"},"observation_digest":"sha256:c6415150b49f05c473e20aae3d2db0c5c1d87c5a584439bf3808dcb4fe11d27f","observation_id":"6f6f2d7c-e9c7-4efa-b376-80326965d1f3","resolution":{"observed_at":"2026-08-07T10:33:12.790550Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-06T19:40:04.649752Z","title":"Belgacem et al., Testing modified gravity at cosmological distances with LISA standard sirens, JCAP 2019 (2019) 024 [ 1906.01593]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.05130","last_updated":"2025-07-07T15:42:39Z","snapshot_observed_at":"2026-08-08T08:58:37.504898Z","submitted_at":"2025-07-07T15:42:39Z","title":"Science of the LISA mission: A Summary for the European Strategy for Particle Physics","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.649752Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2507.05130"},"observation_digest":"sha256:c9675f76df8f239ff42915ab0fea14df4f9359190cebf21633a455d06dc1507f","observation_id":"4771ad12-6eee-48b6-a29e-a31461e22d61","resolution":{"observed_at":"2026-08-06T19:40:04.649752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":"1906.01593","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Belgacemet al.(LISA Cosmology Working Group), J","venue":null,"work_id":"36ce1202-ac50-4a17-8333-cfc7d91c3382","year":2019},"citing_paper":{"arxiv_id":"2507.11526","last_updated":"2026-04-13T15:58:35Z","snapshot_observed_at":"2026-08-06T04:32:47.975396Z","submitted_at":"2025-07-15T17:54:46Z","title":"Gravitational wave propagation in bigravity in the late universe","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-19T04:22:07.751835Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2507.11526"},"observation_digest":"sha256:3d17e5e596d055dc7a21f16a2eb1fabfe67ba77f57462f71ca20e9f672e8639d","observation_id":"10d1d3f3-67d7-43ba-8d60-6f9082715c6b","resolution":{"observed_at":"2026-05-19T04:22:58.732295Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-06T15:30:07.474599Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.15791","last_updated":"2025-07-21T16:49:54Z","snapshot_observed_at":"2026-08-07T08:57:10.167437Z","submitted_at":"2025-07-21T16:49:54Z","title":"\\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T15:30:07.474599Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2507.15791"},"observation_digest":"sha256:e5bc35b9653003f5e3622fbfa05fe6d8d6b89f08a9a5b7547b71250913560e3d","observation_id":"cc8c89c8-5c29-4ef0-9c61-7e39300659f4","resolution":{"observed_at":"2026-08-06T15:30:07.474599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-05T21:42:56.783077Z","title":"Belgacem et al., Testing modified gravity at cosmological distances with LISA standard sirens , JCAP 07 (2019) 024 [arXiv:1906.01593]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.08481","last_updated":"2025-08-11T21:34:05Z","snapshot_observed_at":"2026-08-08T22:29:55.585274Z","submitted_at":"2025-08-11T21:34:05Z","title":"Oscillations and parity violation in gravitational wave background from extra tensor modes","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-05T21:42:56.783077Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2508.08481"},"observation_digest":"sha256:2e71fd35e397c6fc23e79e611896a75ab3551ed4a6558fe2d32f33e86755a56d","observation_id":"89834742-29bc-4c1d-9d95-ccfdcd2b76cb","resolution":{"observed_at":"2026-08-05T21:42:56.783077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-03T06:51:32.499202Z","title":"Belgacemet al.(LISA Cosmology Working Group), Testing modified gravity at cosmological distances with LISA standard sirens, JCAP07, 024, arXiv:1906.01593 [astro-ph.CO]","venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2601.21820","last_updated":"2026-05-28T08:19:01Z","snapshot_observed_at":"2026-08-04T07:08:45.728834Z","submitted_at":"2026-01-29T15:04:37Z","title":"Forecasting Constraints on Cosmology and Modified Gravitational-wave Propagation by Combining Strongly Lensed Gravitational Waves and Galaxy Surveys","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-03T06:51:32.499202Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2601.21820"},"observation_digest":"sha256:521c56579a7fa71af4d74dc47f5e30a3b66ff87bbbd2fb9091566657794bbaf7","observation_id":"e4003810-eda1-4c58-a9db-23d9a44d4112","resolution":{"observed_at":"2026-08-03T06:51:32.499202Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":"1906.01593","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Belgacemet al.