{"as_of":"2026-08-10T11:32:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:02448587d28567ab8317b63ab5d05cbd15916d5053739b5756b3b1150adbb150","coverage":[{"denominator":126,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T06:46:19.054759Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"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/2607.29455/citation-record","integrity":"/paper/2607.29455/integrity","json":"/paper/2607.29455/citation-record.json","paper":"/paper/2607.29455"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T06:46:18.212289Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.212289Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:ede4ffa9f89a1b10f54e9177aa1f3aa036cf0f357abde0b75c2cef5073f7aa6a","observation_id":"cb8941c0-97fd-432e-89f4-51af503ca286","resolution":{"observed_at":"2026-08-03T06:46:18.212289Z","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":"2026-08-03T06:46:18.218043Z","title":"NIST Atomic Spectra Database, NIST Standard Reference Database 78 , publisher =","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.218043Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1ab4837aa1ddc3a49b370964fff4b6d15a20844d2424ac11bb4fefa98911ecbf","observation_id":"0e57419d-dc3f-47d1-9009-a4fc067dd323","resolution":{"observed_at":"2026-08-03T06:46:18.218043Z","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":"2026-08-03T06:46:18.223066Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.223066Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:bdac8f98b006a9fd1db71ee67da7228d9750a3398e2d1fdc7594dd5c618d974a","observation_id":"407071cb-c437-470a-8c93-bf43274b654b","resolution":{"observed_at":"2026-08-03T06:46:18.223066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.09824","last_updated":"2026-04-17T14:19:49Z","snapshot_observed_at":"2026-07-06T22:29:01.585836Z","submitted_at":"2025-09-11T19:51:18Z","title":"Sensitivity of spectral lines to granulation: The Sun","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.09824","snapshot_observed_at":"2026-08-03T06:46:18.234936Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.234936Z"},"links":{"cited_paper":"/paper/2509.09824","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1b809bfd937d32fd3b180bcde6b7d98cda63a2f08893eb41b7f549048add4a78","observation_id":"a14e48a6-d1d7-425b-9d5a-b1e3af0a283f","resolution":{"observed_at":"2026-08-03T06:46:18.234936Z","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":"2026-08-03T06:46:18.256073Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.256073Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:839b915d62660b9c94a6a4592eb00c1074947cfaee83ad87614680328abdf1f6","observation_id":"c063bfbe-50ca-47be-9938-c40c1f4edddf","resolution":{"observed_at":"2026-08-03T06:46:18.256073Z","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":"2026-08-03T06:46:18.277569Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.277569Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:2caccd35d4d0a0a596449780c4bb06eb668639b23eb7ec1727c640576f26d9d3","observation_id":"47437e21-04c1-48e9-ae64-47e97774d4ad","resolution":{"observed_at":"2026-08-03T06:46:18.277569Z","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":"2026-08-03T06:46:18.291940Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.291940Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:0743ba8d8fc1ef7dd757c07db9bca31c688de31a11dd16ea92afd3af4e9dee85","observation_id":"ae48848f-25b2-40a6-86ab-7c84221ae4df","resolution":{"observed_at":"2026-08-03T06:46:18.291940Z","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":"2026-08-03T06:46:18.302115Z","title":", year = 2015, month = may, volume =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.302115Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:bf5bfaff59d5e05529e469a9604972e1cd540fbd86ce66fa6667636b9840e002","observation_id":"ef4dd8d3-7535-4e59-9d89-1612efc64908","resolution":{"observed_at":"2026-08-03T06:46:18.302115Z","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":"2026-08-03T06:46:18.306711Z","title":"2026 , note =","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.306711Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:e01fc20a7233106974834bbd0860c7847297e6fa18305c6c15f527ccb48d0405","observation_id":"e5bd9e9f-c27d-46d9-891a-364b6bdfb783","resolution":{"observed_at":"2026-08-03T06:46:18.306711Z","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":"2026-08-03T06:46:18.311389Z","title":"The Open Journal of Astrophysics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.311389Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1d8e233b024a299f2ff64628981bd1220cb1afc57e0ce0a1179c434a99aee606","observation_id":"3a7bc47b-0e71-4e3b-82e9-dd5caa2aa7f5","resolution":{"observed_at":"2026-08-03T06:46:18.311389Z","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":"2026-08-03T06:46:18.325811Z","title":"Main-sequence stars with solar metallicity","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.325811Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:595263fd093e236de0f711f1ce87d93ce56859f481e435148c43169abb88633d","observation_id":"15a841b5-e0fc-469d-84d6-d758f8b897cf","resolution":{"observed_at":"2026-08-03T06:46:18.325811Z","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":"10.1007/bf00712873","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Solar Physics","work_id":"2244e523-f35c-42e0-98dc-580fd45d0e6e","year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.337681Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:9315f346d007b13ed8e7a9e0cffce24334dfa737fa0eef7c60a6684da92704b9","observation_id":"af5d7705-61d4-4fc4-9b4c-1a96b564f63b","resolution":{"observed_at":"2026-08-03T06:49:08.572942Z","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":{"arxiv_id":"2001.01093","last_updated":"2020-01-30T01:48:25Z","snapshot_observed_at":"2026-08-08T21:17:06.640039Z","submitted_at":"2020-01-04T16:14:44Z","title":"Testing the solar activity paradigm in the context of exoplanet transits","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.01093","snapshot_observed_at":"2026-08-03T06:46:18.342183Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.342183Z"},"links":{"cited_paper":"/paper/2001.01093","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:4a08c7e62b9bd8e3661723358d685926a8359709eb9fbc8810ca3e06108625d0","observation_id":"ac1e6f7f-4c1b-4329-adc6-f1d426dbc17a","resolution":{"observed_at":"2026-08-03T06:46:18.342183Z","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":"2026-08-03T06:46:18.347780Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.347780Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:a9b6c25485d4280c5545b3f6e05ead44727171d85b3b2b08b86070dc07fdeed4","observation_id":"f000c472-720e-42c4-8921-5ae49c4a1878","resolution":{"observed_at":"2026-08-03T06:46:18.347780Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.13025","last_updated":"2025-07-17T11:52:50Z","snapshot_observed_at":"2026-08-06T16:30:04.895304Z","submitted_at":"2025-07-17T11:52:50Z","title":"An Atlas of Spectroheliograms from 3641 to 6600 \\AA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.13025","snapshot_observed_at":"2026-08-03T06:46:18.351983Z","title":"RNAAS , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.351983Z"},"links":{"cited_paper":"/paper/2507.13025","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:8dc165601315e58138ad5324c76c664f2ce0ad0e9984ae42fcb2a96a522efc51","observation_id":"f6944537-6520-4e7c-aa7c-f6f1cf71dfc3","resolution":{"observed_at":"2026-08-03T06:46:18.351983Z","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":"2026-08-03T06:46:18.356836Z","title":"Photoniques , year = 2023, month = jul, volume =","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.356836Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:2d77eb3a47f5debd0795e14371f7ad2be4b68a9c5d56c73bd2b92b9c5cc4744d","observation_id":"cb165aaa-c658-44c4-9fcc-b5e2481237d1","resolution":{"observed_at":"2026-08-03T06:46:18.356836Z","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":"2026-08-03T06:46:18.361184Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.361184Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:4e28fe20862002e22f1bc903d6f545e065349b42eb4dde5fe10af3abe44e6f2e","observation_id":"6683e1b9-2294-45db-a7a6-1d2dd564e4fd","resolution":{"observed_at":"2026-08-03T06:46:18.361184Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.00475","last_updated":"2021-06-30T10:58:51Z","snapshot_observed_at":"2026-08-04T10:26:48.529616Z","submitted_at":"2021-06-30T10:58:51Z","title":"The Lightweaver Framework for NLTE Radiative Transfer in Python","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.00475","snapshot_observed_at":"2026-08-03T06:46:18.365490Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.365490Z"},"links":{"cited_paper":"/paper/2107.00475","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1fe2236b6667f77da03b4c4eb55f5ec41286b636fb479bb0b207de2c5101bc8a","observation_id":"fcd3c412-67cb-4c9d-ae9b-cb17e5f17632","resolution":{"observed_at":"2026-08-03T06:46:18.365490Z","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":"2026-08-03T06:46:18.371359Z","title":"doi:10.1017/9781009082136 , adsurl =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.371359Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:08fdbcf0f3c3fb00cf66ec747db1d463ce76c4fc7f75ca16faf806a0717b2c3f","observation_id":"b385a120-0919-4ef6-b72f-756164a28c99","resolution":{"observed_at":"2026-08-03T06:46:18.371359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.08441","last_updated":"2019-02-01T16:21:03Z","snapshot_observed_at":"2026-07-06T07:09:21.768083Z","submitted_at":"2018-10-19T11:07:04Z","title":"STiC -- A multi-atom non-LTE PRD inversion code for full-Stokes solar observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.08441","snapshot_observed_at":"2026-08-03T06:46:18.376014Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.376014Z"},"links":{"cited_paper":"/paper/1810.08441","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:3256203eb1e6ccc41eb892a22173eac6307be0fa019f7dda68010128c4ae133d","observation_id":"1d1edb59-5c28-460d-82a6-c62c8dc0aba6","resolution":{"observed_at":"2026-08-03T06:46:18.376014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09830","last_updated":"2020-04-21T08:54:39Z","snapshot_observed_at":"2026-08-06T20:14:53.062835Z","submitted_at":"2020-04-21T08:54:39Z","title":"The spectral impact of magnetic activity on disk-integrated HARPS-N solar observations: exploring new activity indicators","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09830","snapshot_observed_at":"2026-08-03T06:46:18.389409Z","title":", keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.389409Z"},"links":{"cited_paper":"/paper/2004.09830","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:6080cbc9e480d3c39fef9ea5636222bb1d81a5c72aabffca569e557df53fad29","observation_id":"fb21d708-efd5-486d-8b96-cf8c9372b56f","resolution":{"observed_at":"2026-08-03T06:46:18.389409Z","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":"2026-08-03T06:46:18.407254Z","title":"Ground-based and Airborne Instrumentation for Astronomy IV , year = 2012, editor =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.407254Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:e48c5907d0a863a562824fc99ab510d553556b37700ea028b85aa6c02f1664d1","observation_id":"654dfb3a-20bc-4ba6-9f6d-09b97db1f310","resolution":{"observed_at":"2026-08-03T06:46:18.407254Z","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":"2026-08-03T06:46:18.411744Z","title":"Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II , year = 2016, editor =","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.411744Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:f12b344cd4fc42ca33eb85c145a7e51d0237f067a3bd9da87f2ba5ba022c92e7","observation_id":"05dcbfd0-67cd-48dd-a834-ecc9be092337","resolution":{"observed_at":"2026-08-03T06:46:18.411744Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.02267","last_updated":"2015-11-07T00:00:03Z","snapshot_observed_at":"2026-08-04T16:45:07.288505Z","submitted_at":"2015-11-07T00:00:03Z","title":"HARPS-N observes the Sun as a star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.02267","snapshot_observed_at":"2026-08-03T06:46:18.416231Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.416231Z"},"links":{"cited_paper":"/paper/1511.02267","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:f4ac5ed7df924f93712ac15cead17b79b9d5c33a543243d9a0cd799ba16cab7a","observation_id":"f24eb591-6ba5-47de-9fad-5e65ad0ae481","resolution":{"observed_at":"2026-08-03T06:46:18.416231Z","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":"2026-08-03T06:46:18.421417Z","title":"Equations, methods, and results of the MURaM code","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.421417Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:652f3876d5b71ced7140fc01db5207479e93ecf2d1077752878506f7b1be2cbc","observation_id":"408971ca-60a3-471a-be76-cdb4b9cece9f","resolution":{"observed_at":"2026-08-03T06:46:18.421417Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.2066","last_updated":"2014-07-08T12:37:19Z","snapshot_observed_at":"2026-07-06T03:48:20.911933Z","submitted_at":"2014-07-08T12:37:19Z","title":"Impact of occultations of stellar active regions on transmission spectra: Can occultation of a plage mimic the signature of a blue sky?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.2066","snapshot_observed_at":"2026-08-03T06:46:18.428443Z","title":"Can occultation of a plage mimic the signature of a blue sky?","venue":null,"work_id":null,"year":2066},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.428443Z"},"links":{"cited_paper":"/paper/1407.2066","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:841a0e56693cf894a914dba46caf0555c055e5e2028fd477d8af5ea089d2d45d","observation_id":"1ce20560-9e86-4f72-b546-e82f7f5d15f9","resolution":{"observed_at":"2026-08-03T06:46:18.428443Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.05691","last_updated":"2018-01-24T18:00:59Z","snapshot_observed_at":"2026-08-10T03:59:02.416052Z","submitted_at":"2017-11-15T17:39:59Z","title":"The Transit Light Source Effect: False Spectral Features and Incorrect Densities for M-dwarf Transiting Planets","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.05691","snapshot_observed_at":"2026-08-03T06:46:18.433592Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.433592Z"},"links":{"cited_paper":"/paper/1711.05691","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:35a192c2c28f194fd2fdf27b5d7caf5c192674999a824371e9a73b53a4dc7c55","observation_id":"12ede7a0-aca4-4aac-bea1-3992cf27fb53","resolution":{"observed_at":"2026-08-03T06:46:18.433592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.01647","last_updated":"2017-02-06T15:11:26Z","snapshot_observed_at":"2026-07-06T05:28:58.882304Z","submitted_at":"2017-02-06T15:11:26Z","title":"The Changing Face of $\\alpha$ Centauri B: Probing plage and stellar activity in