{"as_of":"2026-08-18T04:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:07da8290feb46e2aa68adeba2a308d5d00d6c67ab73208208daa1da730b2c7b0","coverage":[{"denominator":184,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T10:57:04.816136Z","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":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2509.03435/citation-record","integrity":"/paper/2509.03435/integrity","json":"/paper/2509.03435/citation-record.json","paper":"/paper/2509.03435"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T10:57:04.454177Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.454177Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:94b119a02a5efa9b255fd5d5681fa03bfc984487c14f27549d2a36d358c70ef1","observation_id":"8c47027b-89a7-4a2b-979c-02d1a198a3c7","resolution":{"observed_at":"2026-08-05T10:57:04.454177Z","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":"2026-08-05T10:57:04.484536Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.484536Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:1985c8e4e0b3ec0bd45e7f8954b123fd55ad395d37a2889fdcbd5da7ae213796","observation_id":"274dff59-38ce-46b5-9a54-1ab2f3e6bcfc","resolution":{"observed_at":"2026-08-05T10:57:04.484536Z","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":"2026-08-05T10:57:04.518123Z","title":"In: Bulletin of the American Astronomical Society, p 268","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.518123Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:5ca80a7589e2b844b9ce998941e90b0c83836f5d02d55e657f98f820cc087ec3","observation_id":"4bbeacb8-473b-40d8-abda-c34d8c4f998a","resolution":{"observed_at":"2026-08-05T10:57:04.518123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.4514","last_updated":"2014-04-17T13:01:19Z","snapshot_observed_at":"2026-08-14T23:37:11.471978Z","submitted_at":"2014-04-17T13:01:19Z","title":"On the origin of stars with and without planets. Tc trends and clues to Galactic evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.4514","snapshot_observed_at":"2026-08-05T10:57:04.521450Z","title":"T _ c trends and clues to Galactic evolution","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.521450Z"},"links":{"cited_paper":"/paper/1404.4514","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:9535af6a3d07f3945c9fc779cc09f9d3793a86bb1bd9cce10212e02c8189fb90","observation_id":"27ce4bcb-ac0b-447c-8d28-e40d5af60054","resolution":{"observed_at":"2026-08-05T10:57:04.521450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.1819","last_updated":"2013-11-07T21:00:01Z","snapshot_observed_at":"2026-08-14T23:56:03.747232Z","submitted_at":"2013-11-07T21:00:01Z","title":"The Dispersal of Protoplanetary Disks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.1819","snapshot_observed_at":"2026-08-05T10:57:04.525252Z","title":"In: Beuther H, Klessen RS, Dullemond CP, et al (eds) Protostars and Planets VI, pp 475--496, doi:10.2458/azu_uapress_9780816531240-ch021, 1311.1819","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.525252Z"},"links":{"cited_paper":"/paper/1311.1819","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:019f86b540266e32b2b2d46fc08373072255f901bc0070c617478c330c162be0","observation_id":"178072bc-a3d1-48ed-82c1-07b358bf3daf","resolution":{"observed_at":"2026-08-05T10:57:04.525252Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.10319","last_updated":"2019-10-08T08:45:23Z","snapshot_observed_at":"2026-08-17T00:57:48.426037Z","submitted_at":"2019-08-27T16:48:21Z","title":"Carbon, oxygen, and iron abundances in disk and halo stars. Implications of 3D non-LTE spectral line formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.10319","snapshot_observed_at":"2026-08-05T10:57:04.528776Z","title":"Implications of 3D non-LTE spectral line formation","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.528776Z"},"links":{"cited_paper":"/paper/1908.10319","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:418b8d09f3ed3cb06e29a6593591e108cc62fe5194ec7efb986cbfb38577fbc3","observation_id":"16871188-c148-4a61-a512-3cf6afefdaef","resolution":{"observed_at":"2026-08-05T10:57:04.528776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.04752","last_updated":"2021-09-10T09:33:58Z","snapshot_observed_at":"2026-08-16T17:57:35.529012Z","submitted_at":"2021-09-10T09:33:58Z","title":"The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.04752","snapshot_observed_at":"2026-08-05T10:57:04.532382Z","title":"656:A113","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.532382Z"},"links":{"cited_paper":"/paper/2109.04752","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:641e43104c96a897128fa57f7fcd2b6197d6127c6acf05badcdb8808be30b68c","observation_id":"c15dd44e-a080-4ee7-b5d3-2b1937d525be","resolution":{"observed_at":"2026-08-05T10:57:04.532382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.13449","last_updated":"2022-12-09T09:12:10Z","snapshot_observed_at":"2026-08-17T23:40:56.510311Z","submitted_at":"2022-09-27T15:13:08Z","title":"3D non-LTE iron abundances in FG-type dwarfs","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.13449","snapshot_observed_at":"2026-08-05T10:57:04.536085Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.536085Z"},"links":{"cited_paper":"/paper/2209.13449","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:c2db885079ca3e5bcaed13f3730dc63c7a6d8bf2497c2c5fe889c489f3c15d8b","observation_id":"1f958426-f2c8-4282-89da-9056d6623af8","resolution":{"observed_at":"2026-08-05T10:57:04.536085Z","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":"2026-08-05T10:57:04.539508Z","title":"43(1):481--530","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.539508Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:6ff310b6c515cac12f3db8ad8fdb5062505eba7e75d8b772ee49fbd9148d21c9","observation_id":"49815adb-0d0f-4618-8564-4b0a39076e0d","resolution":{"observed_at":"2026-08-05T10:57:04.539508Z","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":"2026-08-05T10:57:04.542331Z","title":"In: Barnes TGIII, Bash FN (eds) Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, p 25","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.542331Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:2cbb847447cdfcd7fd07104c632e6ad25692e037bb07d3f391595ed27f96fa6e","observation_id":"93245853-0963-453c-9388-731c7e33d856","resolution":{"observed_at":"2026-08-05T10:57:04.542331Z","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":"2026-08-05T10:57:04.545270Z","title":"47(1):481--522","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.545270Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:d752d118c73e2a4b785d9291885d36d99341f832fa1f371576455ed1c9271265","observation_id":"82ecb960-9f3f-44fb-af4d-112decb2393e","resolution":{"observed_at":"2026-08-05T10:57:04.545270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.01661","last_updated":"2021-07-14T15:25:03Z","snapshot_observed_at":"2026-08-17T16:26:20.028011Z","submitted_at":"2021-05-04T18:00:00Z","title":"The chemical make-up of the Sun: A 2020 vision","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.01661","snapshot_observed_at":"2026-08-05T10:57:04.548665Z","title":"653:A141","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.548665Z"},"links":{"cited_paper":"/paper/2105.01661","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:c316131ab4a76414359114a4de2ed8176962cd6c726376270e39a7f28938dc0b","observation_id":"22b708f6-aaca-4a14-a684-efbc3a24ee1e","resolution":{"observed_at":"2026-08-05T10:57:04.548665Z","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":"10.1371/journal.pone.0038024","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"HC (2012) RNA Folding and Catalysis Mediated by Iron (II)","venue":"PLoS ONE","work_id":"27ad3c9e-002f-4fd5-bf1c-411b7d22b9ee","year":2012},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.551764Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:189020e91d423d5ba30953c87aef55e1c5974f773e59bc873fc51705544cbfc6","observation_id":"54431634-971c-465b-9190-97371f8bc96b","resolution":{"observed_at":"2026-08-05T10:57:05.367676Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.10335","last_updated":"2023-10-16T12:19:44Z","snapshot_observed_at":"2026-08-16T14:51:47.498269Z","submitted_at":"2023-10-16T12:19:44Z","title":"Exploring