{"as_of":"2026-08-20T07:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:032f16acc442b76d41b600dfd13431d5f8c05c61c2c75fe74992d739c2cc1e62","coverage":[{"denominator":106,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T20:45:32.134940Z","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":"2026-08-20T06:33:59.587034+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/2507.02059/citation-record","integrity":"/paper/2507.02059/integrity","json":"/paper/2507.02059/citation-record.json","paper":"/paper/2507.02059"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:45:31.862490Z","title":"Dodelson and F","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.862490Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:469f18f9317626de6d8c3a22b1b8c2842dd75818b1779c9e2b57955fbad3bbdd","observation_id":"6960e820-3b64-45bd-a59b-a7dabe45ea51","resolution":{"observed_at":"2026-08-06T20:45:31.862490Z","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":"2026-08-06T20:45:31.865958Z","title":"Dvali, 2011 CERN-Latin-American School of High- Energy Physics, CLASHEP 2011 - Proceedings , 145 (2013)","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.865958Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:bcef1438f2058a740ae1623b044b3f5e2edc8b9664aadb919d414551d2a03c3a","observation_id":"2cec3acd-ea0b-4ecf-a64e-856d578cee21","resolution":{"observed_at":"2026-08-06T20:45:31.865958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9802228","last_updated":"1998-08-15T15:31:52Z","snapshot_observed_at":"2026-07-07T04:28:20.832511Z","submitted_at":"1998-02-03T10:59:26Z","title":"Beyond The Standard Model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9802228","snapshot_observed_at":"2026-08-06T20:45:31.868770Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.868770Z"},"links":{"cited_paper":"/paper/hep-ph/9802228","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:5d44faf3ab10fe71a010f1bb4eed03831434f2ab20a30b9ea66feb09b80ebe03","observation_id":"526f4b4d-14cf-4a0f-8b0d-ae9e95a114e1","resolution":{"observed_at":"2026-08-06T20:45:31.868770Z","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":"2026-08-06T20:45:31.871952Z","title":"de Rham and A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.871952Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:ff501db7343101d00451ff2d6b820c52037e2090528c2cd82a98cd10cd425a96","observation_id":"42798160-a348-4cb8-9a3d-6f2ee8e2b457","resolution":{"observed_at":"2026-08-06T20:45:31.871952Z","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":"2026-08-06T20:45:31.874636Z","title":"Fierz and W","venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.874636Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:4df288547635c275fb4f45aa00ccc71d43aa5fbcf7d0687fcabdb9dfb4828aaf","observation_id":"3f702534-a26c-478f-9ee4-89e96aac5d36","resolution":{"observed_at":"2026-08-06T20:45:31.874636Z","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":"2026-08-06T20:45:31.877234Z","title":"van Dam and M","venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.877234Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:a6f9cf0d4f0f1c0344e4ec232a053c53faaa1f674006c0ec740a1e1a714ce23b","observation_id":"7696e78f-20c6-446d-a018-c032ab666097","resolution":{"observed_at":"2026-08-06T20:45:31.877234Z","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":"2026-08-06T20:45:31.880461Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.880461Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:dbfebea6b280b9c482ca45fa5eda66a4700693c389b467a0f564fa4f3992e394","observation_id":"ddfa1e7a-f883-44be-8cea-5881d6dcb933","resolution":{"observed_at":"2026-08-06T20:45:31.880461Z","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":"2026-08-06T20:45:31.883162Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.883162Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:d9d9423803a7720e69cd3d3376afad910821e8079d120605aacda92f83b0461c","observation_id":"a270dd9c-8971-4aee-8287-152a8208e7d3","resolution":{"observed_at":"2026-08-06T20:45:31.883162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.0601","last_updated":"2013-04-02T11:58:19Z","snapshot_observed_at":"2026-08-17T02:08:51.951573Z","submitted_at":"2013-04-02T11:58:19Z","title":"Exact Solutions in Massive Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.0601","snapshot_observed_at":"2026-08-06T20:45:31.885686Z","title":"Tasinato, K","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.885686Z"},"links":{"cited_paper":"/paper/1304.0601","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:69d57fd7bad0bab02611127527ccde310f4f9d1417b8ce3edd31657e74fe0ed9","observation_id":"05d4c475-8dcd-4d76-86f6-7cc0c39e4035","resolution":{"observed_at":"2026-08-06T20:45:31.885686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.5231","last_updated":"2011-08-26T02:45:01Z","snapshot_observed_at":"2026-08-15T04:37:16.774039Z","submitted_at":"2011-08-26T02:45:01Z","title":"Massive Cosmologies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.5231","snapshot_observed_at":"2026-08-06T20:45:31.888470Z","title":"D’Amico, C","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.888470Z"},"links":{"cited_paper":"/paper/1108.5231","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:d9cba2d9575cbda7f582102126ec4269545931bcd0516029d45e2e17e86eac65","observation_id":"3363ddb1-8610-451a-80b3-dc2ed2921230","resolution":{"observed_at":"2026-08-06T20:45:31.888470Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.1232","last_updated":"2010-11-08T18:31:49Z","snapshot_observed_at":"2026-08-15T05:03:53.059717Z","submitted_at":"2010-11-04T18:24:57Z","title":"Resummation of Massive Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.1232","snapshot_observed_at":"2026-08-06T20:45:31.891289Z","title":"de Rham, G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.891289Z"},"links":{"cited_paper":"/paper/1011.1232","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:267676a65ed88a58184b3d3cab21937913f45f3e3e5ce3325fcb30785b5a0bf6","observation_id":"075a118f-6f33-4755-b19f-1b5d7f828138","resolution":{"observed_at":"2026-08-06T20:45:31.891289Z","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":"2026-08-06T20:45:31.894066Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.894066Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:4647bad47f3c383c5768ff12eba911e9150fb320c82a441a702022905894e709","observation_id":"a70f0198-89f4-4101-9899-1a8d82f4c9be","resolution":{"observed_at":"2026-08-06T20:45:31.894066Z","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":"2026-08-06T20:45:31.896807Z","title":"de Rham and G","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.896807Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:da0e4978da9606fe625f0448e86b22be2f652d01eaf856533dc58663431b2834","observation_id":"961b8f1b-5c3c-4497-bb8a-816e8f24ea00","resolution":{"observed_at":"2026-08-06T20:45:31.896807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.3515","last_updated":"2012-04-03T16:17:42Z","snapshot_observed_at":"2026-08-15T04:35:05.187206Z","submitted_at":"2011-09-16T01:51:46Z","title":"Bimetric Gravity from Ghost-free Massive Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.3515","snapshot_observed_at":"2026-08-06T20:45:31.899346Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.899346Z"},"links":{"cited_paper":"/paper/1109.3515","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:6537c53e01a44935fbeee6c6a25cfdf0ce2a6aa42aa8d8a3334f1302435842c1","observation_id":"80299a1a-ccf6-4dee-93de-80ea5ec2c4f0","resolution":{"observed_at":"2026-08-06T20:45:31.899346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.04876","last_updated":"2023-02-09T19:00:00Z","snapshot_observed_at":"2026-08-16T15:56:26.323020Z","submitted_at":"2023-02-09T19:00:00Z","title":"A dynamical formulation of ghost-free massive gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.04876","snapshot_observed_at":"2026-08-06T20:45:31.902354Z","title":"de Rham, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.902354Z"},"links":{"cited_paper":"/paper/2302.04876","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:34f0ddd5f1441057bff3144fbb15bd11da015efca1dafab9780bef93acc0bde9","observation_id":"25f3c405-6763-4ca1-9985-2c72b00e9d80","resolution":{"observed_at":"2026-08-06T20:45:31.902354Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.3735","last_updated":"2011-10-02T21:31:06Z","snapshot_observed_at":"2026-08-15T04:46:27.246735Z","submitted_at":"2011-05-18T20:02:42Z","title":"Theoretical Aspects of Massive Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.3735","snapshot_observed_at":"2026-08-06T20:45:31.904991Z","title":"Hinterbichler, Rev","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.904991Z"},"links":{"cited_paper":"/paper/1105.3735","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:bd329de209e9e6f7609273dc9246d707c220c74983c65e2ab3b13cb1762c6b63","observation_id":"cb9bbe60-33b2-4bd9-bded-26297ae36cb0","resolution":{"observed_at":"2026-08-06T20:45:31.904991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.4173","last_updated":"2014-03-14T20:27:41Z","snapshot_observed_at":"2026-08-14T23:48:05.360265Z","submitted_at":"2014-01-16T21:00:17Z","title":"Massive Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.4173","snapshot_observed_at":"2026-08-06T20:45:31.907437Z","title":"de