K-dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.01647","snapshot_observed_at":"2026-08-03T06:46:18.438018Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.438018Z"},"links":{"cited_paper":"/paper/1702.01647","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:c08b1399cd7a5f748b4ede90c02d3430b50592b3b485d97b102cf57f992d6690","observation_id":"8394081e-4e78-4592-a4f4-826d1522ef3e","resolution":{"observed_at":"2026-08-03T06:46:18.438018Z","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":"2026-08-03T06:46:18.442562Z","title":", year = 1995, month = nov, volume =","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.442562Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:2918b344d6258afe1618e8892911ee6c4c027c0be84a6a810a00672fd4b490c3","observation_id":"39e11ddb-31a6-46ad-a0d0-1648157b3ff0","resolution":{"observed_at":"2026-08-03T06:46:18.442562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.1638","last_updated":"2010-01-15T08:55:17Z","snapshot_observed_at":"2026-08-02T22:42:50.697525Z","submitted_at":"2010-01-11T11:50:52Z","title":"Using the Sun to estimate Earth-like planets detection capabilities II. Impact of plages","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.1638","snapshot_observed_at":"2026-08-03T06:46:18.454744Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.454744Z"},"links":{"cited_paper":"/paper/1001.1638","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:3da254444e9457851c90a59ca860fc7a5ecfeb3a9984d453ecfd3598a87e6c49","observation_id":"e204ec91-9694-406c-b7c2-adb1d106368a","resolution":{"observed_at":"2026-08-03T06:46:18.454744Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.16076","last_updated":"2023-11-27T18:47:04Z","snapshot_observed_at":"2026-08-03T12:39:13.666778Z","submitted_at":"2023-11-27T18:47:04Z","title":"The magnetically quiet solar surface dominates HARPS-N solar RVs during low activity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.16076","snapshot_observed_at":"2026-08-03T06:46:18.465703Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.465703Z"},"links":{"cited_paper":"/paper/2311.16076","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:568f871088aa592e8aa1ddbb4ecd77008a6291430e97f4e14266774b230e3650","observation_id":"92479caf-8145-414b-9759-037ec8bdf6dd","resolution":{"observed_at":"2026-08-03T06:46:18.465703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.15926","last_updated":"2023-10-24T15:25:59Z","snapshot_observed_at":"2026-07-06T16:37:54.347934Z","submitted_at":"2023-10-24T15:25:59Z","title":"Stellar surface information from the Ca II H&K lines I. Intensity profiles of the solar activity components","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.15926","snapshot_observed_at":"2026-08-03T06:46:18.470067Z","title":"Intensity profiles of the solar activity components","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.470067Z"},"links":{"cited_paper":"/paper/2310.15926","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:eb4a9195d928b90dbc7496a9b5c46e51652fa63d3eca14e12abd0e88f1cf7d09","observation_id":"42a65233-5004-4af4-a02f-9d5945928b16","resolution":{"observed_at":"2026-08-03T06:46:18.470067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05651","last_updated":"2016-01-22T17:01:53Z","snapshot_observed_at":"2026-07-06T04:43:35.671013Z","submitted_at":"2016-01-21T14:20:00Z","title":"The Sun as a planet-host star: Proxies from SDO images for HARPS radial-velocity variations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.05651","snapshot_observed_at":"2026-08-03T06:46:18.475518Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.475518Z"},"links":{"cited_paper":"/paper/1601.05651","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:a0352a9ee97655c7b678d162514e1362082fe77b3f30a022b7fb7ac6575d0303","observation_id":"ebcdee3c-5bd8-4a96-863f-77164f5fd65b","resolution":{"observed_at":"2026-08-03T06:46:18.475518Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04184","last_updated":"2019-02-11T23:46:36Z","snapshot_observed_at":"2026-07-06T07:32:30.290620Z","submitted_at":"2019-02-11T23:46:36Z","title":"HARPS-N Solar Radial-Velocity Variations Are Dominated By Large, Bright Magnetic Regions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04184","snapshot_observed_at":"2026-08-03T06:46:18.479959Z","title":", keywords =","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.479959Z"},"links":{"cited_paper":"/paper/1902.04184","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1aa3c720a32ec35f2088d494fce3dce784004e3a1e39d4a15aa76ce5d25edf08","observation_id":"c905dfff-46b9-4de7-916a-4ff1af53a0cc","resolution":{"observed_at":"2026-08-03T06:46:18.479959Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5632","last_updated":"2013-04-24T11:04:19Z","snapshot_observed_at":"2026-07-06T03:09:25.962992Z","submitted_at":"2013-03-22T14:48:27Z","title":"A new extensive library of PHOENIX stellar atmospheres and synthetic spectra","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5632","snapshot_observed_at":"2026-08-03T06:46:18.484165Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.484165Z"},"links":{"cited_paper":"/paper/1303.5632","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:79db741852b099fa04fa3cd032c95ea716fdb0cc250e7bbad490c84500a31a40","observation_id":"0aef48c3-d2c1-4fa8-ba5f-a88d8a34a085","resolution":{"observed_at":"2026-08-03T06:46:18.484165Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.3594","last_updated":"2014-09-11T21:01:04Z","snapshot_observed_at":"2026-07-06T03:54:16.458401Z","submitted_at":"2014-09-11T21:01:04Z","title":"SOAP 2.0: A tool to estimate the photometric and radial velocity variations induced by stellar spots and plages","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.3594","snapshot_observed_at":"2026-08-03T06:46:18.488160Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.488160Z"},"links":{"cited_paper":"/paper/1409.3594","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:7c1c776bff1bdff80dcc2b1c72a7e1fe04978eb9139310ff3136a38c6207bd69","observation_id":"d7d7e21a-ce8a-4e26-92be-faa83eafc089","resolution":{"observed_at":"2026-08-03T06:46:18.488160Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.04611","last_updated":"2016-08-16T14:23:47Z","snapshot_observed_at":"2026-07-06T05:07:10.046451Z","submitted_at":"2016-08-16T14:23:47Z","title":"HARPS3 for a Roboticized Isaac Newton Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.04611","snapshot_observed_at":"2026-08-03T06:46:18.496765Z","title":"Ground-based and Airborne Instrumentation for Astronomy VI , year = 2016, editor =","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.496765Z"},"links":{"cited_paper":"/paper/1608.04611","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:6ce9cd8d6b94b1a567d7a77e718a4c55f85844b92bb8c0b239dde602c426ee79","observation_id":"4e860892-31d5-44b2-9ac7-c93b16b4145a","resolution":{"observed_at":"2026-08-03T06:46:18.496765Z","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":"2026-08-03T06:46:18.501250Z","title":"Optical and IR Telescope Instrumentation and Detectors , year = 2000, editor =","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.501250Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:71fb4507ed78666a285cf29ab765b7df5b5cda5cca11a9105ed91f03c3653802","observation_id":"90225ec2-75c0-4a11-a1fa-d9413cc395cf","resolution":{"observed_at":"2026-08-03T06:46:18.501250Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.07304","last_updated":"2015-06-24T10:20:23Z","snapshot_observed_at":"2026-07-06T04:21:52.011550Z","submitted_at":"2015-06-24T10:20:23Z","title":"A Gaussian process framework for modelling stellar activity signals in radial velocity