(LISA Cosmology Working Group), J","venue":null,"work_id":"36ce1202-ac50-4a17-8333-cfc7d91c3382","year":2019},"citing_paper":{"arxiv_id":"2604.18669","last_updated":"2026-07-28T01:00:57Z","snapshot_observed_at":"2026-08-03T14:07:40.419983Z","submitted_at":"2026-04-20T17:59:41Z","title":"Hawking area law in quantum gravity","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-10T04:35:35.798089Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2604.18669"},"observation_digest":"sha256:24bcc000cca41f0cdb2eec5f6deb25ecfe09b6b3c9da6d5ec36e41b837e94c79","observation_id":"1a5dd238-5e44-4e3b-9b64-eaa5578b3e65","resolution":{"observed_at":"2026-05-10T12:15:22.641230Z","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":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-02T15:57:48.084997Z","title":"Belgacemet al.[LISA Cosmology Working Group], Testing modified gravity at cosmological distances with LISA standard sirens,JCAP07(2019) 024 [arXiv:1906.01593]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2604.18669","last_updated":"2026-07-28T01:00:57Z","snapshot_observed_at":"2026-08-03T14:07:40.419983Z","submitted_at":"2026-04-20T17:59:41Z","title":"Hawking area law in quantum gravity","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-02T15:57:48.084997Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2604.18669"},"observation_digest":"sha256:b75b3517bb03147d11419e44f641148478d68ee07f173b294ac32134ce9c1dc5","observation_id":"afab1025-50ca-4197-9241-5882ea272b02","resolution":{"observed_at":"2026-08-02T15:57:48.084997Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":"1906.01593","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Belgacemet al.(LISA Cosmology Working Group), J","venue":null,"work_id":"36ce1202-ac50-4a17-8333-cfc7d91c3382","year":2019},"citing_paper":{"arxiv_id":"2605.13036","last_updated":"2026-05-13T05:44:47Z","snapshot_observed_at":"2026-07-06T23:24:37.915639Z","submitted_at":"2026-05-13T05:44:47Z","title":"Inspiral gravitational waveforms from charged compact binaries with scalar hair","version":1},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-05-14T19:13:22.485254Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2605.13036"},"observation_digest":"sha256:f8ff6f7646f2816119130724d95c0a1e55ce40c20a8462cddd99125a57eee537","observation_id":"23598f96-a409-40be-9813-aeb7be3862d8","resolution":{"observed_at":"2026-05-14T19:17:51.230160Z","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":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":"1906.01593","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Belgacemet al.(LISA Cosmology Working Group), J","venue":null,"work_id":"36ce1202-ac50-4a17-8333-cfc7d91c3382","year":2019},"citing_paper":{"arxiv_id":"2605.20112","last_updated":"2026-05-19T16:59:39Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-19T16:59:39Z","title":"Gravitational-wave constraints on $H_0$ are robust to (putative) redshift evolution in the binary black hole mass spectrum at current sensitivity","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-20T03:45:08.000706Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2605.20112"},"observation_digest":"sha256:ac342a33591e91ce17c799c3bd00265164191c53b103fbb4c2f9c216046eeced","observation_id":"029898b2-a98e-4a65-b671-1c64425d30be","resolution":{"observed_at":"2026-05-20T03:48:02.877607Z","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":"1906.01593","last_updated":"2019-07-04T12:23:27Z","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01593","snapshot_observed_at":"2026-08-01T09:44:08.485311Z","title":"Belgacemet al.(LISA Cosmology Working Group), JCAP 07, 024 (2019), arXiv:1906.01593 [astro-ph.CO]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.20689","last_updated":"2026-07-22T19:39:33Z","snapshot_observed_at":"2026-08-01T18:38:10.599796Z","submitted_at":"2026-07-22T19:39:33Z","title":"Gravitational Wave Birefringence in generalized Palatini Chern Simons","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-01T09:44:08.485311Z"},"links":{"cited_paper":"/paper/1906.01593","citing_paper":"/paper/2607.20689"},"observation_digest":"sha256:6b78598cb7ed9767b4f6ed23c2227c90488538cf7dbecc0a2d37cf15ed2cc669","observation_id":"f087052b-4216-4b0b-b2cc-0ad33848097c","resolution":{"observed_at":"2026-08-01T09:44:08.485311Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1906.01593/citation-record","integrity":"/paper/1906.01593/integrity","json":"/paper/1906.01593/citation-record.json","paper":"/paper/1906.01593"},"outbound":[],"paper":{"arxiv_id":"1906.01593","last_updated":"2019-07-04T12:23:27Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T07:57:54.536249Z","submitted_at":"2019-06-04T17:09:36Z","title":"Testing modified gravity at cosmological distances with LISA standard sirens"},"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 16 inbound Pith citation observations for arXiv:1906.01593."}