{"as_of":"2026-08-20T16:38:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5ffec2df5191ba8d355f0f5fe3511b91ae23812415b0e57e78019f5542cbbc3d","coverage":[{"denominator":67,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":67,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-30T11:03:11.626899Z","state":"measured"},{"denominator":67,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":67,"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/2607.27175/citation-record","integrity":"/paper/2607.27175/integrity","json":"/paper/2607.27175/citation-record.json","paper":"/paper/2607.27175"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005036","last_updated":"2000-12-09T02:38:05Z","snapshot_observed_at":"2026-08-16T21:40:44.948452Z","submitted_at":"2000-05-02T20:03:52Z","title":"Acoustic Signatures in the Primary Microwave Background Bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005036","snapshot_observed_at":"2026-07-30T11:03:11.194744Z","title":"Komatsu and D","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.194744Z"},"links":{"cited_paper":"/paper/astro-ph/0005036","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:7a99c5e423b66076ece58a02f2bf1ea7c4b849a889e59fc0e46bb23a53f83331","observation_id":"a5ac155a-20c8-4cf5-a1d3-4f8095694603","resolution":{"observed_at":"2026-07-30T11:03:11.194744Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.1251","last_updated":"2011-05-21T15:56:07Z","snapshot_observed_at":"2026-08-15T04:52:55.504405Z","submitted_at":"2011-03-07T11:25:48Z","title":"Dominance of gauge artifact in the consistency relation for the primordial bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1103.1251","snapshot_observed_at":"2026-07-30T11:03:11.201891Z","title":"Tanaka and Y","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.201891Z"},"links":{"cited_paper":"/paper/1103.1251","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:80ad8198e93bd74b69542277a87941bc52e9ad5d95a12b0dcb7ad28498250dd6","observation_id":"a2e48b47-0a41-48e7-870f-fd80b32d4868","resolution":{"observed_at":"2026-07-30T11:03:11.201891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.0824","last_updated":"2013-10-14T12:37:58Z","snapshot_observed_at":"2026-08-15T00:18:59.811192Z","submitted_at":"2013-05-03T20:00:01Z","title":"The Observed Squeezed Limit of Cosmological Three-Point Functions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.0824","snapshot_observed_at":"2026-07-30T11:03:11.207334Z","title":"Pajer, F","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.207334Z"},"links":{"cited_paper":"/paper/1305.0824","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:bd7e18925dc7d603aa817b89bbb8be16322b13611285276af2fba54d2b10b030","observation_id":"42ab8012-60cb-452d-95e2-2fe54eccd1ab","resolution":{"observed_at":"2026-07-30T11:03:11.207334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.4560","last_updated":"2008-03-27T19:29:35Z","snapshot_observed_at":"2026-08-15T10:29:05.576631Z","submitted_at":"2007-10-25T19:56:52Z","title":"The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.4560","snapshot_observed_at":"2026-07-30T11:03:11.213824Z","title":"Dalal, O","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.213824Z"},"links":{"cited_paper":"/paper/0710.4560","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:f23ff172a91ef7eca5cbf416e4f1443f9141611c48359d76e560732f9be7d10b","observation_id":"30068f0d-09f9-46d4-a97d-04d33b13b8c2","resolution":{"observed_at":"2026-07-30T11:03:11.213824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.3580","last_updated":"2008-08-06T18:46:22Z","snapshot_observed_at":"2026-08-19T20:39:59.821121Z","submitted_at":"2008-05-23T19:59:57Z","title":"Constraints on local primordial non-Gaussianity from large scale structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.3580","snapshot_observed_at":"2026-07-30T11:03:11.220463Z","title":"Slosar, C","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.220463Z"},"links":{"cited_paper":"/paper/0805.3580","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:590d84c923c3d85e67ffe6afe5e9545b78b258f4027eac3e1f1de28a72acca5e","observation_id":"c3a35192-c7b6-430d-a6f8-c3499de5a37b","resolution":{"observed_at":"2026-07-30T11:03:11.220463Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.4826","last_updated":"2008-02-15T17:37:01Z","snapshot_observed_at":"2026-08-15T10:22:30.836371Z","submitted_at":"2008-01-31T18:34:36Z","title":"The effect of primordial non-Gaussianity on halo bias","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.4826","snapshot_observed_at":"2026-07-30T11:03:11.225929Z","title":"Matarrese and L","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.225929Z"},"links":{"cited_paper":"/paper/0801.4826","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:c434fba1f934c44cb4fd29695aae48ce773706e8c1ab7406b699427f1fe83002","observation_id":"447d83dd-870b-4b0c-a58b-833830e1999f","resolution":{"observed_at":"2026-07-30T11:03:11.225929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0609591","last_updated":"2006-09-20T21:20:16Z","snapshot_observed_at":"2026-07-07T01:03:10.885429Z","submitted_at":"2006-09-20T21:20:16Z","title":"Report of the Dark Energy Task Force","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0609591","snapshot_observed_at":"2026-07-30T11:03:11.231727Z","title":"Albrecht, G","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.231727Z"},"links":{"cited_paper":"/paper/astro-ph/0609591","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:5e0b676eca45efa39b0557ca9a04cdd5c88b00a4c539f297b26f5c6b9b5ca579","observation_id":"0274ae58-f3a6-48ad-8b4c-3bde16af26d0","resolution":{"observed_at":"2026-07-30T11:03:11.231727Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.1491","last_updated":"2012-11-08T11:02:08Z","snapshot_observed_at":"2026-08-20T06:21:01.302192Z","submitted_at":"2012-08-07T18:59:26Z","title":"The