{"as_of":"2026-08-14T08:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:74f8054f491a59a84c42961175a1d821851012e11124e5811f41aa2427808444","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":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:15:31.926587Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-07T15:15:31.926587Z","title":"2025, title Positive neutrino masses with DESI DR2 via matter conversion to dark energy , arXiv e-prints, arXiv:2504.20338, 10.48550/arXiv.2504.20338","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.15899","last_updated":"2025-05-21T18:00:02Z","snapshot_observed_at":"2026-08-14T05:07:18.682162Z","submitted_at":"2025-05-21T18:00:02Z","title":"The CMB optical depth constrains the duration of reionization","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-07T15:15:31.926587Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2505.15899"},"observation_digest":"sha256:891ae496a538c1081b16af8c6b7581af03a2b4459ae9d7ec5b34731a35fa3c4c","observation_id":"f62a4ce9-389d-4a40-b674-78c01dd47614","resolution":{"observed_at":"2026-08-07T15:15:31.926587Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-06T15:12:38.109926Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.16589","last_updated":"2026-06-23T13:43:52Z","snapshot_observed_at":"2026-08-08T06:56:16.966820Z","submitted_at":"2025-07-22T13:45:38Z","title":"Cosmological preference for a positive neutrino mass at 2.7$\\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data","version":3},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T15:12:38.109926Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2507.16589"},"observation_digest":"sha256:69f771810df67433ae5bfe5e1ac379af8c43b4a12c940631178eed501663301e","observation_id":"7471884b-0485-4e93-88ae-6925a0f13eea","resolution":{"observed_at":"2026-08-06T15:12:38.109926Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":"2504.20338","doi":"10.48550/arxiv.2504.20338","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Ahlen, A","venue":"arXiv (Cornell University)","work_id":"6aa2b27e-7210-49df-b754-d8186fa0fa6a","year":2025},"citing_paper":{"arxiv_id":"2601.02077","last_updated":"2026-04-04T13:29:01Z","snapshot_observed_at":"2026-08-11T02:41:13.646300Z","submitted_at":"2026-01-05T12:58:36Z","title":"Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity","version":2},"reference_index":113,"source":"pdf_text","source_observed_at":"2026-05-16T18:00:59.984076Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2601.02077"},"observation_digest":"sha256:1cc7f7975a21ce09f72b42f698b790fae438d8f6e3d46441a780cbe6544cc6be","observation_id":"4a5b1f47-bf43-4243-a73f-22a32cce97ee","resolution":{"observed_at":"2026-05-16T18:01:08.933147Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":"2504.20338","doi":"10.48550/arxiv.2504.20338","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Ahlen, A","venue":"arXiv (Cornell University)","work_id":"6aa2b27e-7210-49df-b754-d8186fa0fa6a","year":2025},"citing_paper":{"arxiv_id":"2603.10787","last_updated":"2026-03-11T14:00:06Z","snapshot_observed_at":"2026-08-11T15:40:03.224454Z","submitted_at":"2026-03-11T14:00:06Z","title":"Measuring neutrino mass in light of ACT DR6 and DESI DR2","version":1},"reference_index":111,"source":"pdf_text","source_observed_at":"2026-05-15T13:14:03.491513Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2603.10787"},"observation_digest":"sha256:42aeb19a23f6169a95a91cc1e3847c65f0fcd776fb29eabc56a197cac7a98e1e","observation_id":"43d1b6e0-6c58-48ac-aaf1-65a272cfdd97","resolution":{"observed_at":"2026-05-15T13:15:50.051539Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-02T14:29:22.500586Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.10476","last_updated":"2026-07-21T12:07:55Z","snapshot_observed_at":"2026-08-11T08:05:13.599295Z","submitted_at":"2026-05-11T12:38:17Z","title":"Breaking Free from the Swampland of Impossible Universes through the DESI Portal","version":4},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-02T14:29:22.500586Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2605.10476"},"observation_digest":"sha256:f91e6459a9efca51d8238b5698c47c97686a66866d5ae3e46c70484f6cb583f3","observation_id":"98a0de10-a3ec-429c-a5d6-b3fccb3ce008","resolution":{"observed_at":"2026-08-02T14:29:22.500586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":"2504.20338","doi":"10.48550/arxiv.2504.20338","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Ahlen, A","venue":"arXiv (Cornell University)","work_id":"6aa2b27e-7210-49df-b754-d8186fa0fa6a","year":2025},"citing_paper":{"arxiv_id":"2605.18716","last_updated":"2026-05-18T17:47:36Z","snapshot_observed_at":"2026-08-02T18:37:15.457224Z","submitted_at":"2026-05-18T17:47:36Z","title":"Recoupled Dark Radiation reconciling CMB and DESI BAO