{"as_of":"2026-08-12T04:40:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:374f0fe9da0db5c881ef58f6662facb99dff9531474782a521bbe7a8d64d4d09","coverage":[{"denominator":85,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":85,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T16:14:56.906189Z","state":"measured"},{"denominator":86,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":86,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T21:29:36.872636Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.10310","snapshot_observed_at":"2026-08-03T21:29:36.872636Z","title":"Simulation-based inference on warm dark matter from HERA forecasts,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.15430","last_updated":"2025-11-19T13:36:51Z","snapshot_observed_at":"2026-08-08T07:30:28.738526Z","submitted_at":"2025-11-19T13:36:51Z","title":"21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-03T21:29:36.872636Z"},"links":{"cited_paper":"/paper/2412.10310","citing_paper":"/paper/2511.15430"},"observation_digest":"sha256:4f9b30f116e131c0731eb5f9825dc039ec74ea9d44ea47db26299b5d1881a036","observation_id":"9a3649a4-567f-4ac1-88d6-42a34e999570","resolution":{"observed_at":"2026-08-03T21:29:36.872636Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2412.10310/citation-record","integrity":"/paper/2412.10310/integrity","json":"/paper/2412.10310/citation-record.json","paper":"/paper/2412.10310"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2210.04912","last_updated":"2023-01-19T20:18:42Z","snapshot_observed_at":"2026-08-10T13:42:32.450537Z","submitted_at":"2022-10-10T18:00:01Z","title":"Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.04912","snapshot_observed_at":"2026-08-11T16:14:56.555221Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.555221Z"},"links":{"cited_paper":"/paper/2210.04912","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:9b0b8b8954bc781a544369c7459d84336c135d3949db88aba6c7ec443e6f6f11","observation_id":"7669bd6d-8123-4ad9-a4ae-5619920b7578","resolution":{"observed_at":"2026-08-11T16:14:56.555221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.0197","last_updated":"2013-03-24T13:46:39Z","snapshot_observed_at":"2026-08-10T09:46:59.983772Z","submitted_at":"2012-09-30T13:40:29Z","title":"Reionization and the Cosmic Dawn with the Square Kilometre Array","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.0197","snapshot_observed_at":"2026-08-11T16:14:56.559822Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.559822Z"},"links":{"cited_paper":"/paper/1210.0197","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:46ef7e3a7d65aac4d4fd76da2e081771d982ef9a894a518d9e0661fa6f336ca0","observation_id":"f60169fe-18eb-487c-b185-e783dbfca21c","resolution":{"observed_at":"2026-08-11T16:14:56.559822Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.07568","last_updated":"2015-05-28T07:31:46Z","snapshot_observed_at":"2026-08-02T08:32:11.645299Z","submitted_at":"2015-05-28T07:31:46Z","title":"The Cosmic Dawn and Epoch of Reionization with the Square Kilometre Array","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.07568","snapshot_observed_at":"2026-08-11T16:14:56.563724Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.563724Z"},"links":{"cited_paper":"/paper/1505.07568","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:378dcbd3b0493e6edca1f0825de81dce5125118ec28d2c70a51cb4c9781ae9a3","observation_id":"b87c31e3-18b4-418b-94b9-ec599a1e1988","resolution":{"observed_at":"2026-08-11T16:14:56.563724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.02263","last_updated":"2021-08-04T20:00:24Z","snapshot_observed_at":"2026-08-06T07:25:52.575334Z","submitted_at":"2021-08-04T20:00:24Z","title":"First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.02263","snapshot_observed_at":"2026-08-11T16:14:56.567700Z","title":"Abdurashidova et al., First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum , Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.567700Z"},"links":{"cited_paper":"/paper/2108.02263","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:4e81bdc0f194113a2443ce2746a93b2b7f5d66c78f29e0ed16b09514d711a610","observation_id":"53a64fc1-cf9d-4353-8fee-105db5bb6bd8","resolution":{"observed_at":"2026-08-11T16:14:56.567700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.01496","last_updated":"2019-07-02T16:58:48Z","snapshot_observed_at":"2026-08-08T07:30:39.258113Z","submitted_at":"2019-07-02T16:58:48Z","title":"Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\\alpha$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.01496","snapshot_observed_at":"2026-08-11T16:14:56.572181Z","title":"Archidiacono, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.572181Z"},"links":{"cited_paper":"/paper/1907.01496","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:c8579886db4843565c38a1c8b6c0d52509b4b45d7f52172395e6f1ab92b7348c","observation_id":"89f0aac2-a5c0-4bcf-ab5f-95a1965be30a","resolution":{"observed_at":"2026-08-11T16:14:56.572181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-08-11T16:14:56.576486Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.576486Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:72b2c3f89efc05e0e7268a9adf095a8fb1559466cb87490a16bf9c51608eebcf","observation_id":"2a6bec31-ecc7-498c-86d2-b0db086c9af6","resolution":{"observed_at":"2026-08-11T16:14:56.576486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.00021","last_updated":"2018-09-17T08:34:43Z","snapshot_observed_at":"2026-07-06T06:36:31.526822Z","submitted_at":"2018-04-30T18:00:01Z","title":"Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.00021","snapshot_observed_at":"2026-08-11T16:14:56.581451Z","title":"Schneider, Constraining noncold dark matter models with the global 21-cm signal , Phys","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.581451Z"},"links":{"cited_paper":"/paper/1805.00021","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:d7953dbcbc8c175db7814a810c259bada125dac16133cdb065bc09a37ce04cd6","observation_id":"9857f186-47f5-4ee3-a3cc-4654297831f1","resolution":{"observed_at":"2026-08-11T16:14:56.581451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.0029","last_updated":"2013-12-10T18:36:30Z","snapshot_observed_at":"2026-07-06T03:24:23.773832Z","submitted_at":"2013-09-30T20:03:25Z","title":"The Imprint of Warm Dark Matter on the Cosmological 21-cm Signal","version":2},"cited_work":{"arxiv_id":"1310.0029","doi":null,"metadata_source":"pith","pith_arxiv_id":"1310.0029","snapshot_observed_at":"2026-08-11T16:14:57.850197Z","title":"The Imprint of Warm Dark Matter on the Cosmological 21-cm Signal","venue":"astro-ph.CO","work_id":"15f1b638-e0f9-4762-83b6-596875b5fa7d","year":2013},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.585904Z"},"links":{"cited_paper":"/paper/1310.0029","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:c929dcbac18e8b7bdde55e6a072e1cd97208f583c73aa3bc5441efe6b2b6dcfd","observation_id":"3348516e-311e-45af-b5e0-4508a80002c2","resolution":{"observed_at":"2026-08-11T16:14:57.854736Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.08427","last_updated":"2018-06-07T21:18:20Z","snapshot_observed_at":"2026-08-03T22:28:30.374746Z","submitted_at":"2018-03-22T16:05:44Z","title":"A fresh look into the interacting dark matter scenario","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.08427","snapshot_observed_at":"2026-08-11T16:14:56.590056Z","title":"Escudero, L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.590056Z"},"links":{"cited_paper":"/paper/1803.08427","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:49f969523f5f1840e876b6c31a2ec1772eed0ff1b332194b8ed69a30caafc654","observation_id":"95d964ab-53cb-4c64-bf24-938f693d0d4a","resolution":{"observed_at":"2026-08-11T16:14:56.590056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.15466","last_updated":"2023-05-30T11:42:29Z","snapshot_observed_at":"2026-08-09T19:39:22.719007Z","submitted_at":"2023-05-24T18:00:01Z","title":"BEoRN: A fast and flexible framework to simulate the epoch of reionisation and cosmic