{"as_of":"2026-08-15T03:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ec4d732e3b3af8e2d104127c9b6de203b295c2c98d2b0e7fe86b58c5966267f9","coverage":[{"denominator":177,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:57:58.665129Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/1908.07892/citation-record","integrity":"/paper/1908.07892/integrity","json":"/paper/1908.07892/citation-record.json","paper":"/paper/1908.07892"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"hep-th/0603057","last_updated":"2006-06-16T10:46:50Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2006-03-08T01:25:15Z","title":"Dynamics of dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0603057","snapshot_observed_at":"2026-08-14T11:57:58.237388Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.237388Z"},"links":{"cited_paper":"/paper/hep-th/0603057","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:4b9b4caf132940fbc75628fbb781ae9297e659e4018e07326bcdcec582f1c90f","observation_id":"971426b3-b888-4967-babc-cfee674e4be4","resolution":{"observed_at":"2026-08-14T11:57:58.237388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.2476","last_updated":"2012-03-12T12:39:47Z","snapshot_observed_at":"2026-07-06T02:29:12.672489Z","submitted_at":"2011-06-13T16:06:49Z","title":"Modified Gravity and Cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.2476","snapshot_observed_at":"2026-08-14T11:57:58.242469Z","title":"Clifton, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.242469Z"},"links":{"cited_paper":"/paper/1106.2476","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:11a4bc1f845948ff656bf9ae93f11cf34b8c4f67ab85f26efe1002ed20f74127","observation_id":"a39d8202-e89e-42f3-9524-19da6564da51","resolution":{"observed_at":"2026-08-14T11:57:58.242469Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.0059","last_updated":"2014-12-15T03:38:57Z","snapshot_observed_at":"2026-08-14T23:28:27.549351Z","submitted_at":"2014-06-30T21:20:56Z","title":"Beyond the Cosmological Standard Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.0059","snapshot_observed_at":"2026-08-14T11:57:58.247215Z","title":"Joyce, B","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.247215Z"},"links":{"cited_paper":"/paper/1407.0059","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:099598902d8e1e47d2a91d90452114d893ea6faa56578c8b13fe4d2c9c975645","observation_id":"6f340eb4-04df-4da2-a92b-d78510faf129","resolution":{"observed_at":"2026-08-14T11:57:58.247215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.04623","last_updated":"2016-03-23T18:19:38Z","snapshot_observed_at":"2026-08-14T22:52:01.184620Z","submitted_at":"2015-04-17T20:00:48Z","title":"Cosmological Tests of Modified Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.04623","snapshot_observed_at":"2026-08-14T11:57:58.251650Z","title":"Koyama, Reports on Progress in Physics 79 (April 2016) 046902, arXiv:1504.04623","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.251650Z"},"links":{"cited_paper":"/paper/1504.04623","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:373c770dea48bd676e9467f6ed7e764d43b2b0494cbbca51ec89c58638f20899","observation_id":"f5d37931-b642-4812-a3e1-bd2a11f34acc","resolution":{"observed_at":"2026-08-14T11:57:58.251650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.05356","last_updated":"2016-03-07T17:44:28Z","snapshot_observed_at":"2026-08-14T22:18:10.971021Z","submitted_at":"2015-12-16T21:00:05Z","title":"Beyond $\\Lambda$CDM: Problems, solutions, and the road ahead","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.05356","snapshot_observed_at":"2026-08-14T11:57:58.256873Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.256873Z"},"links":{"cited_paper":"/paper/1512.05356","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:cea53e9d093180a72044f6226a33c4e33cf415710db11bf3b18567bfa0bf9f07","observation_id":"6b669d55-9d10-44d1-84da-68cc8a4f2140","resolution":{"observed_at":"2026-08-14T11:57:58.256873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.06133","last_updated":"2016-06-14T21:52:31Z","snapshot_observed_at":"2026-08-14T22:13:28.709401Z","submitted_at":"2016-01-22T20:03:44Z","title":"Dark Energy vs. Modified Gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.06133","snapshot_observed_at":"2026-08-14T11:57:58.261554Z","title":"Joyce, L","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.261554Z"},"links":{"cited_paper":"/paper/1601.06133","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:7e9d461500208a5aef0bc07ce090db916b645d90d0db6f991d528c1fc9f0371f","observation_id":"4502a2cf-4f78-40d3-a3aa-2f7fe4c8121b","resolution":{"observed_at":"2026-08-14T11:57:58.261554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.10122","last_updated":"2018-12-31T15:05:32Z","snapshot_observed_at":"2026-08-14T18:58:55.704699Z","submitted_at":"2018-06-26T17:40:47Z","title":"Testing General Relativity in Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.10122","snapshot_observed_at":"2026-08-14T11:57:58.266426Z","title":"Ishak, ArXiv e-prints (June 2018) arXiv:1806.10122","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.266426Z"},"links":{"cited_paper":"/paper/1806.10122","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:72ac01aeb2fd9fd5b53beafa8fc1ac378b854d4bf4a9fff9bf8c003df2457913","observation_id":"260204e5-8025-4381-a933-a5f99d0b8655","resolution":{"observed_at":"2026-08-14T11:57:58.266426Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.270517Z","title":null,"venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.270517Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:aaefba05dfcba6a27b033d453abf0523efac8391a803592624c2a0a36f6c732b","observation_id":"2e6154e8-cf98-445f-96cf-318800bd7564","resolution":{"observed_at":"2026-08-14T11:57:58.270517Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.274311Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.274311Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:ea64d0ee56933e27e23ee86100dde1a55f855f6f9c952363681874dda0dd4a88","observation_id":"7ad35eff-3793-481d-93ec-bcb2c0153c19","resolution":{"observed_at":"2026-08-14T11:57:58.274311Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.7377","last_updated":"2014-03-28T14:04:31Z","snapshot_observed_at":"2026-08-12T13:37:17.409976Z","submitted_at":"2014-03-28T14:04:31Z","title":"The Confrontation between General Relativity and Experiment","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.7377","snapshot_observed_at":"2026-08-14T11:57:58.277970Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.277970Z"},"links":{"cited_paper":"/paper/1403.7377","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:5507b2c65bf3bb5e06f0385c2dde0685eb7826306cc0beebc0b4ebb91dd23377","observation_id":"6c2d7452-ca0b-4134-80bc-54c7e80b090f","resolution":{"observed_at":"2026-08-14T11:57:58.277970Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01985","last_updated":"2015-06-26T06:13:15Z","snapshot_observed_at":"2026-08-14T23:04:44.008225Z","submitted_at":"2015-01-08T21:07:01Z","title":"The Parametrized Post-Newtonian-Vainshteinian Formalism","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.01985","snapshot_observed_at":"2026-08-14T11:57:58.282110Z","title":"Avilez-Lopez, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.282110Z"},"links":{"cited_paper":"/paper/1501.01985","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:28eb8a1ce1b1418d7b4f3d18534d6fb994f7d08ca31608f7800dc40edd39a238","observation_id":"2542330c-98be-4674-8009-5f697d425366","resolution":{"observed_at":"2026-08-14T11:57:58.282110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.05324","last_updated":"2017-05-18T13:11:21Z","snapshot_observed_at":"2026-08-14T21:00:37.605205Z","submitted_at":"2017-05-15T16:46:17Z","title":"Parameterised Post-Newtonian Expansion in Screened Regions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.05324","snapshot_observed_at":"2026-08-14T11:57:58.286023Z","title":"McManus, L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.286023Z"},"links":{"cited_paper":"/paper/1705.05324","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:7325bc7d7fe091d17e9a8b3047d7d2934b7fa2080bac1a6292bfff2e63db1099","observation_id":"f12ee744-e114-476a-88d4-d7408d31c4d0","resolution":{"observed_at":"2026-08-14T11:57:58.286023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0605313","last_updated":"2006-05-12T08:14:29Z","snapshot_observed_at":"2026-08-07T15:43:31.455004Z","submitted_at":"2006-05-12T08:14:29Z","title":"The acceleration of the universe and the physics behind