{"as_of":"2026-08-10T11:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8c94556e4881d3a3f4866785a4c5d101c29b9da45165c1e490c3d9d1d055684d","coverage":[{"denominator":90,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":90,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T16:20:10.350973Z","state":"measured"},{"denominator":90,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":90,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+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/2607.18048/citation-record","integrity":"/paper/2607.18048/integrity","json":"/paper/2607.18048/citation-record.json","paper":"/paper/2607.18048"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2511.15823","last_updated":"2026-07-07T22:45:31Z","snapshot_observed_at":"2026-08-05T04:43:18.794298Z","submitted_at":"2025-11-19T19:29:25Z","title":"The SPHEREx Image and Spectrophotometry Processing Pipeline","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.15823","snapshot_observed_at":"2026-08-01T16:20:09.320973Z","title":"P., Crill, B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.320973Z"},"links":{"cited_paper":"/paper/2511.15823","citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:006971f6b50956c60c8f54f2deec731cb71983652874454f5da06b3d00335dab","observation_id":"72efbfb2-eed4-4491-9eff-bdf5db71eade","resolution":{"observed_at":"2026-08-01T16:20:09.320973Z","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":"2026-08-01T16:20:09.328411Z","title":"P., Faisst, A., et al.\\ 2026, SPHEREx Explanatory Supplement, Version 1.4, https://irsa.ipac.caltech.edu/data/SPHEREx/docs/SPHEREx_Expsupp_QR.pdf","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.328411Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:9788814dfefcd36ff92e0c45e1d14e8d4a5111fbb2630ede59087532e264b2ee","observation_id":"a37c82d9-5bcd-4a12-b714-ed48836abef7","resolution":{"observed_at":"2026-08-01T16:20:09.328411Z","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":"2026-08-01T16:20:09.333575Z","title":"doi:10.1098/rsta.2011.0269","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.333575Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:0b7f6d59e2171a5e957fa7abc051654ed5cc08f8f884ff6cf6c85c4f794dedaa","observation_id":"bc9dd884-cec0-4cdf-a8be-8c4fd825f529","resolution":{"observed_at":"2026-08-01T16:20:09.333575Z","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":"2026-08-01T16:20:09.338470Z","title":"F., Argudo-Fern \\'a ndez, M., et al.\\ 2023, , 267, 2, 44","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.338470Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:1c80f00fd6bb0a6b0825572fed0a814e465e851e400354f10f75f998223ee15f","observation_id":"e22a83bb-0036-4492-976a-e1ec65df43d6","resolution":{"observed_at":"2026-08-01T16:20:09.338470Z","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":"10.1051/0004-6361:20021313","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"G.\\ 2002, , 395, 915","venue":"Astronomy and Astrophysics","work_id":"bcb09c6b-3edb-4f47-b73a-17cfb2d9a043","year":2002},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.343864Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:cf9851a98b15e3f2ff87f56e211e34e6ecb9ce4ac2abe76b7db4cc9743dae0f1","observation_id":"148bb6dd-f3e2-429a-9583-b6e6b5099d58","resolution":{"observed_at":"2026-08-01T16:24:17.737957Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/200911703","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1051/0004-6361/200911703","venue":"Astronomy and Astrophysics","work_id":"16e3b60a-8a8d-4c7e-9ddc-2ffc89f999ce","year":2009},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.348921Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:7631e9158eb45117864cf6b80e4fb02ee9b942805ca25f4fa9fdb6b2a39203cf","observation_id":"7ebcc936-7bf7-4176-a8f5-1cd2d303f962","resolution":{"observed_at":"2026-08-01T16:24:17.472934Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-14T05:50:07.161645+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T05:50:07.161645+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-01T16:20:09.355560Z","title":"P., Tollerud, E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.355560Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:13e5aa6f591647000f8495436c111afe12b282f0d067d33de45490d6b02b22db","observation_id":"b300c790-96bf-47a8-90cb-83adfd95b15d","resolution":{"observed_at":"2026-08-01T16:20:09.355560Z","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":"2026-08-01T16:20:09.360617Z","title":"M., Sip o cz, B","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.360617Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:ec77c2f4a5df2f47c8fd9eac9e24cb2a94d2d42de526d8628454d0b1f27e2a4e","observation_id":"d0fbc7f8-de91-4913-af1d-c2ed2994b942","resolution":{"observed_at":"2026-08-01T16:20:09.360617Z","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":"2026-08-01T16:20:09.365349Z","title":"M., Lim, P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.365349Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:bb87c86aeec700182b3c26cfa50d4d99c6b86058414fcb7179f3c160db141f96","observation_id":"930ad4aa-9378-4065-8547-daadd36265fd","resolution":{"observed_at":"2026-08-01T16:20:09.365349Z","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":"2026-08-01T16:20:09.370399Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.370399Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:48d46066741ab80b1c4085e002476a5343d9765e5e836addbb8c0f2e5acad468","observation_id":"a404e3e8-6f6e-4981-9e97-36b3b857e18b","resolution":{"observed_at":"2026-08-01T16:20:09.370399Z","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":"10.1051/0004-6361/202556999","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1051/0004-6361/202556999","venue":"Astronomy