{"as_of":"2026-07-25T01:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:91ecd34f76cf5414c0c06cef4f695f4357f023633ffc613672568b8697381f2b","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-07-24T06:31:00.690269+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-27T08:22:48.704788Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-03T13:18:12.439728Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1607.03148","last_updated":"2017-03-31T19:34:58Z","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:29:45Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions","version":2},"cited_work":{"arxiv_id":"1607.03148","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.03148","snapshot_observed_at":"2026-07-03T13:18:12.439728Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions","venue":"astro-ph.CO","work_id":"f32699d6-2541-4d8c-af6d-d469da162617","year":2016},"citing_paper":{"arxiv_id":"2411.12021","last_updated":"2025-11-24T12:55:36Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-11-18T20:03:34Z","title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","version":5},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-17T06:00:49.044220Z"},"links":{"cited_paper":"/paper/1607.03148","citing_paper":"/paper/2411.12021"},"observation_digest":"sha256:1dbcd3e305720f97d6b76b54c2c82f476c0e2b37a4db1417a9d5003def41d64e","observation_id":"98d2543d-b539-4d2f-970c-6d4ef9705db6","resolution":{"observed_at":"2026-05-17T06:00:49.434343Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03148","last_updated":"2017-03-31T19:34:58Z","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:29:45Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions","version":2},"cited_work":{"arxiv_id":"1607.03148","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.03148","snapshot_observed_at":"2026-07-03T13:18:12.439728Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions","venue":"astro-ph.CO","work_id":"f32699d6-2541-4d8c-af6d-d469da162617","year":2016},"citing_paper":{"arxiv_id":"2411.12022","last_updated":"2024-11-21T16:47:10Z","snapshot_observed_at":"2026-07-06T19:52:15.853216Z","submitted_at":"2024-11-18T20:03:35Z","title":"DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-15T21:36:41.223414Z"},"links":{"cited_paper":"/paper/1607.03148","citing_paper":"/paper/2411.12022"},"observation_digest":"sha256:9fbdb59cc486f19f5784e22a9f4f4e67ebf74ec6028108fcfb13e37f915d1ddf","observation_id":"d09ec496-ef2d-4f38-b88a-fb620f1f4a8f","resolution":{"observed_at":"2026-05-15T21:36:41.763018Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03148","last_updated":"2017-03-31T19:34:58Z","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:29:45Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions","version":2},"cited_work":{"arxiv_id":"1607.03148","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.03148","snapshot_observed_at":"2026-07-03T13:18:12.439728Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions","venue":"astro-ph.CO","work_id":"f32699d6-2541-4d8c-af6d-d469da162617","year":2016},"citing_paper":{"arxiv_id":"2510.14888","last_updated":"2026-04-08T20:26:41Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-16T17:07:57Z","title":"Modeling nonlinear scales for dynamical dark energy cosmologies with COLA","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-18T06:13:13.345307Z"},"links":{"cited_paper":"/paper/1607.03148","citing_paper":"/paper/2510.14888"},"observation_digest":"sha256:07e4cf1bab70b72a11d8fc5e7acb0a9813ecba529d5c6880159f8b6249e65848","observation_id":"7ace65bc-9d60-48af-b429-6ae34605884c","resolution":{"observed_at":"2026-05-18T06:15:58.679250Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03148","last_updated":"2017-03-31T19:34:58Z","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:29:45Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions","version":2},"cited_work":{"arxiv_id":"1607.03148","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.03148","snapshot_observed_at":"2026-07-03T13:18:12.439728Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions","venue":"astro-ph.CO","work_id":"f32699d6-2541-4d8c-af6d-d469da162617","year":2016},"citing_paper":{"arxiv_id":"2606.12565","last_updated":"2026-06-10T18:16:06Z","snapshot_observed_at":"2026-07-06T23:51:27.152983Z","submitted_at":"2026-06-10T18:16:06Z","title":"Galaxy formation in modified gravity -- II. galaxy halo connection and assembly bias","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-06-27T08:22:48.704788Z"},"links":{"cited_paper":"/paper/1607.03148","citing_paper":"/paper/2606.12565"},"observation_digest":"sha256:91bc3b0597271edeb9fd0cb72beac1fdbc05ecbdf804870b8ead0a2eaeb28bf0","observation_id":"6ac98029-2870-42fc-a66e-5b6336dd0c62","resolution":{"observed_at":"2026-07-03T13:18:12.441567Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1607.03148/citation-record","integrity":"/paper/1607.03148/integrity","json":"/paper/1607.03148/citation-record.json","paper":"/paper/1607.03148"},"outbound":[],"paper":{"arxiv_id":"1607.03148","last_updated":"2017-03-31T19:34:58Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:29:45Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"thesis":"As of 25 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1607.03148."}