dawn","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.15466","snapshot_observed_at":"2026-08-11T16:14:56.594590Z","title":"Schaeffer, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.594590Z"},"links":{"cited_paper":"/paper/2305.15466","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:9c00301526787f430f64dae69f48cedec67edac9db42f424d0ef1913fb5655ba","observation_id":"9ce4719a-3193-4be6-92a0-91c0a76f2102","resolution":{"observed_at":"2026-08-11T16:14:56.594590Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.08039","last_updated":"2018-05-16T23:23:59Z","snapshot_observed_at":"2026-07-06T06:29:30.274650Z","submitted_at":"2018-03-19T18:00:08Z","title":"A limit on the warm dark matter particle mass from the redshifted 21 cm absorption line","version":2},"cited_work":{"arxiv_id":"1803.08039","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.08039","snapshot_observed_at":"2026-08-11T16:14:57.808221Z","title":"A limit on the warm dark matter particle mass from the redshifted 21 cm absorption line","venue":"astro-ph.CO","work_id":"70cb9150-6db3-438a-8598-f9bc8669aa7d","year":2018},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.598845Z"},"links":{"cited_paper":"/paper/1803.08039","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:8363733d745c2032723c4a563442fd24086d9db67d14e3ad24390b35f041f7fa","observation_id":"78885809-34cd-4bf7-9485-455d11c4955d","resolution":{"observed_at":"2026-08-11T16:14:57.813146Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.01253","last_updated":"2018-05-03T12:25:25Z","snapshot_observed_at":"2026-07-06T06:37:11.777400Z","submitted_at":"2018-05-03T12:25:25Z","title":"The Implications of a Pre-reionization 21 cm Absorption Signal for Fuzzy Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.01253","snapshot_observed_at":"2026-08-11T16:14:56.602945Z","title":"Lidz and L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.602945Z"},"links":{"cited_paper":"/paper/1805.01253","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:9c61be007c899438f6351da6a863bc8e4870d8398c8d15c430e762fcfd5735d0","observation_id":"2c0438e2-acab-4caf-8cc5-9e2344a883cd","resolution":{"observed_at":"2026-08-11T16:14:56.602945Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.02716","last_updated":"2018-11-07T01:26:08Z","snapshot_observed_at":"2026-08-11T01:34:07.565330Z","submitted_at":"2018-11-07T01:26:08Z","title":"Dark Matter microphysics and 21 cm observations","version":1},"cited_work":{"arxiv_id":"1811.02716","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.02716","snapshot_observed_at":"2026-08-11T16:14:57.778695Z","title":"Dark Matter microphysics and 21 cm observations","venue":"astro-ph.CO","work_id":"4f0d8d4b-b981-48c2-abc7-42c7669f382e","year":2018},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.607742Z"},"links":{"cited_paper":"/paper/1811.02716","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:87de0061739ddce53018500691395d897abd7a4ce8efc1b896f7b3717f87d607","observation_id":"c4c64d15-de41-4292-aa27-0ba85e33ca7d","resolution":{"observed_at":"2026-08-11T16:14:57.783271Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.05333","last_updated":"2020-11-10T19:00:00Z","snapshot_observed_at":"2026-08-09T04:48:09.083789Z","submitted_at":"2020-11-10T19:00:00Z","title":"ETHOS -- An Effective Theory of Structure Formation: Impact of Dark Acoustic Oscillations on Cosmic Dawn","version":1},"cited_work":{"arxiv_id":"2011.05333","doi":null,"metadata_source":"pith","pith_arxiv_id":"2011.05333","snapshot_observed_at":"2026-08-11T16:14:57.760904Z","title":"ETHOS -- An Effective Theory of Structure Formation: Impact of Dark Acoustic Oscillations on Cosmic Dawn","venue":"astro-ph.CO","work_id":"2b42e8c9-d235-4cc7-ba15-8f208f653ea6","year":2020},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.612902Z"},"links":{"cited_paper":"/paper/2011.05333","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:51d2c97d60d6900e0f67eb8c2e167b871adb4bfe068adce48549227810f164e3","observation_id":"ffbdc9e1-4eb8-4758-bad2-bd37c368f0ad","resolution":{"observed_at":"2026-08-11T16:14:57.765439Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.07177","last_updated":"2021-03-21T17:18:33Z","snapshot_observed_at":"2026-08-10T21:04:22.334732Z","submitted_at":"2021-01-18T17:29:39Z","title":"Fuzzy Dark Matter and the 21cm Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.07177","snapshot_observed_at":"2026-08-11T16:14:56.617085Z","title":"Jones, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.617085Z"},"links":{"cited_paper":"/paper/2101.07177","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:513fa2d23b1f994ed4b96e701bf608a5797281172f20a5c23e6da6dc29d1fc3a","observation_id":"22b2efa7-e934-47f3-a9c2-7db3d7ca6c0c","resolution":{"observed_at":"2026-08-11T16:14:56.617085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.02210","last_updated":"2022-04-04T07:54:41Z","snapshot_observed_at":"2026-08-10T21:04:29.911450Z","submitted_at":"2022-01-06T19:00:29Z","title":"Imprints of fermionic and bosonic mixed dark matter on the 21-cm signal at cosmic dawn","version":2},"cited_work":{"arxiv_id":"2201.02210","doi":null,"metadata_source":"pith","pith_arxiv_id":"2201.02210","snapshot_observed_at":"2026-08-11T16:14:57.731781Z","title":"Imprints of fermionic and bosonic mixed dark matter on the 21-cm signal at cosmic dawn","venue":"astro-ph.CO","work_id":"775f634e-c274-427a-8528-ba9e70825ead","year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.621052Z"},"links":{"cited_paper":"/paper/2201.02210","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:cd2b6460a30fe39dcf587a3cf8f5a4f94b39b8d126f2397797e9dace7ec875a8","observation_id":"f376b115-f30a-45dc-8805-eeb1c60cc3cd","resolution":{"observed_at":"2026-08-11T16:14:57.736298Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2201.02638","last_updated":"2022-03-31T19:04:01Z","snapshot_observed_at":"2026-08-10T08:45:38.936286Z","submitted_at":"2022-01-07T19:00:09Z","title":"Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal","version":2},"cited_work":{"arxiv_id":"2201.02638","doi":null,"metadata_source":"pith","pith_arxiv_id":"2201.02638","snapshot_observed_at":"2026-08-11T16:14:57.713230Z","title":"Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal","venue":"astro-ph.CO","work_id":"8ccc4903-30a5-43dd-869e-07aecf7b4887","year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.625126Z"},"links":{"cited_paper":"/paper/2201.02638","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:d8de932747a96727d3577c0953a8ca6cbec5c60eeaec9b3cc676976da46bbfc0","observation_id":"8c090d67-01c1-4e98-9116-d4d336554d79","resolution":{"observed_at":"2026-08-11T16:14:57.718250Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04174","last_updated":"2025-03-20T13:08:09Z","snapshot_observed_at":"2026-08-10T05:13:19.465666Z","submitted_at":"2024-01-08T19:00:05Z","title":"Optimal, fast, and robust inference of reionization-era cosmology with the 21cmPIE-INN","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.04174","snapshot_observed_at":"2026-08-11T16:14:56.628775Z","title":"Schosser, C","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.628775Z"},"links":{"cited_paper":"/paper/2401.04174","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:4c8516de1290e08b6c6ccf053f86b7c73ca180a9dd8ead7e025b9bcca6d9ec72","observation_id":"987bf8d4-fef4-4dc5-8c17-8e4da276b77f","resolution":{"observed_at":"2026-08-11T16:14:56.628775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.17640","last_updated":"2024-04-26T18:01:06Z","snapshot_observed_at":"2026-08-09T08:15:37.021491Z","submitted_at":"2024-04-26T18:01:06Z","title":"Separating Dark Acoustic Oscillations from Astrophysics at Cosmic Dawn","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.17640","snapshot_observed_at":"2026-08-11T16:14:56.633580Z","title":"Verwohlt, C","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.633580Z"},"links":{"cited_paper":"/paper/2404.17640","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:b25fa427c3c5bd5a81dfb543dd1b49eccc21c3414d96c2f96b37959649893231","observation_id":"e16a9f30-ca54-4a7e-b706-ed2bf94a3cdf","resolution":{"observed_at":"2026-08-11T16:14:56.633580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03942","last_updated":"2024-05-28T08:04:58Z","snapshot_observed_at":"2026-08-04T23:59:18.670719Z","submitted_at":"2023-09-07T18:00:01Z","title":"21cmFirstCLASS