it","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0605313","snapshot_observed_at":"2026-08-14T11:57:58.289786Z","title":"Uzan, ArXiv Astrophysics e-prints (May 2006) astro-ph/0605313","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.289786Z"},"links":{"cited_paper":"/paper/astro-ph/0605313","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:aa4c0d2a164efe70971ac3fe222b133081cd3c65298ce97b017f999f9e06f0eb","observation_id":"3b8a1d38-1636-49fc-8f9a-f8525d2cc883","resolution":{"observed_at":"2026-08-14T11:57:58.289786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703375","last_updated":"2007-03-30T17:49:24Z","snapshot_observed_at":"2026-07-07T01:08:03.830352Z","submitted_at":"2007-03-14T21:43:38Z","title":"Constraints on a New Post-General Relativity Cosmological Parameter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703375","snapshot_observed_at":"2026-08-14T11:57:58.293812Z","title":"Caldwell, A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.293812Z"},"links":{"cited_paper":"/paper/astro-ph/0703375","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:02a72e612678c55073f586b08abb11e67f709146583f49a3a0abae7cce8d9471","observation_id":"fb4e165a-9edc-4570-b56a-c25eb16acf15","resolution":{"observed_at":"2026-08-14T11:57:58.293812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.297584Z","title":"Zhang, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.297584Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:4255583b04a13cbc02cc2692b164f86f26a4a746061b5ee39ac3fcf7fedf4c83","observation_id":"5813d239-226b-49f1-b033-d5788cbcdbfb","resolution":{"observed_at":"2026-08-14T11:57:58.297584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0704.2421","last_updated":"2007-04-19T10:12:22Z","snapshot_observed_at":"2026-07-06T01:26:31.626011Z","submitted_at":"2007-04-19T10:12:22Z","title":"Measuring the dark side (with weak lensing)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0704.2421","snapshot_observed_at":"2026-08-14T11:57:58.304920Z","title":"Amendola, M","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.304920Z"},"links":{"cited_paper":"/paper/0704.2421","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:50c7beb348d28f5d1f91576f36eadbe5b600a449815b753c0fae84986ddd474d","observation_id":"873b284f-a6d1-4be1-bd7a-aaccf1c0442d","resolution":{"observed_at":"2026-08-14T11:57:58.304920Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0708.1190","last_updated":"2007-10-12T03:31:48Z","snapshot_observed_at":"2026-07-06T01:32:55.429526Z","submitted_at":"2007-08-08T22:29:27Z","title":"A Parameterized Post-Friedmann Framework for Modified Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0708.1190","snapshot_observed_at":"2026-08-14T11:57:58.308770Z","title":"Hu and I","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.308770Z"},"links":{"cited_paper":"/paper/0708.1190","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:bc91618822292d457e559422b3bf9c0c211926c0abe7195f6ffa569279d5ed47","observation_id":"78f195aa-d042-4c06-97a0-df527184e4f7","resolution":{"observed_at":"2026-08-14T11:57:58.308770Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0101354","last_updated":"2002-09-17T20:59:20Z","snapshot_observed_at":"2026-07-07T00:15:25.881918Z","submitted_at":"2001-01-22T23:53:15Z","title":"Measuring the metric: a parametrized post-Friedmanian approach to the cosmic dark energy problem","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0101354","snapshot_observed_at":"2026-08-14T11:57:58.312882Z","title":"Tegmark, Phys","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.312882Z"},"links":{"cited_paper":"/paper/astro-ph/0101354","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:b73822f49f9c74df00a0e74c7b43ec1b21ece821782800eab3a6073a85e443a7","observation_id":"dc2d7b4b-4440-4e1c-831f-94d8b93d9e9a","resolution":{"observed_at":"2026-08-14T11:57:58.312882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.2117","last_updated":"2013-02-07T17:57:42Z","snapshot_observed_at":"2026-08-15T00:47:12.624567Z","submitted_at":"2012-09-10T20:00:01Z","title":"The Parameterized Post-Friedmann Framework for Theories of Modified Gravity: Concepts, Formalism and Examples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.2117","snapshot_observed_at":"2026-08-14T11:57:58.317072Z","title":"Baker, P","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.317072Z"},"links":{"cited_paper":"/paper/1209.2117","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:c32cfbc0b0706b2233c79c6351ac2c4c81ef682d5d615a4ab3ef097f99f89c57","observation_id":"fe5b3ead-dfef-45ca-9ef6-f485005ae205","resolution":{"observed_at":"2026-08-14T11:57:58.317072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.320591Z","title":null,"venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.320591Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:31d1fa6524db947b574d759bf074faff236caf7c5b2ab16042dcf4696a0d82b7","observation_id":"987bd648-5db6-47e7-b86f-ff950f8255ec","resolution":{"observed_at":"2026-08-14T11:57:58.320591Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507263","last_updated":"2005-08-16T00:28:03Z","snapshot_observed_at":"2026-07-07T00:52:09.097911Z","submitted_at":"2005-07-11T20:00:08Z","title":"Cosmic Growth History and Expansion History","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507263","snapshot_observed_at":"2026-08-14T11:57:58.324216Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.324216Z"},"links":{"cited_paper":"/paper/astro-ph/0507263","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:00109c584ae66ea96821f5a6638377061a8227283d2e1bc850e856e12f80100f","observation_id":"5e459748-1fc5-4602-8fed-5e153824043f","resolution":{"observed_at":"2026-08-14T11:57:58.324216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.0827","last_updated":"2009-02-16T23:40:21Z","snapshot_observed_at":"2026-07-06T01:47:37.043519Z","submitted_at":"2008-11-05T22:25:10Z","title":"The Effective Theory of Quintessence: the w<-1 Side Unveiled","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.0827","snapshot_observed_at":"2026-08-14T11:57:58.328332Z","title":"Creminelli, G","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.328332Z"},"links":{"cited_paper":"/paper/0811.0827","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:a1092d03256fb44ac804350c323862fce7d3c5bdc0fa4ab1a51caa3bb788984a","observation_id":"65285cb1-5469-4471-be4a-e486e4f6b77f","resolution":{"observed_at":"2026-08-14T11:57:58.328332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.1722","last_updated":"2010-03-23T21:03:11Z","snapshot_observed_at":"2026-08-01T19:17:00.699466Z","submitted_at":"2010-03-08T21:01:36Z","title":"A Unified Approach to Cosmic Acceleration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.1722","snapshot_observed_at":"2026-08-14T11:57:58.332246Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.332246Z"},"links":{"cited_paper":"/paper/1003.1722","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:ef5b38a0c03a932603dfa82a08e4d363c589b0dbd8469049600a040244f6686d","observation_id":"592cb20f-6fb5-4f77-84b4-99d5c902eaff","resolution":{"observed_at":"2026-08-14T11:57:58.332246Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.0201","last_updated":"2013-02-17T21:28:56Z","snapshot_observed_at":"2026-08-15T00:44:52.107192Z","submitted_at":"2012-09-30T13:54:32Z","title":"The Effective Field Theory of Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.0201","snapshot_observed_at":"2026-08-14T11:57:58.336124Z","title":"Gubitosi, F","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.336124Z"},"links":{"cited_paper":"/paper/1210.0201","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:5fbdcc43e6d3697817b6fde7e1db8a691370f554bcd2c0c767b59f391b2e4bec","observation_id":"fcdafc33-2ce9-4612-b077-fc1dae691cb7","resolution":{"observed_at":"2026-08-14T11:57:58.336124Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.7054","last_updated":"2013-09-23T16:21:02Z","snapshot_observed_at":"2026-08-15T00:37:41.009869Z","submitted_at":"2012-11-29T20:58:55Z","title":"Dark Energy or Modified Gravity? An Effective Field Theory Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.7054","snapshot_observed_at":"2026-08-14T11:57:58.340193Z","title":"Bloomfield, ´E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.340193Z"},"links":{"cited_paper":"/paper/1211.7054","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:844f01517956cf735713fe8ca8478f31d44fe78d81710f3cd0d60c5ca834c8ff","observation_id":"84e6c2a7-ebea-4264-b112-918e44786b74","resolution":{"observed_at":"2026-08-14T11:57:58.340193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.4840","last_updated":"2013-09-06T16:59:30Z","snapshot_observed_at":"2026-08-15T00:21:07.619987Z","submitted_at":"2013-04-17T14:36:06Z","title":"Essential