{"as_of":"2026-08-17T07:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2f0891638439cd710621ec64b10a4c605ce71a5ca01b30cd4d41e27912a8e098","coverage":[{"denominator":50,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":50,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T17:11:48.226005Z","state":"measured"},{"denominator":50,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":50,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"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":[],"links":{"evidence":"/evidence","html":"/paper/2508.17059/citation-record","integrity":"/paper/2508.17059/integrity","json":"/paper/2508.17059/citation-record.json","paper":"/paper/2508.17059"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:11:49.137668Z","title":null,"venue":null,"work_id":"de46e5fd-2b78-4774-8fd5-c260e3925ab3","year":null},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.870804Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:14a834d128e2d15c972403927f99154ce4d36d8187605a298dcf98c4255fd7f4","observation_id":"d2cc59af-eccc-439b-a05c-145f5e4ff4e0","resolution":{"observed_at":"2026-08-15T17:11:49.143603Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:49.115211Z","title":null,"venue":null,"work_id":"de186e54-8c98-49ab-ba85-072a32c65a01","year":null},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.875723Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:769f60cdf51f6e546ddd6387410a4958f8180091a779f808291dd1c82ea32617","observation_id":"e18718df-d191-4b2d-a1da-a00b4059cfd2","resolution":{"observed_at":"2026-08-15T17:11:49.124700Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:49.097764Z","title":"One is the standard exponential cutoff: Sreg(t) =S(t)e−ε|t|, (28) whereS(t) is the original entropy","venue":null,"work_id":"33ff0784-1ee4-4962-a2c1-c2c734f745ce","year":null},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.880530Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:6526a3844c9b093d453b957a5b53cf7f13b58c7fe4271b76072ec457d7469f6c","observation_id":"9f446eb9-ac0c-4a1d-9592-51ac589b68db","resolution":{"observed_at":"2026-08-15T17:11:49.104153Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:49.082765Z","title":"Constant entanglement, as with constant velocity mo- tion, produces no energy and no particles, in agreement with the total stress-energy, Eq","venue":null,"work_id":"8fb6a18e-0ebe-415f-a874-1726a89fafd8","year":null},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.884741Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:f62e8a0ef2d61f08809af60cab875933d1adcebb3b66d63980f16643d7f4df03","observation_id":"3fc9b5e7-f484-462c-a647-f2511266d572","resolution":{"observed_at":"2026-08-15T17:11:49.088481Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:49.065623Z","title":null,"venue":null,"work_id":"6751999b-3bef-4a50-9b54-2e9da18cad7f","year":null},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.889203Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:15a6e61a8604ccc51e1600ab106a5e610f544b9a04dc0d7ea2963a521668020e","observation_id":"b6f39312-5d82-45b9-a26e-f82aa7eb4553","resolution":{"observed_at":"2026-08-15T17:11:49.070874Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:49.049111Z","title":null,"venue":null,"work_id":"7190a64d-db4c-4b69-8ac2-56b709f84733","year":null},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.893589Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:b1274e793c63ab38ded666cc483f75232a849ddb910950196bc48ae7976f228d","observation_id":"139df2c6-d071-4f69-96e2-d53bdaa44f33","resolution":{"observed_at":"2026-08-15T17:11:49.055575Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:49.035580Z","title":"it from bit,","venue":null,"work_id":"e7f03297-b82b-4461-bb1f-9ef869a2d7a7","year":null},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.898625Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:22ee5f356847aa3b955741849351ad4b88260ad6bdcc1ee86d40b5375c83fe06","observation_id":"9c10d443-d30e-4188-bc1b-66d71c508fa1","resolution":{"observed_at":"2026-08-15T17:11:49.040413Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:47.903673Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.903673Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:b2f44d0fb0493a596f74049fb06c28720b70aba0401ec6083cff1550d2920954","observation_id":"4afb29be-e3fb-4efd-9717-d96d0c090a95","resolution":{"observed_at":"2026-08-15T17:11:47.903673Z","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":"2026-08-15T17:11:49.014055Z","title":"Hawking, Particle