I. Cosmological tool for $\\Lambda$CDM and beyond","version":4},"cited_work":{"arxiv_id":"2309.03942","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.03942","snapshot_observed_at":"2026-08-11T16:14:57.673879Z","title":"21cmFirstCLASS I. Cosmological tool for $\\Lambda$CDM and beyond","venue":"astro-ph.CO","work_id":"e5e8f79a-3cf8-4fba-9626-9bcf323fea5b","year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.637770Z"},"links":{"cited_paper":"/paper/2309.03942","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:f1b36679b8844908b043aa5165fc44ae8e57c5b4ed3fcfa275b0808dd692da6a","observation_id":"f4d4913a-8094-4116-9fa8-5dca7f0b4de8","resolution":{"observed_at":"2026-08-11T16:14:57.677767Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1003.3878","last_updated":"2010-03-19T20:08:53Z","snapshot_observed_at":"2026-08-04T08:35:55.551337Z","submitted_at":"2010-03-19T20:08:53Z","title":"21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.3878","snapshot_observed_at":"2026-08-11T16:14:56.641469Z","title":"Mesinger, S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.641469Z"},"links":{"cited_paper":"/paper/1003.3878","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:d0d30e4a3da4ef91ed7844028c8a37c6e59bf01acee55aa5287f4d1348a8a903","observation_id":"01d9379e-3d72-4288-ac20-7da400f346d0","resolution":{"observed_at":"2026-08-11T16:14:56.641469Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15121","last_updated":"2020-10-28T15:53:27Z","snapshot_observed_at":"2026-08-11T00:27:33.144327Z","submitted_at":"2020-10-28T15:53:27Z","title":"21cmFAST v3: A Python-integrated C code forgenerating 3D realizations of the cosmic 21cm signal","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.15121","snapshot_observed_at":"2026-08-11T16:14:56.644990Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.644990Z"},"links":{"cited_paper":"/paper/2010.15121","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:09fd23e02cdbb3eaca1ff0b82cd8099000068e041c5904639dbf1cdc24255956","observation_id":"3a66c461-3f9d-4cbe-8160-c394a3c122a9","resolution":{"observed_at":"2026-08-11T16:14:56.644990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10616","last_updated":"2024-10-14T15:20:36Z","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T15:20:36Z","title":"Field-level cosmological model selection: field-level simulation-based inference for Stage IV cosmic shear can distinguish dynamical dark energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10616","snapshot_observed_at":"2026-08-11T16:14:56.649005Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.649005Z"},"links":{"cited_paper":"/paper/2410.10616","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:51dc5f85b23ca55165e38a79537733d48be721c8e320e92b1e0641e37c91113b","observation_id":"27353d5d-8e78-4f59-882c-fa1e96da1d25","resolution":{"observed_at":"2026-08-11T16:14:56.649005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.19910","last_updated":"2023-10-30T18:24:25Z","snapshot_observed_at":"2026-08-09T02:38:56.569190Z","submitted_at":"2023-10-30T18:24:25Z","title":"Bayesian Simulation-based Inference for Cosmological Initial Conditions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.19910","snapshot_observed_at":"2026-08-11T16:14:56.652796Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.652796Z"},"links":{"cited_paper":"/paper/2310.19910","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:6913a3b1dc3ef2c11f65bfe73a5f7595756cba16f51910f2a3adb2aad6f397d3","observation_id":"29f9d132-1ec8-46a4-8ee4-bed86f733faf","resolution":{"observed_at":"2026-08-11T16:14:56.652796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.15071","last_updated":"2023-09-26T17:08:24Z","snapshot_observed_at":"2026-07-06T16:23:57.143116Z","submitted_at":"2023-09-26T17:08:24Z","title":"Sensitivity Analysis of Simulation-Based Inference for Galaxy Clustering","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.15071","snapshot_observed_at":"2026-08-11T16:14:56.656966Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.656966Z"},"links":{"cited_paper":"/paper/2309.15071","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:aee49237ae165a53c7e0082c04b8239025212d72328d2953b560517227efd96b","observation_id":"2dd20603-1bf0-4622-bcdb-cdd185091f60","resolution":{"observed_at":"2026-08-11T16:14:56.656966Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.08430","last_updated":"2024-12-06T15:05:23Z","snapshot_observed_at":"2026-07-06T16:19:01.610586Z","submitted_at":"2023-09-15T14:31:53Z","title":"Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds","version":3},"cited_work":{"arxiv_id":"2309.08430","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.08430","snapshot_observed_at":"2026-08-11T16:14:57.600080Z","title":"Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds","venue":"astro-ph.CO","work_id":"dfc8972c-9ec3-40c8-8443-86dd47d88ead","year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.661165Z"},"links":{"cited_paper":"/paper/2309.08430","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:336e942ed1211f20fb68c2e923c15d2e381a308902130e6d0344d4950930ae08","observation_id":"787c2042-3388-47bd-85b9-700ebd37436c","resolution":{"observed_at":"2026-08-11T16:14:57.604765Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.15734","last_updated":"2022-06-10T08:45:43Z","snapshot_observed_at":"2026-08-09T09:56:59.350769Z","submitted_at":"2022-03-29T16:43:43Z","title":"Implicit Likelihood Inference of Reionization Parameters from the 21 cm Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.15734","snapshot_observed_at":"2026-08-11T16:14:56.666082Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.666082Z"},"links":{"cited_paper":"/paper/2203.15734","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:956d18fe8529f28072e456c813a2710575925cbbf050535610e95594831ecaaa","observation_id":"712414a6-0ef6-491e-bde9-a5a239bf8e31","resolution":{"observed_at":"2026-08-11T16:14:56.666082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.07339","last_updated":"2023-08-31T16:38:44Z","snapshot_observed_at":"2026-08-10T12:23:50.558713Z","submitted_at":"2023-03-13T17:59:13Z","title":"Constraining the X-ray heating and reionization using 21-cm power spectra with Marginal Neural Ratio Estimation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.07339","snapshot_observed_at":"2026-08-11T16:14:56.670095Z","title":"Saxena, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.670095Z"},"links":{"cited_paper":"/paper/2303.07339","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:951cf8f6945a1ebc7d7d314c413a3c1ecadee1f3195ebb1aec95448fde458b18","observation_id":"54a45640-ed9f-4970-8871-c62626fb996e","resolution":{"observed_at":"2026-08-11T16:14:56.670095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.03074","last_updated":"2023-07-04T15:58:50Z","snapshot_observed_at":"2026-08-09T03:37:33.287991Z","submitted_at":"2023-05-04T18:00:00Z","title":"Exploring the likelihood of the 21-cm power spectrum with simulation-based inference","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.03074","snapshot_observed_at":"2026-08-11T16:14:56.674038Z","title":"Prelogovi´ c and A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.674038Z"},"links":{"cited_paper":"/paper/2305.03074","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:efa65419d08ec673c2cfa3d079312ca8c9df05a9ecbc75d5a52c3553996a9da0","observation_id":"15aa5ff6-f5e8-4f0d-b002-db071cfe076b","resolution":{"observed_at":"2026-08-11T16:14:56.674038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12277","last_updated":"2024-10-07T11:53:50Z","snapshot_observed_at":"2026-07-06T17:19:00.228875Z","submitted_at":"2024-01-22T19:00:00Z","title":"How informative