Building Blocks of Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.4840","snapshot_observed_at":"2026-08-14T11:57:58.345084Z","title":"Gleyzes, D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.345084Z"},"links":{"cited_paper":"/paper/1304.4840","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:62b86d7aafb84aa83f942caa35476cbc320d970f797db8832ec32f8a025d78d1","observation_id":"ff61f389-2920-4e91-bf88-702893f10db4","resolution":{"observed_at":"2026-08-14T11:57:58.345084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.2684","last_updated":"2014-09-01T05:27:42Z","snapshot_observed_at":"2026-08-14T23:38:00.928850Z","submitted_at":"2014-04-10T03:56:55Z","title":"The effective field theory of inflation/dark energy and the Horndeski theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.2684","snapshot_observed_at":"2026-08-14T11:57:58.348945Z","title":"Tsujikawa, Lect","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.348945Z"},"links":{"cited_paper":"/paper/1404.2684","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:b64e269c400e1e7c2d4fc9523b75cc5c0901c21c1eac798a575a7da75213db0f","observation_id":"f9c08623-b48a-412f-b036-797a4fed1928","resolution":{"observed_at":"2026-08-14T11:57:58.348945Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.3713","last_updated":"2014-06-17T19:40:04Z","snapshot_observed_at":"2026-08-14T23:37:32.949304Z","submitted_at":"2014-04-14T19:51:27Z","title":"Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.3713","snapshot_observed_at":"2026-08-14T11:57:58.353006Z","title":"Bellini and I","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.353006Z"},"links":{"cited_paper":"/paper/1404.3713","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:730ee732c595d26b6f447a6c89b8d8ca28d69970eb25db28fd8348bd7cb9954f","observation_id":"0506c0c9-d89d-421c-992a-42ce6ed9ea68","resolution":{"observed_at":"2026-08-14T11:57:58.353006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.3712","last_updated":"2015-01-22T20:52:39Z","snapshot_observed_at":"2026-08-14T23:11:42.463509Z","submitted_at":"2014-11-13T20:56:05Z","title":"A unifying description of dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.3712","snapshot_observed_at":"2026-08-14T11:57:58.357101Z","title":"Gleyzes, D","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.357101Z"},"links":{"cited_paper":"/paper/1411.3712","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:85335bb3756f3492415b1a28bfc4feb106a2f0b5c253d4bab16468b136243e66","observation_id":"f16543e2-53ee-4f81-8746-186688acd654","resolution":{"observed_at":"2026-08-14T11:57:58.357101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.361135Z","title":"Lagos, E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.361135Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:a4a0ca3a5801345dbaffc6160cfb7d014113020cfbf426e6cfeeb812284c2daf","observation_id":"be072b93-4b20-4df4-bfa2-69973feae335","resolution":{"observed_at":"2026-08-14T11:57:58.361135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0902.0618","last_updated":"2009-06-09T18:54:35Z","snapshot_observed_at":"2026-07-06T01:49:38.051358Z","submitted_at":"2009-02-04T18:55:45Z","title":"Non-linear Evolution of Matter Power Spectrum in Modified Theory of Gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0902.0618","snapshot_observed_at":"2026-08-14T11:57:58.369006Z","title":"Koyama, A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.369006Z"},"links":{"cited_paper":"/paper/0902.0618","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:0e5b2f241bbf1d65451eac6be214cf295219a9f4418785727c29e0c21304e0b1","observation_id":"d27830b7-0995-4ebd-b815-c85ba55835d0","resolution":{"observed_at":"2026-08-14T11:57:58.369006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.4812","last_updated":"2012-03-28T23:42:54Z","snapshot_observed_at":"2026-07-06T02:44:58.674531Z","submitted_at":"2012-03-21T20:00:00Z","title":"A Unified Description of Screened Modified Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.4812","snapshot_observed_at":"2026-08-14T11:57:58.373161Z","title":"Brax, A.-C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.373161Z"},"links":{"cited_paper":"/paper/1203.4812","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:9edaaa1035a1d0a7646d4250d454f73a91ff90cc00fa147a432888cf406c4cda","observation_id":"403fd58f-e03b-4b02-b464-4bb8c5ff6578","resolution":{"observed_at":"2026-08-14T11:57:58.373161Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.04341","last_updated":"2015-05-12T09:14:47Z","snapshot_observed_at":"2026-08-14T22:52:08.460838Z","submitted_at":"2015-04-16T19:07:13Z","title":"Signatures of Horndeski gravity on the Dark Matter Bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.04341","snapshot_observed_at":"2026-08-14T11:57:58.377209Z","title":"Bellini, R","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.377209Z"},"links":{"cited_paper":"/paper/1504.04341","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:15cabad1910dc0040786479172e61dc40834cb14a5fe4c3af00445e53c0e0d9e","observation_id":"a789ac5d-170b-4160-a078-0fbddd2412b4","resolution":{"observed_at":"2026-08-14T11:57:58.377209Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.02168","last_updated":"2016-06-07T15:10:26Z","snapshot_observed_at":"2026-08-14T21:53:50.102574Z","submitted_at":"2016-06-07T15:10:26Z","title":"Constructing perturbation theory kernels for large-scale structure in generalized cosmologies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.02168","snapshot_observed_at":"2026-08-14T11:57:58.381110Z","title":"Taruya, Physical Review D 94 (July 2016) 023504, arXiv:1606.02168","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.381110Z"},"links":{"cited_paper":"/paper/1606.02168","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:5e8d78fd5d5f16635dd7680f3e660934c2ea46e6ae861b7ae027e320c3758af2","observation_id":"57a4252d-5432-4cbf-85ae-95fd4f7ae81e","resolution":{"observed_at":"2026-08-14T11:57:58.381110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.384788Z","title":"Bose and K","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.384788Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:23d89eec77252471ca70a9215074e6425eb15f58cbe66ef39a131618aa2e8caf","observation_id":"137bb6ca-63d7-4e83-b5bc-28dbe6a4fa85","resolution":{"observed_at":"2026-08-14T11:57:58.384788Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.03243","last_updated":"2017-09-11T05:21:41Z","snapshot_observed_at":"2026-08-14T20:34:29.994230Z","submitted_at":"2017-09-11T05:21:41Z","title":"Constraining modified theory of gravity with galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.03243","snapshot_observed_at":"2026-08-14T11:57:58.392436Z","title":"Yamauchi, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.392436Z"},"links":{"cited_paper":"/paper/1709.03243","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:119a2c53c90319164d2874bcf9ef1b096ea6426e84923f45a5f6d8842cfdb2b5","observation_id":"75188eb6-1cfa-4b1b-a5c8-5d37e98c4c32","resolution":{"observed_at":"2026-08-14T11:57:58.392436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.02719","last_updated":"2017-11-29T11:32:54Z","snapshot_observed_at":"2026-08-14T20:55:12.839706Z","submitted_at":"2017-06-08T18:05:43Z","title":"Tackling non-linearities with the effective field theory of dark energy and modified gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.02719","snapshot_observed_at":"2026-08-14T11:57:58.396353Z","title":"Frusciante and G","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.396353Z"},"links":{"cited_paper":"/paper/1706.02719","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:22106450e309c5c575ed4acdf59b5cab77d62d2a3cf3cb53ceb1c6591074f55f","observation_id":"fb9db78c-e3fa-4202-8252-9d18a1d2e762","resolution":{"observed_at":"2026-08-14T11:57:58.396353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.01566","last_updated":"2018-05-07T15:38:58Z","snapshot_observed_at":"2026-08-14T19:48:44.532549Z","submitted_at":"2018-02-05T18:55:05Z","title":"Towards Precision Constraints on Gravity with the Effective Field Theory of Large-Scale Structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.01566","snapshot_observed_at":"2026-08-14T11:57:58.400308Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.400308Z"},"links":{"cited_paper":"/paper/1802.01566","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:ab800e9c9f9a2a4ca61da649f95171747d782412a5aa828a8798b1d355d99625","observation_id":"64d04e16-a66e-49ec-87e3-6a2f54d28276","resolution":{"observed_at":"2026-08-14T11:57:58.400308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.07885","last_updated":"2018-05-23T10:34:28Z","snapshot_observed_at":"2026-08-14T19:52:32.023077Z","submitted_at":"2018-01-24T07:36:41Z","title":"Matter bispectrum beyond Horndeski","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.07885","snapshot_observed_at":"2026-08-14T11:57:58.404122Z","title":"Hirano, T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.404122Z"},"links":{"cited_paper":"/paper/1801.07885","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:2b885f712da9ebcf32b9ce9a2286ef1ee8a9ca0a6b135e09f91bb5328b89fa79","observation_id":"fd85042b-21fe-4144-aada-7a563d349844","resolution":{"observed_at":"2026-08-14T11:57:58.404122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.1257","last_updated":"2010-11-15T16:59:43Z","snapshot_observed_at":"2026-07-06T02:18:44.164256Z","submitted_at":"2010-11-04T20:00:02Z","title":"N-body Simulations for f(R) Gravity using a Self-adaptive Particle-Mesh Code","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.1257","snapshot_observed_at":"2026-08-14T11:57:58.408187Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.408187Z"},"links":{"cited_paper":"/paper/1011.1257","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:2c2a9d6e1fec842a0ce7bc7badab6ed45f050929274fe54f5143e23a7cb88571","observation_id":"83c8d7e2-878e-4f51-952a-4cd58454bc39","resolution":{"observed_at":"2026-08-14T11:57:58.408187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.00522","last_updated":"2016-08-01T18:52:16Z","snapshot_observed_at":"2026-08-14T21:45:54.148495Z","submitted_at":"2016-08-01T18:52:16Z","title":"A parametrisation of modified gravity on nonlinear cosmological scales","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.00522","snapshot_observed_at":"2026-08-14T11:57:58.412182Z","title":"Lombriser, Journal of Cosmology and Astroparticle Physics 11 (November 2016) 039, arXiv:1608.00522","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.412182Z"},"links":{"cited_paper":"/paper/1608.00522","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:51627f3e10c77ec854a695d3ed499a79d488c1e9cecd8acc3a95e8c71ae761a2","observation_id":"1712c1af-6442-440b-ad30-c3509e150066","resolution":{"observed_at":"2026-08-14T11:57:58.412182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.09017","last_updated":"2017-12-25T06:53:17Z","snapshot_observed_at":"2026-08-14T20:00:19.354818Z","submitted_at":"2017-12-25T06:53:17Z","title":"CHAM: a fast algorithm of modelling non-linear matter power spectrum in the sCreened HAlo Model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.09017","snapshot_observed_at":"2026-08-14T11:57:58.416121Z","title":"Hu, X.-W","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.416121Z"},"links":{"cited_paper":"/paper/1712.09017","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:0ff65935dd22da54e72ee49f23ad600c7adfd6650d70b3c4839c17d09f85c24f","observation_id":"c03c6fbf-e4d4-4b6d-a65f-375a5e4ab954","resolution":{"observed_at":"2026-08-14T11:57:58.416121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.08039","last_updated":"2017-02-22T21:39:07Z","snapshot_observed_at":"2026-08-14T21:33:35.303772Z","submitted_at":"2016-10-25T19:46:12Z","title":"Parameterized Post-Newtonian Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.08039","snapshot_observed_at":"2026-08-14T11:57:58.420193Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.420193Z"},"links":{"cited_paper":"/paper/1610.08039","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:b642a70445521cc2c8f4f692d688d8a1aec6c99a3ede4566a8f6a958581b5c14","observation_id":"22886929-4733-47a0-b2bb-f2beb8daab19","resolution":{"observed_at":"2026-08-14T11:57:58.420193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.02985","last_updated":"2015-05-09T18:28:25Z","snapshot_observed_at":"2026-08-14T23:00:35.997053Z","submitted_at":"2015-02-10T16:55:12Z","title":"The missing link: a nonlinear post-Friedmann framework for small and large scales","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.02985","snapshot_observed_at":"2026-08-14T11:57:58.424175Z","title":"Milillo, D","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.424175Z"},"links":{"cited_paper":"/paper/1502.02985","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:24f150fa854c7e1a89290180371ffcff844f4b1bfef97bbc015b8775d20d24e0","observation_id":"d200dbd6-a023-4d1b-bb1a-02e4af38ace0","resolution":{"observed_at":"2026-08-14T11:57:58.424175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03837","last_updated":"2016-02-11T19:26:44Z","snapshot_observed_at":"2026-07-09T16:56:15.649302Z","submitted_at":"2016-02-11T19:26:44Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03837","snapshot_observed_at":"2026-08-14T11:57:58.428178Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.428178Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:60537a443d02ccebf379230604f96ac07fa1b8174d7869e6397870b2f6d7080e","observation_id":"3f475b1f-c3cd-4b4f-b4ea-2fe70063bbed","resolution":{"observed_at":"2026-08-14T11:57:58.428178Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09660","last_updated":"2017-10-13T09:37:56Z","snapshot_observed_at":"2026-08-14T20:28:59.478315Z","submitted_at":"2017-09-27T19:11:34Z","title":"GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.09660","snapshot_observed_at":"2026-08-14T11:57:58.432114Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.432114Z"},"links":{"cited_paper":"/paper/1709.09660","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:8041541952a2ed9cf9acba663e478786d3e4d2944224c1fe21acb94246caf7f9","observation_id":"343900e0-8e59-476f-bb2e-b76398923135","resolution":{"observed_at":"2026-08-14T11:57:58.432114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.3328","last_updated":"2009-12-07T17:14:47Z","snapshot_observed_at":"2026-07-06T01:57:40.790524Z","submitted_at":"2009-09-17T22:16:20Z","title":"Fundamental Theoretical Bias in Gravitational Wave Astrophysics and the Parameterized Post-Einsteinian Framework","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.3328","snapshot_observed_at":"2026-08-14T11:57:58.436419Z","title":"Yunes and F","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.436419Z"},"links":{"cited_paper":"/paper/0909.3328","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:8eb77bb86f00964624835885aa71dcb4848f9d0a9e5f7e920cd65d56345bd3ac","observation_id":"bfd14219-29e8-4b32-aa93-56280d345f11","resolution":{"observed_at":"2026-08-14T11:57:58.436419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.0530","last_updated":"2012-03-04T12:28:05Z","snapshot_observed_at":"2026-07-06T02:35:06.752411Z","submitted_at":"2011-10-03T22:06:11Z","title":"Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.0530","snapshot_observed_at":"2026-08-14T11:57:58.440636Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.440636Z"},"links":{"cited_paper":"/paper/1110.0530","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:621a7088b0e9a8aa1e859cd5911d23c69b87b85e67bb7160c1b0642130638b5e","observation_id":"c2106089-d417-4c1f-a062-c7b1db53fc39","resolution":{"observed_at":"2026-08-14T11:57:58.440636Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.4680","last_updated":"2013-05-12T19:05:47Z","snapshot_observed_at":"2026-08-15T00:31:59.085233Z","submitted_at":"2013-01-20T20:02:38Z","title":"Compact binary systems in scalar-tensor gravity: Equations of motion to 2.5 post-Newtonian order","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.4680","snapshot_observed_at":"2026-08-14T11:57:58.445394Z","title":"Mirshekari and C","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.445394Z"},"links":{"cited_paper":"/paper/1301.4680","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:eb972ac2c965eb907b536bbe7432cfde0cabf3032bd83884793bc4c9c058e81b","observation_id":"024a68d0-858a-423e-b8c0-f1c3e5e1fc7e","resolution":{"observed_at":"2026-08-14T11:57:58.445394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.3320","last_updated":"2014-04-12T01:19:19Z","snapshot_observed_at":"2026-08-14T23:59:15.077164Z","submitted_at":"2013-10-12T00:55:17Z","title":"Compact binary systems in scalar-tensor gravity. II. Tensor gravitational waves to second post-Newtonian