Creation by Black Holes, Commun","venue":null,"work_id":"d2ed4562-d566-478e-8198-ea41ba1a4621","year":1975},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.907765Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:255be871fc399f836c97ca581f456202c71d8234be32fcdb13684f58e5e2ed0b","observation_id":"c2a02b84-f391-4115-8280-a2760e88098d","resolution":{"observed_at":"2026-08-15T17:11:49.017943Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:49.001247Z","title":null,"venue":null,"work_id":"f3faec67-e9b5-4d64-a4f6-6e59294f0d42","year":1975},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.911901Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:5b3f56f14a20f6e857ff5d2878d6ad56bbad1da5e0662ffb7e565ac2bb1de2dc","observation_id":"6962e81c-0eb0-4999-96d0-9e29da13850c","resolution":{"observed_at":"2026-08-15T17:11:49.005724Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:47.916548Z","title":null,"venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.916548Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:f5aa3abe3038a51e91b67856da77b9ec9b37089a888146d4f06a52422dbaf000","observation_id":"416cfc3d-fd00-4811-86d7-2e14a65bccd9","resolution":{"observed_at":"2026-08-15T17:11:47.916548Z","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":"2026-08-15T17:11:48.979844Z","title":null,"venue":null,"work_id":"5841432f-748e-4bb2-be41-4d526b9a1362","year":1975},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.920286Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:8de8fb16db790fbfecb9601518b09495b1c1f573999664b41b62f23782b09d60","observation_id":"81dff4ff-f8c9-46e8-ba1c-43a400f4c53f","resolution":{"observed_at":"2026-08-15T17:11:48.984446Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:48.966104Z","title":null,"venue":null,"work_id":"d5230a23-0486-42c9-9439-da06850ec51d","year":1973},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.924535Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:1b038b62f57e4442b4d0bf8708e4247e52f3e6ac438c061aac81435dd9cba0df","observation_id":"84a12b14-d063-43cb-a2e5-37c68a736200","resolution":{"observed_at":"2026-08-15T17:11:48.970397Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:48.952176Z","title":null,"venue":null,"work_id":"2a88de05-62c9-4abc-a25c-b7d9c8cbab96","year":1976},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.928880Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:eb31b98cc0f2416ce0b91de59705b294d6be2a4d80cf78e6d8ed4df11a9f93c3","observation_id":"3585c4ca-6e16-46c2-a881-2fd8dc3908a9","resolution":{"observed_at":"2026-08-15T17:11:48.957340Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:48.940915Z","title":"Davies and S","venue":null,"work_id":"bc6c210c-cc2b-4a05-921a-da801cd0cfc1","year":1977},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.933588Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:655727c11170d678001f75a808b263df5d67a9b61872cb07f0949309e563afd6","observation_id":"cae4f681-df68-49b5-9cb3-8010349feba3","resolution":{"observed_at":"2026-08-15T17:11:48.944658Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07747","last_updated":"2022-06-10T19:58:21Z","snapshot_observed_at":"2026-08-16T18:02:41.602166Z","submitted_at":"2021-08-17T16:37:28Z","title":"Nonlinear dynamical Casimir effect at weak nonstationarity","version":4},"cited_work":{"arxiv_id":"2108.07747","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.07747","snapshot_observed_at":"2026-08-15T17:11:48.833730Z","title":"Nonlinear dynamical Casimir effect at weak nonstationarity","venue":"hep-th","work_id":"b0d4387d-07fd-48be-99aa-727b0f8ea3e0","year":2021},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.937675Z"},"links":{"cited_paper":"/paper/2108.07747","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:afe262c4d01c2d02c3c45ad8a4ec006c7081124fc894654c29213c76247055ce","observation_id":"2f7727fb-a72d-49f9-ad32-dc43e6e5f4d1","resolution":{"observed_at":"2026-08-15T17:11:48.838793Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.03129","last_updated":"2023-08-06T14:41:38Z","snapshot_observed_at":"2026-08-16T15:10:28.929656Z","submitted_at":"2023-08-06T14:41:38Z","title":"Optomechanical