and Astrophysics","work_id":"b7ee1bf8-2fec-4670-ba5f-f1aa97a07535","year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.376148Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:b05b5732b3cfd8fb5b6865a870d989915f44c0d314ed2bdf9ebd37e8c43c86f1","observation_id":"cf394500-a1e4-4ed9-a83c-26a91ba2b531","resolution":{"observed_at":"2026-08-01T16:24:17.220277Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-01T16:20:09.380684Z","title":"M., Kuntschner, H., et al.\\ 2018, , 473, 4, 4698","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.380684Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:a59a4552b4f0984419a1fb048ff52a5ea8e8b3f208e7eebb16d47fa9761a33f6","observation_id":"7681ef61-4ca0-4060-b0ae-f36a9f9a8237","resolution":{"observed_at":"2026-08-01T16:20:09.380684Z","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":"2026-08-01T16:20:09.385292Z","title":"& Robotham, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.385292Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:8b8d11600fd18762447f93f1331eaef56e99ed0898e45a0e7187579e39b31523","observation_id":"464326b9-304f-49a2-83e7-3e7f404b957b","resolution":{"observed_at":"2026-08-01T16:20:09.385292Z","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":"2026-08-01T16:20:09.389889Z","title":"J., Aboobaker, A","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.389889Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:59d32e3b0d215647d730fef71f35f4e77e2ab69af40a1efca6409698f5e46464","observation_id":"103e4520-a0a1-4af9-a728-50310d5b1ba1","resolution":{"observed_at":"2026-08-01T16:20:09.389889Z","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":"2026-08-01T16:20:09.394507Z","title":"doi:10.1051/0004-6361/201834156","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.394507Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:61ec8cdee072c50ef7113fbbd0cea5e96b3264eaff464de82afeafd0479e5a35","observation_id":"380117c2-f29a-49cc-b7c4-b1f815ce0767","resolution":{"observed_at":"2026-08-01T16:20:09.394507Z","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":"2026-08-01T16:20:09.398923Z","title":"C., & Kothari, H.\\ 2026, Research Notes of the American Astronomical Society, 10, 4, 94","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.398923Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:78309b9d6144d324ea741be6559d4240a9e39b8f8228d9352b129bc494a9bb2e","observation_id":"b0b38cff-3da4-415b-8f53-adf635d6c001","resolution":{"observed_at":"2026-08-01T16:20:09.398923Z","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":"2026-08-01T16:20:09.403249Z","title":"& Charlot, S.\\ 2003, , 344, 4, 1000","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.403249Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:281d3437420ec7ffb41d739c7729a7396fbf0fa49a74ea8d35b45f3255b815d7","observation_id":"272d90df-0a92-46dd-b189-224c64a7e6da","resolution":{"observed_at":"2026-08-01T16:20:09.403249Z","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":"2026-08-01T16:20:09.408546Z","title":"C., et al.\\ 2000, , 533, 2, 682","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.408546Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:96d2db21fb1fa199a34e4b1c7b990608e4eb36602ae04ecec8bb1e0fa7c632aa","observation_id":"5938b4a5-676d-4cca-81db-4bfe2aaf940f","resolution":{"observed_at":"2026-08-01T16:20:09.408546Z","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":"2026-08-01T16:20:09.413202Z","title":"doi:10.1093/mnras/stad2597","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.413202Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:4201dc60dc729f4a0c3eb4da5dd7146b5a0c5c61183114b9d7887e29ab8956d8","observation_id":"ae1762a7-b903-4772-b6fc-35890f6cd700","resolution":{"observed_at":"2026-08-01T16:20:09.413202Z","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":"2026-08-01T16:20:09.417788Z","title":"A., Clayton, G","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.417788Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:21d12bd9dfb9f37b55a1a45801fe1d25b827329adde4dbd1fb006a6e2661c958","observation_id":"fdfd8b3e-c6d9-4ab4-9f45-7b5fdd671ea8","resolution":{"observed_at":"2026-08-01T16:20:09.417788Z","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":"2026-08-01T16:20:09.429244Z","title":"doi:10.1086/376392","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.429244Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:4c3992acccba77cfa92a11ac23b2f937adf43e6a004f52447809853aec0179a9","observation_id":"c2f95cf3-fa50-4f7c-a502-592c0d5e27e3","resolution":{"observed_at":"2026-08-01T16:20:09.429244Z","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":"2026-08-01T16:20:09.480717Z","title":"E., & White, M.