the Sun's birth radius and the distribution of planet building blocks in the Milky Way galaxy: A multi-zone Galactic chemical evolution approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.10335","snapshot_observed_at":"2026-08-05T10:57:04.554758Z","title":"526(4):6088--6102","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.554758Z"},"links":{"cited_paper":"/paper/2310.10335","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:4c3003fac02873e166425aed64ec67cc908508d8ad13312c148bb775675a61d1","observation_id":"79a7f711-7cf1-4bfa-833b-293f66bd1c73","resolution":{"observed_at":"2026-08-05T10:57:04.554758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.13314","last_updated":"2023-01-17T01:58:39Z","snapshot_observed_at":"2026-08-16T16:21:36.955316Z","submitted_at":"2022-10-24T15:08:11Z","title":"Structured Distributions of Gas and Solids in Protoplanetary Disks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.13314","snapshot_observed_at":"2026-08-05T10:57:04.557602Z","title":"In: Inutsuka S, Aikawa Y, Muto T, et al (eds) Protostars and Planets VII, p 423, doi:10.48550/arXiv.2210.13314, 2210.13314","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.557602Z"},"links":{"cited_paper":"/paper/2210.13314","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:77f4a4f80fa7ec84e421e088c8daa0a22428d76c17466e7224d987c0069068ba","observation_id":"7a443d62-acf9-431a-9714-a431c9154e06","resolution":{"observed_at":"2026-08-05T10:57:04.557602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07162","last_updated":"2016-11-22T06:43:09Z","snapshot_observed_at":"2026-08-14T21:29:16.181395Z","submitted_at":"2016-11-22T06:43:09Z","title":"Evidence from stable isotopes and Be-10 for solar system formation triggered by a low-mass supernova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07162","snapshot_observed_at":"2026-08-05T10:57:04.560837Z","title":"Nature Communications 7:13639","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.560837Z"},"links":{"cited_paper":"/paper/1611.07162","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:3861c1ecdb2f2d89a59b13098316a3f30b3d88f09f63a3cdf1caf3568ca0eab0","observation_id":"7d4ba19f-b269-47b1-b39d-7743d28d1dd0","resolution":{"observed_at":"2026-08-05T10:57:04.560837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.4288","last_updated":"2010-08-25T14:15:53Z","snapshot_observed_at":"2026-08-15T05:10:28.498742Z","submitted_at":"2010-08-25T14:15:53Z","title":"Effect of episodic accretion on the structure and the lithium depletion of low-mass stars and planet-hosting stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.4288","snapshot_observed_at":"2026-08-05T10:57:04.563632Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.563632Z"},"links":{"cited_paper":"/paper/1008.4288","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:88850a16df971b37f87f41bf09a3c03d5bb8131b6a6b7710c243b9f09d245ec3","observation_id":"6417e4a5-83a4-4f63-8e1d-812b84ed5802","resolution":{"observed_at":"2026-08-05T10:57:04.563632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.07659","last_updated":"2016-05-09T08:17:28Z","snapshot_observed_at":"2026-08-14T22:00:03.968665Z","submitted_at":"2016-04-26T12:53:29Z","title":"Accurate abundance analysis of late-type stars: advances in atomic physics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.07659","snapshot_observed_at":"2026-08-05T10:57:04.566563Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.566563Z"},"links":{"cited_paper":"/paper/1604.07659","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:7ac5ade97181a1990ee7e00b4bef5fa1b02a13f2ad93f46cb0d3f16422d18790","observation_id":"17cae767-d1bf-407b-8504-1b10b0b3f04e","resolution":{"observed_at":"2026-08-05T10:57:04.566563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.07681","last_updated":"2022-05-16T13:49:00Z","snapshot_observed_at":"2026-08-17T14:09:00.773900Z","submitted_at":"2022-05-16T13:49:00Z","title":"Dust coagulation during the early stages of star formation: molecular cloud collapse and first hydrostatic core evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.07681","snapshot_observed_at":"2026-08-05T10:57:04.569679Z","title":"514(2):2145--2161","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.569679Z"},"links":{"cited_paper":"/paper/2205.07681","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:ff349e198f29971f201130a2c922113142cc0f8c2e0ae76fc533edf25f0081ed","observation_id":"9fef0548-2c8e-42a4-9c06-9c41a7dea6a9","resolution":{"observed_at":"2026-08-05T10:57:04.569679Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.0575","last_updated":"2010-08-03T15:30:56Z","snapshot_observed_at":"2026-08-15T05:12:16.643585Z","submitted_at":"2010-08-03T15:30:56Z","title":"Lithium depletion in solar-like stars: no planet connection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.0575","snapshot_observed_at":"2026-08-05T10:57:04.572797Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.572797Z"},"links":{"cited_paper":"/paper/1008.0575","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:7cdac4e1506da6741dc6634f18710ad6630a23d23a5b65d1dd27e61c694365d7","observation_id":"73e3d2bb-3290-4c7a-89f3-f19273226813","resolution":{"observed_at":"2026-08-05T10:57:04.572797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.02576","last_updated":"2018-08-07T14:28:05Z","snapshot_observed_at":"2026-08-15T18:27:33.207039Z","submitted_at":"2018-02-07T19:00:00Z","title":"The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.02576","snapshot_observed_at":"2026-08-05T10:57:04.576066Z","title":"865(1):68","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.576066Z"},"links":{"cited_paper":"/paper/1802.02576","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:4dd2ccdec5ba36ef209a8c3f44710399dcf04b958b1f6257ba35ad4f8b6edad9","observation_id":"41abbe6c-f530-4862-bd59-90e65e7af681","resolution":{"observed_at":"2026-08-05T10:57:04.576066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.12121","last_updated":"2022-10-21T17:21:01Z","snapshot_observed_at":"2026-08-16T16:22:09.516101Z","submitted_at":"2022-10-21T17:21:01Z","title":"Planet Engulfment Detections are Rare According to Observations and Stellar Modeling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.12121","snapshot_observed_at":"2026-08-05T10:57:04.578901Z","title":"521(2):2969--2987","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.578901Z"},"links":{"cited_paper":"/paper/2210.12121","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:76b389fd904dfe65701848afcfca7d9c090e6adbfbe4fe42e4ee12865a4b2681","observation_id":"3baaad49-029a-4fbd-8343-2b0cdb3ac2d5","resolution":{"observed_at":"2026-08-05T10:57:04.578901Z","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":"10.1007/978-3-319-06956-2_21","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T11:08:14.039542Z","title":"In: Niemczura E, Smalley B, Pych W (eds) Determination of Atmospheric Parameters of B","venue":"GeoPlanet: earth and planetary sciences","work_id":"14c54ad5-b883-4b9c-b120-80a7b2587963","year":2014},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.581637Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:6de2814a74a7156d8a8b30d5fecbe004c0f5b6f19d16cd4ac6cf9a35278391da","observation_id":"2b85bf52-ead7-4ca5-ae39-d2a59b0237bc","resolution":{"observed_at":"2026-08-05T10:57:05.348052Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.05200","last_updated":"2019-07-26T08:53:11Z","snapshot_observed_at":"2026-08-14T19:57:29.413286Z","submitted_at":"2019-05-13T18:00:02Z","title":"Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.05200","snapshot_observed_at":"2026-08-05T10:57:04.584266Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.584266Z"},"links":{"cited_paper":"/paper/1905.05200","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:91a06ac9fe2634f2d467a19b778fb930018a586f0bc56d9c3d02fdda5b41b3ee","observation_id":"0d8d677c-f592-48d4-a70f-c57463a14528","resolution":{"observed_at":"2026-08-05T10:57:04.584266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.01143","last_updated":"2021-09-02T18:00:00Z","snapshot_observed_at":"2026-08-16T17:59:11.464746Z","submitted_at":"2021-09-02T18:00:00Z","title":"Solar oxygen