data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.07304","snapshot_observed_at":"2026-08-03T06:46:18.505353Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.505353Z"},"links":{"cited_paper":"/paper/1506.07304","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:9f3af509cc428ddc13eebdae551b64bdab054104c89be3bd82dfc05f70791821","observation_id":"f626c717-e57a-4e22-8fe7-502c7f7bf35c","resolution":{"observed_at":"2026-08-03T06:46:18.505353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.05810","last_updated":"2022-04-12T13:48:29Z","snapshot_observed_at":"2026-07-06T12:59:35.107673Z","submitted_at":"2022-04-12T13:48:29Z","title":"Into the Depths: a new activity metric for high-precision radial velocity measurements based on line depth variations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.05810","snapshot_observed_at":"2026-08-03T06:46:18.510438Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.510438Z"},"links":{"cited_paper":"/paper/2204.05810","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:e2816d540e70104a2a627133e5a6ecc697fe3cdb38ca209e3684c07cf879279f","observation_id":"bfede1c9-3260-4cf0-a7f1-c0bd3ba66a3c","resolution":{"observed_at":"2026-08-03T06:46:18.510438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12065","last_updated":"2024-05-22T12:51:07Z","snapshot_observed_at":"2026-07-30T22:52:46.073828Z","submitted_at":"2024-05-20T14:36:52Z","title":"Investigating stellar activity through eight years of Sun-as-a-star observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12065","snapshot_observed_at":"2026-08-03T06:46:18.517732Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.517732Z"},"links":{"cited_paper":"/paper/2405.12065","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:aa3b2bcda950147a8b3dab5481f2e03055494eb711cb840079824ce62571a5b1","observation_id":"a4bb4ace-7d16-4b63-bf7b-566609db22a5","resolution":{"observed_at":"2026-08-03T06:46:18.517732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.0696","last_updated":"2014-03-04T13:57:09Z","snapshot_observed_at":"2026-07-06T03:24:36.787347Z","submitted_at":"2013-10-02T13:17:06Z","title":"The PLATO 2.0 Mission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.0696","snapshot_observed_at":"2026-08-03T06:46:18.522244Z","title":"Experimental Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.522244Z"},"links":{"cited_paper":"/paper/1310.0696","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:b025c6fb888f1c187734c6fed6f7cf482253aa0398859a9a43a5fc5d20d9adb1","observation_id":"9dc512ff-99a2-4d32-a9aa-1bec488f8b5e","resolution":{"observed_at":"2026-08-03T06:46:18.522244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.05447","last_updated":"2024-11-18T16:42:09Z","snapshot_observed_at":"2026-08-07T16:30:01.307456Z","submitted_at":"2024-06-08T12:06:49Z","title":"The PLATO Mission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.05447","snapshot_observed_at":"2026-08-03T06:46:18.526831Z","title":"Experimental Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.526831Z"},"links":{"cited_paper":"/paper/2406.05447","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:62ef71c56b532e47f0cb50f0dfac582e770a600d61aec9482907942143ecdee4","observation_id":"623e7b65-2139-4357-a66e-e58e49d5032b","resolution":{"observed_at":"2026-08-03T06:46:18.526831Z","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":"2026-08-03T06:46:18.532711Z","title":", year = 2019, month = aug, volume =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.532711Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:4292e88752720c721dadfa14e5eb5430fd5510cee332862e0c48ca47332247a2","observation_id":"bbd83764-136e-4488-9ddc-529191599502","resolution":{"observed_at":"2026-08-03T06:46:18.532711Z","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":"10.5802/crphys.140","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Comptes Rendus Physique , year = 2024, month = jan, volume =","venue":"Comptes Rendus Physique","work_id":"79c367ab-85c1-4df2-9e8f-226993ee2dea","year":2024},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.537288Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:d9ab87606fd4d0353266ad7e12b470993c8f47fd0b7dea070311e7e9c6f01d58","observation_id":"11699151-f571-4e17-94eb-22a0429474e4","resolution":{"observed_at":"2026-08-03T06:49:08.282522Z","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":{"arxiv_id":"1511.06717","last_updated":"2015-11-20T18:13:50Z","snapshot_observed_at":"2026-07-06T04:37:16.423248Z","submitted_at":"2015-11-20T18:13:50Z","title":"Modelling the photosphere of active stars for planet detection and characterization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.06717","snapshot_observed_at":"2026-08-03T06:46:18.541398Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.541398Z"},"links":{"cited_paper":"/paper/1511.06717","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:27f6b4f046dad40c9d0d46a62ad785d594fd2d5db0a748624062d8862bc133e7","observation_id":"1939fe64-e8bb-4bbd-9030-8ccec1648889","resolution":{"observed_at":"2026-08-03T06:46:18.541398Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.04259","last_updated":"2023-01-11T01:45:16Z","snapshot_observed_at":"2026-08-05T19:27:06.885523Z","submitted_at":"2023-01-11T01:45:16Z","title":"SOAP-GPU: Efficient Spectral Modelling of Stellar Activity Using Graphical Processing Units","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.04259","snapshot_observed_at":"2026-08-03T06:46:18.546288Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.546288Z"},"links":{"cited_paper":"/paper/2301.04259","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:fdeda3b5a86c845129cad278bef3d0024bf481661a0d96b3a9d4e227489a39e3","observation_id":"e0b29300-af16-43e0-90fc-f04afe427f30","resolution":{"observed_at":"2026-08-03T06:46:18.546288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13500","last_updated":"2024-12-18T04:45:24Z","snapshot_observed_at":"2026-07-06T20:09:00.586421Z","submitted_at":"2024-12-18T04:45:24Z","title":"Precise and efficient modeling of stellar-activity-affected solar spectra using SOAP-GPU","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.13500","snapshot_observed_at":"2026-08-03T06:46:18.551578Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.551578Z"},"links":{"cited_paper":"/paper/2412.13500","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:5bc51b66238946adfd59f0bd9f511336c00cea76aa269cce4e7514af8bd416da","observation_id":"ff5ffef6-94d4-4d73-8fd5-8ec0b014b761","resolution":{"observed_at":"2026-08-03T06:46:18.551578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.10035","last_updated":"2024-12-13T10:52:31Z","snapshot_observed_at":"2026-08-05T07:08:29.356286Z","submitted_at":"2024-12-13T10:52:31Z","title":"PAStar: a model for stellar surface from the Sun to active stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.10035","snapshot_observed_at":"2026-08-03T06:46:18.557872Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.557872Z"},"links":{"cited_paper":"/paper/2412.10035","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:4a90a7ede6086022501f2409bdb5e0f442f74dceae3de9b72aef4cb3a690a433","observation_id":"209d6452-4afd-40a2-95f1-f680579d5b95","resolution":{"observed_at":"2026-08-03T06:46:18.557872Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9808182","last_updated":"1998-08-18T18:18:38Z","snapshot_observed_at":"2026-08-03T22:43:07.072226Z","submitted_at":"1998-08-18T18:18:38Z","title":"Numerical Solution of the Expanding Stellar Atmosphere Problem","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9808182","snapshot_observed_at":"2026-08-03T06:46:18.563233Z","title":"Journal of Computational and Applied