are summaries of the cosmic 21-cm signal?","version":2},"cited_work":{"arxiv_id":"2401.12277","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.12277","snapshot_observed_at":"2026-08-11T16:14:57.547059Z","title":"How informative are summaries of the cosmic 21-cm signal?","venue":"astro-ph.CO","work_id":"27a879e7-b298-44e3-9609-cf69c8adbfc7","year":2024},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.678115Z"},"links":{"cited_paper":"/paper/2401.12277","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:8d9603ebecc2f0b10dcd1e280d0790baa63cb8d28118653a842bfdf1a4575e66","observation_id":"06039428-0c6f-4dd3-8cd6-560be02c2e06","resolution":{"observed_at":"2026-08-11T16:14:57.551712Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.14060","last_updated":"2024-03-21T01:11:01Z","snapshot_observed_at":"2026-08-12T03:13:17.949184Z","submitted_at":"2024-03-21T01:11:01Z","title":"Inferring astrophysical parameters using the 2D cylindrical power spectrum from reionisation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.14060","snapshot_observed_at":"2026-08-11T16:14:56.683479Z","title":"Greig, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.683479Z"},"links":{"cited_paper":"/paper/2403.14060","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:72be2df5899373e97aada214db6fa7c54e0caf088fb657ce27faabb82084e8e0","observation_id":"c74bcab5-e03b-4e3a-9b33-a7a9c1982e79","resolution":{"observed_at":"2026-08-11T16:14:56.683479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.14061","last_updated":"2024-03-21T01:11:55Z","snapshot_observed_at":"2026-07-06T17:48:03.807374Z","submitted_at":"2024-03-21T01:11:55Z","title":"Exploring the role of the halo mass function for inferring astrophysical parameters during reionisation","version":1},"cited_work":{"arxiv_id":"2403.14061","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.14061","snapshot_observed_at":"2026-08-11T16:14:57.517432Z","title":"Exploring the role of the halo mass function for inferring astrophysical parameters during reionisation","venue":"astro-ph.CO","work_id":"d783a892-f2f8-4411-92e9-9678bcfa4156","year":2024},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.687672Z"},"links":{"cited_paper":"/paper/2403.14061","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:6b5b56613700e2c6414cdc2b83fb72aa853a05d86d701a6755f2c238fea453ae","observation_id":"b6d50138-6bb2-43a3-95dd-75af7b48f801","resolution":{"observed_at":"2026-08-11T16:14:57.521827Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0102304","last_updated":"2001-05-21T14:52:29Z","snapshot_observed_at":"2026-08-03T15:20:24.720874Z","submitted_at":"2001-02-18T03:01:35Z","title":"Constraints on Warm Dark Matter from Cosmological Reionization","version":2},"cited_work":{"arxiv_id":"astro-ph/0102304","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0102304","snapshot_observed_at":"2026-08-11T16:14:57.499801Z","title":"Constraints on Warm Dark Matter from Cosmological Reionization","venue":"astro-ph","work_id":"7794e316-2db9-413e-8573-9751681172d1","year":2001},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.691835Z"},"links":{"cited_paper":"/paper/astro-ph/0102304","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:781a13ec72e51befa0bd5d1b2d1080819be53cb07bd936be1f06e07930009fa5","observation_id":"2b207b04-0e16-4b4a-a5e9-2987dfaaeffa","resolution":{"observed_at":"2026-08-11T16:14:57.504363Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.0839","last_updated":"2013-06-11T10:21:04Z","snapshot_observed_at":"2026-07-06T03:07:57.150020Z","submitted_at":"2013-03-04T21:00:02Z","title":"Halo Mass Function and the Free Streaming Scale","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.0839","snapshot_observed_at":"2026-08-11T16:14:56.695835Z","title":"Schneider, R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.695835Z"},"links":{"cited_paper":"/paper/1303.0839","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:5069f67dcf389d5cfcfbc927a7d1c342b12f23a210cb4b537ba07d8596b41492","observation_id":"daa0b91a-b3f1-4e6e-b765-af31e80f1ab9","resolution":{"observed_at":"2026-08-11T16:14:56.695835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.3018","last_updated":"2012-10-07T19:50:26Z","snapshot_observed_at":"2026-07-06T02:55:35.722107Z","submitted_at":"2012-09-13T20:00:03Z","title":"Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.3018","snapshot_observed_at":"2026-08-11T16:14:56.699957Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.699957Z"},"links":{"cited_paper":"/paper/1209.3018","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:ef64faf88ef4c3b897cdff7efb7d8b8c7d7138f5ab5ee0349894d9bdccdf7c6b","observation_id":"d1ee7594-6c8c-498c-8ba1-594f08d3b3be","resolution":{"observed_at":"2026-08-11T16:14:56.699957Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.02302","last_updated":"2018-04-23T11:21:10Z","snapshot_observed_at":"2026-07-06T05:32:41.054089Z","submitted_at":"2017-03-07T10:04:28Z","title":"Warm dark matter and the ionization history of the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.02302","snapshot_observed_at":"2026-08-11T16:14:56.704421Z","title":"Lopez-Honorez, O","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.704421Z"},"links":{"cited_paper":"/paper/1703.02302","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:7b8afdabe6998c107ad1e53b847627ddeba337f16ff5577e31fa469871b36482","observation_id":"4f978153-9d72-4612-bc8a-5094b3ab6193","resolution":{"observed_at":"2026-08-11T16:14:56.704421Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.09073","last_updated":"2020-04-06T16:20:03Z","snapshot_observed_at":"2026-08-10T12:32:45.606346Z","submitted_at":"2019-11-20T18:17:57Z","title":"Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-$\\alpha$ and Planck full-survey data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.09073","snapshot_observed_at":"2026-08-11T16:14:56.708358Z","title":"Palanque-Delabrouille, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.708358Z"},"links":{"cited_paper":"/paper/1911.09073","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:7e651b31f86cd9036f0bff7000750ddcb1111ede7360ea3f56370f55383192b5","observation_id":"2a21ee2b-030a-4cc5-854e-9aa5185a063a","resolution":{"observed_at":"2026-08-11T16:14:56.708358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.01620","last_updated":"2024-05-02T17:50:31Z","snapshot_observed_at":"2026-08-04T00:50:28.394911Z","submitted_at":"2024-05-02T17:50:31Z","title":"JWST Lensed quasar dark matter survey II: Strongest gravitational lensing limit on the dark matter free streaming length to date","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.01620","snapshot_observed_at":"2026-08-11T16:14:56.711827Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.711827Z"},"links":{"cited_paper":"/paper/2405.01620","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:e017ec88dea72cba2a20332026029bf80d54bf66533257b027230aec2a66d894","observation_id":"8e337125-8061-446e-8f20-cbc1102e413c","resolution":{"observed_at":"2026-08-11T16:14:56.711827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.18917","last_updated":"2025-03-31T17:59:18Z","snapshot_observed_at":"2026-08-10T12:45:46.288252Z","submitted_at":"2024-09-27T17:04:09Z","title":"Mixed Warm Dark Matter Constraints using Milky Way Satellite Galaxy