{"as_of":"2026-08-04T20:50:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8b54e0fb3678c7d574ca1f8b01bcb34171f4a076cff2003cf04d4c8e82149e3c","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":11,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":11,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":11,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":11,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T07:07:18.855675Z","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":"2026-06-30T15:14:47.132215Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":"1104.2948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-06-30T15:14:47.132215Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","venue":"astro-ph.CO","work_id":"8aa04ef0-ec75-4f3b-a546-bde81c29c80c","year":2011},"citing_paper":{"arxiv_id":"1106.2476","last_updated":"2012-03-12T12:39:47Z","snapshot_observed_at":"2026-07-06T02:29:12.672489Z","submitted_at":"2011-06-13T16:06:49Z","title":"Modified Gravity and Cosmology","version":3},"reference_index":165,"source":"pdf_text","source_observed_at":"2026-05-13T13:08:19.215167Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/1106.2476"},"observation_digest":"sha256:c4b60f01b71eb37a041a78fbdc64cf11afbb0eaa1ee8352ab3d807f3c6fe8fef","observation_id":"fb94383a-95fd-4f43-80c7-4ae4bef7094e","resolution":{"observed_at":"2026-05-13T13:08:19.787093Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":"1104.2948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-06-30T15:14:47.132215Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","venue":"astro-ph.CO","work_id":"8aa04ef0-ec75-4f3b-a546-bde81c29c80c","year":2011},"citing_paper":{"arxiv_id":"2411.07970","last_updated":"2026-05-07T08:20:46Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","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},"reference_index":298,"source":"arxiv_source","source_observed_at":"2026-05-23T17:45:29.240141Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2411.07970"},"observation_digest":"sha256:c4dbefb21028af8f281177bbba694162cfc30b0d3d86f992b516b791aa418761","observation_id":"085a5c9b-0ee7-4072-932e-cbc1a3559d3e","resolution":{"observed_at":"2026-05-23T17:45:45.801452Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":"1104.2948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-06-30T15:14:47.132215Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","venue":"astro-ph.CO","work_id":"8aa04ef0-ec75-4f3b-a546-bde81c29c80c","year":2011},"citing_paper":{"arxiv_id":"2504.20478","last_updated":"2026-04-17T05:39:20Z","snapshot_observed_at":"2026-07-06T21:16:13.624880Z","submitted_at":"2025-04-29T07:19:58Z","title":"Tomographic Alcock-Paczynski Test with Marked Correlation Functions","version":5},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-22T18:56:46.117021Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2504.20478"},"observation_digest":"sha256:0e4597ce7053c809f0a608d538cc0c67734d95c28169e19dd95b04e096e6c8c7","observation_id":"a1c8bbb8-a39e-4cd7-b5cd-97ab61d50576","resolution":{"observed_at":"2026-05-22T18:56:57.894283Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":"1104.2948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-06-30T15:14:47.132215Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","venue":"astro-ph.CO","work_id":"8aa04ef0-ec75-4f3b-a546-bde81c29c80c","year":2011},"citing_paper":{"arxiv_id":"2510.14888","last_updated":"2026-04-08T20:26:41Z","snapshot_observed_at":"2026-08-02T22:21:29.839652Z","submitted_at":"2025-10-16T17:07:57Z","title":"Modeling nonlinear scales for dynamical dark energy cosmologies with COLA","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-18T06:13:13.345307Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2510.14888"},"observation_digest":"sha256:85419c7b4e12474245e57e9e42ec319a7006b7af9960aec7cc0170deedb77de1","observation_id":"c343f49e-c33a-4465-9e4d-3bde5fc102ce","resolution":{"observed_at":"2026-05-18T06:15:58.634105Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-08-03T07:07:18.855675Z","title":"Blakeet al.,Mon","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2601.21274","last_updated":"2026-05-30T03:19:05Z","snapshot_observed_at":"2026-08-04T16:29:32.108259Z","submitted_at":"2026-01-29T05:11:07Z","title":"Realizing the phantom-divide crossing with vector and scalar