Backreaction of Quantum Field Processes in Dynamical Casimir Effect","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.03129","snapshot_observed_at":"2026-08-15T17:11:47.941857Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.941857Z"},"links":{"cited_paper":"/paper/2308.03129","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:f7e0b5c20bac13f309b53c96afcfde16e1237ec413f18cc14b2711ae7f97fc87","observation_id":"521aadec-485a-447e-99e8-68543d2d2c7b","resolution":{"observed_at":"2026-08-15T17:11:47.941857Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.06996","last_updated":"2025-06-09T21:10:14Z","snapshot_observed_at":"2026-08-16T13:00:22.797226Z","submitted_at":"2024-12-09T21:05:28Z","title":"Searching for the classical version of Hawking radiation and screening of Coulomb field by the horizon","version":2},"cited_work":{"arxiv_id":"2412.06996","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.06996","snapshot_observed_at":"2026-08-15T17:11:48.803567Z","title":"Searching for the classical version of Hawking radiation and screening of Coulomb field by the horizon","venue":"gr-qc","work_id":"060c8252-67b3-48d2-acc0-a5baecd11e8d","year":2024},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:47.947630Z"},"links":{"cited_paper":"/paper/2412.06996","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:d5eb82a2f0ab1e064e5ca187aa09d607986a2a2d65bc89e2807f805e693923fb","observation_id":"4a515806-926c-445f-8d40-13cb47a1650c","resolution":{"observed_at":"2026-08-15T17:11:48.808527Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.16244","last_updated":"2024-12-20T16:38:42Z","snapshot_observed_at":"2026-08-16T14:39:54.640716Z","submitted_at":"2023-11-27T19:00:22Z","title":"Black Holes, Cavities and Blinking Islands","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.16244","snapshot_observed_at":"2026-08-15T17:11:48.088797Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.088797Z"},"links":{"cited_paper":"/paper/2311.16244","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:524ab025588a80c2733aa9a0dd4f38b6be314c914e1231fdab6d4610a27c7b61","observation_id":"f1cdb9fe-87e3-43b4-8087-94aad6be1934","resolution":{"observed_at":"2026-08-15T17:11:48.088797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.08357","last_updated":"2023-06-14T08:48:51Z","snapshot_observed_at":"2026-08-17T05:01:20.469823Z","submitted_at":"2023-06-14T08:48:51Z","title":"Entanglement area law violation from field-curvature coupling","version":1},"cited_work":{"arxiv_id":"2306.08357","doi":null,"metadata_source":"pith","pith_arxiv_id":"2306.08357","snapshot_observed_at":"2026-08-15T17:11:48.772007Z","title":"Entanglement area law violation from field-curvature coupling","venue":"gr-qc","work_id":"75f58079-cdcb-4479-bddc-ad44f5ce36dc","year":2023},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.094161Z"},"links":{"cited_paper":"/paper/2306.08357","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:4ff6ee009f040c027262125b6ceddf4b0693a631498a9d826835dbe1689a38b0","observation_id":"45052d8d-b06d-42de-baf0-3414cb03e225","resolution":{"observed_at":"2026-08-15T17:11:48.776367Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.04094","last_updated":"2022-06-08T18:01:05Z","snapshot_observed_at":"2026-08-16T16:54:22.430011Z","submitted_at":"2022-06-08T18:01:05Z","title":"Thermal density matrix breaks down the Page