abundance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.01143","snapshot_observed_at":"2026-08-05T10:57:04.587013Z","title":"508(2):2236--2253","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.587013Z"},"links":{"cited_paper":"/paper/2109.01143","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:a5d1dc0e684dc056f7a20865154c9a326f56900564eab4763bd2551e6e4a5e9b","observation_id":"c477801c-dcf5-4dfc-a612-3f106abae772","resolution":{"observed_at":"2026-08-05T10:57:04.587013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.05402","last_updated":"2025-03-07T13:26:50Z","snapshot_observed_at":"2026-08-16T12:52:10.455516Z","submitted_at":"2025-03-07T13:26:50Z","title":"The Chemical Composition of the Sun","version":1},"cited_work":{"arxiv_id":"2503.05402","doi":"10.48550/arxiv.2503.05402","metadata_source":"pith","pith_arxiv_id":"2503.05402","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"The Chemical Composition of the Sun","venue":"astro-ph.SR","work_id":"03874195-9e93-4c3a-98dd-11374ddf4f7b","year":2025},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.589950Z"},"links":{"cited_paper":"/paper/2503.05402","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:424f4441fa5b202052332721634b6f3e422692e44baa1aad4ffe0a05b7061a91","observation_id":"dd569657-24f0-4e3b-aea5-860246b5410e","resolution":{"observed_at":"2026-08-05T10:57:05.338440Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.09529","last_updated":"2018-02-26T19:00:00Z","snapshot_observed_at":"2026-08-14T19:41:59.174745Z","submitted_at":"2018-02-26T19:00:00Z","title":"Identifying Young $Kepler$ Planet Host Stars from Keck-HIRES Spectra of Lithium","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.09529","snapshot_observed_at":"2026-08-05T10:57:04.592746Z","title":"855(2):115","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.592746Z"},"links":{"cited_paper":"/paper/1802.09529","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:5eb8eb83e028f04c9536c89a9c32eaa10d7d19ef6a073291c9d152ba407dd08c","observation_id":"67c7c9f7-0511-4bc4-b0bf-f03068b6cca2","resolution":{"observed_at":"2026-08-05T10:57:04.592746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.06293","last_updated":"2018-04-17T14:44:01Z","snapshot_observed_at":"2026-08-14T19:25:02.328975Z","submitted_at":"2018-04-17T14:44:01Z","title":"The Gaia-ESO Survey: Evidence of atomic diffusion in M67?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.06293","snapshot_observed_at":"2026-08-05T10:57:04.595586Z","title":"doi:10.1093/mnras/sty1011, https://arxiv.org/abs/1804.06293 https://arxiv.org/abs/arXiv:1804.06293 [astro-ph.SR]","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.595586Z"},"links":{"cited_paper":"/paper/1804.06293","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:2c7290a6520b00674f054ccfff1c5226ef8c2a9af2f175826d7901a0e31b705f","observation_id":"857e8967-6ade-456d-aa0f-fb8615f20895","resolution":{"observed_at":"2026-08-05T10:57:04.595586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.01614","last_updated":"2015-09-07T06:31:18Z","snapshot_observed_at":"2026-08-14T22:45:46.435703Z","submitted_at":"2015-06-04T14:58:55Z","title":"The GAPS Programme with HARPS-N at TNG. X. Differential abundances in the XO-2 planet hosting binary","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.01614","snapshot_observed_at":"2026-08-05T10:57:04.598334Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.598334Z"},"links":{"cited_paper":"/paper/1506.01614","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:df6e53da326c9493eccc036199a38e9d7c826a80d5ef716888c939ce221296ce","observation_id":"59a255d8-11dc-4d31-933d-bc062f837b29","resolution":{"observed_at":"2026-08-05T10:57:04.598334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11135","last_updated":"2020-02-25T19:00:05Z","snapshot_observed_at":"2026-08-08T08:51:24.505831Z","submitted_at":"2020-02-25T19:00:05Z","title":"Fingerprints of giant planets in the composition of solar twins","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.11135","snapshot_observed_at":"2026-08-05T10:57:04.601193Z","title":"493(4):5079--5088","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.601193Z"},"links":{"cited_paper":"/paper/2002.11135","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:242a4ce1c28c1819d0534343713895e8b4aa46994a2a46b22317bfa837b9c64a","observation_id":"d790648c-ecaf-40d2-aed6-de4fad53f5a7","resolution":{"observed_at":"2026-08-05T10:57:04.601193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.04296","last_updated":"2017-03-13T08:56:43Z","snapshot_observed_at":"2026-08-14T21:12:11.031705Z","submitted_at":"2017-03-13T08:56:43Z","title":"Search for giant planets in M67 IV: survey results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.04296","snapshot_observed_at":"2026-08-05T10:57:04.604063Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.604063Z"},"links":{"cited_paper":"/paper/1703.04296","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:f862ac8f6b8541825eb982db5cbc5528c0d631a6a8b841960251ec5919212d44","observation_id":"7fc720b7-3825-424e-a84a-babd748894b1","resolution":{"observed_at":"2026-08-05T10:57:04.604063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.10478","last_updated":"2024-04-16T11:39:40Z","snapshot_observed_at":"2026-08-16T21:18:06.829819Z","submitted_at":"2024-04-16T11:39:40Z","title":"In-depth analysis of solar models with high-metallicity abundances and updated opacity tables","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.10478","snapshot_observed_at":"2026-08-05T10:57:04.607064Z","title":"686:A108","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.607064Z"},"links":{"cited_paper":"/paper/2404.10478","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:ebe2b595f487c11e673ce1a0e3e14b5fd6ce51dad8af76d9850088499744ea65","observation_id":"cb92d462-3ca2-4f44-a065-e0567aec0434","resolution":{"observed_at":"2026-08-05T10:57:04.607064Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.4398","last_updated":"2008-05-28T18:22:47Z","snapshot_observed_at":"2026-08-15T10:14:28.471562Z","submitted_at":"2008-05-28T18:22:47Z","title":"The photospheric solar oxygen project: I. Abundance analysis of atomic lines and influence of atmospheric models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.4398","snapshot_observed_at":"2026-08-05T10:57:04.609891Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.609891Z"},"links":{"cited_paper":"/paper/0805.4398","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:6687e896a4eb011afead03df19ed82c47835ef214d9efa0c66faddc580030e9f","observation_id":"9ea9ec67-014e-4380-9209-95363f170b3d","resolution":{"observed_at":"2026-08-05T10:57:04.609891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.1190","last_updated":"2010-03-05T05:33:59Z","snapshot_observed_at":"2026-08-15T05:24:54.671662Z","submitted_at":"2010-03-05T05:33:59Z","title":"Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.1190","snapshot_observed_at":"2026-08-05T10:57:04.612816Z","title":"Solar Physics 268(2):255--269","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.612816Z"},"links":{"cited_paper":"/paper/1003.1190","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:55224d3db47442df6562fb6ed7f7285bdec0f2da42cf00d15fe6a3d21c161663","observation_id":"f5b7dc2c-f3cb-4e2e-87a7-dc5978fbe672","resolution":{"observed_at":"2026-08-05T10:57:04.612816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.00931","last_updated":"2015-06-02T15:41:51Z","snapshot_observed_at":"2026-08-14T22:46:05.357550Z","submitted_at":"2015-06-02T15:41:51Z","title":"The photospheric solar oxygen project: III. Investigation of the centre-to-limb variation of the 630nm [OI]-NiI blend","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.00931","snapshot_observed_at":"2026-08-05T10:57:04.615614Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.615614Z"},"links":{"cited_paper":"/paper/1506.00931","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:13d945e37dd9200cfe22592db50c737f9a05150601defde5d0dd5b8edd33cd4e","observation_id":"96021705-359a-4214-b2a2-2b0df0cd2dda","resolution":{"observed_at":"2026-08-05T10:57:04.615614Z","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":"2026-08-05T10:57:04.618955Z","title":"Problems of Cosmogeny 