Clustering of Galaxies in SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: Constraints on Primordial Non-Gaussianity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.1491","snapshot_observed_at":"2026-07-30T11:03:11.237500Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.237500Z"},"links":{"cited_paper":"/paper/1208.1491","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:f16161b6e1bd697c41f8dd2cabc2bc5ccaa1a0b356c0ad6ffc027d899ac2a796","observation_id":"c9a419dd-0641-417a-99f3-746ec4236fad","resolution":{"observed_at":"2026-07-30T11:03:11.237500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.1349","last_updated":"2013-12-18T16:48:23Z","snapshot_observed_at":"2026-08-17T22:10:44.528563Z","submitted_at":"2013-03-06T15:09:44Z","title":"Improved Primordial Non-Gaussianity Constraints from Measurements of Galaxy Clustering and the Integrated Sachs-Wolfe Effect","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.1349","snapshot_observed_at":"2026-07-30T11:03:11.243469Z","title":"Giannantonio, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.243469Z"},"links":{"cited_paper":"/paper/1303.1349","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:0c94fa62878ac4395c5df01d865cbf536f879a8150e340fdd39e7772c03eca80","observation_id":"bb8511e0-bf82-4ef0-b3d7-e6e1222260c7","resolution":{"observed_at":"2026-07-30T11:03:11.243469Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.2597","last_updated":"2015-03-25T16:53:27Z","snapshot_observed_at":"2026-08-19T07:30:16.504258Z","submitted_at":"2013-11-11T21:00:29Z","title":"Sloan Digital Sky Survey III Photometric Quasar Clustering: Probing the Initial Conditions of the Universe using the Largest Volume","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.2597","snapshot_observed_at":"2026-07-30T11:03:11.249990Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.249990Z"},"links":{"cited_paper":"/paper/1311.2597","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:84c44446de0652b4e9c763dbf51979e0c36a7b6f6f33012c9bfee5514114fa86","observation_id":"810f86e1-23aa-426f-b842-dc3e2d0fe05e","resolution":{"observed_at":"2026-07-30T11:03:11.249990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.4315","last_updated":"2015-02-09T21:59:45Z","snapshot_observed_at":"2026-08-14T23:33:43.391481Z","submitted_at":"2014-05-16T21:38:06Z","title":"Constraints on primordial non-Gaussianity from 800,000 photometric quasars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.4315","snapshot_observed_at":"2026-07-30T11:03:11.257760Z","title":"Lett.113, 221301 (2014), arXiv:1405.4315 [astro-ph.CO]","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.257760Z"},"links":{"cited_paper":"/paper/1405.4315","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:c17482b93cd7926319d260b14441afa7d34d48dd99d8d2dda8b668dd39ba52fd","observation_id":"a5b56c57-04b3-45b9-8017-1e0eda9424a2","resolution":{"observed_at":"2026-07-30T11:03:11.257760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.08859","last_updated":"2019-04-18T16:00:32Z","snapshot_observed_at":"2026-08-18T11:59:11.968457Z","submitted_at":"2019-04-18T16:00:32Z","title":"Redshift-weighted constraints on primordial non-Gaussianity from the clustering of the eBOSS DR14 quasars in Fourier space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.08859","snapshot_observed_at":"2026-07-30T11:03:11.263506Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.263506Z"},"links":{"cited_paper":"/paper/1904.08859","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:69c2346f339d85d857d773afd8d7dd155678983fc8f0e36f17a3117a8e6540cd","observation_id":"e87a215e-7e5d-430d-8402-aa35582e418f","resolution":{"observed_at":"2026-07-30T11:03:11.263506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.13725","last_updated":"2021-07-02T12:10:58Z","snapshot_observed_at":"2026-08-16T18:14:27.517584Z","submitted_at":"2021-06-25T16:01:20Z","title":"The clustering of galaxies in the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Primordial non-Gaussianity in Fourier Space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.13725","snapshot_observed_at":"2026-07-30T11:03:11.269691Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.269691Z"},"links":{"cited_paper":"/paper/2106.13725","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:2c6f1acae647132cf79a3858ee11fc80055615378e81610b26a364b0e4623aa6","observation_id":"30b6b005-2000-45fa-bc6c-e832d0a54df7","resolution":{"observed_at":"2026-07-30T11:03:11.269691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00036","snapshot_observed_at":"2026-07-30T11:03:11.277149Z","title":"Aghamousa, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.277149Z"},"links":{"cited_paper":"/paper/1611.00036","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:f64b807621053c2dc965a0a0fdd83f070871dcfe9b5b8e1d8faaa1fc570eaff5","observation_id":"47ee7b3e-730c-4f71-8ede-dc85960bb774","resolution":{"observed_at":"2026-07-30T11:03:11.277149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.08657","last_updated":"2019-02-19T17:09:12Z","snapshot_observed_at":"2026-08-19T14:27:07.583433Z","submitted_at":"2018-04-23T18:33:16Z","title":"Overview of the DESI Legacy Imaging Surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.08657","snapshot_observed_at":"2026-07-30T11:03:11.284200Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.284200Z"},"links":{"cited_paper":"/paper/1804.08657","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:c0ff65cc062fc85374522633c2865e8f7629adeae93e9db876888ae4eb94397c","observation_id":"c410ef69-ac2b-4c39-9707-0cb7e02fa8aa","resolution":{"observed_at":"2026-07-30T11:03:11.284200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.01753","last_updated":"2024-06-25T04:39:44Z","snapshot_observed_at":"2026-08-20T08:15:38.633078Z","submitted_at":"2023-07-04T14:49:23Z","title":"Local