curve","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.04094","snapshot_observed_at":"2026-08-15T17:11:48.098568Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.098568Z"},"links":{"cited_paper":"/paper/2206.04094","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:8ff25dd6bd6c24359ec24c7c097730eeb721ffaaff3a8733767c1e8d7b8e15cf","observation_id":"a5d36605-ca33-457e-83ae-3d8b0662766e","resolution":{"observed_at":"2026-08-15T17:11:48.098568Z","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":"2502.14797","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:11:48.730584Z","title":"Belfiglio, O","venue":null,"work_id":"7db25427-00fe-478c-83f6-4955c940dc5f","year":2025},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.103217Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:9c6376641f2ed008be11a37823c93de7ad91638d95427c959a91866037339863","observation_id":"63966ec0-ca65-497c-bae1-d93bee34e487","resolution":{"observed_at":"2026-08-15T17:11:48.739447Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.14642","last_updated":"2025-07-28T20:48:15Z","snapshot_observed_at":"2026-08-16T15:45:19.449974Z","submitted_at":"2023-03-26T06:51:29Z","title":"Experimental observation of a Rindler horizon","version":3},"cited_work":{"arxiv_id":"2303.14642","doi":null,"metadata_source":"pith","pith_arxiv_id":"2303.14642","snapshot_observed_at":"2026-08-15T17:11:48.659537Z","title":"Experimental observation of a Rindler horizon","venue":"hep-ph","work_id":"7f12a883-a5e7-4ffe-a37e-91dd56d7e6e4","year":2023},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.107146Z"},"links":{"cited_paper":"/paper/2303.14642","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:8ced6ff6d4d4b2a26d55afbe491f913c66ded054136f14ab6f7db6fb66f41f76","observation_id":"fda2d157-a147-4dde-afef-1a146ed8ff88","resolution":{"observed_at":"2026-08-15T17:11:48.664122Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.09446","last_updated":"2024-04-15T04:17:57Z","snapshot_observed_at":"2026-08-16T14:00:59.620986Z","submitted_at":"2024-04-15T04:17:57Z","title":"The final burst of the moving mirror is unrelated to the partner mode of analog Hawking radiation","version":1},"cited_work":{"arxiv_id":"2404.09446","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.09446","snapshot_observed_at":"2026-08-15T17:11:48.641680Z","title":"The final burst of the moving mirror is unrelated to the partner mode of analog Hawking radiation","venue":"gr-qc","work_id":"3b26206e-5056-4e9f-842e-d73813a675fe","year":2024},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.111094Z"},"links":{"cited_paper":"/paper/2404.09446","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:041f7e556597eee92f00c34624bf7eba4509c02a7209b6403acef02b5cd1f592","observation_id":"43d30aca-4dc2-4a3b-9faf-2057c1b3f41b","resolution":{"observed_at":"2026-08-15T17:11:48.646313Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.09274","last_updated":"2024-05-07T11:13:41Z","snapshot_observed_at":"2026-08-16T14:01:05.306155Z","submitted_at":"2024-04-14T14:32:55Z","title":"Analysis of the CERN-NA63 radiation reaction data set, assuming the Rindler bath is composed of microscopic black holes","version":2},"cited_work":{"arxiv_id":"2404.09274","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.09274","snapshot_observed_at":"2026-08-15T17:11:48.625361Z","title":"Analysis of the CERN-NA63 radiation reaction data set, assuming the Rindler bath is composed of microscopic black holes","venue":"gr-qc","work_id":"f135d5e6-0286-47aa-af28-fb36d0540004","year":2024},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.115607Z"},"links":{"cited_paper":"/paper/2404.09274","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:998e39d4e2cf2aa3391957747a38284db470ab951d7046353b0aac906f13e9d9","observation_id":"839fe4d7-4f67-4935-a790-3de8259cb60d","resolution":{"observed_at":"2026-08-15T17:11:48.629701Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:48.928037Z","title":null,"venue":null,"work_id":"4581c6e9-9bd8-43fb-901c-fffd3d9065b3","year":1990},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.119286Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:86a5f16c55d194763c0ee1956cea82d397313b9eb03c90e4de16a9b9360a9bde","observation_id":"3d10d99f-c0b3-4fca-833d-1a4b9ac954b3","resolution":{"observed_at":"2026-08-15T17:11:48.932617Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9403108","last_updated":"1994-03-18T15:54:30Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"1994-03-18T15:54:30Z","title":"Geometric and Renormalized Entropy in Conformal