Mathematics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.563233Z"},"links":{"cited_paper":"/paper/astro-ph/9808182","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:ba8ea1b1ac75cb859507cc1573ea32118e54051297ca6ce3b78f25e00d0928d6","observation_id":"23dc06a8-5f0d-44f8-9a37-94f8c6dbb8bd","resolution":{"observed_at":"2026-08-03T06:46:18.563233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.2505","last_updated":"2007-11-15T20:36:02Z","snapshot_observed_at":"2026-07-06T01:32:54.709948Z","submitted_at":"2007-11-15T20:36:02Z","title":"Star Spot Induced Radial Velocity Variability in LkCa 19","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.2505","snapshot_observed_at":"2026-08-03T06:46:18.567707Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.567707Z"},"links":{"cited_paper":"/paper/0711.2505","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:2896fdfca32c78d55051ef5f1d7a8839d7b5e05de97559f0152087d9ae99887d","observation_id":"83f935be-b967-4f86-bedc-8837b891ff4b","resolution":{"observed_at":"2026-08-03T06:46:18.567707Z","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":"2026-08-03T06:46:18.571952Z","title":"AAS/Division for Extreme Solar Systems Abstracts , year = 2024, series =","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.571952Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:c1a6798244a3ea8465117abd802d21c1e8410f984e7158561abf8ed6c712271e","observation_id":"7a2a352f-aca3-488b-b44c-7467843823e4","resolution":{"observed_at":"2026-08-03T06:46:18.571952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.2616","last_updated":"2010-10-13T09:53:19Z","snapshot_observed_at":"2026-07-06T02:17:31.240546Z","submitted_at":"2010-10-13T09:53:19Z","title":"Planetary detection limits taking into account stellar noise. I. Observational strategies to reduce stellar oscillation and granulation effects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.2616","snapshot_observed_at":"2026-08-03T06:46:18.585864Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.585864Z"},"links":{"cited_paper":"/paper/1010.2616","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:c650795655e00ff3980d9aab4b82e5403a1e84d20876d313fb892ef2bb88c472","observation_id":"cc11e295-ba2a-40f4-bebf-6b013d949596","resolution":{"observed_at":"2026-08-03T06:46:18.585864Z","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":"2026-08-03T06:46:18.598173Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.598173Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1bdd8ef034379a3590136be62c88e14747862657eafb16cad83653fb4c5235a8","observation_id":"b4a22cc5-d99b-4572-9af8-04a8eab89714","resolution":{"observed_at":"2026-08-03T06:46:18.598173Z","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":"2026-08-03T06:46:18.603241Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.603241Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:960aeb7afe99b86d0469250601af8eb82e123a8d73835677e5d6633b3fbe4c33","observation_id":"7572add5-86ab-4118-aed0-83d078a86cef","resolution":{"observed_at":"2026-08-03T06:46:18.603241Z","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":"2026-08-03T06:46:18.616456Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.616456Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:d6576325e55d4964d23c39ce5cfddfa67ed9ff8200b114470dce9120a5a980f7","observation_id":"365e5338-60cc-4c50-8e71-13b399b83ec7","resolution":{"observed_at":"2026-08-03T06:46:18.616456Z","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":"2026-08-03T06:46:18.638066Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.638066Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:beff258203a23af7d49f42c718f7226c8d8e00f9116d51d6fbb8e89df7e3f503","observation_id":"5330a7b3-c790-4646-9c6d-4dfa05873c9d","resolution":{"observed_at":"2026-08-03T06:46:18.638066Z","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":"2026-08-03T06:46:18.654748Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.654748Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:40e5df5e3d99dd2d3cdefa6e019d33fbbf4391d4508e7d6e6ac78f7b5760a607","observation_id":"4db01b70-68ae-4fa7-8b48-11efdde64c86","resolution":{"observed_at":"2026-08-03T06:46:18.654748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.02368","last_updated":"2016-06-08T01:21:41Z","snapshot_observed_at":"2026-07-06T04:59:09.337012Z","submitted_at":"2016-06-08T01:21:41Z","title":"Observables Processing for the Helioseismic and Magnetic Imager Instrument on the Solar Dynamics Observatory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.02368","snapshot_observed_at":"2026-08-03T06:46:18.664746Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.664746Z"},"links":{"cited_paper":"/paper/1606.02368","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1c92bf9e7bc41864a14914ec6f4f2e78f8033db91d8072747ecedb1ff0d9894e","observation_id":"5b90e401-a6f4-4879-99e1-3fa7205666d9","resolution":{"observed_at":"2026-08-03T06:46:18.664746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.3168","last_updated":"2010-03-09T23:07:44Z","snapshot_observed_at":"2026-07-06T02:08:19.846136Z","submitted_at":"2010-02-16T21:02:20Z","title":"Transit Probabilities for Stars With Stellar Inclination Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.3168","snapshot_observed_at":"2026-08-03T06:46:18.704752Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.704752Z"},"links":{"cited_paper":"/paper/1002.3168","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:db3c6a578c905e91e36699ffbe22c3dbe42084f63f286c0052686f9e21e6ecdc","observation_id":"d52047f8-94f1-4611-9e77-1fa72895fbe8","resolution":{"observed_at":"2026-08-03T06:46:18.704752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.07939","last_updated":"2016-02-27T12:45:09Z","snapshot_observed_at":"2026-08-10T08:51:19.034686Z","submitted_at":"2016-02-25T14:12:15Z","title":"State of the Field: Extreme Precision Radial Velocities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.07939","snapshot_observed_at":"2026-08-03T06:46:18.719916Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.719916Z"},"links":{"cited_paper":"/paper/1602.07939","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:118f8e4e62d3e3bde53792311807750c813c64561d444a4dc042a8b5e8cf2ba4","observation_id":"f2432a51-e28a-4594-800d-aff5ec3291a4","resolution":{"observed_at":"2026-08-03T06:46:18.719916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.14291","last_updated":"2021-07-29T19:29:59Z","snapshot_observed_at":"2026-08-09T07:29:42.262804Z","submitted_at":"2021-07-29T19:29:59Z","title":"Extreme Precision Radial Velocity Working Group Final Report","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.14291","snapshot_observed_at":"2026-08-03T06:46:18.724559Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.724559Z"},"links":{"cited_paper":"/paper/2107.14291","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:62130bf414e3fcf1ca40c50d8316d18605cec09043ee30e5cef62f0764b74190","observation_id":"4ab32ff4-8eef-4ef6-9b42-78ebde66313b","resolution":{"observed_at":"2026-08-03T06:46:18.724559Z","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":"2026-08-03T06:46:18.734627Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.734627Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:747b3700940cd3d1e60f18861f03b1cbdc3c6a9e4754c3ee22e076c73d75a6cc","observation_id":"0690fa7e-8761-44ee-9760-66e7ba1312de","resolution":{"observed_at":"2026-08-03T06:46:18.734627Z","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":"2026-08-03T06:46:18.741650Z","title":", keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.741650Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:57afa1a2aac002fa8c7b14f29c5dd8bba78ef6c9a075cc85d8af1a96122e5699","observation_id":"fb1831a3-f9c9-48cf-b5a7-33f1650cc5a0","resolution":{"observed_at":"2026-08-03T06:46:18.741650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.12512","last_updated":"2022-04-26T18:00:05Z","snapshot_observed_at":"2026-08-01T16:52:05.880257Z","submitted_at":"2022-04-26T18:00:05Z","title":"Impact