order","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.3320","snapshot_observed_at":"2026-08-14T11:57:58.449667Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.449667Z"},"links":{"cited_paper":"/paper/1310.3320","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:dfd3a3c17358c07dcde694a2575a401490a8d747c36758021dc331cfe10afe9f","observation_id":"a2832f77-130c-4b83-83eb-9a53e0736822","resolution":{"observed_at":"2026-08-14T11:57:58.449667Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03841","last_updated":"2018-10-23T15:08:45Z","snapshot_observed_at":"2026-08-14T22:10:41.610545Z","submitted_at":"2016-02-11T19:26:48Z","title":"Tests of general relativity with GW150914","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03841","snapshot_observed_at":"2026-08-14T11:57:58.454139Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.454139Z"},"links":{"cited_paper":"/paper/1602.03841","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:ac0b31e6dbf8aaa2eb734443bd2f30c0f2194bda6bc7c36fb173e32b33d491b4","observation_id":"91f7bd51-ec01-4d31-be56-b99eb7f2e6da","resolution":{"observed_at":"2026-08-14T11:57:58.454139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.04856","last_updated":"2018-10-23T14:58:34Z","snapshot_observed_at":"2026-08-14T21:52:35.936458Z","submitted_at":"2016-06-15T16:44:05Z","title":"Binary Black Hole Mergers in the first Advanced LIGO Observing Run","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.04856","snapshot_observed_at":"2026-08-14T11:57:58.458235Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.458235Z"},"links":{"cited_paper":"/paper/1606.04856","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:fb0037330e56f1ae41e48f40ca2f0e0184ffe69cd1aaa5bec408c4fe1050fb06","observation_id":"4eed0b95-b82e-46f9-a211-d6248160213f","resolution":{"observed_at":"2026-08-14T11:57:58.458235Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.7139","last_updated":"2014-10-16T20:13:39Z","snapshot_observed_at":"2026-08-14T23:28:51.326633Z","submitted_at":"2014-06-27T10:15:07Z","title":"Anisotropic stress as signature of non-standard propagation of gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.7139","snapshot_observed_at":"2026-08-14T11:57:58.462425Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.462425Z"},"links":{"cited_paper":"/paper/1406.7139","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:5184619752669630213e73b3b723bb2ada9433b97b0ae05ce523d926001c494d","observation_id":"0036f0e3-024b-4f47-8927-b942f26d7692","resolution":{"observed_at":"2026-08-14T11:57:58.462425Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.08458","last_updated":"2016-02-18T20:46:10Z","snapshot_observed_at":"2026-08-14T22:30:29.682898Z","submitted_at":"2015-09-28T20:01:36Z","title":"Breaking a Dark Degeneracy with Gravitational Waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.08458","snapshot_observed_at":"2026-08-14T11:57:58.466650Z","title":"Lombriser and A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.466650Z"},"links":{"cited_paper":"/paper/1509.08458","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:921ce66d0dab147705c244a4a21b3b9740767e9940d88a192d5c446b7d516743","observation_id":"c35561b9-fcec-4d25-8fd0-59fb59f96263","resolution":{"observed_at":"2026-08-14T11:57:58.466650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.04825","last_updated":"2018-04-20T05:45:20Z","snapshot_observed_at":"2026-08-14T20:24:11.018355Z","submitted_at":"2017-10-13T06:56:43Z","title":"Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.04825","snapshot_observed_at":"2026-08-14T11:57:58.470584Z","title":"Nishizawa, ArXiv e-prints (October 2017) arXiv:1710.04825 [gr-qc]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.470584Z"},"links":{"cited_paper":"/paper/1710.04825","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:3af2605e987a5630ef8fe39e09f20ca71818ad08dd78628c7d050393fca1154c","observation_id":"14707ff4-3f5b-4a10-8263-f19f7573d5e0","resolution":{"observed_at":"2026-08-14T11:57:58.470584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0009008","last_updated":"2000-09-25T18:37:17Z","snapshot_observed_at":"2026-07-07T03:13:00.877347Z","submitted_at":"2000-09-04T15:09:00Z","title":"Accelerating Universes with Scaling Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0009008","snapshot_observed_at":"2026-08-14T11:57:58.474836Z","title":"Chevallier and D","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.474836Z"},"links":{"cited_paper":"/paper/gr-qc/0009008","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:491104ca89fb5b4af608af6dd510284c3af92f688bfab3e464126a779d5441f4","observation_id":"37fd01f3-d205-4626-8456-92f9f852f890","resolution":{"observed_at":"2026-08-14T11:57:58.474836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0208512","last_updated":"2002-08-28T23:21:10Z","snapshot_observed_at":"2026-07-07T00:28:09.066072Z","submitted_at":"2002-08-28T23:21:10Z","title":"Exploring the Expansion History of the Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0208512","snapshot_observed_at":"2026-08-14T11:57:58.479038Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.479038Z"},"links":{"cited_paper":"/paper/astro-ph/0208512","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:4a875dcebb6f80888a07a448ff12821ad14d6c87d61ba36e69b2e24ebfeb2228","observation_id":"f6ae2e41-7a6e-4855-9afb-28ce966743da","resolution":{"observed_at":"2026-08-14T11:57:58.479038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.07670","last_updated":"2016-07-06T13:22:43Z","snapshot_observed_at":"2026-08-14T22:08:56.585461Z","submitted_at":"2016-02-24T20:51:09Z","title":"Challenges to Self-Acceleration in Modified Gravity from Gravitational Waves and Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.07670","snapshot_observed_at":"2026-08-14T11:57:58.482996Z","title":"Lombriser and N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.482996Z"},"links":{"cited_paper":"/paper/1602.07670","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:f4b7cb992bda2fece742f165a47e51cfe9426605b74d018f5609e688ece59130","observation_id":"50118666-b27d-48e0-a459-bd79b7a50429","resolution":{"observed_at":"2026-08-14T11:57:58.482996Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03844","last_updated":"2017-11-08T15:29:09Z","snapshot_observed_at":"2026-08-14T20:15:39.634804Z","submitted_at":"2017-11-08T15:29:09Z","title":"Cosmology and the Fate of Dilatation Symmetry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03844","snapshot_observed_at":"2026-08-14T11:57:58.486998Z","title":"Wetterich, Nuclear Physics B 302 (June 1988) 668, arXiv:1711.03844 [hep-th]","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.486998Z"},"links":{"cited_paper":"/paper/1711.03844","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:3fc03258f04e090ad41fbe4761625042ba0d3010c967faba7fc0a5027adfe383","observation_id":"f97462ac-0b00-4e8a-b462-a0f601fa9924","resolution":{"observed_at":"2026-08-14T11:57:58.486998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.490845Z","title":"Ratra and P","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.490845Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:e137c65c198874cb72bfc409f65c519fdfa56da663a3f7778c8c1db3776769e8","observation_id":"d3a5eb83-953c-4a3c-abbf-c551b83c9784","resolution":{"observed_at":"2026-08-14T11:57:58.490845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510293","last_updated":"2009-12-02T19:58:44Z","snapshot_observed_at":"2026-07-07T00:54:52.114296Z","submitted_at":"2005-10-10T20:01:06Z","title":"Investigating dark energy experiments with principal components","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510293","snapshot_observed_at":"2026-08-14T11:57:58.494387Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.494387Z"},"links":{"cited_paper":"/paper/astro-ph/0510293","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:a8f2560a502862e82aee74e66211a9f008a339a789e61dfd8e987b61f2b94cea","observation_id":"968dfdf1-2f73-4796-9f89-08cb150c39fc","resolution":{"observed_at":"2026-08-14T11:57:58.494387Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0806.3415","last_updated":"2008-07-01T09:58:58Z","snapshot_observed_at":"2026-07-06T01:41:33.658168Z","submitted_at":"2008-06-20T15:31:48Z","title":"f(R) Gravity and Chameleon Theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.3415","snapshot_observed_at":"2026-08-14T11:57:58.498247Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.498247Z"},"links":{"cited_paper":"/paper/0806.3415","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:cc09c1b8437481911eec46e3970957bd627aeba1d46b2171cccf52ce1a3035c9","observation_id":"770526e9-e11f-4777-8766-c9b82126a59e","resolution":{"observed_at":"2026-08-14T11:57:58.498247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.1292","last_updated":"2014-11-13T11:49:39Z","snapshot_observed_at":"2026-08-14T23:52:52.711015Z","submitted_at":"2013-12-04T19:28:36Z","title":"Halo modelling in chameleon theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.1292","snapshot_observed_at":"2026-08-14T11:57:58.502024Z","title":"Lombriser, K","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.502024Z"},"links":{"cited_paper":"/paper/1312.1292","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:22b1c24fbece8f20980fc283878fde094071106b2e651362653307f1400c0fba","observation_id":"a57de9a7-9a8b-4ee1-b111-8d7148a52237","resolution":{"observed_at":"2026-08-14T11:57:58.502024Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.00532","last_updated":"2016-09-02T10:16:20Z","snapshot_observed_at":"2026-08-14T21:41:38.856224Z","submitted_at":"2016-09-02T10:16:20Z","title":"Can background cosmology hold the key for modified gravity tests?