\\ 2009, , 699, 1, 486","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.480717Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:07be623a0df3fcdbd7cc5d5b8d9ca0a2bb1dc5d1dde3fcf55a93ee6a258f6920","observation_id":"464e60db-63c3-4634-9243-c04d0d39ab28","resolution":{"observed_at":"2026-08-01T16:20:09.480717Z","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":"2026-08-01T16:20:09.497067Z","title":"& Gunn, J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.497067Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:4964bc83b1474113b777f99ee7a46181e07fa821c19d1ccd5349fdd86481c4d6","observation_id":"a3c389d9-a79c-4f19-8db2-6394952c5e15","resolution":{"observed_at":"2026-08-01T16:20:09.497067Z","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":"2026-08-01T16:20:09.513773Z","title":"& Gunn, J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.513773Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:7a39e53bc1e175304cd26911a4fa3981467da85b5a5acfc8cbc5c6c6573f3434","observation_id":"d24bcbb9-d485-4acd-b7b0-b6df346fea88","resolution":{"observed_at":"2026-08-01T16:20:09.513773Z","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":"2026-08-01T16:20:09.530941Z","title":"& van Dokkum, P.\\ 2012, , 747, 1, 69","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.530941Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:0063df8646b652e52e791f165840f0daa10c83c5b7615b2eb993ed7b90d7aedc","observation_id":"0ebad170-65e0-42ec-88b7-15931bae075b","resolution":{"observed_at":"2026-08-01T16:20:09.530941Z","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":"2026-08-01T16:20:09.549292Z","title":"doi:10.1146/annurev-astro-082812-141017","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.549292Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:63ff0d7ef1de5555f2ba2c023e7b1078e2b6648c4f7a7e8e0dd74a72b47affcf","observation_id":"4932f157-43c1-4a59-963c-4e3825db30c2","resolution":{"observed_at":"2026-08-01T16:20:09.549292Z","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":"2026-08-01T16:20:09.561102Z","title":"G., et al.\\ 2018, , 854, 2, 139","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.561102Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:f8060c5c019d3f532dd0db542a71ec634be8eeb77fdce8b906a875bb31d3c34c","observation_id":"88d43251-e4b7-4051-b012-496ed21401a5","resolution":{"observed_at":"2026-08-01T16:20:09.561102Z","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":"2026-08-01T16:20:09.577898Z","title":"P., Bach, Y","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.577898Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:e398c9cc318d11fd37c5e490df2c03aa5a7b4b8aa23226687200fe55a80f04f0","observation_id":"76eb2129-0003-4853-8178-31bd7d056f59","resolution":{"observed_at":"2026-08-01T16:20:09.577898Z","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":"2026-08-01T16:20:09.596107Z","title":"C., Rayner, J","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.596107Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:4cc90c5f125a9551342f15ef1850314a3212266e2de7fb61ec03b992ac88ccce","observation_id":"aa8278fe-2d79-4ff8-8495-52382710b538","resolution":{"observed_at":"2026-08-01T16:20:09.596107Z","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":"2026-08-01T16:20:09.612946Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.612946Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:ecda4fa01ce941f0658dc0800557592dfedd2dd5eaa441183d20a6d365c79bf1","observation_id":"1992e547-74a7-4716-a0fd-eaeaa4aafdfa","resolution":{"observed_at":"2026-08-01T16:20:09.612946Z","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":"2026-08-01T16:20:09.680774Z","title":"M., Wright, E","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.680774Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:233e1746310b238fd57b02aa4aa7872785c577579b837223901ce8d0fa637f38","observation_id":"15bcea9e-d6b8-4242-b77e-b8b8c059f4ba","resolution":{"observed_at":"2026-08-01T16:20:09.680774Z","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":"2026-08-01T16:20:09.799623Z","title":"doi:10.5303/JKAS.2024.57.1.45","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.799623Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:14fe6d927d4f7433aee661f434014afa583c46a4055d9772b28d06f869055a96","observation_id":"230322d6-97e7-41c9-8dcd-7003d3e96ea2","resolution":{"observed_at":"2026-08-01T16:20:09.799623Z","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":"2026-08-01T16:20:09.987686Z","title":"B., Bosman, S","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:09.987686Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:145050da5c0d5bcf8e21a6bd88bd35b1ad231e6a923586f8a00ee936a0317454","observation_id":"be64c979-b1de-4674-ac88-cb9bbcf3e8fc","resolution":{"observed_at":"2026-08-01T16:20:09.987686Z","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":"10.1051/0004-6361/201629044","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"M., Iglesias-P \\'a ramo, J., et al.