{"as_of":"2026-08-12T22:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5c4da26926fb8ef6c738340ac0f14d1dc9142fd1d50a0854d162c1cf035d13e8","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T19:12:41.526297Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":182,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-10T19:12:41.526297Z","title":"Kimura, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.10659","last_updated":"2025-04-16T03:14:42Z","snapshot_observed_at":"2026-08-10T20:56:43.233393Z","submitted_at":"2025-01-18T05:33:52Z","title":"Gravitomagnetic tidal response of relativistic stars in partially screened scalar-tensor theories","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T19:12:41.526297Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2501.10659"},"observation_digest":"sha256:19b12e28d526e53247b289b22ede4193ba30f34ceacf753fffe31685344fd8e2","observation_id":"8d5f5cc6-d5df-4c0e-a664-39bdd4e217d6","resolution":{"observed_at":"2026-08-10T19:12:41.526297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-10T14:29:27.968561Z","title":"Kimura, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.15298","last_updated":"2025-04-12T08:58:51Z","snapshot_observed_at":"2026-08-10T16:08:01.968504Z","submitted_at":"2025-01-25T18:30:04Z","title":"Scalar-Tensor Gravity and DESI 2024 BAO data","version":2},"reference_index":116,"source":"pdf_text","source_observed_at":"2026-08-10T14:29:27.968561Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2501.15298"},"observation_digest":"sha256:d78b9410fed3c62916113cfdc5682ad28d031a9b5e16219d8f643d72da029885","observation_id":"67221775-e615-4f09-8e72-f440311fe5db","resolution":{"observed_at":"2026-08-10T14:29:27.968561Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":"1111.6749","doi":"10.1103/physrevd.85.024023","metadata_source":"pith","pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","venue":"astro-ph.CO","work_id":"dd2acc4f-3db9-4a21-be7d-472270f38cd1","year":2011},"citing_paper":{"arxiv_id":"2601.05145","last_updated":"2026-04-17T03:28:58Z","snapshot_observed_at":"2026-08-11T12:07:45.730559Z","submitted_at":"2026-01-08T17:32:49Z","title":"How deep can a cosmic void be? Voids-informed theoretical bounds in Galileon gravity","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-16T16:04:11.710388Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2601.05145"},"observation_digest":"sha256:ae2212cc289700a53c7715c97583d024e660af20fc52a69179f07ad4bc3e5118","observation_id":"d286275b-6453-47ae-8fe2-018db1c9a5dc","resolution":{"observed_at":"2026-05-16T16:08:04.651395Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-03T07:07:17.866084Z","title":"Kimura, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2601.21274","last_updated":"2026-05-30T03:19:05Z","snapshot_observed_at":"2026-08-06T03:56:12.411728Z","submitted_at":"2026-01-29T05:11:07Z","title":"Realizing the phantom-divide crossing with vector and scalar fields","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-03T07:07:17.866084Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2601.21274"},"observation_digest":"sha256:c6cd30ca348d3b882cc4f2c0fd4fea8d2f1e59d9c9d1f13f354e44f1f32261fe","observation_id":"55f2c005-1274-4dfe-a7ab-49a27975a502","resolution":{"observed_at":"2026-08-03T07:07:17.866084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-02T22:16:58.002818Z","title":"Kimura, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2602.17644","last_updated":"2026-07-21T14:05:04Z","snapshot_observed_at":"2026-08-06T06:36:14.515098Z","submitted_at":"2026-02-19T18:54:23Z","title":"Cosmic voids evolution in modified gravity via