7:91","venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.618955Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:31caab5bee49caa8bf8611fca1023af91bc33fb6e74cff135fab8bf19769b2f6","observation_id":"4f838781-f5d5-40ad-815c-e4ea154ae9cc","resolution":{"observed_at":"2026-08-05T10:57:04.618955Z","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/bf00172440","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"15(1):121--146","venue":"Space Science Reviews","work_id":"3db35f03-51f6-4a2c-a1a2-2b849a3704c3","year":1973},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.621838Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:2491fb818b9847771cb6e00049c5acb658d50ad28f9ede12f2c33ece6aa4c824","observation_id":"a65d9920-d9e8-46a7-9c80-3834a8d25e0d","resolution":{"observed_at":"2026-08-05T10:57:05.325797Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.22615","last_updated":"2025-05-28T17:31:28Z","snapshot_observed_at":"2026-08-17T22:50:03.168744Z","submitted_at":"2025-05-28T17:31:28Z","title":"The peculiar composition of the Sun is not related to giant planets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.22615","snapshot_observed_at":"2026-08-05T10:57:04.624739Z","title":"arXiv e-prints arXiv:2505.22615","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.624739Z"},"links":{"cited_paper":"/paper/2505.22615","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:43dfcc35c66a875d59acb450a4389100c0e87b03f925f1204976b00b6a253fc8","observation_id":"9f63490b-e19c-48e0-a68e-2ec23310aea0","resolution":{"observed_at":"2026-08-05T10:57:04.624739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.07581","last_updated":"2015-10-26T18:23:06Z","snapshot_observed_at":"2026-08-14T22:26:16.864406Z","submitted_at":"2015-10-26T18:23:06Z","title":"A publicly available simulation of an enhanced network region of the Sun","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.07581","snapshot_observed_at":"2026-08-05T10:57:04.628183Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.628183Z"},"links":{"cited_paper":"/paper/1510.07581","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:e0e6008264ec0179a79dcdfc87e9816974127e3a73549a279767faaaff0bf197","observation_id":"f5257970-aa7f-4763-9a77-7ea4116e2139","resolution":{"observed_at":"2026-08-05T10:57:04.628183Z","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":"2026-08-05T10:57:04.631158Z","title":"94:1--11","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.631158Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:59198ead71734f93e2bfb8b39d431ec243d6467ed4db4df4c6146b75e31aaf13","observation_id":"509ad2f4-07ab-43f8-913d-b75e6cf922d9","resolution":{"observed_at":"2026-08-05T10:57:04.631158Z","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":"2026-08-05T10:57:04.634058Z","title":"724(1):92--97","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.634058Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:5e857e5b97aea2b12ec54964962294d2a68ceb43ac48e7d2ca35a244031eccac","observation_id":"3ae6ae40-8848-4d80-adce-4789ec3a59b7","resolution":{"observed_at":"2026-08-05T10:57:04.634058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.06488","last_updated":"2021-05-14T09:18:53Z","snapshot_observed_at":"2026-08-02T15:10:20.292790Z","submitted_at":"2020-07-13T16:38:09Z","title":"Solar structure and evolution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.06488","snapshot_observed_at":"2026-08-05T10:57:04.636862Z","title":"Living Reviews in Solar Physics 18(1):2","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.636862Z"},"links":{"cited_paper":"/paper/2007.06488","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:18217708e32e4db8086d546636ab0cfc787c128ef5ec8a10bedf3df8e7c4083c","observation_id":"17418d04-b062-4ebc-adeb-7284f2d11d49","resolution":{"observed_at":"2026-08-05T10:57:04.636862Z","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":"2026-08-05T10:57:04.639813Z","title":"121(877):213","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.639813Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:4e8fdc8bc03dc263934d8d79ea446d57c6c49c89f73f362bb68f9b06881713b5","observation_id":"75a40745-9677-4e66-a91f-55b4cccb4d24","resolution":{"observed_at":"2026-08-05T10:57:04.639813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.02305","last_updated":"2020-11-04T14:05:39Z","snapshot_observed_at":"2026-08-16T19:08:10.006114Z","submitted_at":"2020-11-04T14:05:39Z","title":"ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT). IV. Thioformaldehyde (H$_2$CS) in protoplanetary disks: spatial distributions and binding energies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.02305","snapshot_observed_at":"2026-08-05T10:57:04.644139Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.644139Z"},"links":{"cited_paper":"/paper/2011.02305","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:a70405d636230af59233830444edccf9afc241d2959d769ff50cb92fc57d52b7","observation_id":"173b63b0-4908-43db-afd5-35ebca17e575","resolution":{"observed_at":"2026-08-05T10:57:04.644139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.05592","last_updated":"2022-03-10T19:07:52Z","snapshot_observed_at":"2026-08-16T17:15:29.210310Z","submitted_at":"2022-03-10T19:07:52Z","title":"Galactic chemical evolution]{Galactic chemical evolution of the solar neighborhood, solar twins and exoplanet indicators","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.05592","snapshot_observed_at":"2026-08-05T10:57:04.647031Z","title":"512(3):3684--3690","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.647031Z"},"links":{"cited_paper":"/paper/2203.05592","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:673818692661524993aafce466f1d821d4aeece27b618d621afbc51987cbec75","observation_id":"7431bd45-da08-4b0d-9a17-eb1f899e64bb","resolution":{"observed_at":"2026-08-05T10:57:04.647031Z","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":"2026-08-05T10:57:04.650104Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.650104Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:1a4d8e7e29bbd40308c4a0bad16c82ce4b23bdcf5bfed18036cd93c526000463","observation_id":"5c1a0653-cd47-4971-b39b-7d1fdaec1b4f","resolution":{"observed_at":"2026-08-05T10:57:04.650104Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.6414","last_updated":"2013-11-25T19:27:31Z","snapshot_observed_at":"2026-08-14T23:54:00.980829Z","submitted_at":"2013-11-25T19:27:31Z","title":"Li depletion in solar analogues with exoplanets: Extending the sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.6414","snapshot_observed_at":"2026-08-05T10:57:04.652820Z","title":"Extending the sample","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.652820Z"},"links":{"cited_paper":"/paper/1311.6414","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:2483a20a56338ac87e8983fb88e58409dc48c83b202700ac7f6cf2bcea794517","observation_id":"3a9a5f6d-e02f-4ba1-b8b1-6f9de364b82e","resolution":{"observed_at":"2026-08-05T10:57:04.652820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.4618","last_updated":"2014-12-15T14:35:56Z","snapshot_observed_at":"2026-08-14T23:07:33.118220Z","submitted_at":"2014-12-15T14:35:56Z","title":"Li abundances in F stars: planets, rotation and galactic evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.4618","snapshot_observed_at":"2026-08-05T10:57:04.655683Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.655683Z"},"links":{"cited_paper":"/paper/1412.4618","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:4a7fb054cd59855c0c43cb9f3cf348dd7aa915b8207713625d5c26844247e5fd","observation_id":"6865b430-c96b-4e1f-b192-e8d12ed9a2d2","resolution":{"observed_at":"2026-08-05T10:57:04.655683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.07485","last_updated":"2022-12-14T20:06:34Z","snapshot_observed_at":"2026-08-16T16:08:35.923994Z","submitted_at":"2022-12-14T20:06:34Z","title":"The solar photospheric silicon abundance according to CO5BOLD: Investigating line broadening, magnetic fields, and model effects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.07485","snapshot_observed_at":"2026-08-05T10:57:04.658689Z","title":"Investigating line broadening, magnetic fields, and model