Rham, Living Rev","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.907437Z"},"links":{"cited_paper":"/paper/1401.4173","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:ba276c03c896225376b6ea3124ff57d4c4ec6f7a937f6381182c22960464910f","observation_id":"560363f1-b5d5-4a32-9beb-d761863b41f0","resolution":{"observed_at":"2026-08-06T20:45:31.907437Z","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":"2026-08-06T20:45:31.910150Z","title":"Koyama, Rept","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.910150Z"},"links":{"cited_paper":"/paper/1504.04623","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:b05fc328377b38dd4828ff68747b722068f3639e5dbba5320d45bba83930cebb","observation_id":"b307cf5c-8cd9-42e6-816d-13e354ae16f6","resolution":{"observed_at":"2026-08-06T20:45:31.910150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.08462","last_updated":"2017-05-08T15:52:06Z","snapshot_observed_at":"2026-08-14T21:50:56.213462Z","submitted_at":"2016-06-27T20:05:45Z","title":"Graviton Mass Bounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.08462","snapshot_observed_at":"2026-08-06T20:45:31.912921Z","title":"de Rham, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.912921Z"},"links":{"cited_paper":"/paper/1606.08462","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:53cdb7ae93dde46bfdeb961c7d95c6dfe081ea46729ddbee380357228cceee33","observation_id":"19ecdaa5-6922-4884-ba26-e1e641213b52","resolution":{"observed_at":"2026-08-06T20:45:31.912921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.02873","last_updated":"2017-01-11T07:56:00Z","snapshot_observed_at":"2026-08-16T10:45:53.986792Z","submitted_at":"2017-01-11T07:56:00Z","title":"Cosmology of Massive Gravity and its Extensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.02873","snapshot_observed_at":"2026-08-06T20:45:31.915471Z","title":"Hinterbichler, in 51st Rencontres de Moriond on Cosmology (2016) pp","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.915471Z"},"links":{"cited_paper":"/paper/1701.02873","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:89874b49466c6362e2d917bc7c0d85680f96f4f13ed63e23cc0cd54a6ccec52a","observation_id":"a6f62f34-d030-41af-aa54-0db87b6f0ad7","resolution":{"observed_at":"2026-08-06T20:45:31.915471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.06643","last_updated":"2016-12-27T15:33:19Z","snapshot_observed_at":"2026-08-14T23:44:37.931994Z","submitted_at":"2016-08-23T20:08:56Z","title":"On scale-free extensions of massive (bi-)gravity","version":2},"cited_work":{"arxiv_id":"1608.06643","doi":null,"metadata_source":"pith","pith_arxiv_id":"1608.06643","snapshot_observed_at":"2026-08-06T20:45:33.155217Z","title":"On scale-free extensions of massive (bi-)gravity","venue":"hep-th","work_id":"d3a80e9f-fa2d-4446-89a7-4abf1379e1d9","year":2016},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.918106Z"},"links":{"cited_paper":"/paper/1608.06643","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:5b1b84f2104ad9eeb41c254585f65cab768abace7b4e2e7c519461f941937b73","observation_id":"dd043e96-1a8c-4b43-bc9c-d123447e6f4d","resolution":{"observed_at":"2026-08-06T20:45:33.159310Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.08560","last_updated":"2020-03-19T15:17:38Z","snapshot_observed_at":"2026-07-06T08:45:22.918175Z","submitted_at":"2019-12-18T12:22:15Z","title":"Stable Cosmology in Generalised Massive Gravity","version":2},"cited_work":{"arxiv_id":"1912.08560","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.08560","snapshot_observed_at":"2026-08-06T20:45:33.141204Z","title":"Stable Cosmology in Generalised Massive Gravity","venue":"hep-th","work_id":"0bc29052-5ca8-4131-960d-b6ea1a43e888","year":2019},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.920827Z"},"links":{"cited_paper":"/paper/1912.08560","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:4830c61ec12de0f144fe1d4b840d70bb34467473b88694dbdd8c6a8bcf5b9c6c","observation_id":"764af47d-a6c0-4de0-a3ec-cbdcb3491ed0","resolution":{"observed_at":"2026-08-06T20:45:33.145511Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10863","last_updated":"2022-07-15T08:08:08Z","snapshot_observed_at":"2026-08-16T16:58:36.489700Z","submitted_at":"2022-05-22T16:31:59Z","title":"Cosmology of Dirac-Born-Infeld dRGT massive gravity","version":4},"cited_work":{"arxiv_id":"2205.10863","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.10863","snapshot_observed_at":"2026-08-06T20:45:33.129036Z","title":"Cosmology of Dirac-Born-Infeld dRGT massive gravity","venue":"gr-qc","work_id":"9b436bbd-6142-40ec-a496-a3584151f88d","year":2022},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.924112Z"},"links":{"cited_paper":"/paper/2205.10863","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:22456101c0def44a039de234bb40f4b749740a3c63e9bae26e2fdc99d69677de","observation_id":"9e4e1e52-65dc-4580-9217-a11ed62cf836","resolution":{"observed_at":"2026-08-06T20:45:33.132314Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2106.09030","last_updated":"2021-11-03T06:39:22Z","snapshot_observed_at":"2026-08-17T13:21:36.768290Z","submitted_at":"2021-06-16T18:00:00Z","title":"Constraints on bimetric gravity from Big Bang nucleosynthesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.09030","snapshot_observed_at":"2026-08-06T20:45:31.926817Z","title":"H¨ og ˚ as and E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.926817Z"},"links":{"cited_paper":"/paper/2106.09030","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:57a8df40a9d81f35d96ca5a36a3daaf3209a7b92a65bd0aecbf0158edd1d2e9b","observation_id":"7711f47b-7f84-4d46-9cda-48b6aa9a7b4a","resolution":{"observed_at":"2026-08-06T20:45:31.926817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08795","last_updated":"2021-05-10T19:21:24Z","snapshot_observed_at":"2026-08-16T18:50:49.957052Z","submitted_at":"2021-01-21T19:00:04Z","title":"Observational constraints on bimetric gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08795","snapshot_observed_at":"2026-08-06T20:45:31.929650Z","title":"H¨ og ˚ as and E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.929650Z"},"links":{"cited_paper":"/paper/2101.08795","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:9ba6812b649d7c183ba761b979b482110ccfa4f9d69136197b53996d3fd04fe9","observation_id":"2943fd17-19f5-46b9-bc21-9a7e4b48e2b9","resolution":{"observed_at":"2026-08-06T20:45:31.929650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08794","last_updated":"2021-05-10T19:30:08Z","snapshot_observed_at":"2026-08-17T13:13:53.800962Z","submitted_at":"2021-01-21T19:00:03Z","title":"Analytical constraints on bimetric gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08794","snapshot_observed_at":"2026-08-06T20:45:31.932589Z","title":"H¨ og ˚ as and E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.932589Z"},"links":{"cited_paper":"/paper/2101.08794","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:0a5be6b09f1ff3ebb3043ab66c7ca37714af08b1b86e5c71c3306507076d643d","observation_id":"d29c48aa-9ba9-444d-8a6d-cfc5ecacb6b8","resolution":{"observed_at":"2026-08-06T20:45:31.932589Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.01651","last_updated":"2020-04-29T12:54:51Z","snapshot_observed_at":"2026-07-06T08:26:47.571015Z","submitted_at":"2019-10-03T18:00:02Z","title":"On the stability of bimetric structure formation","version":2},"cited_work":{"arxiv_id":"1910.01651","doi":null,"metadata_source":"pith","pith_arxiv_id":"1910.01651","snapshot_observed_at":"2026-08-06T20:45:33.090671Z","title":"On the stability of bimetric structure formation","venue":"gr-qc","work_id":"6ecb48e4-46e2-4de2-ac12-f1c3e7fba09e","year":2019},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.935323Z"},"links":{"cited_paper":"/paper/1910.01651","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:1daf06bf7de96a8d907ca4c0bee4a19ce91954e2bfdb6cbf29df957247caffce","observation_id":"9e7a8a88-424d-49d0-b225-7a3c08f22b8d","resolution":{"observed_at":"2026-08-06T20:45:33.094183Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:45:31.938173Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.938173Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:00919b7035e22d4455a4964f4ceac34a0c6f4a3e08cfb80c5bb7b9109b8be4e4","observation_id":"666e3de9-37be-4e28-a8ac-81fe9c4124ca","resolution":{"observed_at":"2026-08-06T20:45:31.938173Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.14799","last_updated":"2024-03-06T17:06:08Z","snapshot_observed_at":"2026-08-16T14:40:33.718392Z","submitted_at":"2023-11-24T19:00:01Z","title":"On the absence of ghosts in quadratic bigravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.14799","snapshot_observed_at":"2026-08-06T20:45:31.940665Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.940665Z"},"links":{"cited_paper":"/paper/2311.14799","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:e936869eaf3d2a6738505408670a2250a4e97902980ab463761198a657d9f89d","observation_id":"0c963cb8-9b36-4743-9a9d-8ebae3406dd7","resolution":{"observed_at":"2026-08-06T20:45:31.940665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.05673","last_updated":"2023-09-29T09:04:54Z","snapshot_observed_at":"2026-08-16T15:17:02.109318Z","submitted_at":"2023-07-11T18:00:02Z","title":"Bimetric Starobinsky model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.05673","snapshot_observed_at":"2026-08-06T20:45:31.943521Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.943521Z"},"links":{"cited_paper":"/paper/2307.05673","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:de0bfb85e828df98eb455149a6f2411dc3993e423d5ec368b85d2ca43b338c79","observation_id":"238dcf1e-9c68-4cf8-98ee-699dcb39657a","resolution":{"observed_at":"2026-08-06T20:45:31.943521Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.11353","last_updated":"2023-05-02T12:01:48Z","snapshot_observed_at":"2026-08-16T15:46:46.268759Z","submitted_at":"2023-03-20T18:00:02Z","title":"Bimetric-Affine Quadratic Gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.11353","snapshot_observed_at":"2026-08-06T20:45:31.946479Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.946479Z"},"links":{"cited_paper":"/paper/2303.11353","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:d203aa1e6887c2c2d2eabc982c54cb002b8bbf65bb5226a3d57cc328ea2706c7","observation_id":"6a83698e-97d8-49a5-83ba-89a24f2007b1","resolution":{"observed_at":"2026-08-06T20:45:31.946479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.04322","last_updated":"2024-10-31T08:52:17Z","snapshot_observed_at":"2026-08-16T13:36:52.330735Z","submitted_at":"2024-07-05T07:48:09Z","title":"2D BAO vs 3D BAO: solving the Hubble tension with an alternative cosmological model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.04322","snapshot_observed_at":"2026-08-06T20:45:31.949555Z","title":"Dwivedi and M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.949555Z"},"links":{"cited_paper":"/paper/2407.04322","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:0021be3e80b731188f53123e859856896abdb6f7bb0e609bde209806c7d10b0f","observation_id":"727f1c37-b8f4-4602-9f40-2f5c502c1470","resolution":{"observed_at":"2026-08-06T20:45:31.949555Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.4241","last_updated":"2012-10-18T19:26:08Z","snapshot_observed_at":"2026-08-15T00:59:38.744392Z","submitted_at":"2012-05-18T20:00:02Z","title":"Self-accelerating Massive Gravity: Exact solutions for any isotropic matter distribution","version":2},"cited_work":{"arxiv_id":"1205.4241","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.4241","snapshot_observed_at":"2026-08-06T20:45:32.989822Z","title":"Self-accelerating Massive Gravity: Exact solutions for any isotropic matter distribution","venue":"hep-th","work_id":"92db3b53-b71d-4ec5-bf42-6919a491426c","year":2012},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.952179Z"},"links":{"cited_paper":"/paper/1205.4241","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:40f1668bf0251ee12b7137b281aa9518aec03ac34384066fb923e9b2ab1f70ac","observation_id":"2b25b8f6-ea2e-41e3-9d2b-3ef29e4abb57","resolution":{"observed_at":"2026-08-06T20:45:32.993594Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1206.2723","last_updated":"2012-10-01T07:38:06Z","snapshot_observed_at":"2026-08-15T00:57:04.303390Z","submitted_at":"2012-06-13T05:56:34Z","title":"Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.2723","snapshot_observed_at":"2026-08-06T20:45:31.955224Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.955224Z"},"links":{"cited_paper":"/paper/1206.2723","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:5dd106db018ade225c618823b543533a9aaced4916d46ef56853d103913740fa","observation_id":"7a96c8dc-e35d-4c29-991f-441a068747b7","resolution":{"observed_at":"2026-08-06T20:45:31.955224Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.6198","last_updated":"2013-11-07T11:43:21Z","snapshot_observed_at":"2026-08-15T00:27:33.079434Z","submitted_at":"2013-02-25T19:27:33Z","title":"Anisotropic universes in the ghost-free bigravity","version":3},"cited_work":{"arxiv_id":"1302.6198","doi":null,"metadata_source":"pith","pith_arxiv_id":"1302.6198","snapshot_observed_at":"2026-08-06T20:45:32.968886Z","title":"Anisotropic universes in the ghost-free bigravity","venue":"hep-th","work_id":"5fec23e2-3818-4059-8e9e-04beb1f2fb8a","year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.957772Z"},"links":{"cited_paper":"/paper/1302.6198","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:a78a9ee6ae36bf66c3bb6c4d6a780c08d20c75b9df7ecc6f28bdfa29551f04c3","observation_id":"41b02897-813a-4da7-82b8-7d75380f2877","resolution":{"observed_at":"2026-08-06T20:45:32.972263Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1302.5268","last_updated":"2013-02-21T12:56:26Z","snapshot_observed_at":"2026-08-15T00:27:58.304457Z","submitted_at":"2013-02-21T12:56:26Z","title":"Cosmological constraints on ghost-free bigravity: background dynamics and late-time acceleration","version":1},"cited_work":{"arxiv_id":"1302.5268","doi":null,"metadata_source":"pith","pith_arxiv_id":"1302.5268","snapshot_observed_at":"2026-08-06T20:45:32.957333Z","title":"Cosmological constraints on ghost-free bigravity: background dynamics and late-time acceleration","venue":"astro-ph.CO","work_id":"89a62fc7-8efb-42cf-91fc-4db86d01b4a3","year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.960716Z"},"links":{"cited_paper":"/paper/1302.5268","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:8bdcced385584af49865c2900000b5f2498983f6bfe03b38cffee0ff5698ccaf","observation_id":"fc273a86-72ec-4d3f-a1e1-0f748adf44d0","resolution":{"observed_at":"2026-08-06T20:45:32.960583Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1302.6407","last_updated":"2013-03-20T11:51:59Z","snapshot_observed_at":"2026-08-15T00:27:27.523128Z","submitted_at":"2013-02-26T11:52:46Z","title":"Oscillating universe in massive gravity","version":2},"cited_work":{"arxiv_id":"1302.6407","doi":null,"metadata_source":"pith","pith_arxiv_id":"1302.6407","snapshot_observed_at":"2026-08-06T20:45:32.945280Z","title":"Oscillating universe in massive gravity","venue":"gr-qc","work_id":"a48ee616-3e66-4949-9e87-9e8b3f9aebb7","year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.963397Z"},"links":{"cited_paper":"/paper/1302.6407","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:4d5af38a35d226bdb600dfc2f0f2144f9208076eb48ef07367d55091be0f57fb","observation_id":"8bb51a9d-4c63-4b3b-ad5b-6900bf60a75b","resolution":{"observed_at":"2026-08-06T20:45:32.949303Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1208.5512","last_updated":"2012-08-27T21:28:54Z","snapshot_observed_at":"2026-08-15T17:44:12.122294Z","submitted_at":"2012-08-27T21:28:54Z","title":"Constraints on massive gravity theory from big bang nucleosynthesis","version":1},"cited_work":{"arxiv_id":"1208.5512","doi":null,"metadata_source":"pith","pith_arxiv_id":"1208.5512","snapshot_observed_at":"2026-08-06T20:45:32.933333Z","title":"Constraints on massive gravity theory from big bang nucleosynthesis","venue":"gr-qc","work_id":"6284e4a3-0693-46e7-8caa-e85e465a5e23","year":2012},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.966207Z"},"links":{"cited_paper":"/paper/1208.5512","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:be9cac50cb718acab20e9da435d44c6189a12ddc772384956144db02f6d3f9e8","observation_id":"24b227ad-e88c-4d3c-9600-841cd32a2f8c","resolution":{"observed_at":"2026-08-06T20:45:32.937177Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1110.2618","last_updated":"2011-10-12T09:46:46Z","snapshot_observed_at":"2026-08-15T04:32:29.009162Z","submitted_at":"2011-10-12T09:46:46Z","title":"The Self-Accelerating Universe with Vectors in Massive Gravity","version":1},"cited_work":{"arxiv_id":"1110.2618","doi":null,"metadata_source":"pith","pith_arxiv_id":"1110.2618","snapshot_observed_at":"2026-08-06T20:45:32.921726Z","title":"The Self-Accelerating Universe with Vectors in Massive Gravity","venue":"hep-th","work_id":"dce37432-bd42-4467-86e5-9aecdec29148","year":2011},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.969091Z"},"links":{"cited_paper":"/paper/1110.2618","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:f0e566b85957be27a525b34600917b7dfb327616d4cd65a77d33db2c68939553","observation_id":"8a5a7916-3386-4e04-9552-48ccd420d048","resolution":{"observed_at":"2026-08-06T20:45:32.925259Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1210.3627","last_updated":"2012-10-12T20:03:04Z","snapshot_observed_at":"2026-08-15T00:43:18.868486Z","submitted_at":"2012-10-12T20:03:04Z","title":"Vector instabilities and self-acceleration in the decoupling limit of massive gravity","version":1},"cited_work":{"arxiv_id":"1210.3627","doi":null,"metadata_source":"pith","pith_arxiv_id":"1210.3627","snapshot_observed_at":"2026-08-06T20:45:32.909035Z","title":"Vector