hydrodynamics","version":2},"reference_index":171,"source":"pdf_text","source_observed_at":"2026-08-02T22:16:58.002818Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2602.17644"},"observation_digest":"sha256:423850ad1829ee2096a70c9b05e3f65633f1f2eb2ef29acf2143f206d4711285","observation_id":"f324a438-498b-4edc-9674-af77a9828841","resolution":{"observed_at":"2026-08-02T22:16:58.002818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":"1111.6749","doi":"10.1103/physrevd.85.024023","metadata_source":"pith","pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","venue":"astro-ph.CO","work_id":"dd2acc4f-3db9-4a21-be7d-472270f38cd1","year":2011},"citing_paper":{"arxiv_id":"2605.04154","last_updated":"2026-05-05T18:00:07Z","snapshot_observed_at":"2026-08-11T17:34:28.203522Z","submitted_at":"2026-05-05T18:00:07Z","title":"A Master Equation for Screening in Luminal Horndeski Gravity","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-08T18:51:06.425840Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2605.04154"},"observation_digest":"sha256:ac3e3363b0e52aecf954cae8531a006456768c691ad5a47a194e0c426a257242","observation_id":"5aca70e9-ba12-41c9-a4c4-fe66aa9f13c5","resolution":{"observed_at":"2026-05-09T06:10:39.165251Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":"1111.6749","doi":"10.1103/physrevd.85.024023","metadata_source":"pith","pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","venue":"astro-ph.CO","work_id":"dd2acc4f-3db9-4a21-be7d-472270f38cd1","year":2011},"citing_paper":{"arxiv_id":"2605.13937","last_updated":"2026-05-13T16:22:39Z","snapshot_observed_at":"2026-08-10T21:25:12.032485Z","submitted_at":"2026-05-13T16:22:39Z","title":"Spherical collapse and cluster number counts in DHOST theories that pass the constraints from gravitational waves","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-15T02:37:41.419661Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2605.13937"},"observation_digest":"sha256:16625860e9f7cd1f77fc73825add1c81a48c380c6fbfd01e33151780d89879d4","observation_id":"16894c30-5898-4159-8d49-1aa48689ae6f","resolution":{"observed_at":"2026-05-15T02:38:35.655945Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":"1111.6749","doi":"10.1103/physrevd.85.024023","metadata_source":"pith","pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","venue":"astro-ph.CO","work_id":"dd2acc4f-3db9-4a21-be7d-472270f38cd1","year":2011},"citing_paper":{"arxiv_id":"2606.04077","last_updated":"2026-06-16T18:36:18Z","snapshot_observed_at":"2026-08-12T19:14:56.905647Z","submitted_at":"2026-06-02T17:11:03Z","title":"Lagrangian Extensions of Newtonian Gravity constrained by Solar System tests","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-28T08:45:25.884459Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2606.04077"},"observation_digest":"sha256:aadb63aaa6dc259f082ab48a007fba78a6989264d880cb5a3ef0ef71ae8a7b42","observation_id":"690af7cb-a2bb-4051-9c78-63d29bf877e1","resolution":{"observed_at":"2026-07-02T04:56:38.725196Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":"1111.6749","doi":"10.1103/physrevd.85.024023","metadata_source":"pith","pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","venue":"astro-ph.CO","work_id":"dd2acc4f-3db9-4a21-be7d-472270f38cd1","year":2011},"citing_paper":{"arxiv_id":"2606.20794","last_updated":"2026-07-14T10:22:43Z","snapshot_observed_at":"2026-08-12T11:02:16.081093Z","submitted_at":"2026-06-18T18:00:01Z","title":"Constraints on Horndeski Gravity with Phantom Crossing","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2606.20794"},"observation_digest":"sha256:0a107813e65741f33485d719d7891066ad5f66e046588c47720935e10ba3b6d2","observation_id":"62575258-f26f-4472-9cdc-fdb405971302","resolution":{"observed_at":"2026-06-26T15:59:34.744026Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":"1111.6749","doi":"10.1103/physrevd.85.024023","metadata_source":"pith","pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","venue":"astro-ph.CO","work_id":"dd2acc4f-3db9-4a21-be7d-472270f38cd1","year":2011},"citing_paper":{"arxiv_id":"2606.30728","last_updated":"2026-06-29T18:00:03Z","snapshot_observed_at":"2026-08-05T14:45:57.285415Z","submitted_at":"2026-06-29T18:00:03Z","title":"Radial Solutions of Multi-Field de Sitter