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.00532","snapshot_observed_at":"2026-08-14T11:57:58.506135Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.506135Z"},"links":{"cited_paper":"/paper/1609.00532","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:e618c4c39349357e41fcdc4683cc5ac3ddc4eb1707c1c9c25dff125537561b11","observation_id":"ae92b5a1-d9e3-4006-a38b-ff7db7904d22","resolution":{"observed_at":"2026-08-14T11:57:58.506135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.05976","last_updated":"2018-06-14T19:36:36Z","snapshot_observed_at":"2026-08-14T20:03:01.980657Z","submitted_at":"2017-12-16T15:44:45Z","title":"Do cosmological data rule out $f(\\mathcal{R})$ with $w\\neq-1$?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.05976","snapshot_observed_at":"2026-08-14T11:57:58.510086Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.510086Z"},"links":{"cited_paper":"/paper/1712.05976","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:5ac17bcc4400dd9ec3087d70575be8a55dc6efa0619377f55374ae9a3dadae35","observation_id":"127fc1dc-d20c-42ef-95c7-a0b6fe65641f","resolution":{"observed_at":"2026-08-14T11:57:58.510086Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.514017Z","title":"Armend´ ariz-Pic´ on, T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.514017Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:cf64f52499884a354e6f62bf56ea11e1151d070ba06de187c8a387cc5293c414","observation_id":"e2f35e9c-06c5-4baa-be9a-26b4d56eae42","resolution":{"observed_at":"2026-08-14T11:57:58.514017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.0048","last_updated":"2010-09-24T16:00:34Z","snapshot_observed_at":"2026-08-07T20:08:24.365858Z","submitted_at":"2010-07-31T04:03:01Z","title":"Imperfect Dark Energy from Kinetic Gravity Braiding","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.0048","snapshot_observed_at":"2026-08-14T11:57:58.518197Z","title":"Deffayet, O","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.518197Z"},"links":{"cited_paper":"/paper/1008.0048","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:f533909b13fa036001f775838ac021d88a835b786a52289b7e037a9fdddfe3c6","observation_id":"d2747cbe-a845-4236-98b1-6ae309c56c64","resolution":{"observed_at":"2026-08-14T11:57:58.518197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.2197","last_updated":"2009-11-27T10:54:20Z","snapshot_observed_at":"2026-08-14T08:50:19.368647Z","submitted_at":"2008-11-13T20:58:48Z","title":"The galileon as a local modification of gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.2197","snapshot_observed_at":"2026-08-14T11:57:58.522141Z","title":"Nicolis, R","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.522141Z"},"links":{"cited_paper":"/paper/0811.2197","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:48fef3538f4c1820f7b8eae48fc83cba9b37f18b94e8f93a02bcdc0390274fbb","observation_id":"38e36a04-4236-40d5-86bd-85d093da4f5b","resolution":{"observed_at":"2026-08-14T11:57:58.522141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.06180","last_updated":"2015-12-19T02:36:13Z","snapshot_observed_at":"2026-08-14T22:17:48.820706Z","submitted_at":"2015-12-19T02:36:13Z","title":"Is the Effective Field Theory of Dark Energy Effective?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.06180","snapshot_observed_at":"2026-08-14T11:57:58.526533Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.526533Z"},"links":{"cited_paper":"/paper/1512.06180","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:a3f6737ff0c05ace113d00714f6839831fc586637d7030741d53416785616f0e","observation_id":"8354caed-6d29-4e91-ace0-2c4afd7b88f9","resolution":{"observed_at":"2026-08-14T11:57:58.526533Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.4612","last_updated":"2012-08-22T20:14:31Z","snapshot_observed_at":"2026-08-15T00:49:07.964903Z","submitted_at":"2012-08-22T20:14:31Z","title":"No-Go Theorems for Generalized Chameleon Field Theories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.4612","snapshot_observed_at":"2026-08-14T11:57:58.531017Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.531017Z"},"links":{"cited_paper":"/paper/1208.4612","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:a18870f3207cb2407cb314198c68b4f56fe8f10a159daddab51e1ee0135e1229","observation_id":"5cc7d2f0-0fb0-4771-9ece-888f7de01651","resolution":{"observed_at":"2026-08-14T11:57:58.531017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.05481","last_updated":"2015-04-20T19:59:06Z","snapshot_observed_at":"2026-08-14T22:51:44.862967Z","submitted_at":"2015-04-20T19:59:06Z","title":"Effective Theory of Interacting Dark Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.05481","snapshot_observed_at":"2026-08-14T11:57:58.535127Z","title":"Gleyzes, D","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.535127Z"},"links":{"cited_paper":"/paper/1504.05481","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:af780f6b3cc545ae1d663ca45b98dcbafca945ad31c93c5f787d1a930f1ffd3c","observation_id":"0add7fab-6982-4a3b-a37f-7e9bef263422","resolution":{"observed_at":"2026-08-14T11:57:58.535127Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.539401Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.539401Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:b6cd41429782cfc5912210c079b3ff95ea7de3a9b2b2f7d2893614bcfe05f277","observation_id":"64745122-fceb-4efc-b569-0e81ff3ad46a","resolution":{"observed_at":"2026-08-14T11:57:58.539401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.2896","last_updated":"2015-01-31T13:52:40Z","snapshot_observed_at":"2026-08-14T23:34:20.112905Z","submitted_at":"2014-05-12T19:59:51Z","title":"Classifying Linearly Shielded Modified Gravity Models in Effective Field Theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.2896","snapshot_observed_at":"2026-08-14T11:57:58.543117Z","title":"Lombriser and A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.543117Z"},"links":{"cited_paper":"/paper/1405.2896","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:e760755c308e82d13c1a90a54db7914b2c235bd9193fcf4333266a6bdb97d89d","observation_id":"485f1c98-4347-419a-9087-b0e453a81e2b","resolution":{"observed_at":"2026-08-14T11:57:58.543117Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-14T11:57:58.546825Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.546825Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:4c322ef50b2bf7d4431613ae1d606138b78b1a26d65658f5e63a9316355bad98","observation_id":"5487f911-e403-4b69-8495-0d8f35a30969","resolution":{"observed_at":"2026-08-14T11:57:58.546825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05834","last_updated":"2017-11-02T11:19:17Z","snapshot_observed_at":"2026-08-14T20:23:20.089633Z","submitted_at":"2017-10-16T16:57:19Z","title":"Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05834","snapshot_observed_at":"2026-08-14T11:57:58.550863Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.550863Z"},"links":{"cited_paper":"/paper/1710.05834","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:77adaf108c74191306059aaf7bc8ff8656eba2a6f294320f92483028e1ef505a","observation_id":"ac8dd577-7fd2-4a2f-86a6-b729354fd6e2","resolution":{"observed_at":"2026-08-14T11:57:58.550863Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.5544","last_updated":"2014-08-20T21:52:30Z","snapshot_observed_at":"2026-08-14T23:29:35.056030Z","submitted_at":"2014-06-20T21:30:11Z","title":"Measuring Speed of Gravitational Waves by Observations of Photons and Neutrinos from Compact Binary Mergers and Supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.5544","snapshot_observed_at":"2026-08-14T11:57:58.554433Z","title":"Nishizawa and T","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.554433Z"},"links":{"cited_paper":"/paper/1406.5544","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:373d2ff9402e2bd8c52529631e430ad0d72e445a0e4cc4414e5824265fc8b5d4","observation_id":"c4588feb-6bfd-4440-b4e3-1e65091a8a9c","resolution":{"observed_at":"2026-08-14T11:57:58.554433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507184","last_updated":"2006-08-10T19:28:21Z","snapshot_observed_at":"2026-08-10T09:45:15.558035Z","submitted_at":"2005-07-07T20:33:45Z","title":"Probing Cosmic Acceleration Beyond the Equation of State: Distinguishing between Dark Energy and Modified Gravity Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507184","snapshot_observed_at":"2026-08-14T11:57:58.558673Z","title":"Ishak, A","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.558673Z"},"links":{"cited_paper":"/paper/astro-ph/0507184","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:81e875201c8cc855f1931f61834a06edc052c666d9177529c364c2da136571ad","observation_id":"592173fd-a47b-410e-8570-59cdc4c20df6","resolution":{"observed_at":"2026-08-14T11:57:58.558673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.1744","last_updated":"2008-10-09T20:16:22Z","snapshot_observed_at":"2026-07-06T01:44:51.074742Z","submitted_at":"2008-10-09T20:16:22Z","title":"Falsifying Paradigms for Cosmic Acceleration","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.1744","snapshot_observed_at":"2026-08-14T11:57:58.562560Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.562560Z"},"links":{"cited_paper":"/paper/0810.1744","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:9ed2d299dec063315fcfb91b7c0981cc80bd37388884fdd2898f9708ad2963b4","observation_id":"9803b7be-d3ff-46ab-b977-57a213444bee","resolution":{"observed_at":"2026-08-14T11:57:58.562560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.5832","last_updated":"2015-04-08T00:34:41Z","snapshot_observed_at":"2026-08-14T23:14:49.310562Z","submitted_at":"2014-10-21T20:00:36Z","title":"Banana Split: Testing the Dark Energy Consistency with Geometry and Growth","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.5832","snapshot_observed_at":"2026-08-14T11:57:58.566796Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.566796Z"},"links":{"cited_paper":"/paper/1410.5832","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:7a00334a416b00a6f952977a22faa3e90cefa4fbd2fb50602e701df8bd238037","observation_id":"22477dff-23c9-474b-b3b5-59dd713381a0","resolution":{"observed_at":"2026-08-14T11:57:58.566796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.0594","last_updated":"2011-04-11T17:21:46Z","snapshot_observed_at":"2026-08-13T21:59:37.814912Z","submitted_at":"2011-01-03T20:43:31Z","title":"Consistency check of {\\Lambda}CDM phenomenology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.0594","snapshot_observed_at":"2026-08-14T11:57:58.570767Z","title":"Lombriser, Physical Review D 83 (March 2011) 063519, arXiv:1101.0594","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.570767Z"},"links":{"cited_paper":"/paper/1101.0594","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:6259c55494f9c4ac8a3821a0c75c3ed301e1f24a726c083b552e61f46ae48786","observation_id":"a8248ea8-c822-494b-8d07-1beffabcab58","resolution":{"observed_at":"2026-08-14T11:57:58.570767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.3132","last_updated":"2013-10-26T13:44:15Z","snapshot_observed_at":"2026-08-15T00:32:42.029547Z","submitted_at":"2013-01-14T21:00:01Z","title":"Relativistic effects in galaxy clustering in a parametrized post-Friedmann universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.3132","snapshot_observed_at":"2026-08-14T11:57:58.575034Z","title":"Lombriser, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.575034Z"},"links":{"cited_paper":"/paper/1301.3132","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:66a6466845be668fedbb1a19210c464d051576f094a91ee1969e9fb81bfd7e1a","observation_id":"241cad31-4e9e-4c15-9188-fc6618bc5ddf","resolution":{"observed_at":"2026-08-14T11:57:58.575034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.05915","last_updated":"2015-09-07T16:02:23Z","snapshot_observed_at":"2026-08-14T22:47:34.858014Z","submitted_at":"2015-05-21T22:05:35Z","title":"Semi-dynamical perturbations of unified dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.05915","snapshot_observed_at":"2026-08-14T11:57:58.579128Z","title":"Lombriser and A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.579128Z"},"links":{"cited_paper":"/paper/1505.05915","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:b33776670b671d8d8eb34fa988b1df597aa7f6718207d6fd1b356bfd10c54791","observation_id":"3b28db92-6d92-4a1f-8179-e803c314bb7e","resolution":{"observed_at":"2026-08-14T11:57:58.579128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.582852Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.582852Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:c8cef74200b424eacbe895fc213b8b95e168777cc084025786b528a288ca6de1","observation_id":"4bbfdd94-b6a7-442b-8ec5-ae5d85f958e1","resolution":{"observed_at":"2026-08-14T11:57:58.582852Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.1962","last_updated":"2010-06-10T01:40:15Z","snapshot_observed_at":"2026-07-06T02:06:42.120857Z","submitted_at":"2010-02-10T18:28:08Z","title":"Testing General Relativity with Current Cosmological Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.1962","snapshot_observed_at":"2026-08-14T11:57:58.590329Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.590329Z"},"links":{"cited_paper":"/paper/1002.1962","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:68ad3888cc8340ffdb0ffc2026213fcdf4913f14d930a2db684407a07aeb58ac","observation_id":"2d70f41f-b5e5-49be-8ea8-4bce30984c64","resolution":{"observed_at":"2026-08-14T11:57:58.590329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.4583","last_updated":"2011-12-23T18:42:22Z","snapshot_observed_at":"2026-07-06T02:34:23.023626Z","submitted_at":"2011-09-21T16:39:22Z","title":"Testing General Relativity at Cosmological Scales: Implementation and Parameter Correlations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.4583","snapshot_observed_at":"2026-08-14T11:57:58.594129Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.594129Z"},"links":{"cited_paper":"/paper/1109.4583","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:408a17fc34a1791a703644d3622e3c4e12e86744a3878c3ccecf01fab27f8eab","observation_id":"fcdf59d3-411e-49f4-8151-2d2480402b3b","resolution":{"observed_at":"2026-08-14T11:57:58.594129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.597828Z","title":"Bonvin and P","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.597828Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:fcd1f1271caef61ac5c72ee61eb83c44e945f1903b5ee9018094075ef07186df","observation_id":"eeddc3f7-e456-4de4-a7e3-0b3d443c8ae4","resolution":{"observed_at":"2026-08-14T11:57:58.597828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0604485","last_updated":"2006-05-13T01:40:01Z","snapshot_observed_at":"2026-07-07T00:59:54.787519Z","submitted_at":"2006-04-23T12:07:20Z","title":"On the Growth of Perturbations as a Test of Dark Energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0604485","snapshot_observed_at":"2026-08-14T11:57:58.605623Z","title":"Bertschinger, Astrophysical Journal 648 (September 2006) 797, astro-ph/0604485","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.605623Z"},"links":{"cited_paper":"/paper/astro-ph/0604485","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:0c94a626c5bbc823342fada8fd9bcc2cdf9bcf02875b7ca6b87875c1cc2c8488","observation_id":"cfe72484-5922-45ae-98fa-bb9b8afe5d63","resolution":{"observed_at":"2026-08-14T11:57:58.605623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.0398","last_updated":"2012-06-28T14:34:03Z","snapshot_observed_at":"2026-07-06T02:43:54.165797Z","submitted_at":"2012-03-02T09:16:49Z","title":"Effective action approach to cosmological perturbations in dark energy and modified gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.0398","snapshot_observed_at":"2026-08-14T11:57:58.609486Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.609486Z"},"links":{"cited_paper":"/paper/1203.0398","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:1eeaadbb19905d6ffdad92bc368258b42f713e10adbddfb5ac6413bb6a65b3d6","observation_id":"dd381e7d-41ad-4540-b904-bd1198b4b5e0","resolution":{"observed_at":"2026-08-14T11:57:58.609486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.5742","last_updated":"2014-05-01T19:58:17Z","snapshot_observed_at":"2026-08-14T23:50:55.349433Z","submitted_at":"2013-12-19T20:59:47Z","title":"Effective