instabilities and self-acceleration in the decoupling limit of massive gravity","venue":"hep-th","work_id":"d004429a-27b0-4994-be44-081923801a34","year":2012},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.971892Z"},"links":{"cited_paper":"/paper/1210.3627","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:83c73214ef252d24a89f434b9b1fc2d660dad904df59374d4195261e1c3302a5","observation_id":"335bc938-61b0-417b-b0df-9accc54c5ce3","resolution":{"observed_at":"2026-08-06T20:45:32.912279Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.8300","last_updated":"2015-04-20T14:54:12Z","snapshot_observed_at":"2026-08-14T23:17:39.304100Z","submitted_at":"2014-09-29T20:00:19Z","title":"Cosmological viability of massive gravity with generalized matter coupling","version":3},"cited_work":{"arxiv_id":"1409.8300","doi":null,"metadata_source":"pith","pith_arxiv_id":"1409.8300","snapshot_observed_at":"2026-08-06T20:45:32.897758Z","title":"Cosmological viability of massive gravity with generalized matter coupling","venue":"astro-ph.CO","work_id":"a299ce5d-81e5-4b50-b29a-33b66ab080c6","year":2014},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.974904Z"},"links":{"cited_paper":"/paper/1409.8300","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:2b9b533d422fc7b913151c77ab765a30a09bb8ecf84982e40bbe1e65a6a154b1","observation_id":"b295ec5f-4066-4cea-823e-b6e1e99b11b7","resolution":{"observed_at":"2026-08-06T20:45:32.900932Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1306.0004","last_updated":"2013-10-24T13:50:39Z","snapshot_observed_at":"2026-08-15T00:15:38.184125Z","submitted_at":"2013-05-31T20:00:01Z","title":"Bimetric gravity doubly coupled to matter: theory and cosmological implications","version":2},"cited_work":{"arxiv_id":"1306.0004","doi":null,"metadata_source":"pith","pith_arxiv_id":"1306.0004","snapshot_observed_at":"2026-08-06T20:45:32.886075Z","title":"Bimetric gravity doubly coupled to matter: theory and cosmological implications","venue":"hep-th","work_id":"854b2a21-6060-4597-8921-a329d4a0c38d","year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.977624Z"},"links":{"cited_paper":"/paper/1306.0004","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:720fdef24aceb6c16cc0c957d64fe343d2cbb33eadf41675e46d858f7a7f7797","observation_id":"02be208b-469e-4ff3-9ae0-016058d7f066","resolution":{"observed_at":"2026-08-06T20:45:32.889500Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1407.4331","last_updated":"2014-12-09T08:32:48Z","snapshot_observed_at":"2026-08-14T23:26:32.031543Z","submitted_at":"2014-07-16T14:56:06Z","title":"Stable and unstable cosmological models in bimetric massive gravity","version":3},"cited_work":{"arxiv_id":"1407.4331","doi":null,"metadata_source":"pith","pith_arxiv_id":"1407.4331","snapshot_observed_at":"2026-08-06T20:45:32.873970Z","title":"Stable and unstable cosmological models in bimetric massive gravity","venue":"astro-ph.CO","work_id":"6ccf4fa7-b076-48a0-b1bb-4f481d8b5ed5","year":2014},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.980384Z"},"links":{"cited_paper":"/paper/1407.4331","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:9121407e9fe7b43ff02076e9ece943a81551f922fef69a240a28c18c6d38d999","observation_id":"793d079e-11a2-4462-8ee0-067d3099f494","resolution":{"observed_at":"2026-08-06T20:45:32.877365Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.03562","last_updated":"2016-11-23T14:24:44Z","snapshot_observed_at":"2026-08-15T22:21:04.301289Z","submitted_at":"2016-10-11T23:42:17Z","title":"Role of matter in extended quasidilaton massive gravity","version":2},"cited_work":{"arxiv_id":"1610.03562","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.03562","snapshot_observed_at":"2026-08-06T20:45:32.861964Z","title":"Role of matter in extended quasidilaton massive gravity","venue":"hep-th","work_id":"1bf230b7-80f8-4298-9cc4-54baf2aa30c7","year":2016},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.983156Z"},"links":{"cited_paper":"/paper/1610.03562","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:279ace7f709d080d1518b7fa7fb742371788f7b296a65ed7c361b1d47785acba","observation_id":"5495728f-3c52-4260-af11-c03343cdaf23","resolution":{"observed_at":"2026-08-06T20:45:32.865198Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.19873","last_updated":"2024-11-29T17:34:13Z","snapshot_observed_at":"2026-08-13T18:15:49.602100Z","submitted_at":"2024-11-29T17:34:13Z","title":"To the Problem of Cosmic Expansion in Massive Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.19873","snapshot_observed_at":"2026-08-06T20:45:31.985900Z","title":"Heisenberg, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.985900Z"},"links":{"cited_paper":"/paper/2411.19873","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:5dc1d72ad24f19691d7fcb1c02e730ab7ffeaf412377da6597d259c772f3aeea","observation_id":"74346e10-024d-48f3-82e3-2c57d8cd1a04","resolution":{"observed_at":"2026-08-06T20:45:31.985900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.03870","last_updated":"2025-05-25T17:07:36Z","snapshot_observed_at":"2026-08-16T10:59:08.075923Z","submitted_at":"2025-05-06T18:00:00Z","title":"Dynamical Dark Energy Emerges from Massive Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.03870","snapshot_observed_at":"2026-08-06T20:45:31.988914Z","title":"Smirnov, arXiv e-prints , arXiv:2505.03870 (2025), arXiv:2505.03870 [astro-ph.CO]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.988914Z"},"links":{"cited_paper":"/paper/2505.03870","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:df45de3e47f52910533d14f7ae0b486e8ab48ee0713677dbe5098543c8292e98","observation_id":"82ae0244-f423-46b8-b957-63ab89e1d074","resolution":{"observed_at":"2026-08-06T20:45:31.988914Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.8329","last_updated":"2014-05-27T15:12:05Z","snapshot_observed_at":"2026-08-15T00:08:21.171743Z","submitted_at":"2013-07-31T14:18:56Z","title":"Cosmology in General Massive Gravity Theories","version":2},"cited_work":{"arxiv_id":"1307.8329","doi":null,"metadata_source":"pith","pith_arxiv_id":"1307.8329","snapshot_observed_at":"2026-08-06T20:45:32.834854Z","title":"Cosmology in General Massive Gravity Theories","venue":"hep-th","work_id":"2e3f3ace-58be-4bc4-a766-3b15e095531b","year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.991684Z"},"links":{"cited_paper":"/paper/1307.8329","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:3af8d68e17244a61c227931dad169b3e8b9c45e1ad58d310e06085b6f0f37c45","observation_id":"3b71f268-5744-496d-85ef-ab0351246940","resolution":{"observed_at":"2026-08-06T20:45:32.838162Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.4154","last_updated":"2013-06-04T09:40:35Z","snapshot_observed_at":"2026-08-15T00:24:52.677940Z","submitted_at":"2013-03-18T04:33:19Z","title":"Nonlinear stability of cosmological solutions in massive gravity","version":2},"cited_work":{"arxiv_id":"1303.4154","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.4154","snapshot_observed_at":"2026-08-06T20:45:32.823209Z","title":"Nonlinear stability of cosmological solutions in massive gravity","venue":"hep-th","work_id":"f911dd4c-3b13-4fda-85e8-ac61f1c7422b","year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.995013Z"},"links":{"cited_paper":"/paper/1303.4154","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:fdd614cf1ba5178d2220a92ebfdbb008b440237cbd22a89e592bece3af67054c","observation_id":"cd2304ad-23bf-4cf0-bda3-cd0afaa37038","resolution":{"observed_at":"2026-08-06T20:45:32.826469Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1304.0449","last_updated":"2013-04-01T20:00:00Z","snapshot_observed_at":"2026-08-15T00:23:00.966159Z","submitted_at":"2013-04-01T20:00:00Z","title":"Cosmological Perturbations in Extended Massive Gravity","version":1},"cited_work":{"arxiv_id":"1304.0449","doi":null,"metadata_source":"pith","pith_arxiv_id":"1304.0449","snapshot_observed_at":"2026-08-06T20:45:32.811881Z","title":"Cosmological Perturbations in Extended Massive Gravity","venue":"hep-th","work_id":"2e1f389e-e3af-4a55-ba81-8b66d2409340","year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:31.997769Z"},"links":{"cited_paper":"/paper/1304.0449","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:98514875f21afb989269602440671a8639ba97f62f5e3741b4972bb7f2d5fb85","observation_id":"2313b112-072d-46fd-9cf5-0c154993284b","resolution":{"observed_at":"2026-08-06T20:45:32.814872Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1304.0484","last_updated":"2013-09-11T11:43:05Z","snapshot_observed_at":"2026-08-15T00:23:00.112800Z","submitted_at":"2013-04-01T21:31:08Z","title":"On the cosmology of massive gravity","version":2},"cited_work":{"arxiv_id":"1304.0484","doi":null,"metadata_source":"pith","pith_arxiv_id":"1304.0484","snapshot_observed_at":"2026-08-06T20:45:32.799604Z","title":"On the cosmology of massive