Galileons","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-01T01:54:53.803870Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2606.30728"},"observation_digest":"sha256:da687252d39c9e0dcfe3565ad5abc87636ab902f085aa5f6be2d7474b7035b73","observation_id":"d87d0729-51d1-44cc-b28c-121d16802b9b","resolution":{"observed_at":"2026-07-01T12:35:44.341835Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":"1111.6749","doi":"10.1103/physrevd.85.024023","metadata_source":"pith","pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","venue":"astro-ph.CO","work_id":"dd2acc4f-3db9-4a21-be7d-472270f38cd1","year":2011},"citing_paper":{"arxiv_id":"2606.31274","last_updated":"2026-06-30T07:47:03Z","snapshot_observed_at":"2026-08-05T16:57:52.442817Z","submitted_at":"2026-06-30T07:47:03Z","title":"Fragility of stealth solutions in mimetic gravity","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-01T04:46:42.967488Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2606.31274"},"observation_digest":"sha256:aad529583fbd16ff3a18ce31f02d05bf0f7b71cc7b266ee0d01a1e0fe6b6e445","observation_id":"2722744b-5c01-4823-9742-c1937b1a75b7","resolution":{"observed_at":"2026-07-01T11:05:41.767101Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":"1111.6749","doi":"10.1103/physrevd.85.024023","metadata_source":"pith","pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","venue":"astro-ph.CO","work_id":"dd2acc4f-3db9-4a21-be7d-472270f38cd1","year":2011},"citing_paper":{"arxiv_id":"2606.31977","last_updated":"2026-06-30T17:17:50Z","snapshot_observed_at":"2026-08-02T18:59:37.715063Z","submitted_at":"2026-06-30T17:17:50Z","title":"Constraining dark energy with complementary probes of large-scale structure","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-01T03:37:13.804621Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2606.31977"},"observation_digest":"sha256:5e7df342aa60b12343152e2ea1cf80c01ebeecc6c8ad05dfd3e804db766979ad","observation_id":"604f74a2-6a30-41f3-bb9b-1cfcabe31975","resolution":{"observed_at":"2026-07-01T11:55:42.884808Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-01T21:09:45.999865Z","title":"Kimura, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.16395","last_updated":"2026-07-17T18:00:01Z","snapshot_observed_at":"2026-08-09T00:53:14.785477Z","submitted_at":"2026-07-17T18:00:01Z","title":"Rolling Galileons: Evolving Braiding Strength for Viable Dark Energy","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-01T21:09:45.999865Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2607.16395"},"observation_digest":"sha256:c04429799618e81d439202169ca0f057136f68c4ee306babe545c36e739f2bbf","observation_id":"4eca5fa2-33f5-4fa5-b13f-ba92689de424","resolution":{"observed_at":"2026-08-01T21:09:45.999865Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6749","snapshot_observed_at":"2026-08-01T15:41:46.953319Z","title":"Kimura, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.26447","last_updated":"2026-07-29T03:52:12Z","snapshot_observed_at":"2026-08-09T00:15:56.534898Z","submitted_at":"2026-07-29T03:52:12Z","title":"Phantom-divide crossing and suppressed structure growth in kinetically braided dark energy with momentum exchange","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-01T15:41:46.953319Z"},"links":{"cited_paper":"/paper/1111.6749","citing_paper":"/paper/2607.26447"},"observation_digest":"sha256:b1a6be599d96d49b78e085460d7b61aa4cb5a01ae48fdb99b0537f5e8d9c9ffc","observation_id":"751d1113-9699-4b3d-9624-2a0dbefae327","resolution":{"observed_at":"2026-08-01T15:41:46.953319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1111.6749/citation-record","integrity":"/paper/1111.6749/integrity","json":"/paper/1111.6749/citation-record.json","paper":"/paper/1111.6749"},"outbound":[],"paper":{"arxiv_id":"1111.6749","last_updated":"2012-01-19T02:27:10Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:38:25.549929Z","submitted_at":"2011-11-29T10:15:57Z","title":"Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1111.6749."}