effects","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.658689Z"},"links":{"cited_paper":"/paper/2212.07485","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:4fc3a0eb6f254b37fa8f676e51ce0c5566cd9e8a72410c708a4f2369845c8e98","observation_id":"e40fc9cb-f545-47ba-a5a3-a0e7bf20bd37","resolution":{"observed_at":"2026-08-05T10:57:04.658689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.03465","last_updated":"2017-04-11T18:00:05Z","snapshot_observed_at":"2026-08-17T21:39:07.555139Z","submitted_at":"2017-04-11T18:00:05Z","title":"The influence of atomic diffusion on stellar ages and chemical tagging","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.03465","snapshot_observed_at":"2026-08-05T10:57:04.662051Z","title":"840(2):99","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.662051Z"},"links":{"cited_paper":"/paper/1704.03465","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:4673dcfd5c5a36ef6ff4cdca0033c9fabd1159f4f0f10012160e5859a31c5a45","observation_id":"f95e3be2-9969-4b0e-b8d0-8d6c74e52550","resolution":{"observed_at":"2026-08-05T10:57:04.662051Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703213","last_updated":"2007-03-09T17:39:47Z","snapshot_observed_at":"2026-07-07T01:07:50.296173Z","submitted_at":"2007-03-09T17:39:47Z","title":"Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703213","snapshot_observed_at":"2026-08-05T10:57:04.665170Z","title":"663(2):866--894","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.665170Z"},"links":{"cited_paper":"/paper/astro-ph/0703213","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:e698be69b1703034b09e4522c882ae662b3256290d2a91d7911755efc4646c62","observation_id":"389bee5a-3c8f-43fb-aceb-84f295970309","resolution":{"observed_at":"2026-08-05T10:57:04.665170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.3028","last_updated":"2013-03-12T21:01:24Z","snapshot_observed_at":"2026-08-15T07:08:45.661639Z","submitted_at":"2013-03-12T21:01:24Z","title":"Stellar Multiplicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.3028","snapshot_observed_at":"2026-08-05T10:57:04.668889Z","title":"51(1):269--310","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.668889Z"},"links":{"cited_paper":"/paper/1303.3028","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:c9a2e49369b09d5c36b2ee6cfeae83048b96737d3181dbbbf2039f39d57b8fd4","observation_id":"584ab1d2-1e69-48c3-bcda-3cb721fb8f94","resolution":{"observed_at":"2026-08-05T10:57:04.668889Z","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":"10.1007/3-540-54752-5_186","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T11:08:14.039542Z","title":"p 39--43, doi:10.1007/3-540-54752-5_186","venue":"Lecture notes in physics","work_id":"9ea0930a-6d2a-4e9e-b50f-14fc85e7c8b7","year":1991},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.671705Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:0336d5d6f3971d01de7f6d8713bafb8e33a1fdc74c2b750c1205ff50c8523b73","observation_id":"45d327dd-3414-47fa-9b61-69ae4c42123a","resolution":{"observed_at":"2026-08-05T10:57:05.305042Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1209.2771","last_updated":"2012-09-13T03:18:55Z","snapshot_observed_at":"2026-08-15T00:46:54.433730Z","submitted_at":"2012-09-13T03:18:55Z","title":"Solar Fe abundance and magnetic fields - Towards a consistent reference metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.2771","snapshot_observed_at":"2026-08-05T10:57:04.674637Z","title":"Towards a consistent reference metallicity","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.674637Z"},"links":{"cited_paper":"/paper/1209.2771","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:69db44ed0b7a0539e3448a27c2ca04e28b6380dd55e5d31bab0973109a917728","observation_id":"cda75d8d-beb2-4b3f-b3cc-b996d51bd8fe","resolution":{"observed_at":"2026-08-05T10:57:04.674637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.05569","last_updated":"2019-01-29T19:12:14Z","snapshot_observed_at":"2026-08-14T17:44:01.441269Z","submitted_at":"2018-12-13T18:43:54Z","title":"Hints for a Turnover at the Snow Line in the Giant Planet Occurrence Rate","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.05569","snapshot_observed_at":"2026-08-05T10:57:04.677842Z","title":"874(1):81","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.677842Z"},"links":{"cited_paper":"/paper/1812.05569","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:0188aeb60fd2abe1c9d9ea8539ba7f2c790d3993aac081e9d10822b21dc81dac","observation_id":"2c012eff-0023-45fd-8f9a-5b5512afa0c9","resolution":{"observed_at":"2026-08-05T10:57:04.677842Z","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":"2026-08-05T10:57:04.680875Z","title":"In: Gomes N, Ascenso J (eds) 24th Portuguese National Astronomy and Astrophysics Meeting, p 51","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.680875Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:59fa4fa89e69d4fa8682c4d03fd513a2883817f2d452e303c19c23f91be7fed5","observation_id":"1137814b-0beb-4575-898c-7862a51aa364","resolution":{"observed_at":"2026-08-05T10:57:04.680875Z","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":"2026-08-05T10:57:04.683663Z","title":"Astronomische Nachrichten 323:213--219","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.683663Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:a394e59075c19f89de605ce1dd5fbd16eedc2a16c912669bda02e95b763b69e7","observation_id":"6eb2b646-28bb-4922-989f-dae2f6d517bd","resolution":{"observed_at":"2026-08-05T10:57:04.683663Z","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":"2026-08-05T10:57:04.686498Z","title":"922(2):129","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.686498Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:f40327bba18ea2a8467d989d600b17a9c02f523aaa58b5e2467e7452b633099d","observation_id":"0a40e9ff-342b-4095-86be-a580dda69c66","resolution":{"observed_at":"2026-08-05T10:57:04.686498Z","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":"2026-08-05T10:57:04.689316Z","title":"Cell 168(6)","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.689316Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:a8907c1476ad7e4fd38c2401f33ece003a786abd98bcc1bd5d2007fe75a82f69","observation_id":"84521fda-b9dc-4663-87c0-5526e22f52fc","resolution":{"observed_at":"2026-08-05T10:57:04.689316Z","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":"2026-08-05T10:57:04.692297Z","title":"285(2):403--412","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.692297Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:82894ab01abecb4ec2c238973ffab825271db27ae3c874b126d46250d6e3349b","observation_id":"0d47bfe4-2667-47e2-aa60-4084229885d1","resolution":{"observed_at":"2026-08-05T10:57:04.692297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0609829","last_updated":"2006-09-29T18:06:12Z","snapshot_observed_at":"2026-07-07T01:03:24.785292Z","submitted_at":"2006-09-29T18:06:12Z","title":"The Chemical Compositions of Stars with Planets: A Review","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0609829","snapshot_observed_at":"2026-08-05T10:57:04.695058Z","title":"118(849):1494--1505","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.695058Z"},"links":{"cited_paper":"/paper/astro-ph/0609829","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:bc930a9363cf1d374608cf2e430cfc09a15fde0ce91d93b815cdb626c8db2fa9","observation_id":"b7c0f852-ed7e-436d-b314-6f63cc38a736","resolution":{"observed_at":"2026-08-05T10:57:04.695058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.0480","last_updated":"2014-06-02T19:17:54Z","snapshot_observed_at":"2026-08-14T23:31:51.540921Z","submitted_at":"2014-06-02T19:17:54Z","title":"Solar System chemical abundances corrected for systematics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.0480","snapshot_observed_at":"2026-08-05T10:57:04.698258Z","title":"443:L99--L103","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.698258Z"},"links":{"cited_paper":"/paper/1406.0480","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:a04d62a39e0c9eb5788a72319e4b65c96c02ebe960985698148cc40fda742027","observation_id":"aefc9494-45b5-4306-831d-4dd89f176689","resolution":{"observed_at":"2026-08-05T10:57:04.698258Z","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":"2026-08-05T10:57:04.701103Z","title":"In: Holt SS, Sonneborn G (eds) Cosmic Abundances, p 117","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.701103Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:f1640f761702c3c2cf3eed7d8946dab502fa26ed7bc6489aae6ee96ffd1bc4a0","observation_id":"a8dd385f-608f-415d-b9a1-9e7b23dec4b2","resolution":{"observed_at":"2026-08-05T10:57:04.701103Z","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":"10.1023/a:1005164331058","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"doi:10.1023/A:1005164331058","venue":"Space Science Reviews","work_id":"b6a70c16-6a45-48e8-ae13-afbe46f0bdf9","year":1998},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.704057Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:fadf3bb4e3e44dd0b1b57fed8a990c32db77485d18210b42f09067dc4243c930","observation_id":"fe64d4b9-f0d7-48c6-832c-d97ecb5d4234","resolution":{"observed_at":"2026-08-05T10:57:05.276394Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.00547","last_updated":"2018-05-01T20:47:01Z","snapshot_observed_at":"2026-08-14T19:19:55.632024Z","submitted_at":"2018-05-01T20:47:01Z","title":"Dust cleansing of star-forming gas I: Did radiation from bright stars affect the chemical composition of the Sun and of M67?