gravity","venue":"hep-th","work_id":"18113eda-6ef8-4e5c-b207-0e0b0a10bc75","year":2013},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.000661Z"},"links":{"cited_paper":"/paper/1304.0484","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:20c5b6d5a9e1bff6aef50ea609852074e3f1f83b422852080e78adb0c66e7c8c","observation_id":"c4fd42db-819a-4af8-a116-66245a80df9a","resolution":{"observed_at":"2026-08-06T20:45:32.803385Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1512.04008","last_updated":"2017-07-22T04:06:54Z","snapshot_observed_at":"2026-08-17T23:20:36.465510Z","submitted_at":"2015-12-13T06:04:26Z","title":"Phenomenology in minimal theory of massive gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.04008","snapshot_observed_at":"2026-08-06T20:45:32.003210Z","title":"De Felice and S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.003210Z"},"links":{"cited_paper":"/paper/1512.04008","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:011342c06bb51a5cf6165a21d7e4c45fb5b35baa07722218223a2991ee33359f","observation_id":"a629a595-0045-483b-960c-2202f19b85b6","resolution":{"observed_at":"2026-08-06T20:45:32.003210Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.07529","last_updated":"2015-07-15T15:45:01Z","snapshot_observed_at":"2026-08-14T22:54:54.595359Z","submitted_at":"2015-03-25T20:00:39Z","title":"Black holes in massive gravity","version":2},"cited_work":{"arxiv_id":"1503.07529","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.07529","snapshot_observed_at":"2026-08-06T20:45:32.780513Z","title":"Black holes in massive gravity","venue":"gr-qc","work_id":"631e2134-987a-4c90-8415-859adafe30c3","year":2015},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.005954Z"},"links":{"cited_paper":"/paper/1503.07529","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:21cb230588dd3aa9b48d2af4d846361238f1ff98df0e2f8c8242c506f96d502b","observation_id":"a3db9646-a388-4c46-9a59-0caaef417c77","resolution":{"observed_at":"2026-08-06T20:45:32.783370Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1704.02425","last_updated":"2017-07-24T17:52:42Z","snapshot_observed_at":"2026-08-14T21:07:42.359561Z","submitted_at":"2017-04-08T02:34:07Z","title":"Tests of Gravity Theories Using Supermassive Black Holes","version":2},"cited_work":{"arxiv_id":"1704.02425","doi":null,"metadata_source":"pith","pith_arxiv_id":"1704.02425","snapshot_observed_at":"2026-08-06T20:45:32.765969Z","title":"Tests of Gravity Theories Using Supermassive Black Holes","venue":"astro-ph.CO","work_id":"95e91bae-0a53-46bf-9494-92fb43c7d9c9","year":2017},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.008362Z"},"links":{"cited_paper":"/paper/1704.02425","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:c81097179ab5c2b208584b1561affb85687485f84971b19033be58819e09f136","observation_id":"430a8d50-64be-477e-aac3-6366e98f603f","resolution":{"observed_at":"2026-08-06T20:45:32.768903Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2026-08-06T20:45:32.011429Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.011429Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:82c71ed8c5d3744e4629806579304ce2e372bfc84dc7d2806518d5590665ba9f","observation_id":"efd47803-8116-4146-9526-d87e9e67409d","resolution":{"observed_at":"2026-08-06T20:45:32.011429Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.04855","last_updated":"2016-06-15T16:44:04Z","snapshot_observed_at":"2026-08-14T21:52:35.855236Z","submitted_at":"2016-06-15T16:44:04Z","title":"GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.04855","snapshot_observed_at":"2026-08-06T20:45:32.014687Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.014687Z"},"links":{"cited_paper":"/paper/1606.04855","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:9997e4ceaa90a0e2461f94c260136a83d81071d08f8614efde82a12171ff54c9","observation_id":"279ef63e-1db9-46ed-86ee-45a2da54f187","resolution":{"observed_at":"2026-08-06T20:45:32.014687Z","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":"2026-08-06T20:45:32.017909Z","title":"Akutsu et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.017909Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:4a80a99b2c3d490cd7ac6a96fd3266d8bc9e5aac88d8594ae8ce6d009fcb2be6","observation_id":"0bcbe881-7ff7-4a94-8bcb-1a64b543e682","resolution":{"observed_at":"2026-08-06T20:45:32.017909Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3978","last_updated":"2014-10-16T13:24:29Z","snapshot_observed_at":"2026-08-12T13:34:29.588273Z","submitted_at":"2014-08-18T11:19:22Z","title":"Advanced Virgo: a 2nd generation interferometric gravitational wave detector","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.3978","snapshot_observed_at":"2026-08-06T20:45:32.020440Z","title":"Acernese et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.020440Z"},"links":{"cited_paper":"/paper/1408.3978","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:f71c4a93662745697ea7a11c84fd92fad36ae5833d682ac1e2b9675173768f7f","observation_id":"49fc58aa-186c-4deb-a33c-a1afb56f1e22","resolution":{"observed_at":"2026-08-06T20:45:32.020440Z","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":"2026-08-06T20:45:32.023831Z","title":"Agazie, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.023831Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:b325f3473a13031a562d797b43e452f667550550d579878a9e922ae91d2606f4","observation_id":"bc2e697b-7e6b-40a3-ac30-96b972a94f08","resolution":{"observed_at":"2026-08-06T20:45:32.023831Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16216","last_updated":"2023-06-28T13:51:04Z","snapshot_observed_at":"2026-08-08T13:18:07.452026Z","submitted_at":"2023-06-28T13:51:04Z","title":"Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16216","snapshot_observed_at":"2026-08-06T20:45:32.026389Z","title":"Xu et al., Res","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.026389Z"},"links":{"cited_paper":"/paper/2306.16216","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:f0a0a15eb03a6f1be46d66c3fd1d30b541eaba9e8e3a5f5f703aec66ca3f19e0","observation_id":"33bcc9b5-f829-4def-aeb2-87ff6bd6bafd","resolution":{"observed_at":"2026-08-06T20:45:32.026389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16224","last_updated":"2023-06-28T13:51:12Z","snapshot_observed_at":"2026-08-18T17:15:24.425540Z","submitted_at":"2023-06-28T13:51:12Z","title":"The second data release from the European Pulsar Timing Array I. The dataset and timing analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16224","snapshot_observed_at":"2026-08-06T20:45:32.029144Z","title":"Antoniadis, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.029144Z"},"links":{"cited_paper":"/paper/2306.16224","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:2b47b7b984866276534ef8097e10144d1171711351de744f1a973c65322cdc2a","observation_id":"d9d869c1-20cf-483f-baf4-212328347137","resolution":{"observed_at":"2026-08-06T20:45:32.029144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16225","last_updated":"2023-06-28T13:51:13Z","snapshot_observed_at":"2026-08-18T17:14:10.501057Z","submitted_at":"2023-06-28T13:51:13Z","title":"The second data release from the European Pulsar Timing Array II. Customised pulsar noise models for spatially correlated gravitational waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16225","snapshot_observed_at":"2026-08-06T20:45:32.031929Z","title":"Antoniadis et al.(EPTA and InPTA Collaborations), Astron","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.031929Z"},"links":{"cited_paper":"/paper/2306.16225","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:38c64fc2355bcf4f709c37c506d4280d2edba92243ea0203f3880dfe0ddff9f7","observation_id":"21513153-0959-4340-9d68-022c8e5168d4","resolution":{"observed_at":"2026-08-06T20:45:32.031929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16214","last_updated":"2023-06-28T13:51:02Z","snapshot_observed_at":"2026-08-17T09:03:17.044903Z","submitted_at":"2023-06-28T13:51:02Z","title":"The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16214","snapshot_observed_at":"2026-08-06T20:45:32.034880Z","title":"Antoniadis et al.