fields","version":2},"reference_index":115,"source":"pdf_text","source_observed_at":"2026-08-03T07:07:18.855675Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2601.21274"},"observation_digest":"sha256:2d8c4d536e1002940e5e2580c4a593a39cc1cbf9cb1a2b3c73160fd3cd338e8b","observation_id":"c6672995-81e9-4d78-b979-5c60738f446c","resolution":{"observed_at":"2026-08-03T07:07:18.855675Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":"1104.2948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-06-30T15:14:47.132215Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","venue":"astro-ph.CO","work_id":"8aa04ef0-ec75-4f3b-a546-bde81c29c80c","year":2011},"citing_paper":{"arxiv_id":"2605.22309","last_updated":"2026-07-15T09:02:22Z","snapshot_observed_at":"2026-08-03T09:50:36.320966Z","submitted_at":"2026-05-21T10:55:25Z","title":"Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background","version":1},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-05-22T05:36:41.912431Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2605.22309"},"observation_digest":"sha256:4641429b1541e289be0f6b8bcddf1e470cf5c52530671d04814c97ff4aec19ce","observation_id":"af9cabe8-6376-46f6-909a-0e7c7385b0c5","resolution":{"observed_at":"2026-05-22T05:41:08.976862Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-08-02T13:30:04.850379Z","title":"Blakeet al., The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9, Mon","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2605.22309","last_updated":"2026-07-15T09:02:22Z","snapshot_observed_at":"2026-08-03T09:50:36.320966Z","submitted_at":"2026-05-21T10:55:25Z","title":"Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background","version":2},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-08-02T13:30:04.850379Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2605.22309"},"observation_digest":"sha256:22e87d89d87e78cadbbfde8c1421043a7e8e9da8bcc5054515e36cd14f5cb79b","observation_id":"fb983d51-962e-45c0-9fa7-37cdc34ab411","resolution":{"observed_at":"2026-08-02T13:30:04.850379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":"1104.2948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-06-30T15:14:47.132215Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","venue":"astro-ph.CO","work_id":"8aa04ef0-ec75-4f3b-a546-bde81c29c80c","year":2011},"citing_paper":{"arxiv_id":"2605.23367","last_updated":"2026-06-08T11:28:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-22T08:33:44Z","title":"Cosmological constraints from neighbor-density-weighted marked correlation functions","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-25T03:27:13.896349Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2605.23367"},"observation_digest":"sha256:9fd502013a0210517638a6360bcacf61f03b64640add881e8a8833b3a571d15d","observation_id":"570e99fb-985d-4de0-a82a-4a92ffa7b1bc","resolution":{"observed_at":"2026-05-25T03:30:17.265427Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":"1104.2948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-06-30T15:14:47.132215Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","venue":"astro-ph.CO","work_id":"8aa04ef0-ec75-4f3b-a546-bde81c29c80c","year":2011},"citing_paper":{"arxiv_id":"2605.23367","last_updated":"2026-06-08T11:28:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-22T08:33:44Z","title":"Cosmological constraints from neighbor-density-weighted marked correlation functions","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-06-30T15:08:32.960489Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2605.23367"},"observation_digest":"sha256:f8b39b8ca1f92a1813658a2b5cae44d37ef3fdbc5cdd71c3977f8d3b4a3427bb","observation_id":"60d49ea0-b673-4fe3-bba4-09a620cb47af","resolution":{"observed_at":"2026-06-30T15:14:47.133379Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":"1104.2948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-06-30T15:14:47.132215Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","venue":"astro-ph.CO","work_id":"8aa04ef0-ec75-4f3b-a546-bde81c29c80c","year":2011},"citing_paper":{"arxiv_id":"2605.27087","last_updated":"2026-06-02T03:39:14Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-26T14:35:10Z","title":"Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-06-29T15:49:18.200446Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2605.27087"},"observation_digest":"sha256:ec5af38ea20cfaf1cc48ff76b0e5125974a97f1400eedf7275761a7ab16e3955","observation_id":"8896f70d-a104-48fb-a6f6-1166affce3f3","resolution":{"observed_at":"2026-06-29T16:33:39.561136Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2948","snapshot_observed_at":"2026-07-14T16:44:02.461654Z","title":"Blake, S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.09732","last_updated":"2026-07-02T07:56:02Z","snapshot_observed_at":"2026-08-04T12:51:14.408110Z","submitted_at":"2026-07-02T07:56:02Z","title":"Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-07-14T16:44:02.461654Z"},"links":{"cited_paper":"/paper/1104.2948","citing_paper":"/paper/2607.09732"},"observation_digest":"sha256:55daed52024e75d95434a06d849ff8ce1dc33e04473f55fea1e3c2270cf265f2","observation_id":"2bfe305b-ece7-4364-a184-21aae11f5ede","resolution":{"observed_at":"2026-07-14T16:44:02.461654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1104.2948/citation-record","integrity":"/paper/1104.2948/integrity","json":"/paper/1104.2948/citation-record.json","paper":"/paper/1104.2948"},"outbound":[],"paper":{"arxiv_id":"1104.2948","last_updated":"2011-04-15T00:20:34Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-15T00:20:34Z","title":"The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:1104.2948."}