measurements","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-20T09:01:32.945533Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2605.18716"},"observation_digest":"sha256:824cb02b0c22897bec9907e6c7d43debaacf749120906ddfd1f6388189f7a8fb","observation_id":"695f6cff-2b29-4ad2-b210-5930eb2ef33e","resolution":{"observed_at":"2026-05-20T09:03:10.043540Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":"2504.20338","doi":"10.48550/arxiv.2504.20338","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Ahlen, A","venue":"arXiv (Cornell University)","work_id":"6aa2b27e-7210-49df-b754-d8186fa0fa6a","year":2025},"citing_paper":{"arxiv_id":"2606.05005","last_updated":"2026-06-03T15:26:36Z","snapshot_observed_at":"2026-07-06T23:45:02.342193Z","submitted_at":"2026-06-03T15:26:36Z","title":"Neutrino mass constraints in interacting dark energy models after DESI DR2","version":1},"reference_index":129,"source":"pdf_text","source_observed_at":"2026-06-28T04:52:33.342231Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2606.05005"},"observation_digest":"sha256:b8bbe4c4c21a4064887fa96dc4b0b3736afae6a28ef19443e3bb9d769e35ee29","observation_id":"e145cf7f-b0e3-45a0-ae30-e5bec0de8cbe","resolution":{"observed_at":"2026-07-02T10:56:52.513437Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":"2504.20338","doi":"10.48550/arxiv.2504.20338","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Ahlen, A","venue":"arXiv (Cornell University)","work_id":"6aa2b27e-7210-49df-b754-d8186fa0fa6a","year":2025},"citing_paper":{"arxiv_id":"2606.19449","last_updated":"2026-06-17T18:00:07Z","snapshot_observed_at":"2026-08-12T22:07:51.773940Z","submitted_at":"2026-06-17T18:00:07Z","title":"A self-consistent analytical model for both the photoionization rate and reionization history","version":1},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-06-26T19:42:03.383235Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2606.19449"},"observation_digest":"sha256:0684e1a684a287ff3e747d8f4c43ada6d9ea0ae3ebe2c46535672b5c50671025","observation_id":"35a9f108-135d-4939-a6e3-5411775b117d","resolution":{"observed_at":"2026-07-04T02:29:23.391191Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":"2504.20338","doi":"10.48550/arxiv.2504.20338","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Ahlen, A","venue":"arXiv (Cornell University)","work_id":"6aa2b27e-7210-49df-b754-d8186fa0fa6a","year":2025},"citing_paper":{"arxiv_id":"2606.19459","last_updated":"2026-06-17T18:01:12Z","snapshot_observed_at":"2026-08-13T21:31:19.365989Z","submitted_at":"2026-06-17T18:01:12Z","title":"Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-06-26T19:37:19.656550Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2606.19459"},"observation_digest":"sha256:166c110aaead54d9ab06512750b7abc9eb6d7b8f1cc19e350c0e521d7a915030","observation_id":"f63a7874-f35a-4704-9082-a3abc67e9a44","resolution":{"observed_at":"2026-06-26T19:39:50.636299Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":182,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:e46794552e6107297e8eedad98e06d7f656946f652e0cc4004c425e569fd8673","observation_id":"8a8ae46f-262a-4990-94fb-b57bdfefd77d","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-02T03:35:56.423266Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.13857","last_updated":"2026-07-15T14:02:52Z","snapshot_observed_at":"2026-08-12T18:06:39.936614Z","submitted_at":"2026-07-15T14:02:52Z","title":"Evaporating cosmologically coupled black holes","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-02T03:35:56.423266Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2607.13857"},"observation_digest":"sha256:915487ac536438fa00243d9c45b6ff436fcd0957f842ce688e2b2495a36ebdb3","observation_id":"03b7810b-cc84-41f6-9ee6-58e2d9bd88d8","resolution":{"observed_at":"2026-08-02T03:35:56.423266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.20338","snapshot_observed_at":"2026-08-01T01:25:44.291475Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.25841","last_updated":"2026-07-28T15:18:43Z","snapshot_observed_at":"2026-08-14T07:16:00.788206Z","submitted_at":"2026-07-28T15:18:43Z","title":"General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints","version":1},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-08-01T01:25:44.291475Z"},"links":{"cited_paper":"/paper/2504.20338","citing_paper":"/paper/2607.25841"},"observation_digest":"sha256:f2ea76135509c1307cdd9c45ff2386f84c9e6c76b01305f553a9e3200cac79ba","observation_id":"b4afb2c0-3640-4964-ba1d-602d645c4cb9","resolution":{"observed_at":"2026-08-01T01:25:44.291475Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2504.20338/citation-record","integrity":"/paper/2504.20338/integrity","json":"/paper/2504.20338/citation-record.json","paper":"/paper/2504.20338"},"outbound":[],"paper":{"arxiv_id":"2504.20338","last_updated":"2025-09-08T20:18:27Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T15:58:24.960182Z","submitted_at":"2025-04-29T01:13:41Z","title":"Positive neutrino masses with DESI DR2 via matter conversion to dark energy"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2504.20338."}