(EPTA and InPTA Collaborations), Astron","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.034880Z"},"links":{"cited_paper":"/paper/2306.16214","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:9fd1db653dbbcc6ca712bb6d8b9114fda56874afc396d669edc2499fbcde684b","observation_id":"b97b387f-cfa6-4844-bd66-65e48d6907c8","resolution":{"observed_at":"2026-08-06T20:45:32.034880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16230","last_updated":"2023-10-18T03:46:43Z","snapshot_observed_at":"2026-08-16T15:20:24.185912Z","submitted_at":"2023-06-28T13:51:18Z","title":"The Parkes Pulsar Timing Array Third Data Release","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16230","snapshot_observed_at":"2026-08-06T20:45:32.037712Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.037712Z"},"links":{"cited_paper":"/paper/2306.16230","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:c0921a6471ad274bfa1027bd6f324e19b4dd2f6648ec661e88c5ae2549f95f15","observation_id":"221614f2-29a5-4335-888e-a29435333cff","resolution":{"observed_at":"2026-08-06T20:45:32.037712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16215","last_updated":"2023-06-28T13:51:03Z","snapshot_observed_at":"2026-08-12T23:01:24.461267Z","submitted_at":"2023-06-28T13:51:03Z","title":"Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16215","snapshot_observed_at":"2026-08-06T20:45:32.040285Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.040285Z"},"links":{"cited_paper":"/paper/2306.16215","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:d4083d719e1d1dd57cedfef4103ac1dc507a3ed92580bf09e64a36cdc4f98a70","observation_id":"20635fb4-2961-49f7-9b09-eb2fd140340d","resolution":{"observed_at":"2026-08-06T20:45:32.040285Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.05344","last_updated":"2026-07-24T01:40:05Z","snapshot_observed_at":"2026-08-16T18:03:47.667497Z","submitted_at":"2021-08-11T17:53:08Z","title":"Detecting the Stochastic Gravitational Wave Background from Massive Gravity with Pulsar Timing Arrays","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.05344","snapshot_observed_at":"2026-08-06T20:45:32.042720Z","title":"Liang and M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.042720Z"},"links":{"cited_paper":"/paper/2108.05344","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:00629fea6476f384805151f210960c373d81ff5483a82609043fafdb19ffcb39","observation_id":"29850003-53a2-4172-94db-187348bf8755","resolution":{"observed_at":"2026-08-06T20:45:32.042720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.0701","last_updated":"2008-12-16T23:31:23Z","snapshot_observed_at":"2026-08-16T08:09:10.440792Z","submitted_at":"2008-09-03T20:12:48Z","title":"Optimal strategies for gravitational wave stochastic background searches in pulsar timing data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.0701","snapshot_observed_at":"2026-08-06T20:45:32.045282Z","title":"Anholm, S","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.045282Z"},"links":{"cited_paper":"/paper/0809.0701","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:276ab73e6d226281a26a223c148ed0602e39ac670ab3f6186469d39282a30d2d","observation_id":"9d6a8269-f0f7-414e-843c-cffd63e9a2dc","resolution":{"observed_at":"2026-08-06T20:45:32.045282Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12975","last_updated":"2024-12-17T14:57:18Z","snapshot_observed_at":"2026-08-15T08:35:37.226275Z","submitted_at":"2024-12-17T14:57:18Z","title":"Comparative analysis of the NANOgrav Hellings-Downs as a window into new physics","version":1},"cited_work":{"arxiv_id":"2412.12975","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12975","snapshot_observed_at":"2026-08-06T20:45:32.613057Z","title":"Comparative analysis of the NANOgrav Hellings-Downs as a window into new physics","venue":"astro-ph.CO","work_id":"9fcead59-7db0-4df7-b1b0-604aaeec7e95","year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.047852Z"},"links":{"cited_paper":"/paper/2412.12975","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:44b8e9e0086c00b0a0040357b13efbe92e4cc963c5c058e69278a232e24ee6a5","observation_id":"bb8ba045-ef34-4270-b44a-6e52c9e2901a","resolution":{"observed_at":"2026-08-06T20:45:32.616213Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.2090","last_updated":"2014-04-08T11:01:32Z","snapshot_observed_at":"2026-08-14T23:38:16.334201Z","submitted_at":"2014-04-08T11:01:32Z","title":"Pulsar Timing Arrays and Gravity Tests in the Radiative Regime","version":1},"cited_work":{"arxiv_id":"1404.2090","doi":null,"metadata_source":"pith","pith_arxiv_id":"1404.2090","snapshot_observed_at":"2026-08-06T20:45:32.601944Z","title":"Pulsar Timing Arrays and Gravity Tests in the Radiative Regime","venue":"astro-ph.CO","work_id":"cb86b8fa-867a-4e41-a2cb-c7e1c2cc5d06","year":2014},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.050329Z"},"links":{"cited_paper":"/paper/1404.2090","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:4e38d1aeb2bc43ac260976d7e14c4fcf436765660680dc4e8adbe460a489f1cc","observation_id":"0cc81f97-2aa0-47e7-acbc-45c74672476d","resolution":{"observed_at":"2026-08-06T20:45:32.604733Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.11796","last_updated":"2023-05-11T16:37:13Z","snapshot_observed_at":"2026-08-16T15:53:21.465536Z","submitted_at":"2023-02-23T06:20:10Z","title":"Constraining gravitational wave propagation using pulsar timing array correlations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.11796","snapshot_observed_at":"2026-08-06T20:45:32.053129Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.053129Z"},"links":{"cited_paper":"/paper/2302.11796","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:28106244faaf6c70efffee02055b9a613b13edf822e3d8f13f4076b18480d69f","observation_id":"31c23c88-610e-4834-93e4-c1b74c62538f","resolution":{"observed_at":"2026-08-06T20:45:32.053129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.13593","last_updated":"2024-05-22T04:21:03Z","snapshot_observed_at":"2026-08-16T15:21:37.166413Z","submitted_at":"2023-06-23T16:33:18Z","title":"Testing gravity with cosmic variance-limited pulsar timing array correlations","version":4},"cited_work":{"arxiv_id":"2306.13593","doi":null,"metadata_source":"pith","pith_arxiv_id":"2306.13593","snapshot_observed_at":"2026-08-06T20:45:32.582471Z","title":"Testing gravity with cosmic variance-limited pulsar timing array correlations","venue":"gr-qc","work_id":"63976fe4-3758-45c4-a6d2-cf98e0e4f482","year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.055895Z"},"links":{"cited_paper":"/paper/2306.13593","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:00a9933f32957912e637686e5e8a98cabef2df30e8e27d8091e1213642c84565","observation_id":"e2aa964d-cf0d-4ae4-9fd2-8ab43d97b177","resolution":{"observed_at":"2026-08-06T20:45:32.585551Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07537","last_updated":"2024-10-01T07:45:37Z","snapshot_observed_at":"2026-08-16T14:53:03.008668Z","submitted_at":"2023-10-11T14:40:52Z","title":"Beyond the Hellings-Downs curve: Non-Einsteinian gravitational waves in pulsar timing array correlations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.07537","snapshot_observed_at":"2026-08-06T20:45:32.058545Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.058545Z"},"links":{"cited_paper":"/paper/2310.07537","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:e6634cb02bd5f5705fa7ba5c3891f3b0d2d6819f641f2d8d424c684eb5986973","observation_id":"eb49bf66-5625-4f2c-8b16-0c42c81fea4b","resolution":{"observed_at":"2026-08-06T20:45:32.058545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.07955","last_updated":"2024-09-18T13:41:41Z","snapshot_observed_at":"2026-08-16T13:19:10.563641Z","submitted_at":"2024-09-12T11:34:18Z","title":"Charting the Nanohertz Gravitational Wave Sky with Pulsar Timing Arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.07955","snapshot_observed_at":"2026-08-06T20:45:32.061161Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.061161Z"},"links":{"cited_paper":"/paper/2409.07955","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:23a24d9e805e46ffd7ac5a844ac9c9e77ff827305d0decc505394221ed5bc024","observation_id":"ac8bfc94-b78c-4c97-be37-4f5fde58b336","resolution":{"observed_at":"2026-08-06T20:45:32.061161Z","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":"2026-08-06T20:45:32.064064Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.064064Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:8fa97530d9cdb4121e8ee60dca5f5099401f4d30043abc35ef03320295c7ddf6","observation_id":"cbea7475-12d5-46cc-9c47-c56ac57c32cc","resolution":{"observed_at":"2026-08-06T20:45:32.064064Z","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":"2026-08-06T20:45:32.066429Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.066429Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:8b3d85e23b11be415eb4cda327c770c424af470173fed59ddf120b2049cf96f8","observation_id":"757da361-6508-4653-a3c1-8657bae8d016","resolution":{"observed_at":"2026-08-06T20:45:32.066429Z","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":"2026-08-15T21:57:31.832991Z","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":"2026-08-06T20:45:32.069119Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.069119Z"},"links":{"cited_paper":"/paper/1710.05834","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:0671bf10b77f467de457ee9b6673c0fe26b267b2845ebf0a2818e3220b6617b5","observation_id":"54e0ad76-57ca-407c-b008-49cc951aeb9a","resolution":{"observed_at":"2026-08-06T20:45:32.069119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05833","last_updated":"2017-10-24T12:03:18Z","snapshot_observed_at":"2026-08-19T15:24:12.152497Z","submitted_at":"2017-10-16T16:57:18Z","title":"Multi-messenger Observations of a Binary Neutron Star Merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05833","snapshot_observed_at":"2026-08-06T20:45:32.071559Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.071559Z"},"links":{"cited_paper":"/paper/1710.05833","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:caf0dd4cb871a8a20f2e6f3b79f0d2d32998a066a57930f2681f2709a3c15f17","observation_id":"586b77ab-3688-430e-a9cd-bc71969ec06a","resolution":{"observed_at":"2026-08-06T20:45:32.071559Z","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":"2026-08-06T20:45:32.074099Z","title":"De