Counts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.18917","snapshot_observed_at":"2026-08-11T16:14:56.715416Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.715416Z"},"links":{"cited_paper":"/paper/2409.18917","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:6277d3325618336e7cb3530ec6bf3f3b2375e69cb42edee1d2a406be835595f7","observation_id":"a3fa9a56-1e56-494f-bb14-aced885effae","resolution":{"observed_at":"2026-08-11T16:14:56.715416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-11T16:14:56.718988Z","title":"Aghanim, Y","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.718988Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:d9d8612f9c56743a8476f50501770f1ec68899672e3d85666bca9eeae9fe2f43","observation_id":"c414061e-dddd-40f7-96d3-7cfb98849136","resolution":{"observed_at":"2026-08-11T16:14:56.718988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.08995","last_updated":"2019-01-23T14:33:04Z","snapshot_observed_at":"2026-08-09T15:33:15.158962Z","submitted_at":"2018-09-24T15:18:35Z","title":"Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.08995","snapshot_observed_at":"2026-08-11T16:14:56.722499Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.722499Z"},"links":{"cited_paper":"/paper/1809.08995","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:28165831c056ebb497ba1b507fc79174f1c179710c115451740a82af37622d57","observation_id":"85bda62c-2c49-4d21-999d-b0b1fa4eb58b","resolution":{"observed_at":"2026-08-11T16:14:56.722499Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.2413","last_updated":"2013-01-30T19:50:51Z","snapshot_observed_at":"2026-07-06T02:57:13.626734Z","submitted_at":"2012-10-08T20:28:40Z","title":"The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.2413","snapshot_observed_at":"2026-08-11T16:14:56.726678Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.726678Z"},"links":{"cited_paper":"/paper/1210.2413","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:8ecfc3efe8a1405039f47c0c920c46534c257ee9bc559235eb4e1c9220465850","observation_id":"b89614b8-6dff-4298-a576-2b172b745ccf","resolution":{"observed_at":"2026-08-11T16:14:56.726678Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.7031","last_updated":"2014-09-16T19:07:20Z","snapshot_observed_at":"2026-08-07T08:37:01.823613Z","submitted_at":"2013-10-25T20:01:24Z","title":"What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of Reionization","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.7031","snapshot_observed_at":"2026-08-11T16:14:56.731581Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.731581Z"},"links":{"cited_paper":"/paper/1310.7031","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:cb27884c749087bc8cb6e70e6f2dfc254e2e83032382f3f101b0a6de90568d82","observation_id":"89c80d73-fb38-48c9-b5ab-5ecaccc93c81","resolution":{"observed_at":"2026-08-11T16:14:56.731581Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0010468","last_updated":"2001-05-11T19:48:06Z","snapshot_observed_at":"2026-07-07T00:13:40.301989Z","submitted_at":"2000-10-24T02:14:57Z","title":"In the Beginning: The First Sources of Light and the Reionization of the Universe","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0010468","snapshot_observed_at":"2026-08-11T16:14:56.735602Z","title":"Barkana and A","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.735602Z"},"links":{"cited_paper":"/paper/astro-ph/0010468","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:0dda7ed7f8fd54978f8a9a76cfa2d47f922d721a6210bf165f720b9c95130810","observation_id":"30918ad7-225b-4245-b13b-747e054ae72f","resolution":{"observed_at":"2026-08-11T16:14:56.735602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.16828","last_updated":"2020-09-24T05:09:22Z","snapshot_observed_at":"2026-08-05T13:28:38.337108Z","submitted_at":"2020-06-30T14:05:39Z","title":"Reionization inference from the CMB optical depth and E-mode polarization power spectra","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.16828","snapshot_observed_at":"2026-08-11T16:14:56.739797Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.739797Z"},"links":{"cited_paper":"/paper/2006.16828","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:95e8e9b4e75785955357c319827870070783a580e5831ac60a7dbf81e84efdf0","observation_id":"9541a06b-b4ce-4cd5-a4bf-bb75ed3082dd","resolution":{"observed_at":"2026-08-11T16:14:56.739797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608032","last_updated":"2006-09-20T14:34:27Z","snapshot_observed_at":"2026-08-05T10:28:30.702983Z","submitted_at":"2006-08-01T20:02:05Z","title":"Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0608032","snapshot_observed_at":"2026-08-11T16:14:56.743718Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.743718Z"},"links":{"cited_paper":"/paper/astro-ph/0608032","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:f32cc9d3cffa99b94d9b43b1bab7d81e1ab27b38fc034c0fded7f9555491d212","observation_id":"b0b0a6b9-2384-49e8-b1ba-6a9970c612ba","resolution":{"observed_at":"2026-08-11T16:14:56.743718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.16571","last_updated":"2021-03-30T18:00:00Z","snapshot_observed_at":"2026-08-03T13:43:48.954362Z","submitted_at":"2021-03-30T18:00:00Z","title":"Galaxy Stellar Mass Functions from z~10 to z~6 using the Deepest Spitzer/IRAC Data: No Significant Evolution in the Stellar-to-Halo Mass Ratio of Galaxies in the First Gyr of Cosmic Time","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.16571","snapshot_observed_at":"2026-08-11T16:14:56.748176Z","title":"Stefanon, R","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.748176Z"},"links":{"cited_paper":"/paper/2103.16571","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:adbaa2fa48c7aa829ca3af1330b7f39c99579abe27949b553842d99e71406e62","observation_id":"265ff9eb-5c1b-41e3-a4d0-9c6e600a3dc7","resolution":{"observed_at":"2026-08-11T16:14:56.748176Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.10895","last_updated":"2022-08-05T11:52:14Z","snapshot_observed_at":"2026-08-06T14:26:46.233893Z","submitted_at":"2022-03-21T11:40:53Z","title":"COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.10895","snapshot_observed_at":"2026-08-11T16:14:56.752010Z","title":"Shuntov, H","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.752010Z"},"links":{"cited_paper":"/paper/2203.10895","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:aa5cda4d238d21974cd3208e486d3256aed4738a5a007ee667b814b4ef11cb13","observation_id":"2595794a-fd0d-456a-9a8c-d983f7a6c9ad","resolution":{"observed_at":"2026-08-11T16:14:56.752010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.04442","last_updated":"2020-05-13T21:12:11Z","snapshot_observed_at":"2026-07-06T09:03:28.399877Z","submitted_at":"2020-03-09T22:44:40Z","title":"A tale of two sites -- I: Inferring the properties of minihalo-hosted galaxies from current observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.04442","snapshot_observed_at":"2026-08-11T16:14:56.756041Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.756041Z"},"links":{"cited_paper":"/paper/2003.04442","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:a6159518168b58b022f9d0a8be751fa1332ffe0122cdbd5e688f22e7c76d87ee","observation_id":"c84e8693-9959-435f-b266-cc6c99c2e5e8","resolution":{"observed_at":"2026-08-11T16:14:56.756041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9907024","last_updated":"1999-07-02T09:23:48Z","snapshot_observed_at":"2026-07-07T01:27:04.258766Z","submitted_at":"1999-07-02T09:23:48Z","title":"Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9907024","snapshot_observed_at":"2026-08-11T16:14:56.759944Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.759944Z"},"links":{"cited_paper":"/paper/astro-ph/9907024","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:f846dd9b08fc7270f8f4fd2353c9f7d41ba1e3d6997f4dc6350425a6f0b3f25b","observation_id":"f0a28498-cc0d-4b42-957a-512a4316b7f9","resolution":{"observed_at":"2026-08-11T16:14:56.759944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.03586","last_updated":"2016-04-12T21:05:34Z","snapshot_observed_at":"2026-08-10T12:35:12.381048Z","submitted_at":"2016-04-12T21:05:34Z","title":"Late Pop III Star Formation During the Epoch of Reionization: Results from the Renaissance Simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.03586","snapshot_observed_at":"2026-08-11T16:14:56.763750Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.763750Z"},"links":{"cited_paper":"/paper/1604.03586","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:c0e2edd6dfadaa165b970145b661259b2d2631a34a22dddb557d326aac385570","observation_id":"dba8aa94-90e9-4d17-a751-f7f440795f0a","resolution":{"observed_at":"2026-08-11T16:14:56.763750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.6776","last_updated":"2013-01-28T21:23:31Z","snapshot_observed_at":"2026-07-06T03:05:06.660056Z","submitted_at":"2013-01-28T21:23:31Z","title":"The