\\ 2017, , 599, A71","venue":"Astronomy and Astrophysics","work_id":"b2941368-5794-42b0-9fd2-6d06377eb1ae","year":2017},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.115468Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:288b72525a8638664cc13b83f4580e4936cf38268c3b2e2f7242bbbe9872cab8","observation_id":"c1450df1-d8c0-4c31-ba4d-c63c524f39a1","resolution":{"observed_at":"2026-08-01T16:24:16.860256Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-01T16:20:10.120603Z","title":"J., Stanway, E","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.120603Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:28ccd259cf98c702053ce73d871b4450f4ecb4a886ba9a265dd2d8ef734494ee","observation_id":"cb3906d5-2d48-45ef-a74c-a71d95a13cc2","resolution":{"observed_at":"2026-08-01T16:20:10.120603Z","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":"2026-08-01T16:20:10.124908Z","title":"M., Masters, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.124908Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:94429d40dbc4d664ce3d98dac7b3dc4428a57ef7c7f4720865f576cc814169ad","observation_id":"2d9ae300-a758-4a88-b157-c97e89b42576","resolution":{"observed_at":"2026-08-01T16:20:10.124908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9707017","last_updated":"1997-07-02T16:33:57Z","snapshot_observed_at":"2026-08-05T16:37:26.102409Z","submitted_at":"1997-07-02T16:33:57Z","title":"PEGASE: a UV to NIR spectral evolution model of galaxies - Application to the calibration of bright galaxy counts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9707017","snapshot_observed_at":"2026-08-01T16:20:10.128830Z","title":"& Rocca-Volmerange, B.\\ 1997, , 326, 950","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.128830Z"},"links":{"cited_paper":"/paper/astro-ph/9707017","citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:ced808a5eafa3e2b8ca7a0174e491a68f4e93c38382f3dccb3ddc90dab168e9f","observation_id":"cdbd1f91-3148-4755-9183-00d1d0ff4608","resolution":{"observed_at":"2026-08-01T16:20:10.128830Z","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":"2026-08-01T16:20:10.133677Z","title":"doi:10.1093/mnras/stz418","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.133677Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:0aebed38b68dde3867f3aa772864f660d64539bb93c854d1d2ddbdf4142992e8","observation_id":"7a6db023-f1bc-4333-9428-d89c2e2965b1","resolution":{"observed_at":"2026-08-01T16:20:10.133677Z","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":"2026-08-01T16:20:10.137881Z","title":"M.\\ 2018, The Journal of Open Source Software, 3, 26, 695","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.137881Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:e63c296ac56275b8a5eff7b7aa9e4215583d0ae61606469b879187f90476cf7d","observation_id":"e6e7994d-29ba-464b-b7aa-8387ad84c12a","resolution":{"observed_at":"2026-08-01T16:20:10.137881Z","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":"2026-08-01T16:20:10.143580Z","title":"R., Millman, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.143580Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:bc471ef738e2c8fdf84573470ce8effe3fb505d2e2de503ced6258c831c463b9","observation_id":"cf1b0451-5555-4aed-b7b8-e08527536d64","resolution":{"observed_at":"2026-08-01T16:20:10.143580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.15060","last_updated":"2021-06-07T04:24:51Z","snapshot_observed_at":"2026-08-08T16:12:08.537015Z","submitted_at":"2021-03-28T06:24:00Z","title":"PnG BERT: Augmented BERT on Phonemes and Graphemes for Neural TTS","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.15060","snapshot_observed_at":"2026-08-01T16:20:10.148151Z","title":"doi:10.1146/annurev.astro.43.072103.150600","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.148151Z"},"links":{"cited_paper":"/paper/2103.15060","citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:df02ad258f617b548e82e18bf40b92af58bf3da7f88d7383acb1352eb24fc8c4","observation_id":"1e1bc176-ab95-45e5-9cf4-144be10124a3","resolution":{"observed_at":"2026-08-01T16:20:10.148151Z","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":"2026-08-01T16:20:10.152520Z","title":"& Olofsson, H.\\ 2018, , 26, 1, 1","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.152520Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:d9ec88b6ecf500202e88ea96e60239c9d3b91ed39bdd62d93561ccd3dc6f1b3b","observation_id":"b1ef1654-b8be-47ba-90f3-b321649336c5","resolution":{"observed_at":"2026-08-01T16:20:10.152520Z","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":"2026-08-01T16:20:10.156574Z","title":"J., Cheng, Y.-T., et al.\\ 2026, , 1000, 1, 56","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.156574Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:93192daf2926afcc9d2e5d33aadf81bc703de4578aff40e351a5b47b06ee05c0","observation_id":"70ebe3c6-aeb2-43f8-80b2-ce85285de095","resolution":{"observed_at":"2026-08-01T16:20:10.156574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2602.09139","last_updated":"2026-04-21T15:44:55Z","snapshot_observed_at":"2026-08-02T10:52:09.099972Z","submitted_at":"2026-02-09T19:37:35Z","title":"Spectral response of SPHEREx","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2602.09139","snapshot_observed_at":"2026-08-01T16:20:10.160581Z","title":"J., Condon, S., et al.\\ 2026, arXiv:2602.09139","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.160581Z"},"links":{"cited_paper":"/paper/2602.09139","citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:61384b9f0c268cdfad929c3354bf8324f8dd0ef767f4299befdb8d119cf36d17","observation_id":"4d987a76-e1ca-4d86-b530-897924321e82","resolution":{"observed_at":"2026-08-01T16:20:10.160581Z","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":"2026-08-01T16:20:10.164838Z","title":"D.