{"as_of":"2026-08-14T02:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6f12654c0a6449bb385c949ccd95b800fb136c34234a07614a9ec7ab3c68435a","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T18:11:36.049361Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-03T16:18:38.381386Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04117","snapshot_observed_at":"2026-08-12T18:11:36.049361Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.11973","last_updated":"2025-03-17T17:44:48Z","snapshot_observed_at":"2026-08-13T05:40:49.955207Z","submitted_at":"2024-11-18T19:01:25Z","title":"Boosted Dark Matter Driven by Cosmic Rays and Diffuse Supernova Neutrinos","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T18:11:36.049361Z"},"links":{"cited_paper":"/paper/2309.04117","citing_paper":"/paper/2411.11973"},"observation_digest":"sha256:bcb32d113e0962cff3f691e22633407ef4737ea6c19f5d81c15f8c8d47465b7b","observation_id":"ce6e7eee-39bd-4e1e-83e5-92e561906bff","resolution":{"observed_at":"2026-08-12T18:11:36.049361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04117","snapshot_observed_at":"2026-08-12T05:07:16.311317Z","title":"De Romeri, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.00805","last_updated":"2024-12-01T13:26:44Z","snapshot_observed_at":"2026-08-13T14:04:36.147745Z","submitted_at":"2024-12-01T13:26:44Z","title":"Neutrino Diffusion within Dark Matter Spikes","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T05:07:16.311317Z"},"links":{"cited_paper":"/paper/2309.04117","citing_paper":"/paper/2412.00805"},"observation_digest":"sha256:52bdc1867b306a272b3a62a2399d1928c9d9be4012f14db13b15c6f38c98e657","observation_id":"8e4787ef-41c9-4244-a405-356387ba24a2","resolution":{"observed_at":"2026-08-12T05:07:16.311317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04117","snapshot_observed_at":"2026-08-10T18:15:41.209240Z","title":"De Romeri, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11569","last_updated":"2025-04-23T17:57:49Z","snapshot_observed_at":"2026-08-13T10:42:36.732852Z","submitted_at":"2025-01-20T16:18:51Z","title":"Blazar Boosted ALP and vector portal Dark matter confronting light mediator searches","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T18:15:41.209240Z"},"links":{"cited_paper":"/paper/2309.04117","citing_paper":"/paper/2501.11569"},"observation_digest":"sha256:52ef373f231eb67a3b2883352515f44b03b8e408099fd6db7224afbb288b3145","observation_id":"852c4d81-14d2-4198-b8bb-790b8fe8fc56","resolution":{"observed_at":"2026-08-10T18:15:41.209240Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04117","snapshot_observed_at":"2026-08-03T08:35:40.219661Z","title":"De Romeri, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2601.16903","last_updated":"2026-07-23T09:17:53Z","snapshot_observed_at":"2026-08-10T11:08:10.863356Z","submitted_at":"2026-01-23T17:12:56Z","title":"Cosmic-ray-electron boosted light dark matter: Implications of LZ 2025 data","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-03T08:35:40.219661Z"},"links":{"cited_paper":"/paper/2309.04117","citing_paper":"/paper/2601.16903"},"observation_digest":"sha256:49402d0a8b2c396aed90b082f543278d4bdea9df17c6a2c18b478739af365a68","observation_id":"1cea2039-6a10-4286-a817-0c2edf6f198c","resolution":{"observed_at":"2026-08-03T08:35:40.219661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter","version":3},"cited_work":{"arxiv_id":"2309.04117","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.04117","snapshot_observed_at":"2026-07-03T16:18:38.381386Z","title":"De Romeri, A","venue":null,"work_id":"f413f4ee-8013-41da-ac2a-7894bba0cdb6","year":2024},"citing_paper":{"arxiv_id":"2602.04858","last_updated":"2026-06-23T09:20:24Z","snapshot_observed_at":"2026-08-03T04:31:42.595842Z","submitted_at":"2026-02-04T18:43:59Z","title":"Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-05-16T06:48:35.787193Z"},"links":{"cited_paper":"/paper/2309.04117","citing_paper":"/paper/2602.04858"},"observation_digest":"sha256:5b9403fe34ee2f3fff6f13f5fd2aaac0edd0bacb89c0409d9030c61742aac615","observation_id":"ac1ac5d6-1fd2-49ff-8fc7-37d469120ba8","resolution":{"observed_at":"2026-05-16T06:50:42.792877Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04117","snapshot_observed_at":"2026-08-03T04:31:58.618333Z","title":"De Romeri, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.04858","last_updated":"2026-06-23T09:20:24Z","snapshot_observed_at":"2026-08-03T04:31:42.595842Z","submitted_at":"2026-02-04T18:43:59Z","title":"Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints","version":3},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-03T04:31:58.618333Z"},"links":{"cited_paper":"/paper/2309.04117","citing_paper":"/paper/2602.04858"},"observation_digest":"sha256:819eed5bbcdb7291086da131b66c9d9395bae4a0863391707c43448068f4be4e","observation_id":"8559fd49-1122-4ab8-b5d8-05ddbdb1b537","resolution":{"observed_at":"2026-08-03T04:31:58.618333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04117","snapshot_observed_at":"2026-08-03T04:14:46.746962Z","title":"De Romeri, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.06111","last_updated":"2026-06-24T08:31:42Z","snapshot_observed_at":"2026-08-06T14:38:27.293620Z","submitted_at":"2026-02-05T19:00:00Z","title":"Dark Matter Heating of Compact Stars Beyond Capture: A Relativistic Framework for Energy Deposition by Particle Beams","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-03T04:14:46.746962Z"},"links":{"cited_paper":"/paper/2309.04117","citing_paper":"/paper/2602.06111"},"observation_digest":"sha256:7e773200b3146ede1e3aa017c55a0272eb19b7dcfb941d1d053ff9255018060d","observation_id":"c4bb06d7-9561-46ff-902f-c3c32ac15eda","resolution":{"observed_at":"2026-08-03T04:14:46.746962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter","version":3},"cited_work":{"arxiv_id":"2309.04117","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.04117","snapshot_observed_at":"2026-07-03T16:18:38.381386Z","title":"De Romeri, A","venue":null,"work_id":"f413f4ee-8013-41da-ac2a-7894bba0cdb6","year":2024},"citing_paper":{"arxiv_id":"2606.13469","last_updated":"2026-06-11T15:20:50Z","snapshot_observed_at":"2026-08-02T03:38:17.954750Z","submitted_at":"2026-06-11T15:20:50Z","title":"Simulations of 3-Dimensional Recoil Response to Coherent Elastic Neutrino-Nucleus Scattering Events in Directional Direct Dark Matter Detectors","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-27T05:51:41.874094Z"},"links":{"cited_paper":"/paper/2309.04117","citing_paper":"/paper/2606.13469"},"observation_digest":"sha256:ccd1f00f3ed5447171eeea436b33405c7b71636b058e5eb22e0472d96b0b3b3d","observation_id":"55c48107-927b-4684-95d0-198dcfc00af6","resolution":{"observed_at":"2026-07-03T16:18:38.382928Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2309.04117/citation-record","integrity":"/paper/2309.04117/integrity","json":"/paper/2309.04117/citation-record.json","paper":"/paper/2309.04117"},"outbound":[],"paper":{"arxiv_id":"2309.04117","last_updated":"2024-03-14T08:43:24Z","latest_version":3,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-13T10:18:07.734741Z","submitted_at":"2023-09-08T04:39:12Z","title":"XENONnT and LUX-ZEPLIN constraints on DSNB-boosted dark matter"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2309.04117."}