depletion of gas in high-redshift dwarf galaxies from an inhomogeneous reionization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.6776","snapshot_observed_at":"2026-08-11T16:14:56.768064Z","title":"Sobacchi and A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.768064Z"},"links":{"cited_paper":"/paper/1301.6776","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:f54c5c743faa5278562cbe5f8e819fe4b056afd2af4cecd8e2931e26f601d06d","observation_id":"cda20a42-cbeb-4141-904a-0be74e9aa0cd","resolution":{"observed_at":"2026-08-11T16:14:56.768064Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.01110","last_updated":"2015-06-12T10:41:52Z","snapshot_observed_at":"2026-07-06T04:10:55.883019Z","submitted_at":"2015-03-03T21:00:07Z","title":"Probing The Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.01110","snapshot_observed_at":"2026-08-11T16:14:56.776217Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.776217Z"},"links":{"cited_paper":"/paper/1503.01110","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:22e76adcca4a0ffa73f230a3bc7be3bcfe0e8a5999014d07b5958aa7b1b850b2","observation_id":"456302cf-6c92-48ca-9263-69f490c26c28","resolution":{"observed_at":"2026-08-11T16:14:56.776217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:14:56.780479Z","title":"Barkana and A","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.780479Z"},"links":{"citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:3e6d600c5299bb81d2c01985b57cf32a4961f6dbb034884d6277485b4d6dc933","observation_id":"cf11bfac-3fc0-45b4-a41e-88e294e7c0aa","resolution":{"observed_at":"2026-08-11T16:14:56.780479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.6781","last_updated":"2013-01-28T21:34:49Z","snapshot_observed_at":"2026-07-06T03:05:06.660056Z","submitted_at":"2013-01-28T21:34:49Z","title":"How does radiative feedback from a UV background impact reionization?","version":1},"cited_work":{"arxiv_id":"1301.6781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1301.6781","snapshot_observed_at":"2026-08-11T16:14:57.258132Z","title":"How does radiative feedback from a UV background impact reionization?","venue":"astro-ph.CO","work_id":"27b5ad4d-56a3-456b-8c4c-058d52f26d19","year":2013},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.784192Z"},"links":{"cited_paper":"/paper/1301.6781","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:da24fcb9c37e74df49b9f07e421d335bbee10eec8b80d8bb56474f408c0c772f","observation_id":"e38054ad-b3f3-4a2b-8da3-06d475dc5740","resolution":{"observed_at":"2026-08-11T16:14:57.262672Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.13919","last_updated":"2022-03-10T19:24:22Z","snapshot_observed_at":"2026-08-10T13:41:56.560122Z","submitted_at":"2021-10-26T18:00:00Z","title":"The Impact of the First Galaxies on Cosmic Dawn and Reionization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.13919","snapshot_observed_at":"2026-08-11T16:14:56.788205Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.788205Z"},"links":{"cited_paper":"/paper/2110.13919","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:0f62b0247462e347f2d7a5fd6e7eedd99e7311c7b41457c0fe96fcb96df33410","observation_id":"722a5807-92d7-46f2-ab50-717f15ecf7be","resolution":{"observed_at":"2026-08-11T16:14:56.788205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07282","last_updated":"2022-12-20T16:38:53Z","snapshot_observed_at":"2026-08-10T04:31:00.862009Z","submitted_at":"2021-08-16T18:00:07Z","title":"HERA Phase I Limits on the Cosmic 21-cm Signal: Constraints on Astrophysics and Cosmology During the Epoch of Reionization","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.07282","snapshot_observed_at":"2026-08-11T16:14:56.792075Z","title":"Abdurashidova et al., HERA Phase I Limits on the Cosmic 21 cm Signal: Constraints on Astrophysics and Cosmology during the Epoch of Reionization , Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.792075Z"},"links":{"cited_paper":"/paper/2108.07282","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:631802c9cddc947db489d8146f9f7e853b8cf894777eb7decac83815795aeaf9","observation_id":"3fb6c228-89f5-4114-b9aa-765354501f43","resolution":{"observed_at":"2026-08-11T16:14:56.792075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0501562","last_updated":"2005-04-01T11:30:12Z","snapshot_observed_at":"2026-07-07T00:47:49.541205Z","submitted_at":"2005-01-26T14:49:17Z","title":"Constraining Warm Dark Matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0501562","snapshot_observed_at":"2026-08-11T16:14:56.795751Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.795751Z"},"links":{"cited_paper":"/paper/astro-ph/0501562","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:3dac694621267c64993cbcf93307ed0c47c56aa0b7b3b36696d2320bea6e4be2","observation_id":"018de219-2a90-4fc8-8275-9aceed4c5698","resolution":{"observed_at":"2026-08-11T16:14:56.795751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0010389","last_updated":"2001-05-29T13:43:10Z","snapshot_observed_at":"2026-07-07T00:13:35.834290Z","submitted_at":"2000-10-19T20:05:39Z","title":"Halo Formation in Warm Dark Matter Models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0010389","snapshot_observed_at":"2026-08-11T16:14:56.800346Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.800346Z"},"links":{"cited_paper":"/paper/astro-ph/0010389","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:fded7eb014ad67be764e2a088f7cfe5d51673559d97af9fcc6f2c8bbfeae07e5","observation_id":"c7ec1893-c329-4539-a2a5-4b7593adcf13","resolution":{"observed_at":"2026-08-11T16:14:56.800346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.09321","last_updated":"2022-03-23T10:28:32Z","snapshot_observed_at":"2026-08-09T03:01:12.238792Z","submitted_at":"2021-11-17T19:00:01Z","title":"Lyman-$\\alpha$ constraints on freeze-in and superWIMPs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.09321","snapshot_observed_at":"2026-08-11T16:14:56.804189Z","title":"Decant, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.804189Z"},"links":{"cited_paper":"/paper/2111.09321","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:2bca61334dbdd60d3a21dbe63b3f79a91e9ce3d809d4fa9300c7b776415762fd","observation_id":"9152451c-9821-4698-82b8-5cead11f20dd","resolution":{"observed_at":"2026-08-11T16:14:56.804189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005260","last_updated":"2000-09-25T14:18:33Z","snapshot_observed_at":"2026-07-07T00:11:18.128450Z","submitted_at":"2000-05-12T15:41:05Z","title":"Mass function of dark matter halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005260","snapshot_observed_at":"2026-08-11T16:14:56.808135Z","title":"Jenkins, C","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.808135Z"},"links":{"cited_paper":"/paper/astro-ph/0005260","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:3209a636e7c0195fdade04cf06397ae1fd33f92de5f5530af2e24bfb11efd11a","observation_id":"d16f86f5-7d1f-4ad4-b411-17d649e65371","resolution":{"observed_at":"2026-08-11T16:14:56.808135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9901122","last_updated":"1999-01-13T09:30:56Z","snapshot_observed_at":"2026-07-07T01:23:56.519140Z","submitted_at":"1999-01-11T13:50:02Z","title":"Large scale bias and the peak background split","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9901122","snapshot_observed_at":"2026-08-11T16:14:56.813412Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.813412Z"},"links":{"cited_paper":"/paper/astro-ph/9901122","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:0e31508757e7e9750c50a08b97dc804dc4d9822e7c5ac8f80b7ebe8f94894584","observation_id":"d0c98e5a-656e-48e3-8ac9-a77b9f64eb54","resolution":{"observed_at":"2026-08-11T16:14:56.813412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.2133","last_updated":"2015-04-10T10:36:46Z","snapshot_observed_at":"2026-07-06T04:02:46.798336Z","submitted_at":"2014-12-05T21:00:05Z","title":"Structure formation with