primordial non-Gaussianity from the large-scale clustering of photometric DESI luminous red galaxies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.01753","snapshot_observed_at":"2026-07-30T11:03:11.289416Z","title":"Rezaie, A","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.289416Z"},"links":{"cited_paper":"/paper/2307.01753","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:47da680825478517f1e196193de7dcf2cf28db965c83670aca241eb80f7da680","observation_id":"8c33243b-3e3b-4f68-a08c-8e874bc64cdb","resolution":{"observed_at":"2026-07-30T11:03:11.289416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.17623","last_updated":"2025-07-02T21:49:19Z","snapshot_observed_at":"2026-08-12T11:52:26.779890Z","submitted_at":"2024-11-26T17:34:01Z","title":"Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.17623","snapshot_observed_at":"2026-07-30T11:03:11.294954Z","title":"Chaussidon, C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.294954Z"},"links":{"cited_paper":"/paper/2411.17623","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:9303ccd86aa17f248555af8616f1bede1ecc8f8e1dcae568e95721bb8f59e5f7","observation_id":"15f62553-8fc0-4988-a819-0a3e2a4cfe07","resolution":{"observed_at":"2026-07-30T11:03:11.294954Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.05213","last_updated":"2026-04-06T22:18:36Z","snapshot_observed_at":"2026-08-14T13:54:15.019824Z","submitted_at":"2026-04-06T22:18:36Z","title":"Local primordial non-Gaussianity using cross-correlations of DESI tracers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.05213","snapshot_observed_at":"2026-07-30T11:03:11.301359Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.301359Z"},"links":{"cited_paper":"/paper/2604.05213","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:374a850f78d5d73ab5fe070f007b5ad037d3682bec799c0579972cc12205b832","observation_id":"b5a496a1-77c6-4526-b839-9b6404d62142","resolution":{"observed_at":"2026-07-30T11:03:11.301359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2512.17865","last_updated":"2026-04-15T20:56:43Z","snapshot_observed_at":"2026-08-17T03:03:43.545196Z","submitted_at":"2025-12-19T18:14:50Z","title":"Constraining primordial non-Gaussianity from DESI DR1 quasars and Planck PR4 CMB Lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2512.17865","snapshot_observed_at":"2026-07-30T11:03:11.307359Z","title":"Chiarenza, A","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.307359Z"},"links":{"cited_paper":"/paper/2512.17865","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:747168e454dd705f475e21d31c8f1ebce1fa530bc81a329ea40bf5aede62d46e","observation_id":"4bccc9cc-521c-488d-8e7e-1977e6092eac","resolution":{"observed_at":"2026-07-30T11:03:11.307359Z","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":"2026-07-30T11:03:11.312854Z","title":"Chudaykin, M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.312854Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:09364995844119d0d26b367558223ba2ad6f5dcb5311aa6bbac07e4c68dd4837","observation_id":"aeb90a48-8bcd-4abc-8b23-5e0d4d471144","resolution":{"observed_at":"2026-07-30T11:03:11.312854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.05398","last_updated":"2024-04-12T13:42:59Z","snapshot_observed_at":"2026-08-19T17:30:39.458747Z","submitted_at":"2024-03-08T15:52:50Z","title":"The Wide-field Spectroscopic Telescope (WST) Science White Paper","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.05398","snapshot_observed_at":"2026-07-30T11:03:11.319454Z","title":"Mainieri, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.319454Z"},"links":{"cited_paper":"/paper/2403.05398","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:fd4861deb151b18b9ef04daf1e3e312c216102b9e9fb7fffc4aba51ce2078b2e","observation_id":"07f5c10e-a135-4de1-8ac2-e0a4209dd001","resolution":{"observed_at":"2026-07-30T11:03:11.319454Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.07970","last_updated":"2026-05-07T08:20:46Z","snapshot_observed_at":"2026-08-13T19:17:16.209565Z","submitted_at":"2024-11-12T17:51:21Z","title":"MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.07970","snapshot_observed_at":"2026-07-30T11:03:11.325865Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.325865Z"},"links":{"cited_paper":"/paper/2411.07970","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:878bf55102bf6193213204bcdc147a49181ce87de232487c9f604b737945beac","observation_id":"b568609f-e019-4d8b-bc81-1e05bfb2fde8","resolution":{"observed_at":"2026-07-30T11:03:11.325865Z","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":"2026-07-30T11:03:11.331226Z","title":"Besuner, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.331226Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:c6d56af49406e320d3362a082175f9f2ba1bd573b1595e17e34bbd58b8856f12","observation_id":"7b0b8919-1061-47ea-b2db-9075ffbd39ee","resolution":{"observed_at":"2026-07-30T11:03:11.331226Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03569","last_updated":"2024-09-02T09:27:58Z","snapshot_observed_at":"2026-08-16T14:03:34.829145Z","submitted_at":"2024-04-04T16:29:53Z","title":"High redshift LBGs from deep broadband imaging for future spectroscopic