of Correlated Noise on the Mass Precision of Earth-analog Planets in Radial Velocity Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.12512","snapshot_observed_at":"2026-08-03T06:46:18.746677Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.746677Z"},"links":{"cited_paper":"/paper/2204.12512","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:03e8ccbc4c048c9ac4df2edc000b528fa83ba117569556360dbad1e0359cc94b","observation_id":"39f73e60-a253-4fad-977e-a86079ee0046","resolution":{"observed_at":"2026-08-03T06:46:18.746677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.05970","last_updated":"2021-06-03T03:00:15Z","snapshot_observed_at":"2026-08-04T09:03:40.342573Z","submitted_at":"2020-08-13T15:36:48Z","title":"Detection Limits of Low-mass, Long-period Exoplanets Using Gaussian Processes Applied to HARPS-N Solar RVs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.05970","snapshot_observed_at":"2026-08-03T06:46:18.752459Z","title":", keywords =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.752459Z"},"links":{"cited_paper":"/paper/2008.05970","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:91a997993e12d7349802de065a74190c1764ca448b424e504eeb9bf496c50243","observation_id":"da5afb54-db79-4be1-8d77-e1adc7c97018","resolution":{"observed_at":"2026-08-03T06:46:18.752459Z","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":"2026-08-03T06:46:18.772522Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.772522Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:c223011e9fb68e4d6a6770d8d6f834c1a06c7527fd21be2331ef82056d8736c0","observation_id":"27981031-fd88-4261-8759-05a1df067cde","resolution":{"observed_at":"2026-08-03T06:46:18.772522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03373","last_updated":"2024-02-01T19:07:53Z","snapshot_observed_at":"2026-07-06T16:15:27.717075Z","submitted_at":"2023-09-06T21:48:01Z","title":"A comparative study of two X2.2 and X9.3 solar flares observed with HARPS-N: Reconciling Sun-as-a-star spectroscopy and high-spatial resolution solar observations in the context of the solar-stellar connection","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.03373","snapshot_observed_at":"2026-08-03T06:46:18.780513Z","title":"Reconciling Sun-as-a-star spectroscopy and high-spatial resolution solar observations in the context of the solar-stellar connection","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.780513Z"},"links":{"cited_paper":"/paper/2309.03373","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:b135ffec6be1b898d0f98ae479abcaa3a38ccfe68c67443adf0ae236ce0fb1dc","observation_id":"fe8dbb56-d2d9-4b54-b19b-2c49136d40fc","resolution":{"observed_at":"2026-08-03T06:46:18.780513Z","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":"10.5281/zenodo.5130046","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Posters from the TESS Science Conference II (TSC2) , year = 2021, month = jul, eid =","venue":"Zenodo (CERN European Organization for Nuclear Research)","work_id":"298b70ea-cd2e-4825-8cd8-09193c9cbeff","year":2021},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.786270Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:56aa8f8c2cced9b2877c0c983aa1893753df34c164eee39a92919a70f77c66fc","observation_id":"78ade741-cd15-4ffc-b86b-c17f164929d8","resolution":{"observed_at":"2026-08-03T06:49:07.923417Z","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":"2026-08-03T06:46:18.794978Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.794978Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:0c252ccfe565ed0624ab4529cd7cea2f955e8dc3d66e3bcb96491684f5f47a7a","observation_id":"dca3f879-51b8-4165-b0af-3a055bede7df","resolution":{"observed_at":"2026-08-03T06:46:18.794978Z","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":"2026-08-03T06:46:18.811052Z","title":"2015 , note =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.811052Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:bcfc2f84253667c203be3723c6b52849da4e11330d67bbb24ae30e8e6c439cac","observation_id":"98233f11-b9ef-4a52-9fc7-c9c3fe50b55d","resolution":{"observed_at":"2026-08-03T06:46:18.811052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13611","last_updated":"2021-05-28T06:39:50Z","snapshot_observed_at":"2026-08-05T02:49:21.574236Z","submitted_at":"2021-05-28T06:39:50Z","title":"MPS-ATLAS: A fast all-in-one code for synthesising stellar spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13611","snapshot_observed_at":"2026-08-03T06:46:18.816295Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.816295Z"},"links":{"cited_paper":"/paper/2105.13611","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1c9fde21de2ada89750b96e2e842a7c620b1f081107a27e7265e257ba82b1d33","observation_id":"a9e950fb-00cc-4a81-8039-a267a4de93b2","resolution":{"observed_at":"2026-08-03T06:46:18.816295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.02860","last_updated":"2022-11-05T09:27:53Z","snapshot_observed_at":"2026-07-06T14:14:46.573987Z","submitted_at":"2022-11-05T09:27:53Z","title":"Can 1D radiative equilibrium models of faculae be used for calculating contamination of transmission spectra?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.02860","snapshot_observed_at":"2026-08-03T06:46:18.826724Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.826724Z"},"links":{"cited_paper":"/paper/2211.02860","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:dcb2a919555c980e0eed9ac217f97ce1c2e7153a0e1350139ea0590926e6f287","observation_id":"b06dc382-e61c-4445-8794-454bdefd1d39","resolution":{"observed_at":"2026-08-03T06:46:18.826724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.08532","last_updated":"2015-07-30T15:07:35Z","snapshot_observed_at":"2026-07-06T04:25:22.664904Z","submitted_at":"2015-07-30T15:07:35Z","title":"The HARPS-N Rocky Planet Search I. HD219134b: A transiting rocky planet in a multi-planet system at 6.5 pc from the Sun","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.08532","snapshot_observed_at":"2026-08-03T06:46:18.836394Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.836394Z"},"links":{"cited_paper":"/paper/1507.08532","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:01aa70548e5f1f570774423cc288885e803314bb320803b69538dbb35920189c","observation_id":"b5644bd2-c7f1-4d5b-bbf4-f4024b46bcf2","resolution":{"observed_at":"2026-08-03T06:46:18.836394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.04627","last_updated":"2019-08-16T12:12:06Z","snapshot_observed_at":"2026-08-05T17:03:16.034529Z","submitted_at":"2019-08-13T13:20:28Z","title":"Catalog for the ESPRESSO blind radial velocity exoplanet survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.04627","snapshot_observed_at":"2026-08-03T06:46:18.854745Z","title":", keywords =","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.854745Z"},"links":{"cited_paper":"/paper/1908.04627","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:f1138eb19d884eab758c75332fbb77b66f8283b57dd57a791eec9c6dd18e49a6","observation_id":"ad30f410-755b-4941-b57d-8de6cf3279a0","resolution":{"observed_at":"2026-08-03T06:46:18.854745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.02303","last_updated":"2020-06-03T14:43:13Z","snapshot_observed_at":"2026-07-06T09:25:44.674803Z","submitted_at":"2020-06-03T14:43:13Z","title":"EXPRES