{"as_of":"2026-08-22T11:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a8dd024fd54b1e0c617c174d5aab8bb0f346383f0386054f0dda80936cbec82d","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T23:07:54.110110Z","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":"2026-07-04T07:09:38.845151Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2111.13137","last_updated":"2023-01-19T21:40:55Z","snapshot_observed_at":"2026-08-16T17:39:19.838425Z","submitted_at":"2021-11-25T15:49:40Z","title":"Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling","version":2},"cited_work":{"arxiv_id":"2111.13137","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2111.13137","snapshot_observed_at":"2026-07-04T07:09:38.845151Z","title":"A., & Ng, K","venue":null,"work_id":"812557a2-bc5e-4093-8374-36f08dadd93c","year":2022},"citing_paper":{"arxiv_id":"2510.07511","last_updated":"2026-04-17T13:58:36Z","snapshot_observed_at":"2026-08-11T10:32:53.120621Z","submitted_at":"2025-10-08T20:18:43Z","title":"Robust Measurement of Stellar Streams Around the Milky Way: Correcting Spatially Variable Observational Selection Effects in Optical Imaging Surveys","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-18T08:58:11.931376Z"},"links":{"cited_paper":"/paper/2111.13137","citing_paper":"/paper/2510.07511"},"observation_digest":"sha256:de4144a9d37d2b247ba5a5a5f9fffba514debf56720c1d2ccbc0200b1a889223","observation_id":"7f398d38-6775-447b-b09d-3f70ca743519","resolution":{"observed_at":"2026-05-18T09:01:09.613267Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.13137","last_updated":"2023-01-19T21:40:55Z","snapshot_observed_at":"2026-08-16T17:39:19.838425Z","submitted_at":"2021-11-25T15:49:40Z","title":"Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.13137","snapshot_observed_at":"2026-08-03T23:07:54.110110Z","title":"Dekker, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.07513","last_updated":"2026-07-01T19:58:59Z","snapshot_observed_at":"2026-08-17T11:54:41.459636Z","submitted_at":"2025-11-10T19:00:00Z","title":"JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios","version":5},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.110110Z"},"links":{"cited_paper":"/paper/2111.13137","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:213e59745491e9bcb97d41da52889dd56d38e6562c2bacc611ba6b1b5d09355b","observation_id":"950a0f7e-4f1e-4922-bb9f-b6f32d896a4c","resolution":{"observed_at":"2026-08-03T23:07:54.110110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.13137","last_updated":"2023-01-19T21:40:55Z","snapshot_observed_at":"2026-08-16T17:39:19.838425Z","submitted_at":"2021-11-25T15:49:40Z","title":"Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.13137","snapshot_observed_at":"2026-08-03T07:37:35.527724Z","title":"Dekker, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2601.19863","last_updated":"2026-07-15T15:48:17Z","snapshot_observed_at":"2026-08-18T13:02:18.217217Z","submitted_at":"2026-01-27T18:21:08Z","title":"Prompt cusps in hierarchical dark matter halos: Implications for annihilation boost","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-03T07:37:35.527724Z"},"links":{"cited_paper":"/paper/2111.13137","citing_paper":"/paper/2601.19863"},"observation_digest":"sha256:4a2b5183d71b36ead04ce99caf5ec1fb45bb2654f7447de47c63f2aa70e55198","observation_id":"5676323a-3e2c-45ee-a86a-7867f468d0b5","resolution":{"observed_at":"2026-08-03T07:37:35.527724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.13137","last_updated":"2023-01-19T21:40:55Z","snapshot_observed_at":"2026-08-16T17:39:19.838425Z","submitted_at":"2021-11-25T15:49:40Z","title":"Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling","version":2},"cited_work":{"arxiv_id":"2111.13137","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2111.13137","snapshot_observed_at":"2026-07-04T07:09:38.845151Z","title":"A., & Ng, K","venue":null,"work_id":"812557a2-bc5e-4093-8374-36f08dadd93c","year":2022},"citing_paper":{"arxiv_id":"2606.21519","last_updated":"2026-06-19T15:16:42Z","snapshot_observed_at":"2026-08-15T14:41:44.719071Z","submitted_at":"2026-06-19T15:16:42Z","title":"Wave-optics imprints of dark matter subhalos on strongly lensed gravitational waves. II. Saddle images and detectability","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-06-26T13:34:00.717067Z"},"links":{"cited_paper":"/paper/2111.13137","citing_paper":"/paper/2606.21519"},"observation_digest":"sha256:3d7ce496ab779540b2c8b5cbccede96bd22b7db9c724a7f8c875f752bb700d3a","observation_id":"9c59f8b3-283c-44c0-8fe9-b6161a3f3628","resolution":{"observed_at":"2026-07-04T07:09:38.846699Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.13137","last_updated":"2023-01-19T21:40:55Z","snapshot_observed_at":"2026-08-16T17:39:19.838425Z","submitted_at":"2021-11-25T15:49:40Z","title":"Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.13137","snapshot_observed_at":"2026-08-01T11:22:03.765828Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19938","last_updated":"2026-07-22T09:12:33Z","snapshot_observed_at":"2026-08-21T11:34:57.797028Z","submitted_at":"2026-07-22T09:12:33Z","title":"Ringing of the Reionization: A first direct measurement of the intergalactic pressure smoothing scale at redshift z>4.2 as imprinted onto small-scale peculiar velocities in the Lyman-alpha forest","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-01T11:22:03.765828Z"},"links":{"cited_paper":"/paper/2111.13137","citing_paper":"/paper/2607.19938"},"observation_digest":"sha256:e4f34400479f76dbde6dff228351bda72a36974daafe1effedcd5905d639d268","observation_id":"0955f5be-345a-490e-9701-1eb5a8fe7137","resolution":{"observed_at":"2026-08-01T11:22:03.765828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.13137","last_updated":"2023-01-19T21:40:55Z","snapshot_observed_at":"2026-08-16T17:39:19.838425Z","submitted_at":"2021-11-25T15:49:40Z","title":"Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.13137","snapshot_observed_at":"2026-08-01T09:11:24.213307Z","title":"Dekker, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.20884","last_updated":"2026-07-23T03:18:02Z","snapshot_observed_at":"2026-08-18T12:54:40.217704Z","submitted_at":"2026-07-23T03:18:02Z","title":"A lower bound on primordial power spectrum from halo substructure","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-01T09:11:24.213307Z"},"links":{"cited_paper":"/paper/2111.13137","citing_paper":"/paper/2607.20884"},"observation_digest":"sha256:a25f842e027b2d08c3dc600858e907b0a217dc4dcf451effa3015f34e00e1874","observation_id":"913be03f-e24f-454c-b11d-38abfb1395e3","resolution":{"observed_at":"2026-08-01T09:11:24.213307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2111.13137/citation-record","integrity":"/paper/2111.13137/integrity","json":"/paper/2111.13137/citation-record.json","paper":"/paper/2111.13137"},"outbound":[],"paper":{"arxiv_id":"2111.13137","last_updated":"2023-01-19T21:40:55Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T17:39:19.838425Z","submitted_at":"2021-11-25T15:49:40Z","title":"Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2111.13137."}