surveys","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03569","snapshot_observed_at":"2026-07-30T11:03:11.336959Z","title":"Ruhlmann-Kleider, C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.336959Z"},"links":{"cited_paper":"/paper/2404.03569","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:0bedfe680f2e83e9bed50c38e3bf978641c7fe3dcc4b34ea401adad0735bbd2f","observation_id":"425ab96c-dd06-4fec-b40d-45854f86f9dd","resolution":{"observed_at":"2026-07-30T11:03:11.336959Z","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":"2026-07-30T11:03:11.342945Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.342945Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:08d4ac9866840923454d9e2f87a955a86b289afb5e4edfc79ecef5c2be39505c","observation_id":"a7417f4e-13fd-484f-b4ec-6c1560035fb7","resolution":{"observed_at":"2026-07-30T11:03:11.342945Z","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":"2026-07-30T11:03:11.350278Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.350278Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:c600a6ad21687d2e52acd313e0956c3938d78c34af6e3f46056e1259b5645f92","observation_id":"2729b448-8cb3-49f3-8316-60438e896fa3","resolution":{"observed_at":"2026-07-30T11:03:11.350278Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2511.22243","last_updated":"2026-03-30T15:37:29Z","snapshot_observed_at":"2026-07-06T22:37:08.086095Z","submitted_at":"2025-11-27T09:14:33Z","title":"Forecasting local Primordial Non-Gaussianities from UNIONS Lyman-Break Galaxies and Planck CMB lensing","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.22243","snapshot_observed_at":"2026-07-30T11:03:11.358756Z","title":"de Boer, and S","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.358756Z"},"links":{"cited_paper":"/paper/2511.22243","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:81a9ad1687fe037fde78e8e3fc0476746ae31c16799cb8dbb6f1e303e029dddd","observation_id":"3440dac4-caa2-4b13-adb3-4a2e91476905","resolution":{"observed_at":"2026-07-30T11:03:11.358756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.05697","last_updated":"2019-05-14T16:19:37Z","snapshot_observed_at":"2026-08-17T17:14:51.900117Z","submitted_at":"2019-05-14T16:19:37Z","title":"Planck 2018 results. IX. Constraints on primordial non-Gaussianity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.05697","snapshot_observed_at":"2026-07-30T11:03:11.364997Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.364997Z"},"links":{"cited_paper":"/paper/1905.05697","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:0521343fbb50f570f4f9e56fb6e356b29d54c4ccb982483cdd2336d3a016c45d","observation_id":"13b49dee-ceee-4550-ac5b-1c1bc841aa11","resolution":{"observed_at":"2026-07-30T11:03:11.364997Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.02289","last_updated":"2024-01-10T10:35:23Z","snapshot_observed_at":"2026-08-16T16:04:09.143018Z","submitted_at":"2023-01-05T20:46:21Z","title":"Cosmological Fisher forecasts for next-generation spectroscopic surveys","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.02289","snapshot_observed_at":"2026-07-30T11:03:11.371574Z","title":"d’Assignies D, C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.371574Z"},"links":{"cited_paper":"/paper/2301.02289","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:8a01943e72fc834379bdd3f971a3675aea5e780ee9e9d6f1329c502415761808","observation_id":"b8431a53-c701-4320-8192-e1ab61f05786","resolution":{"observed_at":"2026-07-30T11:03:11.371574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.3380","last_updated":"2010-04-24T15:03:29Z","snapshot_observed_at":"2026-08-15T05:33:40.837974Z","submitted_at":"2009-11-17T19:20:45Z","title":"Quasi-Single Field Inflation and Non-Gaussianities","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.3380","snapshot_observed_at":"2026-07-30T11:03:11.378515Z","title":"Chen and Y","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.378515Z"},"links":{"cited_paper":"/paper/0911.3380","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:9c2b8cc3794fd96921f74f54fb5c0aed970e6fc57b76d579ae4df74565148d9d","observation_id":"a1d5b3b1-1b2d-483c-976a-defd7c39b8cb","resolution":{"observed_at":"2026-07-30T11:03:11.378515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.2630","last_updated":"2013-01-11T23:21:42Z","snapshot_observed_at":"2026-08-15T00:32:55.791695Z","submitted_at":"2013-01-11T23:21:42Z","title":"Anomalous Dimensions and Non-Gaussianity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.2630","snapshot_observed_at":"2026-07-30T11:03:11.384545Z","title":"Green, M","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.384545Z"},"links":{"cited_paper":"/paper/1301.2630","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:64f6e0887a27d418e4aa4a0306132398d38659a22ba1ada85fdff6118e435294","observation_id":"fcf4b90a-b109-4484-9268-0a861381e5da","resolution":{"observed_at":"2026-07-30T11:03:11.384545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.6324","last_updated":"2012-08-27T12:36:12Z","snapshot_observed_at":"2026-08-15T04:11:41.064757Z","submitted_at":"2012-04-27T20:09:52Z","title":"Prospects for constraining the shape of non-Gaussianity with the scale-dependent bias","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.6324","snapshot_observed_at":"2026-07-30T11:03:11.392497Z","title":"Noreña, L","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.392497Z"},"links":{"cited_paper":"/paper/1204.6324","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:ebcb5dd61eec7cc0ca0c9d6cae7206db5861c802ebf46ecd6c5aeda92ffc6455","observation_id":"965b9f07-40c0-4d4e-a485-3d106cd2c8b7","resolution":{"observed_at":"2026-07-30T11:03:11.392497Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.6318","last_updated":"2012-04-27T20:00:08Z","snapshot_observed_at":"2026-08-16T22:36:46.009471Z","submitted_at":"2012-04-27T20:00:08Z","title":"Effects and Detectability of Quasi-Single Field Inflation in the Large-Scale Structure and Cosmic Microwave