\\ 2007, Computing in Science and Engineering, 9, 90","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.164838Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:758608778d8b11eb8835f4b96fd2d0fde9037a3056256c55a1425fa91b78a890","observation_id":"b99ffced-65a2-4845-b3c7-108c51f9d1ac","resolution":{"observed_at":"2026-08-01T16:20:10.164838Z","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":"2026-08-01T16:20:10.168922Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.168922Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:b937605807422de1197fe57b15714f711ac5c52ed1e5672787334d8c938b678d","observation_id":"5e215655-db7d-41b2-998e-75f751a6a22a","resolution":{"observed_at":"2026-08-01T16:20:10.168922Z","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":"2026-08-01T16:20:10.172813Z","title":"M., Tyson, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.172813Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:e2a58545f724f3262b2cb30ceeca4515a47377e868cb7e306424f8323535a121","observation_id":"03832074-3732-4412-8fbc-49db1dc87278","resolution":{"observed_at":"2026-08-01T16:20:10.172813Z","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":"2026-08-01T16:20:10.177307Z","title":"H., Masci, F., Tsai, C","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.177307Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:a87030652f2876f562a6eec07b4c930cd211a8c43a5e1a2dc8eee57482beae68","observation_id":"089f43f2-5496-493b-93be-03d88b4f9cfc","resolution":{"observed_at":"2026-08-01T16:20:10.177307Z","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":"2026-08-01T16:20:10.181302Z","title":"H., Cluver, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.181302Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:f29baaa43384e95bb9968bdcc24ba7e2331a28866bd35336ec13301a78c7d426","observation_id":"53ea3293-53a0-41c2-bfa9-a798c1c594c0","resolution":{"observed_at":"2026-08-01T16:20:10.181302Z","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":"10.3847/1538-4357/ae5c9a","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"K., Melchior, P., Spergel, D","venue":"The Astrophysical Journal","work_id":"a0565a93-3ef3-4988-b306-07ae5eaeebc5","year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.186245Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:e272d9af6b7dc094b87896aad931fca31a3ec73ec51b429ed20a6357688069f5","observation_id":"032e9a0e-c66c-4b0d-9431-43932f7cf366","resolution":{"observed_at":"2026-08-01T16:24:16.496445Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-01T16:20:10.189984Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.189984Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:438fb377227bad3775223b934fed5600bd6c6fabba150c934ce72346124fa26d","observation_id":"8b2d20e4-523f-4af0-9bbc-d2a130e986c2","resolution":{"observed_at":"2026-08-01T16:20:10.189984Z","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":"2026-08-01T16:20:10.193875Z","title":"doi:10.1088/2041-8205/722/1/L64","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.193875Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:01301e5800fca5eca8bb10babc22fe6e847c6d359e165c6c0687d360980bc45f","observation_id":"89827418-92b5-4031-98e4-793185fe649a","resolution":{"observed_at":"2026-08-01T16:20:10.193875Z","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":"10.1088/0004-637x/777/2/82","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"G., & Lim, S.\\ 2013, , 777, 2, 82","venue":"The Astrophysical Journal","work_id":"3d9db6b8-0e01-46e1-b175-c95a9d05ceef","year":2013},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.197948Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:e6de41ada2f27431f217e78f328548647c59d4b5fa97768c48bbff107d910193","observation_id":"762335ad-46f4-4e42-905e-158a5f554c1e","resolution":{"observed_at":"2026-08-01T16:24:16.208144Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-01T16:20:10.202002Z","title":"doi:10.1111/j.1365-2966.2008.12908.x","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.202002Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:3cc72abeb668b49f06d7e82c367e1a348fb8a3162f022fb2507deb695e0f4263","observation_id":"e94698fb-0761-4e4c-adf3-6888049465db","resolution":{"observed_at":"2026-08-01T16:20:10.202002Z","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":"2026-08-01T16:20:10.205812Z","title":"H., Kim, M., Kim, T., et al.\\ 2025, , 169, 3, 185","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.205812Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:b844790dc8d6ce37784344622d8c445b232d7125ca00eab0a5dcc5278588012c","observation_id":"8b1d063e-6ff5-45ff-88ea-e917d7ed9f04","resolution":{"observed_at":"2026-08-01T16:20:10.205812Z","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":"10.5303/jkas.2025.58.1.43","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T16:24:15.787180Z","title":"doi:10.5303/JKAS.2025.58.1.43","venue":null,"work_id":"e7c2ab0d-6230-4188-b40f-efe3b373a798","year":2025},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.210235Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:5ebebc48ae74f09a0f4a399aedddbac93011ee08390f8bb2cf0d5daaba89c3f5","observation_id":"1553c0a9-5dd1-4b67-99f2-44ef34a25d36","resolution":{"observed_at":"2026-08-01T16:24:15.916423Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/adf3a9","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.3847/1538-4357/adf3a9","venue":"The