I. HD~3651 an Ideal RV Benchmark","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.02303","snapshot_observed_at":"2026-08-03T06:46:18.866342Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.866342Z"},"links":{"cited_paper":"/paper/2006.02303","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:c7ec74aaf47c2e67f8e337122112eed171fe703be4d2e668e19e69e89be5920f","observation_id":"9e1db459-9e11-453f-b5fa-c27b414c1e92","resolution":{"observed_at":"2026-08-03T06:46:18.866342Z","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":"2026-08-03T06:46:18.876845Z","title":"American Astronomical Society Meeting \\#240 , year = 2022, series =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.876845Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1f2f8ca1c9bc84e386a1a02c75f153a97b86ca727ac58bd9baa2c01e9f7adb1a","observation_id":"d4241d95-638c-4d3a-8f19-5c1ffa5b51bc","resolution":{"observed_at":"2026-08-03T06:46:18.876845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11689","last_updated":"2021-01-27T21:07:54Z","snapshot_observed_at":"2026-07-06T10:36:14.502129Z","submitted_at":"2021-01-27T21:07:54Z","title":"Target Prioritization and Observing Strategies for the NEID Earth Twin Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11689","snapshot_observed_at":"2026-08-03T06:46:18.881714Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.881714Z"},"links":{"cited_paper":"/paper/2101.11689","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:d9f5ca105347c8ad1f59cfe342729a4aaddcce9f1a502c7f146f4ab2413aa24d","observation_id":"e73648b7-e08e-4994-82b3-6c097bdb91bb","resolution":{"observed_at":"2026-08-03T06:46:18.881714Z","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":"2026-08-03T06:46:18.897881Z","title":"American Astronomical Society Meeting Abstracts , year = 2026, series =","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.897881Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:d6e254c8bd5b658c165e22855bb22b0e27fb508a7b02d654585f780345269054","observation_id":"e863436c-b23a-4a6f-91b0-d7716dab7b64","resolution":{"observed_at":"2026-08-03T06:46:18.897881Z","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":"2026-08-03T06:46:18.907963Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.907963Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:1a587fbc847e7e681361bcfdd8ef13058da313660470e16b023a80df33dfd52e","observation_id":"cc194368-c21f-4638-aa6c-17d8a188c4ea","resolution":{"observed_at":"2026-08-03T06:46:18.907963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.10639","last_updated":"2022-01-25T21:34:36Z","snapshot_observed_at":"2026-08-08T12:15:56.780644Z","submitted_at":"2022-01-25T21:34:36Z","title":"The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.10639","snapshot_observed_at":"2026-08-03T06:46:18.912624Z","title":"State of the Field in Disentangling Photospheric Velocities","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.912624Z"},"links":{"cited_paper":"/paper/2201.10639","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:48759484ced296aa66efa7df17ec378a778932019d51b982e8f092a5554c2ba8","observation_id":"2739f2f0-6d41-4e73-9ea2-19e03cbb508d","resolution":{"observed_at":"2026-08-03T06:46:18.912624Z","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":"2026-08-03T06:46:18.924882Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.924882Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:0f878783e3cd306b505968b6e401315647fa994d28ae846f96688ae51945bc03","observation_id":"8f5844e7-2038-4812-88a3-6644bfdaaaea","resolution":{"observed_at":"2026-08-03T06:46:18.924882Z","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":"2026-08-03T06:46:18.941560Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.941560Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:62f317d8a9097c2917c93840d794bb1f8adcc355e53ddf19bf146ac98476f7d3","observation_id":"a4b5a5a3-950e-4991-a7ef-638b847569bc","resolution":{"observed_at":"2026-08-03T06:46:18.941560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.12186","last_updated":"2019-04-27T17:33:26Z","snapshot_observed_at":"2026-08-10T07:12:26.181834Z","submitted_at":"2019-04-27T17:33:26Z","title":"Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.12186","snapshot_observed_at":"2026-08-03T06:46:18.945414Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.945414Z"},"links":{"cited_paper":"/paper/1904.12186","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:414519a90d8ecd5d82f4edaec25da4ea39de8199609291ff9258f3e0c3ca4653","observation_id":"89fc997e-15f6-4766-9917-9fdae1ab0386","resolution":{"observed_at":"2026-08-03T06:46:18.945414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.05955","last_updated":"2018-11-23T16:54:41Z","snapshot_observed_at":"2026-07-06T07:14:44.317338Z","submitted_at":"2018-11-14T18:42:27Z","title":"A candidate super-Earth planet orbiting near the snow line of Barnard's star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.05955","snapshot_observed_at":"2026-08-03T06:46:18.950483Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.950483Z"},"links":{"cited_paper":"/paper/1811.05955","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:a0843ba24231212ec04d9136214a27db6b2c39f739da77491aed76fb7aef2082","observation_id":"542d9ee1-16e7-4ad4-832b-d52da4515336","resolution":{"observed_at":"2026-08-03T06:46:18.950483Z","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":"2026-08-03T06:46:18.954856Z","title":"Bulletin of the American Astronomical Society , year = 2022, volume =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.954856Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:2ccd342aaeccd8ef1cfd2923962d8f6fd804250d2974e578f5c5f169f3d5ae88","observation_id":"bcd61167-e0a4-44e8-bc94-215dba7a97f9","resolution":{"observed_at":"2026-08-03T06:46:18.954856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.02778","last_updated":"2015-06-01T17:07:09Z","snapshot_observed_at":"2026-08-09T04:58:49.017135Z","submitted_at":"2015-05-11T20:00:44Z","title":"Stellar activity mimics a habitable-zone planet around Kapteyn's star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.02778","snapshot_observed_at":"2026-08-03T06:46:18.961611Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.961611Z"},"links":{"cited_paper":"/paper/1505.02778","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:9c5bbb7796efcef76ffae0c57c1a3f3bb76d2bb5f005fe0df0383866b32824f7","observation_id":"2c0571ec-8631-4a94-9abe-106157e00482","resolution":{"observed_at":"2026-08-03T06:46:18.961611Z","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":"2026-08-03T06:46:18.971178Z","title":"American Astronomical Society Meeting Abstracts \\#234 , year = 2019, series =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.971178Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:de53c49514eab710922afb524a3d54efa17cfdbf93fa95e33b784e538804d531","observation_id":"1bbb7291-c99f-473d-8458-7bc07a079dc5","resolution":{"observed_at":"2026-08-03T06:46:18.971178Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.7374","last_updated":"2013-04-30T11:17:07Z","snapshot_observed_at":"2026-08-01T18:37:04.352274Z","submitted_at":"2013-04-27T14:19:05Z","title":"Two Super-Earths Orbiting the Solar Analogue HD41248 on the edge of a 7:5 Mean Motion