Background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.6318","snapshot_observed_at":"2026-07-30T11:03:11.400100Z","title":"Sefusatti, J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.400100Z"},"links":{"cited_paper":"/paper/1204.6318","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:c8958fd69c0a43d6331123b500a8e87d0363c7fd3ca883b14563c6ebf32bb9ef","observation_id":"30991f01-e2b0-4f02-9fb3-bd6477e48632","resolution":{"observed_at":"2026-07-30T11:03:11.400100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06366","last_updated":"2017-03-13T01:30:43Z","snapshot_observed_at":"2026-08-17T15:44:41.756999Z","submitted_at":"2016-12-19T20:54:54Z","title":"Biasing and the search for primordial non-Gaussianity beyond the local type","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.06366","snapshot_observed_at":"2026-07-30T11:03:11.407700Z","title":"Gleyzes, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.407700Z"},"links":{"cited_paper":"/paper/1612.06366","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:a1a8ab31b23b6ff49a96cac86e8bc708ada820fbe760fc5bde0784effd2b9d18","observation_id":"ace5e30c-b9ae-454f-a565-a7ce3ca619c8","resolution":{"observed_at":"2026-07-30T11:03:11.407700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.2606","last_updated":"2014-02-20T21:03:24Z","snapshot_observed_at":"2026-08-14T23:55:43.377192Z","submitted_at":"2013-11-11T21:07:46Z","title":"Constraining the initial conditions of the Universe using large scale structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.2606","snapshot_observed_at":"2026-07-30T11:03:11.414083Z","title":"Agarwal, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.414083Z"},"links":{"cited_paper":"/paper/1311.2606","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:7e1af7d526612a8eb541e004d1f193a390a345c57f76e455d0a4c17b0325f17f","observation_id":"1e17d30f-3c48-45b6-9303-10bd91beb1be","resolution":{"observed_at":"2026-07-30T11:03:11.414083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.04882","last_updated":"2024-05-24T12:30:00Z","snapshot_observed_at":"2026-08-17T05:56:22.725947Z","submitted_at":"2023-11-08T18:39:12Z","title":"Light Fields during Inflation from BOSS and Future Galaxy Surveys","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.04882","snapshot_observed_at":"2026-07-30T11:03:11.419619Z","title":"Green, Y","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.419619Z"},"links":{"cited_paper":"/paper/2311.04882","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:be523d0991a7dec54f82f63a911e224003e919ff2353dcc21c42bf6bbab00b93","observation_id":"d8f2a1be-db35-4329-ba88-1654382321ae","resolution":{"observed_at":"2026-07-30T11:03:11.419619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07187","last_updated":"2023-04-18T11:15:50Z","snapshot_observed_at":"2026-08-16T16:32:20.742234Z","submitted_at":"2022-09-15T10:03:41Z","title":"Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07187","snapshot_observed_at":"2026-07-30T11:03:11.425416Z","title":"Riquelme, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.425416Z"},"links":{"cited_paper":"/paper/2209.07187","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:cc68b63f204e88a1804a2459a6dc58988793ba912f30de260fe24c6638254d4f","observation_id":"e3b8feae-faa0-40e4-b9fb-09c6814378df","resolution":{"observed_at":"2026-07-30T11:03:11.425416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.08515","last_updated":"2022-10-25T21:46:01Z","snapshot_observed_at":"2026-08-19T14:26:41.945305Z","submitted_at":"2022-08-17T20:11:48Z","title":"Target Selection and Validation of DESI Luminous Red Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.08515","snapshot_observed_at":"2026-07-30T11:03:11.430742Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.430742Z"},"links":{"cited_paper":"/paper/2208.08515","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:fdf3b1206d19688e0cfe76eefe7805e9e472719f4bb1b1f05a66c0a9e8c47549","observation_id":"00b465e5-4f55-4224-980b-b81d10a03eb7","resolution":{"observed_at":"2026-07-30T11:03:11.430742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00024","last_updated":"2019-10-30T18:04:11Z","snapshot_observed_at":"2026-08-14T18:06:11.466837Z","submitted_at":"2018-10-31T18:00:02Z","title":"The Cosmological Bootstrap: Inflationary Correlators from Symmetries and Singularities","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.00024","snapshot_observed_at":"2026-07-30T11:03:11.437207Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.437207Z"},"links":{"cited_paper":"/paper/1811.00024","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:44e8948751b38224802f14a451b98b46026930336bda03ae19412d112c773293","observation_id":"cd799d31-5e4d-4386-a55e-f59b0c5205af","resolution":{"observed_at":"2026-07-30T11:03:11.437207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.09787","last_updated":"2019-01-14T18:30:24Z","snapshot_observed_at":"2026-08-14T21:28:02.510116Z","submitted_at":"2016-11-29T18:57:56Z","title":"Large-Scale Galaxy Bias","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.09787","snapshot_observed_at":"2026-07-30T11:03:11.442902Z","title":"Desjacques, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.442902Z"},"links":{"cited_paper":"/paper/1611.09787","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:b21ba999c372dad497009a6bf49765e9a6ae8c5eb83c358eef5a3cd56886cb20","observation_id":"a1045c5c-58c9-452e-be8d-3e8fd528a6af","resolution":{"observed_at":"2026-07-30T11:03:11.442902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.3224","last_updated":"2009-11-08T19:07:06Z","snapshot_observed_at":"2026-08-15T05:38:52.225767Z","submitted_at":"2009-09-17T14:03:12Z","title":"Detectability of the effect of Inflationary non-Gaussianity on halo bias","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.3224","snapshot_observed_at":"2026-07-30T11:03:11.448915Z","title":"Verde