suppressed small-scale perturbations","version":2},"cited_work":{"arxiv_id":"1412.2133","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.2133","snapshot_observed_at":"2026-08-11T16:14:57.149673Z","title":"Structure formation with suppressed small-scale perturbations","venue":"astro-ph.CO","work_id":"72143a40-f8af-4eec-afd6-e62b627212bc","year":2014},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.817856Z"},"links":{"cited_paper":"/paper/1412.2133","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:83ed7e33c40ffb471f2dab0075b13024f189e907a74e3c196a176ce3f194511a","observation_id":"24539fa9-d29a-403d-a986-3fe9a78f4c8e","resolution":{"observed_at":"2026-08-11T16:14:57.153545Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1403.6125","last_updated":"2014-06-20T12:41:40Z","snapshot_observed_at":"2026-07-06T03:39:19.222383Z","submitted_at":"2014-03-24T20:00:22Z","title":"The X-ray spectra of the first galaxies: 21cm signatures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.6125","snapshot_observed_at":"2026-08-11T16:14:56.822106Z","title":"Pacucci, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.822106Z"},"links":{"cited_paper":"/paper/1403.6125","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:f2fb21b17d7dfd1605d4a29af147be94c61edfa8d78da328ed041c18026bb85f","observation_id":"eb6a9949-29de-48ed-bce8-fc916aaa1ecf","resolution":{"observed_at":"2026-08-11T16:14:56.822106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.03471","last_updated":"2018-02-28T06:07:39Z","snapshot_observed_at":"2026-08-10T10:21:07.184985Z","submitted_at":"2017-05-09T18:00:06Z","title":"Simultaneously constraining the astrophysics of reionisation and the epoch of heating with 21CMMC","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.03471","snapshot_observed_at":"2026-08-11T16:14:56.826584Z","title":"Greig and A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.826584Z"},"links":{"cited_paper":"/paper/1705.03471","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:dc9ff1017e3c876f06be566abe9066661d543203255e20727ac863bf0366e567","observation_id":"d440e7b8-ef0a-4788-85fa-075815a75b2a","resolution":{"observed_at":"2026-08-11T16:14:56.826584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:14:56.830989Z","title":"Mirocha, S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.830989Z"},"links":{"citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:d14b56d3581469935ef1b77159f0cf5b691a602e05037b2b60e67bd0a06b7792","observation_id":"fc9a4270-0af8-4254-8fa1-f0dbfc24a8f9","resolution":{"observed_at":"2026-08-11T16:14:56.830989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.07775","last_updated":"2021-02-15T19:00:00Z","snapshot_observed_at":"2026-07-06T10:41:34.776588Z","submitted_at":"2021-02-15T19:00:00Z","title":"New Determinations of the UV Luminosity Functions from z~9 to z~2 show a remarkable consistency with halo growth and a constant star formation efficiency","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.07775","snapshot_observed_at":"2026-08-11T16:14:56.835261Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.835261Z"},"links":{"cited_paper":"/paper/2102.07775","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:f450dd37bb2b6d758748f5aa1e478a61c76bb9b11d8a7cc6f788004b846a4803","observation_id":"2a0a1e95-0b6e-49d0-b23f-cb501ba48552","resolution":{"observed_at":"2026-08-11T16:14:56.835261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.01245","last_updated":"2021-01-03T21:39:44Z","snapshot_observed_at":"2026-08-07T05:13:22.477503Z","submitted_at":"2020-09-02T18:00:01Z","title":"First Constraints on Small-Scale Non-Gaussianity from UV Galaxy Luminosity Functions","version":2},"cited_work":{"arxiv_id":"2009.01245","doi":null,"metadata_source":"pith","pith_arxiv_id":"2009.01245","snapshot_observed_at":"2026-08-11T16:14:57.097251Z","title":"First Constraints on Small-Scale Non-Gaussianity from UV Galaxy Luminosity Functions","venue":"astro-ph.CO","work_id":"ec5a44df-0bb2-4cca-a4be-695325ea1569","year":2020},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.839467Z"},"links":{"cited_paper":"/paper/2009.01245","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:bf5e01b4bf26bb19d50ea0e5687bba273ab5642b171dd9e5a05229d58262098b","observation_id":"87603f7f-f262-479d-93a2-9d573e2e64f1","resolution":{"observed_at":"2026-08-11T16:14:57.101453Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1606.07473","last_updated":"2016-09-13T00:38:50Z","snapshot_observed_at":"2026-08-04T17:53:43.597487Z","submitted_at":"2016-06-23T20:54:28Z","title":"Hydrogen Epoch of Reionization Array (HERA)","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.07473","snapshot_observed_at":"2026-08-11T16:14:56.843731Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.843731Z"},"links":{"cited_paper":"/paper/1606.07473","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:8000978cd13fc3a9a4c29adcbb11380f939ecc2e078137f2fa35a2304f3d2600","observation_id":"e94584df-c7e8-4ccc-a205-434d4ff13b37","resolution":{"observed_at":"2026-08-11T16:14:56.843731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:14:56.848463Z","title":null,"venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.848463Z"},"links":{"citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:544a84a860942a38245c708019c9e3e18768e1135f6da7ca04cf4357bae0b782","observation_id":"3452e528-f6ca-4e32-b8df-dfc5b62da0f3","resolution":{"observed_at":"2026-08-11T16:14:56.848463Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.15256","last_updated":"2023-10-23T18:05:32Z","snapshot_observed_at":"2026-08-10T11:03:12.970916Z","submitted_at":"2023-10-23T18:05:32Z","title":"SimBIG: Field-level Simulation-Based Inference of Galaxy Clustering","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.15256","snapshot_observed_at":"2026-08-11T16:14:56.852265Z","title":"Lemos, L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.852265Z"},"links":{"cited_paper":"/paper/2310.15256","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:83886789267ff2ebec026689511da50308f40d8123cb8cd7c21142f5b8d8ff07","observation_id":"6a0cea1f-32e4-4284-af9f-6388dd78e372","resolution":{"observed_at":"2026-08-11T16:14:56.852265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:14:56.856546Z","title":"Bhardwaj, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.856546Z"},"links":{"citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:a19336b1f646fc97385fa725b68ef5377931e611586ed1a23e942e8d8bf71dbb","observation_id":"59146b44-596d-4009-8ac3-ec6a1f2d074f","resolution":{"observed_at":"2026-08-11T16:14:56.856546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07954","last_updated":"2024-07-02T07:37:14Z","snapshot_observed_at":"2026-08-04T03:45:38.223520Z","submitted_at":"2023-09-14T18:00:01Z","title":"Simulation-based inference for stochastic gravitational wave background data analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07954","snapshot_observed_at":"2026-08-11T16:14:56.860307Z","title":"Alvey, U","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.860307Z"},"links":{"cited_paper":"/paper/2309.07954","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:94fd693de9f6734ab41204765957e3991039d1d535ce27531970607df0ad42e2","observation_id":"d26502ec-784f-42f5-a8c9-23f81785bffe","resolution":{"observed_at":"2026-08-11T16:14:56.860307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.14618","last_updated":"2025-06-12T19:28:07Z","snapshot_observed_at":"2026-08-09T16:39:14.263765Z","submitted_at":"2024-03-21T17:59:10Z","title":"Simulation-Based Inference of the sky-averaged 21-cm signal from CD-EoR with REACH","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.14618","snapshot_observed_at":"2026-08-11T16:14:56.864353Z","title":"Saxena, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.864353Z"},"links":{"cited_paper":"/paper/2403.14618","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:9845a45d973a7a93f0fdebccc838759747abf97e25dddd92a982003c6052670c","observation_id":"c041f4f8-cd78-4cbe-bdef-68950885f310","resolution":{"observed_at":"2026-08-11T16:14:56.864353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.11373","last_updated":"2024-12-03T11:03:28Z","snapshot_observed_at":"2026-08-05T17:00:42.667900Z","submitted_at":"2024-04-17T13:31:51Z","title":"Simulation-based