Astrophysical Journal","work_id":"90a9a9cf-7be8-4dc1-bde2-0a6c22d986e8","year":2025},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.214438Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:7d8be1e521a080bbca43963b5d0fd5a42964961df8dc2703776d6d4918db68db","observation_id":"80066ca6-b0a5-49e5-9016-31a44721da87","resolution":{"observed_at":"2026-08-01T16:24:15.613414Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-01T16:20:10.218730Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.218730Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:26df23228fd18847a17efb21e5ad89295de6fcfaed094eb4769186ac7d1c25bd","observation_id":"c823d9e5-f197-4fa1-9d68-4c03b78ba481","resolution":{"observed_at":"2026-08-01T16:20:10.218730Z","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":"2026-08-01T16:20:10.222625Z","title":"doi:10.1046/j.1365-8711.1998.01947.x","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.222625Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:fd98242088b9466e7e6337abdd4a50eaab5a0231e6db8e24f739c70b11433624","observation_id":"0a8c99dc-d4a4-4a2b-95fc-dae4de070d99","resolution":{"observed_at":"2026-08-01T16:20:10.222625Z","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":"2026-08-01T16:20:10.226471Z","title":"doi:10.1111/j.1365-2966.2005.09270.x","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.226471Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:7676693005e0b0a3ad24037efe5322e28611f5f4cacd038aef6a8cfd5be36019","observation_id":"7ffeb6ee-d984-45e8-ad38-9eb8666f6615","resolution":{"observed_at":"2026-08-01T16:20:10.226471Z","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":"2026-08-01T16:20:10.230284Z","title":"doi:10.1086/508143","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.230284Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:a458bc4c267b370b5e4373a01ff03ffcfb6c41b30aa6dc04f63d8835cda7c2fd","observation_id":"cbf41c2c-1eeb-423d-b32a-d18ca7d6eca6","resolution":{"observed_at":"2026-08-01T16:20:10.230284Z","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":"2026-08-01T16:20:10.234988Z","title":"& Str \\\"o mb \\\"a ck, G.\\ 2011, , 418, 4, 2785","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.234988Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:f438cc91076a9dd1a0e9774a90df3d999943497892ae801d4060cbf196fcd296","observation_id":"cef31a2d-3614-4552-89c5-c53d0d963679","resolution":{"observed_at":"2026-08-01T16:20:10.234988Z","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":"2026-08-01T16:20:10.238514Z","title":"doi:10.1093/mnras/staa1489","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.238514Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:3d4611b1b552203e1f5ad3144e9a5fbd3235b510fef08330072f1ec06005d0d1","observation_id":"3608eb3f-e8f6-48af-967d-2fd938049b3d","resolution":{"observed_at":"2026-08-01T16:20:10.238514Z","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":"10.1051/0004-6361/202142812","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"M., Garc \\' a-Benito, R., et al.\\ 2022, , 661, A99","venue":"Astronomy and Astrophysics","work_id":"7c9c6fe6-41a4-4d60-9868-bce8afcf4e24","year":2022},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.243371Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:9430512adb31ed5439896c4ea77a3a7f3719f3be2897c16b36fec8fdd09f9fdb","observation_id":"5604a95e-ce39-498d-8266-cefd25ffcfc1","resolution":{"observed_at":"2026-08-01T16:24:15.273060Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-01T16:20:10.247451Z","title":"doi:10.3847/1538-4357/ab9eb0","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.247451Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:924f22848b13db30335165839946301667e44ac0f6e863f8db5db6d49b3457c8","observation_id":"4fa321ed-c2ce-4671-9751-ec3d6cdf6ea5","resolution":{"observed_at":"2026-08-01T16:20:10.247451Z","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":"2026-08-01T16:20:10.251578Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.251578Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:dfa9596ee1161061fd87c8f20c7f57a8d124ba05f37553eff18d0227323ad0ed","observation_id":"41261ac6-c4a3-46c1-a218-86d2b531384e","resolution":{"observed_at":"2026-08-01T16:20:10.251578Z","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":"2026-08-01T16:20:10.255568Z","title":"doi:10.1111/j.1365-2966.2012.20431.x","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.255568Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:f9b1aed6f00476965a854106349a323a47aaffefba40b60964b93b9fc6fb6681","observation_id":"74fbd072-2920-4e5f-9e77-0e8948016427","resolution":{"observed_at":"2026-08-01T16:20:10.255568Z","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":"2026-08-01T16:20:10.259370Z","title":"J.