Field Theory of Cosmic Acceleration: an implementation in CAMB","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.5742","snapshot_observed_at":"2026-08-14T11:57:58.613098Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.613098Z"},"links":{"cited_paper":"/paper/1312.5742","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:7d87dff6de4beff61f2739d52d55a73dd49e478ea4cda9ddf1577976fc4501a0","observation_id":"671168b4-214e-485e-9a11-2a7682b5d929","resolution":{"observed_at":"2026-08-14T11:57:58.613098Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.06102","last_updated":"2017-05-02T20:42:01Z","snapshot_observed_at":"2026-08-14T21:56:37.018158Z","submitted_at":"2016-05-19T19:53:30Z","title":"hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.06102","snapshot_observed_at":"2026-08-14T11:57:58.617314Z","title":"Zumalac´ arregui, E","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.617314Z"},"links":{"cited_paper":"/paper/1605.06102","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:414758f296bb88c489fc21dcb8e101def1f829815d4676752682cc9ec1ec7777","observation_id":"a4e009b2-e3f2-4f10-a866-02d3e58eb07f","resolution":{"observed_at":"2026-08-14T11:57:58.617314Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.6712","last_updated":"2014-03-21T03:38:56Z","snapshot_observed_at":"2026-08-15T00:20:03.440883Z","submitted_at":"2013-04-24T19:59:52Z","title":"A Simplified Approach to General Scalar-Tensor Theories","version":3},"cited_work":{"arxiv_id":"1304.6712","doi":null,"metadata_source":"pith","pith_arxiv_id":"1304.6712","snapshot_observed_at":"2026-08-14T11:57:59.883109Z","title":"A Simplified Approach to General Scalar-Tensor Theories","venue":"astro-ph.CO","work_id":"78144325-9418-4807-b3a5-f25f0ba2112b","year":2013},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.621246Z"},"links":{"cited_paper":"/paper/1304.6712","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:af43a8b38d0bd204823e4447ade78a77322569cfb89204b29086833ffbadf38c","observation_id":"515a52e0-161c-4391-a9d1-11bd9de70ead","resolution":{"observed_at":"2026-08-14T11:57:59.887287Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0901.3775","last_updated":"2009-03-02T22:57:45Z","snapshot_observed_at":"2026-08-12T15:18:49.540673Z","submitted_at":"2009-01-26T18:11:46Z","title":"Quantum Gravity at a Lifshitz Point","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.3775","snapshot_observed_at":"2026-08-14T11:57:58.624981Z","title":"Hoˇ rava,Physical Review D 79 (April 2009) 084008, arXiv:0901.3775 [hep-th]","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.624981Z"},"links":{"cited_paper":"/paper/0901.3775","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:268678dc7e88743da1a052af1f900c901d89ff3b973f4bb38a4a5356e42f6c37","observation_id":"68c43cd9-f7b2-4fd8-8af0-0126cdda5ac4","resolution":{"observed_at":"2026-08-14T11:57:58.624981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0106220","last_updated":"2001-09-11T18:47:20Z","snapshot_observed_at":"2026-07-07T03:52:45.282073Z","submitted_at":"2001-06-19T22:31:06Z","title":"Lower Bound on the Propagation Speed of Gravity from Gravitational Cherenkov Radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0106220","snapshot_observed_at":"2026-08-14T11:57:58.628736Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.628736Z"},"links":{"cited_paper":"/paper/hep-ph/0106220","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:bfe7c137d6fd0648efcd8e910012e34afbe63f1968b599f806b4e1053a97f079","observation_id":"a69fe6a6-7337-43d7-9182-83280eca00c1","resolution":{"observed_at":"2026-08-14T11:57:58.628736Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.632934Z","title":null,"venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.632934Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:9afb41fdefe8a1ef45a4a9957b0839e1bdcfd909a89647bf3d41b3d2cbdd5ce3","observation_id":"ee3f679a-11da-4d74-a1ab-36e784ea6188","resolution":{"observed_at":"2026-08-14T11:57:58.632934Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.636862Z","title":"Beltr´ an Jim´ enez, F","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.636862Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:1c4011f412fdd81bcb3bf91c6b91d3705e24b041957a2990fc438a94e2f8521c","observation_id":"52cc2e03-d384-4e34-9011-818f7f5a8637","resolution":{"observed_at":"2026-08-14T11:57:58.636862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.09447","last_updated":"2018-07-24T18:30:07Z","snapshot_observed_at":"2026-08-14T19:42:03.161529Z","submitted_at":"2018-02-26T16:46:02Z","title":"Gravitational wave constraints on dark sector models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.09447","snapshot_observed_at":"2026-08-14T11:57:58.644437Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.644437Z"},"links":{"cited_paper":"/paper/1802.09447","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:5bc2d364503d2c86812b971ae7d7ff131318ae5b4ba7384b45f73083d0e89541","observation_id":"e3b681f3-3584-4c80-9b5a-7a0e3191e610","resolution":{"observed_at":"2026-08-14T11:57:58.644437Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.03701","last_updated":"2015-10-09T17:14:52Z","snapshot_observed_at":"2026-08-14T22:28:31.977725Z","submitted_at":"2015-10-09T17:14:52Z","title":"The Speed of Galileon Gravity","version":1},"cited_work":{"arxiv_id":"1510.03701","doi":null,"metadata_source":"pith","pith_arxiv_id":"1510.03701","snapshot_observed_at":"2026-08-14T11:57:59.820594Z","title":"The Speed of Galileon Gravity","venue":"gr-qc","work_id":"d8ca5c94-74a5-411a-bc36-4e5dc6fae8e8","year":2015},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.648992Z"},"links":{"cited_paper":"/paper/1510.03701","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:46fd835ba62acc844abf096f36fb1ca8e69ef4a6544ca14e8cc3af1a73186da3","observation_id":"adad0b7c-9b97-4e59-8bfa-5f4649de0fd9","resolution":{"observed_at":"2026-08-14T11:57:59.824753Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1406.0485","last_updated":"2014-06-26T19:03:19Z","snapshot_observed_at":"2026-08-14T23:31:51.444063Z","submitted_at":"2014-06-02T19:26:23Z","title":"The observational status of Galileon gravity after Planck","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.0485","snapshot_observed_at":"2026-08-14T11:57:58.652833Z","title":"Barreira, B","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.652833Z"},"links":{"cited_paper":"/paper/1406.0485","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:b24a6f614863b6d93931603c72fb15a787fe724311e4f992793d9c595f9202cf","observation_id":"775990bf-9cee-4bab-8935-6cde439c23d3","resolution":{"observed_at":"2026-08-14T11:57:58.652833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:57:58.656869Z","title":"Lombriser, W","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.656869Z"},"links":{"citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:a7d662d39c436053362422b5ff770b980a82f46695986a15ef18d4ae581464af","observation_id":"683c22f9-1413-4971-8452-c1ce455bee71","resolution":{"observed_at":"2026-08-14T11:57:58.656869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.3598","last_updated":"2012-05-11T00:16:08Z","snapshot_observed_at":"2026-07-06T02:35:53.691786Z","submitted_at":"2011-10-17T08:26:34Z","title":"Observational Constraints on Kinetic Gravity Braiding from the Integrated Sachs-Wolfe Effect","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.3598","snapshot_observed_at":"2026-08-14T11:57:58.665129Z","title":"Kimura, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:58.665129Z"},"links":{"cited_paper":"/paper/1110.3598","citing_paper":"/paper/1908.07892"},"observation_digest":"sha256:d122d603294e2a4fe1afdf18a001cfeeb3faea1ebfd20b0f36905e41923d728f","observation_id":"30ca9926-696a-46c2-af59-a8555917484b","resolution":{"observed_at":"2026-08-14T11:57:58.665129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.07892","last_updated":"2019-08-21T14:27:19Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T02:16:28.816319Z","submitted_at":"2019-08-21T14:27:19Z","title":"Parametrizations for tests of gravity"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":98,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":177},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 100 of 177 outbound references and 0 inbound Pith citation observations for arXiv:1908.07892."}