Felice and S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.074099Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:331466f8d708d3650aa3c84122e7484742aa4c754561862ae9b02eeb3111c0d6","observation_id":"b98b746a-bc4f-4524-a650-1d191d215e90","resolution":{"observed_at":"2026-08-06T20:45:32.074099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.02123","last_updated":"2018-07-05T18:00:12Z","snapshot_observed_at":"2026-08-14T18:55:16.745867Z","submitted_at":"2018-07-05T18:00:12Z","title":"Measuring stochastic gravitational-wave energy beyond general relativity","version":1},"cited_work":{"arxiv_id":"1807.02123","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.02123","snapshot_observed_at":"2026-08-06T20:45:32.466323Z","title":"Measuring stochastic gravitational-wave energy beyond general relativity","venue":"gr-qc","work_id":"f25ec620-e85a-453a-838d-c113fff7d9e5","year":2018},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.076448Z"},"links":{"cited_paper":"/paper/1807.02123","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:acf56341b380be61e5a954651a18af63c8a6f497e47aeb40ad34b271402bc19a","observation_id":"b0885480-dd15-4ef5-b34e-e7a51a2faa55","resolution":{"observed_at":"2026-08-06T20:45:32.469199Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:45:32.079495Z","title":"Proca, J","venue":null,"work_id":null,"year":1936},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.079495Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:36302d8416e28401277baff366a6170e58a74e1bf2170afae5144bebe5da84e2","observation_id":"5b94d8db-db7a-4c89-96c7-b719433f0ed7","resolution":{"observed_at":"2026-08-06T20:45:32.079495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.04672","last_updated":"2024-09-07T01:29:43Z","snapshot_observed_at":"2026-08-16T13:20:36.656265Z","submitted_at":"2024-09-07T01:29:43Z","title":"The Dispersion Relation of Massive Photons in Plasma: A Comment on \"Bounding the Photon Mass with Ultrawide Bandwidth Pulsar Timing Data and Dedispersed Pulses of Fast Radio Bursts\"","version":1},"cited_work":{"arxiv_id":"2409.04672","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.04672","snapshot_observed_at":"2026-08-06T20:45:32.455160Z","title":"The Dispersion Relation of Massive Photons in Plasma: A Comment on \"Bounding the Photon Mass with Ultrawide Bandwidth Pulsar Timing Data and Dedispersed Pulses of Fast Radio Bursts\"","venue":"astro-ph.HE","work_id":"f961731c-9a97-4a6c-919a-e0dd668e8106","year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.081889Z"},"links":{"cited_paper":"/paper/2409.04672","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:a5cef4d76993d52feb4162f20b09f62bb57b51450fb971dfb5d339a32e4e68e9","observation_id":"f8251872-95e3-4915-a9c6-82e80c4507d7","resolution":{"observed_at":"2026-08-06T20:45:32.458124Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1208.5975","last_updated":"2012-12-12T07:43:01Z","snapshot_observed_at":"2026-08-15T00:48:29.158485Z","submitted_at":"2012-08-29T17:41:43Z","title":"Gravitational wave signal from massive gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.5975","snapshot_observed_at":"2026-08-06T20:45:32.084441Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.084441Z"},"links":{"cited_paper":"/paper/1208.5975","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:ebd958f107be667fc420a4b55a1521004c0864d4b8f317683c8df7e81ff7255e","observation_id":"8d5dfd5f-73f5-43ea-a769-b273e4868848","resolution":{"observed_at":"2026-08-06T20:45:32.084441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.01954","last_updated":"2020-03-20T05:56:02Z","snapshot_observed_at":"2026-08-05T02:34:16.583093Z","submitted_at":"2020-02-04T11:44:49Z","title":"Review of Pulsar Timing Array for Gravitational Wave Research","version":2},"cited_work":{"arxiv_id":"2002.01954","doi":null,"metadata_source":"pith","pith_arxiv_id":"2002.01954","snapshot_observed_at":"2026-08-06T20:45:32.435767Z","title":"Review of Pulsar Timing Array for Gravitational Wave Research","venue":"astro-ph.IM","work_id":"739425a3-b9e9-4848-bbdb-892cdd468132","year":2020},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.087019Z"},"links":{"cited_paper":"/paper/2002.01954","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:21a37dbb92a3ef09a8ccacde186ad1653edae0531da7855eb6b3508b1899ada1","observation_id":"e930905a-970a-4372-a641-fcf8e3f6ed6b","resolution":{"observed_at":"2026-08-06T20:45:32.438908Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.05847","last_updated":"2024-08-01T15:16:05Z","snapshot_observed_at":"2026-08-20T04:05:45.390090Z","submitted_at":"2023-08-10T20:03:18Z","title":"Answers to frequently asked questions about the pulsar timing array Hellings and Downs curve","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.05847","snapshot_observed_at":"2026-08-06T20:45:32.089607Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.089607Z"},"links":{"cited_paper":"/paper/2308.05847","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:bbdcdd3b350c7bf780c3cc8485c273578cfc261e46a840d91ac18e8e43f5766d","observation_id":"8304adf6-4ec1-4e4d-bc8c-6d71eb10e9ab","resolution":{"observed_at":"2026-08-06T20:45:32.089607Z","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":"2026-08-06T20:45:32.092147Z","title":null,"venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.092147Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:12dd1b1d2ef709357b8fe3f2c75e7955974743dd7ef25b2381281ecc86ce3343","observation_id":"9e807ca0-e5e7-458a-bee1-ca7e6a153e73","resolution":{"observed_at":"2026-08-06T20:45:32.092147Z","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":"2026-08-06T20:45:32.094534Z","title":null,"venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.094534Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:6d9cbba660c5ee4bcf5168640dba78305df527f8a07719e94a424b50b9df825a","observation_id":"e90ea10a-08a9-4e7d-91c5-63cafcea6b25","resolution":{"observed_at":"2026-08-06T20:45:32.094534Z","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":"2026-08-06T20:45:32.097075Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.097075Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:ef807b9146d15953c2cfea390a90c10d43f4ada8a197bbfa574f182753d11387","observation_id":"4b4e5b2b-8e54-430f-bb3d-61d2f5f0699c","resolution":{"observed_at":"2026-08-06T20:45:32.097075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.03932","last_updated":"2024-08-28T19:44:48Z","snapshot_observed_at":"2026-08-16T14:37:00.090509Z","submitted_at":"2023-12-06T22:19:35Z","title":"Stochastic gravitational wave background detection using NANOGrav 15-year data set in the context of massive gravity","version":3},"cited_work":{"arxiv_id":"2312.03932","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.03932","snapshot_observed_at":"2026-08-06T20:45:32.415849Z","title":"Stochastic gravitational wave background detection using NANOGrav 15-year data set in the context of massive gravity","venue":"astro-ph.CO","work_id":"c82545a5-888e-44f1-8485-3cacbb857031","year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.099731Z"},"links":{"cited_paper":"/paper/2312.03932","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:669517a9774dad9df686ad3e5c8ea3f2e4a23dd824b104b5d75dd40bd5306922","observation_id":"88e48d0b-e86b-4ce9-bb37-8e1aad631a37","resolution":{"observed_at":"2026-08-06T20:45:32.419226Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07469","last_updated":"2023-10-11T13:15:46Z","snapshot_observed_at":"2026-08-16T14:53:04.907612Z","submitted_at":"2023-10-11T13:15:46Z","title":"Constraining the Graviton Mass with the NANOGrav 15-Year Data Set","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.07469","snapshot_observed_at":"2026-08-06T20:45:32.102292Z","title":"Wu, Z.