Field Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9403108","snapshot_observed_at":"2026-08-15T17:11:48.123304Z","title":"Holzhey, F","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.123304Z"},"links":{"cited_paper":"/paper/hep-th/9403108","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:b721e182ed950a50a1f1a774fbc8301f21688fface640a39d6a642a7574e2481","observation_id":"7bede412-d44c-4b32-ac62-db2f1d31d0e6","resolution":{"observed_at":"2026-08-15T17:11:48.123304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.07016","last_updated":"2020-03-16T04:21:37Z","snapshot_observed_at":"2026-07-06T09:04:55.326634Z","submitted_at":"2020-03-16T04:21:37Z","title":"Extreme Hawking Radiation","version":1},"cited_work":{"arxiv_id":"2003.07016","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.07016","snapshot_observed_at":"2026-08-15T17:11:48.589474Z","title":"Extreme Hawking Radiation","venue":"gr-qc","work_id":"6532d816-0bfc-4853-a14e-dfcee2810375","year":2020},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.127331Z"},"links":{"cited_paper":"/paper/2003.07016","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:5b2c34108f832cb1bd9522f957829ed5bc2848e583c3df61a1caddca5f22248f","observation_id":"18e041af-cf82-42a8-a52f-94d802b8cf49","resolution":{"observed_at":"2026-08-15T17:11:48.593736Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.13745","last_updated":"2020-10-12T19:39:42Z","snapshot_observed_at":"2026-08-05T01:13:44.544216Z","submitted_at":"2020-04-28T18:00:11Z","title":"Dilaton gravity with a boundary: from unitarity to black hole evaporation","version":3},"cited_work":{"arxiv_id":"2004.13745","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.13745","snapshot_observed_at":"2026-08-15T17:11:48.570459Z","title":"Dilaton gravity with a boundary: from unitarity to black hole evaporation","venue":"hep-th","work_id":"4612bf94-c3af-454b-b06e-ccdba8fdd809","year":2020},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.131473Z"},"links":{"cited_paper":"/paper/2004.13745","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:a86b41078c3e817bd0e8fca23585f1a19491e585c1e6c2a34a992593529b1e5f","observation_id":"d92105b0-2fdb-4b38-8c45-c63f23e6fa88","resolution":{"observed_at":"2026-08-15T17:11:48.576064Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08139","last_updated":"2021-01-19T06:03:39Z","snapshot_observed_at":"2026-08-16T18:51:28.727623Z","submitted_at":"2021-01-19T06:03:39Z","title":"Relativistic quantum information as radiation reaction: entanglement entropy and self-force of a moving mirror analog to the CGHS black hole","version":1},"cited_work":{"arxiv_id":"2101.08139","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08139","snapshot_observed_at":"2026-08-15T17:11:48.548629Z","title":"Relativistic quantum information as radiation reaction: entanglement entropy and self-force of a moving mirror analog to the CGHS black hole","venue":"gr-qc","work_id":"c3c220f8-315a-4f10-86f7-8231ed64f4c6","year":2021},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.135736Z"},"links":{"cited_paper":"/paper/2101.08139","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:112f3e298417731affa4dbfa6daeee0503e61afa56d4fbd9de754a81da4017ce","observation_id":"51ef9fb2-141f-476a-bcb4-ad8562a57f05","resolution":{"observed_at":"2026-08-15T17:11:48.554202Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.0602","last_updated":"2014-08-13T20:39:56Z","snapshot_observed_at":"2026-08-14T23:38:56.071376Z","submitted_at":"2014-04-02T16:15:16Z","title":"Entanglement entropy and negative energy in two dimensions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.0602","snapshot_observed_at":"2026-08-15T17:11:48.140055Z","title":"Bianchi and M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.140055Z"},"links":{"cited_paper":"/paper/1404.0602","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:92a0b75d8ca3ff9633cfe67447959f8ab770420f367ffd547d6a5bb1c6724cf3","observation_id":"05a5d73c-a526-45da-8756-78a9ab97bee3","resolution":{"observed_at":"2026-08-15T17:11:48.140055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.08613","last_updated":"2017-07-24T05:38:12Z","snapshot_observed_at":"2026-08-14T21:04:17.303183Z","submitted_at":"2017-04-27T15:01:35Z","title":"Entropy evolution of moving mirrors and the information loss problem","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.08613","snapshot_observed_at":"2026-08-15T17:11:48.144245Z","title":"Chen and D.