and S","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.448915Z"},"links":{"cited_paper":"/paper/0909.3224","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:480c5a2960cd4918201877de73ae19e7c18e1f89a1eb4dc2ab3f6b842c3e34cc","observation_id":"0b749150-32d1-4dca-bd7b-bfcded530588","resolution":{"observed_at":"2026-07-30T11:03:11.448915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.2173","last_updated":"2012-09-10T22:56:45Z","snapshot_observed_at":"2026-08-15T00:47:11.147467Z","submitted_at":"2012-09-10T22:56:45Z","title":"Stochastic Bias from Non-Gaussian Initial Conditions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.2173","snapshot_observed_at":"2026-07-30T11:03:11.455013Z","title":"Baumann, S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.455013Z"},"links":{"cited_paper":"/paper/1209.2173","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:2c7222aaf86c49bd1efa760b62328e4ce6002f86ce4b13ee9c7c25279ed103c9","observation_id":"7ce33519-d961-4b64-b254-80608515cee3","resolution":{"observed_at":"2026-07-30T11:03:11.455013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.03723","last_updated":"2015-11-25T23:05:26Z","snapshot_observed_at":"2026-08-14T22:28:04.963987Z","submitted_at":"2015-10-13T15:03:06Z","title":"Galaxy Bias and Primordial Non-Gaussianity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.03723","snapshot_observed_at":"2026-07-30T11:03:11.461334Z","title":"Assassi, D","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.461334Z"},"links":{"cited_paper":"/paper/1510.03723","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:e55648230509347e94aab30429fa4f3aa352faadcda50c66f85f9a84e7be6f51","observation_id":"ae589bc3-98fa-4832-8409-65f04d7dcb33","resolution":{"observed_at":"2026-07-30T11:03:11.461334Z","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":"2026-07-30T11:03:11.468383Z","title":null,"venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.468383Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:dc0eea81fcfe6a322c2922268fee17a2205b019a7f5ceb26f5880e45d0335056","observation_id":"be5f15a4-10ef-4b1d-8644-76df3bb65177","resolution":{"observed_at":"2026-07-30T11:03:11.468383Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.05088","last_updated":"2017-02-16T18:53:37Z","snapshot_observed_at":"2026-08-14T21:16:08.126372Z","submitted_at":"2017-02-16T18:53:37Z","title":"Optimising primordial non-Gaussianity measurements from galaxy surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.05088","snapshot_observed_at":"2026-07-30T11:03:11.477548Z","title":"Mueller, W","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.477548Z"},"links":{"cited_paper":"/paper/1702.05088","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:710c67a50a45b99bf23b5f0d2a29b96dffe922a56c9b68e28eeba8e9db576330","observation_id":"34df0019-89ae-4094-b6a4-f5e3598bbc50","resolution":{"observed_at":"2026-07-30T11:03:11.477548Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9911177","last_updated":"2000-06-01T12:13:06Z","snapshot_observed_at":"2026-07-07T01:29:40.678750Z","submitted_at":"1999-11-10T17:57:36Z","title":"Efficient Computation of CMB anisotropies in closed FRW models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9911177","snapshot_observed_at":"2026-07-30T11:03:11.484195Z","title":"Lewis, A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.484195Z"},"links":{"cited_paper":"/paper/astro-ph/9911177","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:b1cfa87b355a4ddd86845cf386953e1edc15b047065097d21816e331582a49d7","observation_id":"539af2fa-4766-43d4-a2a0-6a0a6b5d3b30","resolution":{"observed_at":"2026-07-30T11:03:11.484195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.3654","last_updated":"2012-04-19T11:36:17Z","snapshot_observed_at":"2026-08-19T23:50:01.657916Z","submitted_at":"2012-01-17T22:12:30Z","title":"CMB power spectrum parameter degeneracies in the era of precision cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.3654","snapshot_observed_at":"2026-07-30T11:03:11.491880Z","title":"Howlett, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.491880Z"},"links":{"cited_paper":"/paper/1201.3654","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:2ad226b55320e064341b3e4bb984e9c4f96ef7c726c0bc73be99e679082e7b1a","observation_id":"c0acdd83-0c6e-4c16-9d5c-4814207aa45d","resolution":{"observed_at":"2026-07-30T11:03:11.491880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507263","last_updated":"2005-08-16T00:28:03Z","snapshot_observed_at":"2026-07-07T00:52:09.097911Z","submitted_at":"2005-07-11T20:00:08Z","title":"Cosmic Growth History and Expansion History","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507263","snapshot_observed_at":"2026-07-30T11:03:11.499474Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.499474Z"},"links":{"cited_paper":"/paper/astro-ph/0507263","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:96c1fed649e9b6b7b08f6ac37ef0d10bca56bc3ea6ac426c0d3847ed0c924376","observation_id":"b763a8bf-9535-4669-8ccd-b67cb3049405","resolution":{"observed_at":"2026-07-30T11:03:11.499474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-07-30T11:03:11.506192Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.506192Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:d3d991402ac9c5c4982b3da0344a40b36653a38e879cf4e350df437a6eba89d9","observation_id":"3158114d-a667-4242-b90d-b0d8cd544aea","resolution":{"observed_at":"2026-07-30T11:03:11.506192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-08-14T22:13:38.637603Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-07-30T11:03:11.512417Z","title":"Krause and