Resonance","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.7374","snapshot_observed_at":"2026-08-03T06:46:18.976887Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.976887Z"},"links":{"cited_paper":"/paper/1304.7374","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:567a39d740e1049dea69cfde563ada11cbce9a1059b79114ebf77a771d58a059","observation_id":"400ad505-672a-4bb5-956b-ccbd576b94fd","resolution":{"observed_at":"2026-08-03T06:46:18.976887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.3093","last_updated":"2014-06-12T01:12:49Z","snapshot_observed_at":"2026-08-02T00:03:36.437921Z","submitted_at":"2014-06-12T01:12:49Z","title":"The curious case of HD41248. A pair of static signals buried behind red-noise","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.3093","snapshot_observed_at":"2026-08-03T06:46:18.982992Z","title":"A Pair of Static Signals Buried Behind Red Noise","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.982992Z"},"links":{"cited_paper":"/paper/1406.3093","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:63515a4e7f814f07c62402b09a4cd279ad968aac9eb6e55232dcb72c830a06b7","observation_id":"68123131-68ff-426c-909d-4cb9e7a89dee","resolution":{"observed_at":"2026-08-03T06:46:18.982992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.6135","last_updated":"2014-04-24T14:47:35Z","snapshot_observed_at":"2026-08-04T11:56:01.660203Z","submitted_at":"2014-04-24T14:47:35Z","title":"The HARPS search for southern extra-solar planets XXXV. The interesting case of HD41248: stellar activity, no planets?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.6135","snapshot_observed_at":"2026-08-03T06:46:18.988207Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.988207Z"},"links":{"cited_paper":"/paper/1404.6135","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:5afb235c26fd0ec3ed6121db3aeda1dd5285d8d8e2e22ca0858d4a608756ab1a","observation_id":"837c78a9-a8f8-4b71-8382-d96a3a732152","resolution":{"observed_at":"2026-08-03T06:46:18.988207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.03089","last_updated":"2017-05-08T21:13:42Z","snapshot_observed_at":"2026-07-06T05:41:47.469609Z","submitted_at":"2017-05-08T21:13:42Z","title":"Agatha: disentangling periodic signals from correlated noise in a periodogram framework","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.03089","snapshot_observed_at":"2026-08-03T06:46:18.994775Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.994775Z"},"links":{"cited_paper":"/paper/1705.03089","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:4730bfd17174268f9e0df5a3c23ac3e18335c3f7268ed7ece97f59b28939d4ab","observation_id":"a164c2fc-4eb6-4c18-8185-25c2cf2c9175","resolution":{"observed_at":"2026-08-03T06:46:18.994775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.11714","last_updated":"2019-11-26T17:39:04Z","snapshot_observed_at":"2026-08-04T14:36:34.562958Z","submitted_at":"2019-11-26T17:39:04Z","title":"Decoding the radial velocity variations of HD41248 with ESPRESSO","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.11714","snapshot_observed_at":"2026-08-03T06:46:18.999612Z","title":", keywords =","venue":null,"work_id":null,"year":1911},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:18.999612Z"},"links":{"cited_paper":"/paper/1911.11714","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:21d6dd200b0f45e42ab191f83c67c8fe5cf10f60f66f993606dc41d2194ce65e","observation_id":"8ed8b97a-e173-4441-88d1-2b3855543ad8","resolution":{"observed_at":"2026-08-03T06:46:18.999612Z","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":"2026-08-03T06:46:19.016188Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:19.016188Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:b16417d2f7f4855fde7a075ff3aca79e58c7999a76bfd76ade1bb6b96975e9cc","observation_id":"c22b3c76-a6de-4f9e-9e5d-06ef3e2a6327","resolution":{"observed_at":"2026-08-03T06:46:19.016188Z","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":"2026-08-03T06:46:19.020771Z","title":", year = 1984, month = jan, volume =","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:19.020771Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:9375981bfc268738f01231440f2e9d204deffa422cfac3708b404f7fb3c0d296","observation_id":"42f81508-b8b7-44a0-aebe-4080f5d240ce","resolution":{"observed_at":"2026-08-03T06:46:19.020771Z","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":"2026-08-03T06:46:19.026430Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:19.026430Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:88f50e1f36ba7f898d2841d1d8ce625f1983c70689471819b8f07c14e9774596","observation_id":"ef2c3d82-1d65-4638-93ee-c81a3d7c0b89","resolution":{"observed_at":"2026-08-03T06:46:19.026430Z","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":"2026-08-03T06:46:19.031897Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:19.031897Z"},"links":{"citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:a3a7d8c75480af9b18b14a1b9f62fc30cac634f280e954973190f62f763d81a0","observation_id":"1a833847-80d5-45ab-a7ef-1841abe7a091","resolution":{"observed_at":"2026-08-03T06:46:19.031897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.18663","last_updated":"2024-10-24T11:48:02Z","snapshot_observed_at":"2026-08-07T20:38:30.358441Z","submitted_at":"2024-10-24T11:48:02Z","title":"Detection of faculae in the transit and transmission spectrum of WASP-69b","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.18663","snapshot_observed_at":"2026-08-03T06:46:19.037544Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:19.037544Z"},"links":{"cited_paper":"/paper/2410.18663","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:72367e392b0245000945eb0d975722e0bfdc23e274d957855db71d9e20184c4c","observation_id":"579e449c-0974-4aa8-b962-226d36b632d8","resolution":{"observed_at":"2026-08-03T06:46:19.037544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.07020","last_updated":"2015-02-25T00:54:37Z","snapshot_observed_at":"2026-07-06T04:10:10.990919Z","submitted_at":"2015-02-25T00:54:37Z","title":"The Solar Cycle","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.07020","snapshot_observed_at":"2026-08-03T06:46:19.044995Z","title":"Living Reviews in Solar Physics , keywords =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:19.044995Z"},"links":{"cited_paper":"/paper/1502.07020","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:045ef7ccb7cb00e639c478413565554944abc239cca3a3f707f120adca86cde0","observation_id":"54470b57-e8cc-4340-b5a6-1b3b2ca1d197","resolution":{"observed_at":"2026-08-03T06:46:19.044995Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.1452","last_updated":"2011-01-14T14:24:04Z","snapshot_observed_at":"2026-07-06T02:20:18.010624Z","submitted_at":"2010-12-07T10:39:35Z","title":"Disentangling stellar activity and planetary signals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.1452","snapshot_observed_at":"2026-08-03T06:46:19.054759Z","title":"Physics of Sun and Star Spots , year = 2011, editor =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-03T06:46:19.054759Z"},"links":{"cited_paper":"/paper/1012.1452","citing_paper":"/paper/2607.29455"},"observation_digest":"sha256:16c83b0dbe0931e258dce8a232cb676507f1ca57fc16493312ca79530b5c5862","observation_id":"3ee5753f-5836-409f-91e9-5cd5ed772066","resolution":{"observed_at":"2026-08-03T06:46:19.054759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.29455","last_updated":"2026-07-31T14:19:33Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-08T00:15:53.192565Z","submitted_at":"2026-07-31T14:19:33Z","title":"The Fe I 4377 {\\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":97,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":126},"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 100 of 126 outbound references and 0 inbound Pith citation observations for arXiv:2607.29455."}