-h","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.144245Z"},"links":{"cited_paper":"/paper/1704.08613","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:6c0fb2b41b5c32f0b87ae2fe69cd954031f05f5764a4d46a27aee6a20d2d1417","observation_id":"ad4d4f08-1b78-4127-a7a1-2b0ddb97a2a4","resolution":{"observed_at":"2026-08-15T17:11:48.144245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.08072","last_updated":"2015-06-24T11:33:08Z","snapshot_observed_at":"2026-08-14T22:43:08.502430Z","submitted_at":"2015-06-24T11:33:08Z","title":"Signatures of Energy Flux in Particle Production: A Black Hole Birth Cry and Death Gasp","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.08072","snapshot_observed_at":"2026-08-15T17:11:48.148815Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.148815Z"},"links":{"cited_paper":"/paper/1506.08072","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:51017261de4d1625a1f34a7700eebc235ffc824e6fc44470c8c4e0d75e95d316","observation_id":"567fb262-440a-46f0-a25a-870f9feddd2b","resolution":{"observed_at":"2026-08-15T17:11:48.148815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07451","last_updated":"2021-08-17T05:33:15Z","snapshot_observed_at":"2026-08-16T18:02:49.456421Z","submitted_at":"2021-08-17T05:33:15Z","title":"M\\\"obius Mirrors","version":1},"cited_work":{"arxiv_id":"2108.07451","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.07451","snapshot_observed_at":"2026-08-15T17:11:48.487900Z","title":"M\\\"obius Mirrors","venue":"gr-qc","work_id":"120dcbe5-2568-40cc-a2df-cd91e45801ec","year":2021},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.154659Z"},"links":{"cited_paper":"/paper/2108.07451","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:917e87c5961e73a27ded809f951c95ad56ff5cf780cc5ecf8b7e10f2dd217024","observation_id":"dbd72ad4-6292-45f1-a999-740765f5f4dc","resolution":{"observed_at":"2026-08-15T17:11:48.492600Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.03521","last_updated":"2024-11-05T21:55:54Z","snapshot_observed_at":"2026-08-16T13:02:37.041568Z","submitted_at":"2024-11-05T21:55:54Z","title":"There and Back Again: Quantum Radiation from Round-trip Flying Mirrors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.03521","snapshot_observed_at":"2026-08-15T17:11:48.159951Z","title":"Mujtaba, E","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.159951Z"},"links":{"cited_paper":"/paper/2411.03521","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:00a758e957cb107f276dfcc97ca153561a950520e25987017e69ce9f7647f9a4","observation_id":"1e3ed5af-3645-4b19-a10d-0a9be64ea467","resolution":{"observed_at":"2026-08-15T17:11:48.159951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.15148","last_updated":"2021-11-30T06:13:34Z","snapshot_observed_at":"2026-08-16T17:38:21.201037Z","submitted_at":"2021-11-30T06:13:34Z","title":"Quantum power: a Lorentz invariant approach to Hawking radiation","version":1},"cited_work":{"arxiv_id":"2111.15148","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.15148","snapshot_observed_at":"2026-08-15T17:11:48.452518Z","title":"Quantum power: a Lorentz invariant approach to Hawking radiation","venue":"gr-qc","work_id":"5a9956c9-c1f8-4c32-bbc0-22fecd01e01b","year":2021},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.164747Z"},"links":{"cited_paper":"/paper/2111.15148","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:30c8cedd7a5a7876a2a77d8d5767dc2bd2ae65a22630177ec2646cf55809eac3","observation_id":"ac084d8f-53a8-40ea-92b8-732340c117c1","resolution":{"observed_at":"2026-08-15T17:11:48.458510Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:48.909805Z","title":null,"venue":null,"work_id":"e359459e-aa64-4100-942d-3339052b1690","year":1996},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.169410Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:0271c13c6bec8ec37981604cdfb42b09604a99ae0fb82899a4e80463753be72c","observation_id":"e4995275-1ab3-47b8-ba04-e2669de2b080","resolution":{"observed_at":"2026-08-15T17:11:48.916404Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:48.896097Z","title":null,"venue":null,"work_id":"628ba924-2133-4eaf-86e9-e09a6ed71d57","year":1985},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.173847Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:ccc78775a012fbcdbbf8d646bc6ec0f782c88985228dcc72359a678d469983f1","observation_id":"dc57d509-f05a-41a1-8c74-710ee697c7a8","resolution":{"observed_at":"2026-08-15T17:11:48.900540Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.5235","last_updated":"2014-05-16T17:40:45Z","snapshot_observed_at":"2026-08-14T23:33:45.559212Z","submitted_at":"2014-05-16T17:40:45Z","title":"Last gasp of a black hole: unitary evaporation implies non-monotonic mass loss","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.5235","snapshot_observed_at":"2026-08-15T17:11:48.178772Z","title":"Bianchi and M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.178772Z"},"links":{"cited_paper":"/paper/1405.5235","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:c5fa4c2dc4f719d020f908cda15ffd6cb8aff0cf4064b10a3de3e679986da29f","observation_id":"f66157fc-ea29-4ae9-8f65-acb36d72eac3","resolution":{"observed_at":"2026-08-15T17:11:48.178772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9306083","last_updated":"1993-08-26T22:59:01Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"1993-06-18T01:10:14Z","title":"Information in Black Hole Radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9306083","snapshot_observed_at":"2026-08-15T17:11:48.183958Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.183958Z"},"links":{"cited_paper":"/paper/hep-th/9306083","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:88313a9e10f96489f67dfd22403d88aa47ac5245236db8a49533e9e0f67a89a7","observation_id":"0c7f1af1-676a-4e4f-bbb9-eece8be29a2c","resolution":{"observed_at":"2026-08-15T17:11:48.183958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.01129","last_updated":"2019-08-30T04:00:54Z","snapshot_observed_at":"2026-08-16T10:52:08.084888Z","submitted_at":"2019-08-30T04:00:54Z","title":"Remnant-free Moving Mirror Model for Black Hole Radiation Field","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.01129","snapshot_observed_at":"2026-08-15T17:11:48.188651Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.188651Z"},"links":{"cited_paper":"/paper/1909.01129","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:7eed85949de8a4ca416dfaefc2335423eefc6aa14e2837abf571af367e7e81e8","observation_id":"b3423be7-e138-40bd-b479-15eecc73b648","resolution":{"observed_at":"2026-08-15T17:11:48.188651Z","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":"2026-08-15T17:11:48.192702Z","title":null,"venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.192702Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:9f74df9bde2f339d3762ca9c006b31a8bb0c73f8589421ddf04704cedbb612a4","observation_id":"9fd1d02b-7c73-456e-a268-f18e5969df9e","resolution":{"observed_at":"2026-08-15T17:11:48.192702Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.03676","last_updated":"2023-03-07T06:25:00Z","snapshot_observed_at":"2026-08-16T15:50:14.743446Z","submitted_at":"2023-03-07T06:25:00Z","title":"Thermal Larmor radiation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.03676","snapshot_observed_at":"2026-08-15T17:11:48.197483Z","title":"Ievlev and M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.197483Z"},"links":{"cited_paper":"/paper/2303.03676","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:44c9c4713bd413f5c75e65813e58f9bc2995626947116163917f3c97a00fdc56","observation_id":"322cb1ff-61a1-4917-8be1-2f15cb18b665","resolution":{"observed_at":"2026-08-15T17:11:48.197483Z","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":"2026-08-15T17:11:48.876099Z","title":null,"venue":null,"work_id":"e397aa66-7aa8-4f6f-b03f-fbfebd3dd7c4","year":1949},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.202264Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:6e6ecc701f714b8da09034196cf68bbe09834122ea84ff74e76bebf3ee613682","observation_id":"540838cb-6100-46ba-a94e-922ee9830b00","resolution":{"observed_at":"2026-08-15T17:11:48.879918Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:48.206701Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.206701Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:8bfd2d71a0e5b311014fc4a63cde5130669abc7276844765d84b37f94ce322cb","observation_id":"3ae6ccb8-f38c-47ed-b453-c14ad2088125","resolution":{"observed_at":"2026-08-15T17:11:48.206701Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.07291","last_updated":"2022-07-02T03:51:05Z","snapshot_observed_at":"2026-08-16T16:52:55.377140Z","submitted_at":"2022-06-15T04:19:26Z","title":"Infrared