\\ 1998, , 110, 749, 863","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.259370Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:f17e0bda9a781f4274e32e743df64be08d9c482d2fb36e51daf37a1eb6ff07d1","observation_id":"6886810f-23a1-4064-baaf-d03399d05b1d","resolution":{"observed_at":"2026-08-01T16:20:10.259370Z","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":"2026-08-01T16:20:10.263255Z","title":"doi:10.1086/422498","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.263255Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:1f4ea7d7d1e0587b0350385bd17c38112c47d79acd77de54fd23aff2eb8f9996","observation_id":"185ea257-5735-43bd-8451-7682c9354cdd","resolution":{"observed_at":"2026-08-01T16:20:10.263255Z","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":"2026-08-01T16:20:10.267416Z","title":"doi:10.1093/mnras/stz2616","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.267416Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:3494424fddf6648f9b75f40514dcbe27e5cedd2bf29178f14d368d03bf39beb4","observation_id":"f3a59a65-7a73-466e-94d7-0a3c62de4c4b","resolution":{"observed_at":"2026-08-01T16:20:10.267416Z","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":"2026-08-01T16:20:10.271406Z","title":"T., Toomey, D","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.271406Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:6e98d5cfa64406408fef6ee58c6b97631313a555b014f09262a521da88e8fa2e","observation_id":"5a246ee3-663b-4a67-95ce-e43c9cc4e0b3","resolution":{"observed_at":"2026-08-01T16:20:10.271406Z","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":"2026-08-01T16:20:10.276106Z","title":"T., Cushing, M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.276106Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:b0615c55005493707ee7cfc9393ce5f99b0c3b74934621cf495d934475c6b71d","observation_id":"88775a8b-2dd5-4f57-a7a2-9a4e896417b1","resolution":{"observed_at":"2026-08-01T16:20:10.276106Z","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":"2026-08-01T16:20:10.280020Z","title":"F., et al.\\ 2015, , 449, 3, 2853","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.280020Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:fb8d53a62c79d37fdc3a1f5112e6326f64945d3ed6c30a64005f1ce5f2499665","observation_id":"0ab98fe3-0bee-4bcc-b93d-d8983fa57b13","resolution":{"observed_at":"2026-08-01T16:20:10.280020Z","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":"2026-08-01T16:20:10.283952Z","title":"doi:10.1051/0004-6361/201527570","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.283952Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:c13e7031a051c72aae0ef6150dc289d428bbbbc74ce6d2aca9928d219e2c8413","observation_id":"82c38e70-13bd-4a01-be97-f4d05edde220","resolution":{"observed_at":"2026-08-01T16:20:10.283952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.00543","last_updated":"2026-07-01T07:34:48Z","snapshot_observed_at":"2026-07-07T00:06:14.968413Z","submitted_at":"2026-07-01T07:34:48Z","title":"SPHEREx 0.75 to 5 $\\mu$m Spectra for a Sequence of Nearby Brown Dwarfs","version":1},"cited_work":{"arxiv_id":"2607.00543","doi":"10.48550/arxiv.2607.00543","metadata_source":"pith","pith_arxiv_id":"2607.00543","snapshot_observed_at":"2026-08-01T18:16:15.623592Z","title":"SPHEREx 0.75 to 5 $\\mu$m Spectra for a Sequence of Nearby Brown Dwarfs","venue":"astro-ph.SR","work_id":"50aa2824-213b-402d-803c-6e5c10a8e914","year":2026},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.287962Z"},"links":{"cited_paper":"/paper/2607.00543","citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:ce220c669b558b282ef8323b36b24d06ec2a24ccd0e02205617a5e6ead1cec0c","observation_id":"b9b504d2-48a3-4c7f-a24b-c1617dee0999","resolution":{"observed_at":"2026-08-01T16:24:14.979168Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+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":"2026-08-01T16:20:10.292264Z","title":"E.\\ 1955, , 121, 161","venue":null,"work_id":null,"year":1955},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.292264Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:f8f207e1e045a095220a44408248f799fc2c0e45989897c9a1873c1476f0e566","observation_id":"86592eda-4883-4e7f-b462-f4f2f89f22d6","resolution":{"observed_at":"2026-08-01T16:20:10.292264Z","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":"2026-08-01T16:20:10.296306Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.296306Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:a8b5055020a5495bd2cb5ea66f39c2af466b085defaf1ded72807f2d49dd2bfa","observation_id":"ba45b691-0d5e-494c-95d8-24d517d73dbe","resolution":{"observed_at":"2026-08-01T16:20:10.296306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.06374","last_updated":"2016-06-21T00:31:20Z","snapshot_observed_at":"2026-08-03T16:50:58.479827Z","submitted_at":"2016-06-21T00:31:20Z","title":"An Empirical Approach to Cosmological Galaxy Survey Simulation: Application to SPHEREx Low-Resolution Spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.06374","snapshot_observed_at":"2026-08-01T16:20:10.300628Z","title":"R., Capak, P., Masters, D., et al.