T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.512417Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:b56f6d9c23a1d9405b48b2154a18bb7df9bb399ddbefa05e40ed5d0ec92c7a92","observation_id":"b61cffad-c907-4e09-8c7b-0771dcf3c4e1","resolution":{"observed_at":"2026-07-30T11:03:11.512417Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.04833","last_updated":"2021-02-20T00:11:53Z","snapshot_observed_at":"2026-08-13T04:27:14.953344Z","submitted_at":"2020-04-09T22:02:02Z","title":"2D-FFTLog: Efficient computation of real space covariance matrices for galaxy clustering and weak lensing","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.04833","snapshot_observed_at":"2026-07-30T11:03:11.521154Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.521154Z"},"links":{"cited_paper":"/paper/2004.04833","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:0b4dec835b02743c6873f4a4cd2f64c26baf333750c191cbaafac1c2a6a9a418","observation_id":"4a66a692-06f1-4933-8d20-fc7438cfdb7a","resolution":{"observed_at":"2026-07-30T11:03:11.521154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0307460","last_updated":"2003-07-26T00:20:17Z","snapshot_observed_at":"2026-08-19T10:41:20.567499Z","submitted_at":"2003-07-26T00:20:17Z","title":"Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0307460","snapshot_observed_at":"2026-07-30T11:03:11.527659Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.527659Z"},"links":{"cited_paper":"/paper/astro-ph/0307460","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:1f25e5ca1aa1fdf62eb0d59994cb237e84dd02ec70ae95f0506cf6e074a77740","observation_id":"6065a9b9-1b0c-402a-b027-e7467ddd4409","resolution":{"observed_at":"2026-07-30T11:03:11.527659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.3854","last_updated":"2014-12-11T22:59:01Z","snapshot_observed_at":"2026-08-20T07:07:15.101001Z","submitted_at":"2014-12-11T22:59:01Z","title":"Designing an Inflation Galaxy Survey: how to measure $\\sigma(f_{\\rm NL}) \\sim 1$ using scale-dependent galaxy bias","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.3854","snapshot_observed_at":"2026-07-30T11:03:11.533685Z","title":"de Putter and O","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.533685Z"},"links":{"cited_paper":"/paper/1412.3854","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:01432a0a3d1f1296ca0031d6d75d2b758fc79c901ccc1557e8244c7217df7287","observation_id":"98e64d0b-c17c-43d4-a991-e4e853418cd0","resolution":{"observed_at":"2026-07-30T11:03:11.533685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16923","last_updated":"2023-06-29T13:18:57Z","snapshot_observed_at":"2026-08-16T15:20:03.820137Z","submitted_at":"2023-06-29T13:18:57Z","title":"NAUTILUS: boosting Bayesian importance nested sampling with deep learning","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16923","snapshot_observed_at":"2026-07-30T11:03:11.539310Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.539310Z"},"links":{"cited_paper":"/paper/2306.16923","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:dfd97e3a475702571bd7cafc4753f06abf01ff5ed007a87c2f166e206b99c10c","observation_id":"c21e794f-b3b1-4cad-b0e8-b111c5d0a959","resolution":{"observed_at":"2026-07-30T11:03:11.539310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13970","last_updated":"2025-07-09T12:22:45Z","snapshot_observed_at":"2026-08-12T19:40:10.586390Z","submitted_at":"2019-10-30T16:38:10Z","title":"GetDist: a Python package for analysing Monte Carlo samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13970","snapshot_observed_at":"2026-07-30T11:03:11.545547Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.545547Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:83651c302c02bbfe96343c347b14bae2da68d514db2c801c0bd4201297dac326","observation_id":"8db66b62-6aca-4ced-a912-26c395c0c193","resolution":{"observed_at":"2026-07-30T11:03:11.545547Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07700","last_updated":"2025-04-04T17:52:32Z","snapshot_observed_at":"2026-08-19T15:20:25.392135Z","submitted_at":"2024-08-14T17:57:18Z","title":"Profile Likelihoods in Cosmology: When, Why and How illustrated with $\\Lambda$CDM, Massive Neutrinos and Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.07700","snapshot_observed_at":"2026-07-30T11:03:11.554931Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.554931Z"},"links":{"cited_paper":"/paper/2408.07700","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:1360d819c68a8ae0699834f7a051ee8397733c0b07fda6246b45fbc3dec73e46","observation_id":"88cd134b-2fb1-4a46-91c2-2efdb9e59e31","resolution":{"observed_at":"2026-07-30T11:03:11.554931Z","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":"2026-07-30T11:03:11.562200Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.562200Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:ff1ac9d2601ed46ea2faeb2bd700aea338ab390c80e9413e9719263ad820d932","observation_id":"05475830-d416-4ae6-a721-bd453b527936","resolution":{"observed_at":"2026-07-30T11:03:11.562200Z","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":"2026-07-30T11:03:11.570385Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.570385Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:0fff9b44cabab041da79b2dd4d26a4a8d7dd97bd22349cfabc56ad48e5642302","observation_id":"be4e5af9-abee-43bd-93c9-840c97c65cd2","resolution":{"observed_at":"2026-07-30T11:03:11.570385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.03653","last_updated":"2017-02-14T06:07:22Z","snapshot_observed_at":"2026-08-19T21:16:39.670904Z","submitted_at":"2017-02-13T07:07:13Z","title":"Project Overview of the Beijing-Arizona