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.00547","snapshot_observed_at":"2026-08-05T10:57:04.706846Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.706846Z"},"links":{"cited_paper":"/paper/1805.00547","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:f9c8add184573c384bde4fe69596f4d9d9aa0c0e0bf5676045f3cf978e396a4e","observation_id":"671fead2-9bff-4140-b002-e94a03e76de6","resolution":{"observed_at":"2026-08-05T10:57:04.706846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.02361","last_updated":"2018-10-12T11:42:10Z","snapshot_observed_at":"2026-08-17T08:48:25.409948Z","submitted_at":"2018-09-07T08:56:09Z","title":"Dust cleansing of star-forming gas: II. Did late accretion flows change the chemical composition of the solar atmosphere?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.02361","snapshot_observed_at":"2026-08-05T10:57:04.709772Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.709772Z"},"links":{"cited_paper":"/paper/1809.02361","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:fc2db34e18794611583c74c2392b8cb84aea79c68bfab68916146489c4f3f561","observation_id":"8d56708a-cb25-40a1-a999-e733dbf74be2","resolution":{"observed_at":"2026-08-05T10:57:04.709772Z","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":"2026-08-05T10:57:04.712725Z","title":"328(1-2):185--191","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.712725Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:aaef270e16dc095e9c7b11bc9e65e692433b361e570f33fb9d6f3506dc5f1a95","observation_id":"623fdcb5-9807-4a41-8f11-36f36f82de3d","resolution":{"observed_at":"2026-08-05T10:57:04.712725Z","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":"10.1143/ptps.96.107","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Condensation of Dust Particles","venue":"Progress of Theoretical Physics Supplement","work_id":"835db4f8-1105-424f-96f8-2289ad718e1e","year":1988},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.715799Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:7e50aa42716a697eb43d5e93f8e135e995ec2027c852ab1fa9ebb706bc247a9e","observation_id":"df809858-d31a-4ab1-8da9-3a7e24c32664","resolution":{"observed_at":"2026-08-05T10:57:05.260212Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0112196","last_updated":"2001-12-07T22:46:46Z","snapshot_observed_at":"2026-08-10T06:40:25.179919Z","submitted_at":"2001-12-07T22:46:46Z","title":"The abundance pattern of the lambda Bootis stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0112196","snapshot_observed_at":"2026-08-05T10:57:04.718691Z","title":"381:959--970","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.718691Z"},"links":{"cited_paper":"/paper/astro-ph/0112196","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:2bee9de5d40c994132d15ae1afd9829f9083a28e7259ff456172a54887820e9b","observation_id":"391d5044-05dc-4f8b-b75b-bf27c331373b","resolution":{"observed_at":"2026-08-05T10:57:04.718691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0112198","last_updated":"2001-12-07T23:14:56Z","snapshot_observed_at":"2026-08-09T08:17:05.564683Z","submitted_at":"2001-12-07T23:14:56Z","title":"The accretion/diffusion theory for lambda Bootis stars in the light of spectroscopic data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0112198","snapshot_observed_at":"2026-08-05T10:57:04.721590Z","title":"381:971--981","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.721590Z"},"links":{"cited_paper":"/paper/astro-ph/0112198","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:43fa46726ea32870c1715a2ae15f4a799555f3f5d3cdae2d337160fe52e38592","observation_id":"9cf6d7e0-a194-4b96-bd66-f8f626c605a2","resolution":{"observed_at":"2026-08-05T10:57:04.721590Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.10941","last_updated":"2023-08-21T18:00:02Z","snapshot_observed_at":"2026-08-16T15:06:54.734685Z","submitted_at":"2023-08-21T18:00:02Z","title":"Stellar Wind Yields of Very Massive Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.10941","snapshot_observed_at":"2026-08-05T10:57:04.724433Z","title":"526(1):534--547","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.724433Z"},"links":{"cited_paper":"/paper/2308.10941","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:07703db4c38e376bd589a573e1efcb5e9fc7a7a287043a1de921b2aaa81aa8bd","observation_id":"bfee1ac9-1463-4a2c-b6ff-3dbc7b8657f3","resolution":{"observed_at":"2026-08-05T10:57:04.724433Z","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":"2026-08-05T10:57:04.727306Z","title":"In: Dworetsky MM, Castelli F, Faraggiana R (eds) IAU Colloq","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.727306Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:1e960ad5fa07f28cb9325aa97e9f5bceb295b18fe1a3b03cc939cf45c3dfcf28","observation_id":"d63fb063-283b-4f57-8812-4a0431db9bf5","resolution":{"observed_at":"2026-08-05T10:57:04.727306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.02477","last_updated":"2015-12-13T23:44:20Z","snapshot_observed_at":"2026-08-14T22:28:59.264721Z","submitted_at":"2015-10-08T20:04:43Z","title":"The Fundamentally Different Dynamics of Dust and Gas in Molecular Clouds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.02477","snapshot_observed_at":"2026-08-05T10:57:04.730098Z","title":"456(4):4174--4190","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.730098Z"},"links":{"cited_paper":"/paper/1510.02477","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:62f062db4fb3717e3550c553c6efc857b03938a1a0b1f6d5ee12656c9bc695f5","observation_id":"5dba7fa7-4f1d-4435-a647-791b28640acd","resolution":{"observed_at":"2026-08-05T10:57:04.730098Z","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":"10.1016/j.epsl.2018.01.018","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Earth and Planetary Science Letters 487:9--20","venue":"Earth and Planetary Science Letters","work_id":"5c169f60-21b1-4bfe-9df1-0e067d85b0e6","year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.732976Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:5a76db9793849e11a3629b92f9e39ad92f8b7df2639353a818443f1fd157cfd5","observation_id":"865304a9-1621-445d-8d6e-f46aff615d66","resolution":{"observed_at":"2026-08-05T10:57:05.250824Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16461","last_updated":"2023-06-28T18:00:04Z","snapshot_observed_at":"2026-08-16T15:20:17.474909Z","submitted_at":"2023-06-28T18:00:04Z","title":"How does accretion of planet-forming disks influence stellar abundances?