-C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.102292Z"},"links":{"cited_paper":"/paper/2310.07469","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:8410df489626b8e6c4a65a36d8c347433e52d7dd473310dac561bb1c3a8528ae","observation_id":"46a9509d-af1b-4eef-a7a6-ba5c4f9ccc57","resolution":{"observed_at":"2026-08-06T20:45:32.102292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09658","last_updated":"2025-05-16T18:29:35Z","snapshot_observed_at":"2026-08-16T13:09:59.772040Z","submitted_at":"2024-10-12T21:37:10Z","title":"Connecting Inflation to the NANOGrav 15-year Data Set via Massive Gravity","version":2},"cited_work":{"arxiv_id":"2410.09658","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.09658","snapshot_observed_at":"2026-08-06T20:45:32.393338Z","title":"Connecting Inflation to the NANOGrav 15-year Data Set via Massive Gravity","venue":"astro-ph.CO","work_id":"298f0e8e-b406-4875-b267-6afb65cd2848","year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.105219Z"},"links":{"cited_paper":"/paper/2410.09658","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:4c50e82c4f9a3eeddc54d006e3a57cfaa5f8f9057dd301867988dbd7101e25c2","observation_id":"af4fa4dc-630c-4b9d-baae-3217821cfe61","resolution":{"observed_at":"2026-08-06T20:45:32.397233Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.03192","last_updated":"2021-07-06T09:39:10Z","snapshot_observed_at":"2026-08-16T18:33:16.540405Z","submitted_at":"2021-04-07T15:31:47Z","title":"Tensor spectrum of turbulence-sourced gravitational waves as a constraint on graviton mass","version":2},"cited_work":{"arxiv_id":"2104.03192","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.03192","snapshot_observed_at":"2026-08-06T20:45:32.381672Z","title":"Tensor spectrum of turbulence-sourced gravitational waves as a constraint on graviton mass","venue":"gr-qc","work_id":"7832110c-e4b7-43a1-9e69-895037d05dfc","year":2021},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.108010Z"},"links":{"cited_paper":"/paper/2104.03192","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:c00caeb6aa5c8c2635253c9a6f8d63bbfff20fd0208900e3fd3207aa02a43629","observation_id":"0ce49e73-4031-4347-9677-ade41ff04f73","resolution":{"observed_at":"2026-08-06T20:45:32.384879Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.0740","last_updated":"2014-12-11T16:35:39Z","snapshot_observed_at":"2026-08-14T23:24:17.723128Z","submitted_at":"2014-08-04T16:37:05Z","title":"Gravitational-wave sensitivity curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.0740","snapshot_observed_at":"2026-08-06T20:45:32.110836Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.110836Z"},"links":{"cited_paper":"/paper/1408.0740","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:8e361784966052bae2986ecbc30e6ef0adc6cf4de8d0fa4376e5371bccb45cdf","observation_id":"e75de4e6-b223-4b02-bce0-2f088bdf3468","resolution":{"observed_at":"2026-08-06T20:45:32.110836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.07230","last_updated":"2023-08-24T17:14:41Z","snapshot_observed_at":"2026-08-19T20:00:35.252144Z","submitted_at":"2022-08-15T14:40:29Z","title":"Hellings and Downs correlation of an arbitrary set of pulsars","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.07230","snapshot_observed_at":"2026-08-06T20:45:32.113323Z","title":"Allen and J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.113323Z"},"links":{"cited_paper":"/paper/2208.07230","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:e40eb1713461ded45cd67aed507fdfc0366f925845a3bc6b63a5c055049f49f8","observation_id":"a2a04091-d9fc-4ded-a727-4a78049970f2","resolution":{"observed_at":"2026-08-06T20:45:32.113323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.14460","last_updated":"2024-08-30T16:50:46Z","snapshot_observed_at":"2026-08-20T01:49:31.386738Z","submitted_at":"2024-07-19T17:03:29Z","title":"Pulsar timing array sensitivity to anisotropies in the gravitational wave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14460","snapshot_observed_at":"2026-08-06T20:45:32.116220Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.116220Z"},"links":{"cited_paper":"/paper/2407.14460","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:9a574b91576c1da6fee5fd7aeb18c6d80570b5feb52b60ab7a4024c02474129d","observation_id":"d94c35cc-7324-4e24-8083-a4129b309dd0","resolution":{"observed_at":"2026-08-06T20:45:32.116220Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.15084","last_updated":"2025-05-21T04:12:42Z","snapshot_observed_at":"2026-08-16T08:38:00.896687Z","submitted_at":"2025-05-21T04:12:42Z","title":"Imprints of Large-Scale Structures in the Anisotropies of the Cosmological Gravitational Wave Background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.15084","snapshot_observed_at":"2026-08-06T20:45:32.118806Z","title":"Bravo and W","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.118806Z"},"links":{"cited_paper":"/paper/2505.15084","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:9031cd0fed8083582208726ee458eaffad41b721e2f7d9b5f3b3fa2b6e2552a5","observation_id":"556e5f7b-348a-4364-9a2d-0332484561ef","resolution":{"observed_at":"2026-08-06T20:45:32.118806Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.17401","last_updated":"2025-04-11T15:16:16Z","snapshot_observed_at":"2026-08-16T12:55:38.405859Z","submitted_at":"2025-02-24T18:29:34Z","title":"Measuring anisotropies in the PTA band with cross-correlations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.17401","snapshot_observed_at":"2026-08-06T20:45:32.121510Z","title":"Cusin, C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.121510Z"},"links":{"cited_paper":"/paper/2502.17401","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:0c032be353bf7328ebe85c93fa573c8b8c47523f8c964c494386bde66cf25b1a","observation_id":"8b894547-8988-43d5-9891-67d6482a13ff","resolution":{"observed_at":"2026-08-06T20:45:32.121510Z","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":"2411.19761","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:45:32.329172Z","title":"Kuwahara and L","venue":null,"work_id":"bbf912ea-1f5a-4f23-a81e-0cfadfae0d0d","year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.124059Z"},"links":{"citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:f6f17a121a0f6f61e7018656bdc35357fc9bec10257f80baf2cf98482e2bc85b","observation_id":"d05173fa-3e42-486a-bf36-354ad700450b","resolution":{"observed_at":"2026-08-06T20:45:32.333130Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.11245","last_updated":"2024-09-17T14:50:36Z","snapshot_observed_at":"2026-08-16T13:17:48.700730Z","submitted_at":"2024-09-17T14:50:36Z","title":"Mapping Anisotropies in the Stochastic Gravitational-Wave Background with TianQin","version":1},"cited_work":{"arxiv_id":"2409.11245","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.11245","snapshot_observed_at":"2026-08-06T20:45:32.245607Z","title":"Mapping Anisotropies in the Stochastic Gravitational-Wave Background with TianQin","venue":"gr-qc","work_id":"b5dfe139-7508-44b1-be80-6d62c59d6817","year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.126725Z"},"links":{"cited_paper":"/paper/2409.11245","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:ef62b50a21dcf31de477f14ba990aaf4623d2a4324146f2504ae3c851d55d93f","observation_id":"e096ebf7-f27b-446c-83e0-60d572995235","resolution":{"observed_at":"2026-08-06T20:45:32.249953Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.05677","last_updated":"2024-09-04T19:12:39Z","snapshot_observed_at":"2026-08-16T14:02:39.341963Z","submitted_at":"2024-04-08T16:56:45Z","title":"Pulsar Timing Array Harmonic Analysis and Source Angular Correlations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.05677","snapshot_observed_at":"2026-08-06T20:45:32.129433Z","title":"Allen, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.129433Z"},"links":{"cited_paper":"/paper/2404.05677","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:83df83f4801b0dcca6ca6cf4f5ad5f11c6959f32a42e6e78c20b85af9603bde1","observation_id":"5bf906e7-f427-4d15-b209-5dc5ef62a20f","resolution":{"observed_at":"2026-08-06T20:45:32.129433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.4664","last_updated":"2014-09-16T20:54:55Z","snapshot_observed_at":"2026-08-15T18:48:59.540829Z","submitted_at":"2014-06-18T09:59:14Z","title":"Mapping gravitational-wave backgrounds using methods from CMB analysis: Application to pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.4664","snapshot_observed_at":"2026-08-06T20:45:32.132393Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.132393Z"},"links":{"cited_paper":"/paper/1406.4664","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:7b9716064a92e69a2530d455fa3aad651218e907af6d028a0f8f217390ef50aa","observation_id":"53922177-21d0-4698-9b74-a25b0668ae78","resolution":{"observed_at":"2026-08-06T20:45:32.132393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.14570","last_updated":"2020-11-30T19:43:22Z","snapshot_observed_at":"2026-08-13T06:50:03.447148Z","submitted_at":"2020-06-25T17:16:20Z","title":"Fisher formalism for anisotropic gravitational-wave background searches with pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.14570","snapshot_observed_at":"2026-08-06T20:45:32.134940Z","title":"Ali-Ha ¨ ımoud, T","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-06T20:45:32.134940Z"},"links":{"cited_paper":"/paper/2006.14570","citing_paper":"/paper/2507.02059"},"observation_digest":"sha256:0ce7dc874a0626a7e675deed18ca274a39631825d7ff6a3db345a8993d3c8b9f","observation_id":"4d3a8faf-5838-41f5-a003-e24590ed2346","resolution":{"observed_at":"2026-08-06T20:45:32.134940Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.02059","last_updated":"2025-08-01T13:18:29Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T04:58:22.596969Z","submitted_at":"2025-07-02T18:01:11Z","title":"Do Pulsar Timing Datasets Favor Massive Gravity?"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":68,"verified_exact":31,"verified_fuzzy":0},"total_outbound_references":106},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 100 of 106 outbound references and 0 inbound Pith citation observations for arXiv:2507.02059."}