\\ 2016, arXiv:1606.06374","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.300628Z"},"links":{"cited_paper":"/paper/1606.06374","citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:515e10bbc2011306fd5752fa555f1c514ffa3124eecb926c5243041b60deb9ec","observation_id":"3bb86814-f568-42df-96e8-d6807074e58a","resolution":{"observed_at":"2026-08-01T16:20:10.300628Z","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":"2026-08-01T16:20:10.304863Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.304863Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:38dd9efb4e4036ee428d8b957d18598371b4fe6e607016c90dfcaf8f47f32425","observation_id":"7e862ad7-b928-4582-80c9-dbff12b33786","resolution":{"observed_at":"2026-08-01T16:20:10.304863Z","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":"2026-08-01T16:20:10.309074Z","title":"doi:10.1093/mnras/stw2231","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.309074Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:bcfc2f585d22ee9dec15cda7ed5e95cc535f5263a108fb6c5fb9774a9595b43d","observation_id":"02e62ff0-fc8a-4961-9e9e-b7dbfcf8b4e5","resolution":{"observed_at":"2026-08-01T16:20:10.309074Z","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":"2026-08-01T16:20:10.313465Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.313465Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:ea64413d64e7f2a581c3a57431d5872b9cfb51fec0c0acac7f782bbedfe0361d","observation_id":"1ac866af-d4e9-4d44-b3b3-810693850438","resolution":{"observed_at":"2026-08-01T16:20:10.313465Z","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":"2026-08-01T16:20:10.317685Z","title":"doi:10.3847/1538-4365/aa72ed","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.317685Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:1ff92eee3037a85958c2729e976482ebd7cbc78183992568298027bc52bdc3f8","observation_id":"8ec48c7c-6105-4e7d-a8b6-a3ac9dcb261f","resolution":{"observed_at":"2026-08-01T16:20:10.317685Z","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":"2026-08-01T16:20:10.321828Z","title":"E., et al.\\ 2020, Nature Methods, 17, 261","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.321828Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:4c8da851075e07be1431d62ed06e72f2a01a30665a7523971b80ecc4e479ef3f","observation_id":"19904657-7088-4102-84ac-44424351a347","resolution":{"observed_at":"2026-08-01T16:20:10.321828Z","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":"2026-08-01T16:20:10.325952Z","title":"doi:10.1007/s10509-010-0458-z","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.325952Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:8bdffd2c6cdb2d202287b10d50335f554f438d68e4ac4ac52e76881069a20370","observation_id":"9778714f-a4bf-4b62-b4fd-75df433aada0","resolution":{"observed_at":"2026-08-01T16:20:10.325952Z","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":"2026-08-01T16:20:10.329947Z","title":"doi:10.1051/0004-6361:20011493","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.329947Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:31e68dd9c71133b0b09d3f4e5ee09cfbba698680e5600d104f491e8af1042ffb","observation_id":"47275748-0579-4f09-9e08-04d9624053fb","resolution":{"observed_at":"2026-08-01T16:20:10.329947Z","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":"2026-08-01T16:20:10.333893Z","title":"M., Maraston, C., Goddard, D., et al.\\ 2017, , 472, 4, 4297","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.333893Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:fad744761006157973e4216d96855cfc1172b54ebaf8adce81f5272da374fcde","observation_id":"2cd6953d-7d96-42c7-ba01-4588eb5bdfc0","resolution":{"observed_at":"2026-08-01T16:20:10.333893Z","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":"2026-08-01T16:20:10.337854Z","title":"L., Eisenhardt, P","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.337854Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:1f38036ad7b8cc7d3310e66ba8cd8b439e0b6101b2623e1686e7a880c81e7582","observation_id":"ff20dd61-dd20-4aa9-8979-d14de4d1f032","resolution":{"observed_at":"2026-08-01T16:20:10.337854Z","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":"2026-08-01T16:20:10.342252Z","title":"doi:10.3847/1538-4357/ab3ebc","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.342252Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:dabc44d0e6a56094dd5f98b0ea7cac702f3785e07e839936854049bcb8c5cc24","observation_id":"08523a9f-15e1-4cdc-9e8e-93ce559114d7","resolution":{"observed_at":"2026-08-01T16:20:10.342252Z","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":"2026-08-01T16:20:10.346469Z","title":"L., Crill, B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.346469Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:5b8def04ab2dd71fb9170a27ece4221fd3ca2a3b8a384f959770cb4df67c1c51","observation_id":"bedbba38-353d-45d9-bdb4-532f9450c638","resolution":{"observed_at":"2026-08-01T16:20:10.346469Z","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":"2026-08-01T16:20:10.350973Z","title":"doi:10.1093/mnras/sts126","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-01T16:20:10.350973Z"},"links":{"citing_paper":"/paper/2607.18048"},"observation_digest":"sha256:6533a7b07e5d8ab2a4d4f7124680a4b367c86fffe8e65201104201a913fcb851","observation_id":"43b21870-2ebc-452a-a628-9bb617f6f720","resolution":{"observed_at":"2026-08-01T16:20:10.350973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.18048","last_updated":"2026-07-20T15:18:49Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-09T19:02:03.200446Z","submitted_at":"2026-07-20T15:18:49Z","title":"Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations"},"reference_resolution":{"displayed":90,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":80,"verified_exact":9,"verified_fuzzy":0},"total_outbound_references":90},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 90 of 90 outbound references and 0 inbound Pith citation observations for arXiv:2607.18048."}