acceleration radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.07291","snapshot_observed_at":"2026-08-15T17:11:48.210388Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.210388Z"},"links":{"cited_paper":"/paper/2206.07291","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:f7cc967b054226e67703fabbe7680ce3c7ecb8d3e03fc6cd9bb34c605ded4247","observation_id":"27b19456-3e14-457b-b7aa-fa0121408b56","resolution":{"observed_at":"2026-08-15T17:11:48.210388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.09869","last_updated":"2020-09-03T09:58:42Z","snapshot_observed_at":"2026-07-06T08:46:01.828120Z","submitted_at":"2019-12-20T15:11:09Z","title":"Quantum radiation in dielectric media with dispersion and dissipation","version":2},"cited_work":{"arxiv_id":"1912.09869","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.09869","snapshot_observed_at":"2026-08-15T17:11:48.276555Z","title":"Quantum radiation in dielectric media with dispersion and dissipation","venue":"quant-ph","work_id":"a16f4cf0-065d-4bb0-ba19-ed4d8a57038f","year":2019},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.214374Z"},"links":{"cited_paper":"/paper/1912.09869","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:9f6b65065337a8ec164e38985225c1d7bae8736e3649548bf01814a76b62a6fd","observation_id":"5a823ef1-8e05-4b76-a653-8b9d3e466ea3","resolution":{"observed_at":"2026-08-15T17:11:48.283946Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.6756","last_updated":"2013-03-27T07:34:01Z","snapshot_observed_at":"2026-08-15T00:23:41.937337Z","submitted_at":"2013-03-27T07:34:01Z","title":"Time Dependence of Particle Creation from Accelerating Mirrors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.6756","snapshot_observed_at":"2026-08-15T17:11:48.218168Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.218168Z"},"links":{"cited_paper":"/paper/1303.6756","citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:f5110dba502c8de5a77897a17d9147f58d19d0b605632d1d11eeedbd35b5a614","observation_id":"0ed6f4d2-f2c3-470a-a7ae-1ad6611798d5","resolution":{"observed_at":"2026-08-15T17:11:48.218168Z","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":"2026-08-15T17:11:48.863297Z","title":null,"venue":null,"work_id":"ca340849-e514-427a-8c6b-c862677ce180","year":2017},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.222257Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:10a48415675064a8cb82e5be77a5a1f2d2f616746e923147699f3eed017a6016","observation_id":"5426e089-2d10-47ec-8aa9-23a525e7f35c","resolution":{"observed_at":"2026-08-15T17:11:48.867639Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-15T17:11:48.848479Z","title":"Fabbri and J","venue":null,"work_id":"04fffbdc-5ef9-4d6c-8e72-c81a7be72636","year":2005},"citing_paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T17:11:48.226005Z"},"links":{"citing_paper":"/paper/2508.17059"},"observation_digest":"sha256:197c3074a009289b285a11683f543c38897cebc778a3088ebcc148ba7d012485","observation_id":"81d14334-8cc3-4794-b63d-0600c37e6573","resolution":{"observed_at":"2026-08-15T17:11:48.853569Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2508.17059","last_updated":"2025-08-23T15:21:28Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-15T17:05:42.283774Z","submitted_at":"2025-08-23T15:21:28Z","title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra"},"reference_resolution":{"displayed":50,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":31,"verified_exact":13,"verified_fuzzy":6},"total_outbound_references":50},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 50 of 50 outbound references and 0 inbound Pith citation observations for arXiv:2508.17059."}