inference of black hole ringdowns in the time domain","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.11373","snapshot_observed_at":"2026-08-11T16:14:56.868433Z","title":"Pacilio, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.868433Z"},"links":{"cited_paper":"/paper/2404.11373","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:a8dccd5a8e937828c607d1edbfd674b8bdfbf3d7322cc8c1983be90664c35bb0","observation_id":"3badf4b8-0bfe-4ae2-907e-7e3d077cf4c6","resolution":{"observed_at":"2026-08-11T16:14:56.868433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.02652","last_updated":"2024-09-24T14:10:13Z","snapshot_observed_at":"2026-07-06T15:23:10.114682Z","submitted_at":"2023-05-04T08:45:51Z","title":"Angular power spectrum of gravitational-wave transient sources as a probe of the large-scale structure","version":2},"cited_work":{"arxiv_id":"2305.02652","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.02652","snapshot_observed_at":"2026-08-11T16:14:57.020116Z","title":"Angular power spectrum of gravitational-wave transient sources as a probe of the large-scale structure","venue":"astro-ph.CO","work_id":"9cdf497d-0491-42c6-af63-c1fbcf8ca5cc","year":2023},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.872489Z"},"links":{"cited_paper":"/paper/2305.02652","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:a967eaa9eaa530c3b350426282846b47ea6f444403339e4ecfdaec0611178652","observation_id":"7bf96465-c1ed-416c-9c61-05cf9a0b6719","resolution":{"observed_at":"2026-08-11T16:14:57.024607Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:14:56.876034Z","title":"Stachurski, C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.876034Z"},"links":{"citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:b786d7d17c5022543e9d5e606de4a8c9d0491bd705dcb3ecdb93760fb08ec00e","observation_id":"7403f7ef-046a-4d80-a127-f173d784fe63","resolution":{"observed_at":"2026-08-11T16:14:56.876034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:14:57.960060Z","title":null,"venue":null,"work_id":"ecb7642f-a7d8-4075-a570-949f0c8441b5","year":2024},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.879452Z"},"links":{"citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:66affd6008d8ac4a028733c5c75e92dadd405c1ce1689ecb12a063b559e1c25c","observation_id":"7105ee2c-3225-496c-87eb-9fea4e555d36","resolution":{"observed_at":"2026-08-11T16:14:57.964921Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.13951","last_updated":"2020-11-27T19:00:07Z","snapshot_observed_at":"2026-08-11T11:13:54.680527Z","submitted_at":"2020-11-27T19:00:07Z","title":"Simulation-efficient marginal posterior estimation with swyft: stop wasting your precious time","version":1},"cited_work":{"arxiv_id":"2011.13951","doi":null,"metadata_source":"pith","pith_arxiv_id":"2011.13951","snapshot_observed_at":"2026-08-11T16:14:57.000115Z","title":"Simulation-efficient marginal posterior estimation with swyft: stop wasting your precious time","venue":"astro-ph.IM","work_id":"ad1e3859-2b7e-4956-bcac-db8f4a5ccfbc","year":2020},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.882843Z"},"links":{"cited_paper":"/paper/2011.13951","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:9e5d6f8a59b9e25fa82cd74a48ebbaa421dd209bb35d5dd57592572be2bb08fd","observation_id":"2521370e-8924-485b-89b0-e0a150cc2fff","resolution":{"observed_at":"2026-08-11T16:14:57.006794Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:14:57.947766Z","title":null,"venue":null,"work_id":"47718e6c-24b4-442d-b2cf-5c85c596db2f","year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.886524Z"},"links":{"citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:0c3b4c8f0073622bb9d449fc647425ee77517f2337b0aedfcdc0b9f8ecbe1ed6","observation_id":"31838d40-7d7f-412c-a0b2-f56bf7dae681","resolution":{"observed_at":"2026-08-11T16:14:57.951728Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.06581","last_updated":"2022-12-04T19:18:32Z","snapshot_observed_at":"2026-07-06T11:57:21.548494Z","submitted_at":"2021-10-13T08:50:05Z","title":"A Trust Crisis In Simulation-Based Inference? Your Posterior Approximations Can Be Unfaithful","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.06581","snapshot_observed_at":"2026-08-11T16:14:56.889828Z","title":"Hermans, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.889828Z"},"links":{"cited_paper":"/paper/2110.06581","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:0df2a1cb9a9fe405f4cfc7de18fbd184c96536aa2a755b15ed67ddd5556a7589","observation_id":"8710f681-d50f-4b74-9e09-2d37e76bab3e","resolution":{"observed_at":"2026-08-11T16:14:56.889828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.6980","last_updated":"2017-01-30T01:27:54Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2014-12-22T13:54:29Z","title":"Adam: A Method for Stochastic Optimization","version":9},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.6980","snapshot_observed_at":"2026-08-11T16:14:56.893414Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.893414Z"},"links":{"cited_paper":"/paper/1412.6980","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:3ac9dfe9c6427e16f6c3da0e751f8d4392d772defcf152801c059de774a1d1d1","observation_id":"70400d83-3450-46a3-a659-569f954fceaf","resolution":{"observed_at":"2026-08-11T16:14:56.893414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01214","last_updated":"2021-10-26T08:19:44Z","snapshot_observed_at":"2026-07-06T11:25:32.650351Z","submitted_at":"2021-07-02T18:00:03Z","title":"Truncated Marginal Neural Ratio Estimation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.01214","snapshot_observed_at":"2026-08-11T16:14:56.897371Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.897371Z"},"links":{"cited_paper":"/paper/2107.01214","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:68b8d1d974b3fe23bb35827921934655b034c8efe0c70e998fd17c622e7aa701","observation_id":"01bc1c05-a86a-4cd2-b563-b38ecf8b1e5a","resolution":{"observed_at":"2026-08-11T16:14:56.897371Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.7319","last_updated":"2013-04-17T16:32:47Z","snapshot_observed_at":"2026-08-04T08:31:25.108034Z","submitted_at":"2012-10-27T13:20:28Z","title":"Signatures of X-rays in the early Universe","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.7319","snapshot_observed_at":"2026-08-11T16:14:56.901503Z","title":"Mesinger, A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.901503Z"},"links":{"cited_paper":"/paper/1210.7319","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:5aa75a0b5d45e9e40e7444e9b458aff6c54aedd0c3593aad98384061a8bb4b05","observation_id":"e7119ae8-f54f-4f5a-b75f-cc41e5124521","resolution":{"observed_at":"2026-08-11T16:14:56.901503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.08030","last_updated":"2022-11-08T15:38:25Z","snapshot_observed_at":"2026-08-04T06:47:23.182797Z","submitted_at":"2021-11-15T19:00:09Z","title":"Fast and Credible Likelihood-Free Cosmology with Truncated Marginal Neural Ratio Estimation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.08030","snapshot_observed_at":"2026-08-11T16:14:56.906189Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.906189Z"},"links":{"cited_paper":"/paper/2111.08030","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:75483c74828d0f5900e5b3efa15314a40bb62f83a3da52e9c6f38c4fd98f9746","observation_id":"82b53db2-8010-421b-b5e0-8144d957c33b","resolution":{"observed_at":"2026-08-11T16:14:56.906189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts"},"reference_resolution":{"displayed":85,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":69,"verified_exact":16,"verified_fuzzy":0},"total_outbound_references":85},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 85 of 85 outbound references and 1 inbound Pith citation observation for arXiv:2412.10310."}