Sky Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.03653","snapshot_observed_at":"2026-07-30T11:03:11.579226Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.579226Z"},"links":{"cited_paper":"/paper/1702.03653","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:7bd864904bcc34f032222935ae0da330d06fdb60fa9b72840d3dfb3182224567","observation_id":"487b1f7d-38d5-4a3e-93b5-7b06a0fd98f7","resolution":{"observed_at":"2026-07-30T11:03:11.579226Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.02900","last_updated":"2015-04-11T17:45:05Z","snapshot_observed_at":"2026-08-19T23:57:29.167790Z","submitted_at":"2015-04-11T17:45:05Z","title":"The Dark Energy Camera","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.02900","snapshot_observed_at":"2026-07-30T11:03:11.584757Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.584757Z"},"links":{"cited_paper":"/paper/1504.02900","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:5941723e4a76a87d75028fb3a2a80be950ddd2c4a5987e78c345d37a592510fe","observation_id":"3d89241a-6cf9-4f56-bae9-ddaf5be9c6e5","resolution":{"observed_at":"2026-07-30T11:03:11.584757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.11355","last_updated":"2020-04-29T17:01:30Z","snapshot_observed_at":"2026-08-14T16:02:09.251432Z","submitted_at":"2019-07-26T01:38:40Z","title":"Improving Galaxy Clustering Measurements with Deep Learning: analysis of the DECaLS DR7 data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.11355","snapshot_observed_at":"2026-07-30T11:03:11.591959Z","title":"Rezaie, H.-J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.591959Z"},"links":{"cited_paper":"/paper/1907.11355","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:e33bf01959d6c3c8832ad6687e9450c49ffc3094e67b3eecdd1d7dfa675ddc96","observation_id":"41dbb925-6ed8-4e44-ad63-4a6b3c9cb9f4","resolution":{"observed_at":"2026-07-30T11:03:11.591959Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.13724","last_updated":"2021-06-25T16:01:19Z","snapshot_observed_at":"2026-08-16T18:14:27.554665Z","submitted_at":"2021-06-25T16:01:19Z","title":"Primordial non-Gaussianity from the Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey I: Catalogue Preparation and Systematic Mitigation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.13724","snapshot_observed_at":"2026-07-30T11:03:11.597548Z","title":"Rezaie, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.597548Z"},"links":{"cited_paper":"/paper/2106.13724","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:41e70f0ae2f1a3868000b7c18158561b14ed0ae646cbb59b76062b6a903df003","observation_id":"e0e7c34c-c6cd-4cc6-bf29-b05438d66566","resolution":{"observed_at":"2026-07-30T11:03:11.597548Z","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":"2026-07-30T11:03:11.602772Z","title":"Jarvis, G","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.602772Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:09d6b9b71a274bf941ed129f5e068c12e910ddcfe227419b7cab08be82895e8b","observation_id":"099aeb93-c31e-4f6b-aa2d-b8026b473736","resolution":{"observed_at":"2026-07-30T11:03:11.602772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.2366","last_updated":"2018-05-23T19:18:23Z","snapshot_observed_at":"2026-08-19T09:13:46.659953Z","submitted_at":"2008-05-15T18:10:13Z","title":"LSST: from Science Drivers to Reference Design and Anticipated Data Products","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.2366","snapshot_observed_at":"2026-07-30T11:03:11.608165Z","title":"Ivezić, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.608165Z"},"links":{"cited_paper":"/paper/0805.2366","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:e348df85041d6316fa61d8ea2c357e6e67fce2bcca09c7a21cc531dc436b5063","observation_id":"d7212873-996d-4eff-82ef-96ece4033066","resolution":{"observed_at":"2026-07-30T11:03:11.608165Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.13378","last_updated":"2019-08-27T16:22:44Z","snapshot_observed_at":"2026-08-16T04:53:02.942507Z","submitted_at":"2019-04-30T17:22:56Z","title":"Cosmology with dropout selection: Straw-man surveys and CMB lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.13378","snapshot_observed_at":"2026-07-30T11:03:11.613827Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.613827Z"},"links":{"cited_paper":"/paper/1904.13378","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:2004859e1071a038b709ab5ceea87cad895df88fb249e299cd7efb16735025b5","observation_id":"007c5335-d6bc-428d-b67c-8fa124490cf2","resolution":{"observed_at":"2026-07-30T11:03:11.613827Z","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":"2026-07-30T11:03:11.620034Z","title":"Chernoff, On the Distribution of the Likelihood Ratio, The Annals of Mathematical Statistics25, 573 (1954)","venue":null,"work_id":null,"year":1954},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.620034Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:666c851daa37e513d13b8eadc19e6ff165b85257bc67d14c16ccd6bcf0763666","observation_id":"98a13210-fdc8-4bec-9c1e-f25c296f83cf","resolution":{"observed_at":"2026-07-30T11:03:11.620034Z","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":"2026-07-30T11:03:11.626899Z","title":null,"venue":null,"work_id":null,"year":1938},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.626899Z"},"links":{"citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:fe55a7684acbf606f4b5a5bd98d7e543d2ecee81dc8ded350ab1900a050aaf26","observation_id":"84eeb866-c4f7-4375-a1d3-e76b11bba430","resolution":{"observed_at":"2026-07-30T11:03:11.626899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T22:46:02.271170Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys"},"reference_resolution":{"displayed":67,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":67,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":67},"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 67 of 67 outbound references and 0 inbound Pith citation observations for arXiv:2607.27175."}