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16461","snapshot_observed_at":"2026-08-05T10:57:04.735744Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.735744Z"},"links":{"cited_paper":"/paper/2306.16461","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:149c91f6f0895a203988fab31438616121625e8cc1a75d32183efaa8db04adc6","observation_id":"9eaedb19-e94a-42cd-879a-656ce52634c4","resolution":{"observed_at":"2026-08-05T10:57:04.735744Z","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":"2026-08-05T10:57:04.739619Z","title":"363(1):293--314","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.739619Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:e164b415962aa8f819e3de591b59aa8da0e1bedf27160ba056eb3e0cb1592b60","observation_id":"caac975e-54b0-4d87-b37f-8f389f91b2e0","resolution":{"observed_at":"2026-08-05T10:57:04.739619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.4198","last_updated":"2009-11-21T20:23:32Z","snapshot_observed_at":"2026-08-15T05:33:20.505269Z","submitted_at":"2009-11-21T20:23:32Z","title":"Enhanced lithium depletion in Sun-like stars with orbiting planets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.4198","snapshot_observed_at":"2026-08-05T10:57:04.742460Z","title":"462(7270):189--191","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.742460Z"},"links":{"cited_paper":"/paper/0911.4198","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:1efbea16d040a896a687c75f0ac15d5f172c9c585a88e4e9d12bd237a6a1bffc","observation_id":"2ec82342-fea9-4a89-b9d8-9300c2eb34ea","resolution":{"observed_at":"2026-08-05T10:57:04.742460Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.06308","last_updated":"2015-01-26T10:16:00Z","snapshot_observed_at":"2026-08-14T23:02:45.290967Z","submitted_at":"2015-01-26T10:16:00Z","title":"Gas giant planets as dynamical barriers to inward-migrating super-Earths","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.06308","snapshot_observed_at":"2026-08-05T10:57:04.745866Z","title":"800(2):L22","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.745866Z"},"links":{"cited_paper":"/paper/1501.06308","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:45a8b9b355dcbac3542703a3794c69f784589ed68d7b3dc22454d8f85562b8b4","observation_id":"a1ff75db-5ed4-4db1-9fd0-58e81072761e","resolution":{"observed_at":"2026-08-05T10:57:04.745866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.03634","last_updated":"2017-05-24T17:20:57Z","snapshot_observed_at":"2026-08-14T21:12:30.529911Z","submitted_at":"2017-03-10T11:34:20Z","title":"Breaking the Chains: Hot Super-Earth systems from migration and disruption of compact resonant chains","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.03634","snapshot_observed_at":"2026-08-05T10:57:04.749153Z","title":"470(2):1750--1770","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.749153Z"},"links":{"cited_paper":"/paper/1703.03634","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:724fbb2ec710bbcf6eb64ecc1a6cc3c6251f9ecc1ee4e64be07a2c313fa013ff","observation_id":"af20abcc-032d-4b44-b35f-c4900789fc6c","resolution":{"observed_at":"2026-08-05T10:57:04.749153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.00027","last_updated":"2015-06-30T20:29:04Z","snapshot_observed_at":"2026-08-14T22:42:15.967765Z","submitted_at":"2015-06-30T20:29:04Z","title":"Gaia FGK benchmark stars: abundances of alpha and iron-peak elements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.00027","snapshot_observed_at":"2026-08-05T10:57:04.752237Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.752237Z"},"links":{"cited_paper":"/paper/1507.00027","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:41e60fdbbbf70d105f3dcee8454a22b5e88c014c43737145c45a73dd272f5eb0","observation_id":"bd18b216-ddbb-4f39-9255-4f1005caf2c9","resolution":{"observed_at":"2026-08-05T10:57:04.752237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.08041","last_updated":"2018-11-20T01:30:36Z","snapshot_observed_at":"2026-08-14T17:56:27.614758Z","submitted_at":"2018-11-20T01:30:36Z","title":"Accuracy and precision of industrial stellar abundances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.08041","snapshot_observed_at":"2026-08-05T10:57:04.755542Z","title":"57:571--616","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.755542Z"},"links":{"cited_paper":"/paper/1811.08041","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:5111057ecea7f09f618f72dea290134125c9d53a53a8d85ae44dea252253e4f3","observation_id":"f51a9b59-0cb6-484c-ae85-888d4440c019","resolution":{"observed_at":"2026-08-05T10:57:04.755542Z","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":"2026-08-05T10:57:04.758694Z","title":"In: American Astronomical Society Meeting Abstracts, p 340.04D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.758694Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:7b69b76e0127af3e2cfc470c0ebb33c68b03bfed4a871fc99fbc553fb4f07cf0","observation_id":"aa43aea1-57b4-4f96-b7fb-3d2f64b87fda","resolution":{"observed_at":"2026-08-05T10:57:04.758694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.01484","last_updated":"2018-09-13T16:23:28Z","snapshot_observed_at":"2026-08-17T12:17:54.477654Z","submitted_at":"2018-05-03T18:00:41Z","title":"Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.01484","snapshot_observed_at":"2026-08-05T10:57:04.762790Z","title":"863(2):191","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.762790Z"},"links":{"cited_paper":"/paper/1805.01484","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:7d0da64dcae2ac85301da37f1a6dae35c0994e4957a50a9b329c86549aa13684","observation_id":"1e60c769-7c33-4d94-8dfc-56ac540bd007","resolution":{"observed_at":"2026-08-05T10:57:04.762790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.04672","last_updated":"2015-09-16T21:32:30Z","snapshot_observed_at":"2026-08-14T22:32:16.201566Z","submitted_at":"2015-09-15T18:33:17Z","title":"Lambda Boo Abundance Patterns: Accretion from Orbiting Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.04672","snapshot_observed_at":"2026-08-05T10:57:04.766560Z","title":"150(6):166","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.766560Z"},"links":{"cited_paper":"/paper/1509.04672","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:da0b214c65573b9880b98efb8ad9deaa39c6c8ccf2743036e4ba67f8ddc31c0c","observation_id":"42a6e45b-7400-44d7-b4d4-be7d8a51c3f5","resolution":{"observed_at":"2026-08-05T10:57:04.766560Z","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":"10.1111/maps.14272","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Meteoritics & Planetary Science 59(12):3193--3214","venue":"Meteoritics and Planetary Science","work_id":"d539c335-fcab-4e3c-b842-0a83ffb0a518","year":2024},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.769527Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:53808717de1c1e396697a624574bec34a28265e433881dda9ce1dd06da21a202","observation_id":"e554936f-eea0-43dd-a27b-3aa6af2cb088","resolution":{"observed_at":"2026-08-05T10:57:05.241055Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[{"edge_observation":{"observed_at":"2026-08-05T12:18:18.660265+00:00","source":"paper_reference_links","state":"open"},"event_date":"2025-11-11","event_type":"correction","notice_doi":"10.1111/maps.70059","provenance":{"observed_at":"2026-07-11T02:55:43.045809+00:00","source":"crossref","source_record_id":"10.1111/maps.70059->10.1111/maps.14272:correction"}}],"reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T10:57:04.772273Z","title":"335(2):L45--L49","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.772273Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:03386112342babc1e024f9c4b6c6ab7afe2b187865c13bd8a7b3aeca2d5ee87a","observation_id":"07c34379-ad89-493d-bf11-d49651443cc1","resolution":{"observed_at":"2026-08-05T10:57:04.772273Z","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":"2026-08-05T10:57:04.775042Z","title":"91(1-2):175--180","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.775042Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:e8fa969247946a173a46a5c512d0fd1d83109c7bda4a17dc0756748246071f2c","observation_id":"a5c608cc-6560-47b3-abe6-25dca3e76880","resolution":{"observed_at":"2026-08-05T10:57:04.775042Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.4527","last_updated":"2011-08-25T10:44:44Z","snapshot_observed_at":"2026-08-15T04:37:34.258022Z","submitted_at":"2011-08-23T08:54:04Z","title":"Is the solar spectrum latitude dependent? An investigation with SST/TRIPPEL","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.4527","snapshot_observed_at":"2026-08-05T10:57:04.778338Z","title":"An investigation with SST/TRIPPEL","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.778338Z"},"links":{"cited_paper":"/paper/1108.4527","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:8b1210752cf7a18072ad7a8a521b978524c1d43113fbc4eb2b92179f1a16dfd1","observation_id":"2fcd3489-9c7c-4303-8289-ad2308b07e54","resolution":{"observed_at":"2026-08-05T10:57:04.778338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.0639","last_updated":"2007-09-05T13:16:45Z","snapshot_observed_at":"2026-08-16T04:44:28.003694Z","submitted_at":"2007-09-05T13:16:45Z","title":"Atomic Diffusion and Mixing in Old Stars I. VLT/FLAMES-UVES Observations of Stars in NGC 6397","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.0639","snapshot_observed_at":"2026-08-05T10:57:04.781406Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.781406Z"},"links":{"cited_paper":"/paper/0709.0639","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:8ba0d6386fafae717bd639b39fc2cedb9152d4215538bc617c29948ae33da8e8","observation_id":"548b6fe2-9ae4-401f-be39-1e51c3976c39","resolution":{"observed_at":"2026-08-05T10:57:04.781406Z","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":"10.1002/chem.201801847","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T11:08:14.039542Z","title":"doi:10.1002/chem.201801847","venue":"Chemistry - A European Journal","work_id":"13c664c2-f3de-4867-ae83-6f545831b31c","year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.784503Z"},"links":{"citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:4ab2140dbe54521720b908ef9587b3fb26041b4ba51b9f8f9230707a033d587b","observation_id":"971d826c-885a-4c35-b1cd-c5ea3b8be6ca","resolution":{"observed_at":"2026-08-05T10:57:05.231157Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1412.0585","last_updated":"2015-05-27T10:47:17Z","snapshot_observed_at":"2026-08-14T23:09:28.234907Z","submitted_at":"2014-12-01T18:46:45Z","title":"Evolution of the Milky Way with radial motions of stars and gas I. The solar neighborhood and the thin and thick disk","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.0585","snapshot_observed_at":"2026-08-05T10:57:04.787515Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.787515Z"},"links":{"cited_paper":"/paper/1412.0585","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:35087dcf141e82139aec83ed94c1380d288987bda5f4ed2c3a7fa3700e8aabfd","observation_id":"ab4d9009-27d8-4d6c-9c59-d881c7794c53","resolution":{"observed_at":"2026-08-05T10:57:04.787515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.10360","last_updated":"2017-06-26T21:14:26Z","snapshot_observed_at":"2026-08-14T21:27:47.793875Z","submitted_at":"2016-11-30T20:59:21Z","title":"Zoom-Simulations of Protoplanetary Disks starting from GMC scales","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.10360","snapshot_observed_at":"2026-08-05T10:57:04.791244Z","title":"846(1):7","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.791244Z"},"links":{"cited_paper":"/paper/1611.10360","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:35abad2d996ffd4f0d55f66069826a5b1ba55059ddd4747b58f2d1f97a24bb0e","observation_id":"9d0ba377-0239-4012-aa6b-059675bffa2c","resolution":{"observed_at":"2026-08-05T10:57:04.791244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.07901","last_updated":"2017-02-25T15:00:41Z","snapshot_observed_at":"2026-08-14T21:14:48.038293Z","submitted_at":"2017-02-25T15:00:41Z","title":"Revisiting the pre-main-sequence evolution of stars I. Importance of accretion efficiency and deuterium abundance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.07901","snapshot_observed_at":"2026-08-05T10:57:04.794516Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.794516Z"},"links":{"cited_paper":"/paper/1702.07901","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:5728ab85939cd2157ba1a372766dbf6bbbe5b3320b09984367f6c3194233392c","observation_id":"bedc2a06-0ae7-4f81-b0a2-a6f3ae2234e3","resolution":{"observed_at":"2026-08-05T10:57:04.794516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.07396","last_updated":"2018-08-22T14:54:19Z","snapshot_observed_at":"2026-08-14T18:38:18.818894Z","submitted_at":"2018-08-22T14:54:19Z","title":"Revisiting the pre-main-sequence evolution of stars II. Consequences of planet formation on stellar surface composition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.07396","snapshot_observed_at":"2026-08-05T10:57:04.797435Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.797435Z"},"links":{"cited_paper":"/paper/1808.07396","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:b305b9b8484c0cea655597095524a6889971c167782466955c692b6d06202f66","observation_id":"39195dde-5d8f-418b-be8d-ed8a1d1702e1","resolution":{"observed_at":"2026-08-05T10:57:04.797435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.19089","last_updated":"2024-07-16T08:17:47Z","snapshot_observed_at":"2026-08-16T13:48:13.018371Z","submitted_at":"2024-05-29T13:52:36Z","title":"Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.19089","snapshot_observed_at":"2026-08-05T10:57:04.800748Z","title":"533(1):538--550","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.800748Z"},"links":{"cited_paper":"/paper/2405.19089","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:60981e0444400f434a8890c7b72bbd3f60a696ed750207c5a46f7d049aa01ef0","observation_id":"94dc4cc7-38b2-44d9-999b-f7db0c145a47","resolution":{"observed_at":"2026-08-05T10:57:04.800748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.04057","last_updated":"2024-05-07T06:59:48Z","snapshot_observed_at":"2026-08-16T13:54:48.401615Z","submitted_at":"2024-05-07T06:59:48Z","title":"Super-Earths and Earth-like Exoplanets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.04057","snapshot_observed_at":"2026-08-05T10:57:04.803883Z","title":"Treatise on Geochemistry 7:51--112","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.803883Z"},"links":{"cited_paper":"/paper/2405.04057","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:3f82aa3364c80385b7dc6efefe0971e51bd11bfab72178da394f6f43c4a57e1e","observation_id":"c5785cfb-6b2c-4f7b-9da3-e701f08d1543","resolution":{"observed_at":"2026-08-05T10:57:04.803883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.00697","last_updated":"2024-01-01T08:25:33Z","snapshot_observed_at":"2026-08-16T14:30:31.856685Z","submitted_at":"2024-01-01T08:25:33Z","title":"3D non-LTE abundance analyses of late-type stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.00697","snapshot_observed_at":"2026-08-05T10:57:04.806913Z","title":"62(1):475--527","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.806913Z"},"links":{"cited_paper":"/paper/2401.00697","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:9ad3f70bc0900758b3cd6519adb465cdd4f0b3a4bc39e9d7990612479c450214","observation_id":"5219234d-cb4d-4e32-8d2e-b41df4150ee1","resolution":{"observed_at":"2026-08-05T10:57:04.806913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.03788","last_updated":"2016-08-12T13:32:57Z","snapshot_observed_at":"2026-08-14T21:44:23.704714Z","submitted_at":"2016-08-12T13:32:57Z","title":"The chemical compositions of solar twins in the open cluster M67","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.03788","snapshot_observed_at":"2026-08-05T10:57:04.809974Z","title":"463(1):696--704","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.809974Z"},"links":{"cited_paper":"/paper/1608.03788","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:75b1692bc7c32ecc780a2df009b62a96619b0f3da1a12c00a2a76fcd1f5142da","observation_id":"85aea0b7-61d1-45bd-8ad4-a008b4232c37","resolution":{"observed_at":"2026-08-05T10:57:04.809974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.07354","last_updated":"2016-03-02T02:13:23Z","snapshot_observed_at":"2026-08-14T22:12:54.262598Z","submitted_at":"2016-01-27T13:13:46Z","title":"The Hyades open cluster is chemically inhomogeneous","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.07354","snapshot_observed_at":"2026-08-05T10:57:04.812927Z","title":"457(4):3934--3948","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.812927Z"},"links":{"cited_paper":"/paper/1601.07354","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:83c8d427a4b40a4bf445cd6d776d26d50152c99fc658c5d68143e69c15160986","observation_id":"147f2a17-8959-448d-8b0c-15ace6691018","resolution":{"observed_at":"2026-08-05T10:57:04.812927Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.11008","last_updated":"2019-06-06T13:34:24Z","snapshot_observed_at":"2026-08-14T17:09:45.298232Z","submitted_at":"2019-02-28T10:52:50Z","title":"Chemical (in)homogeneity and atomic diffusion in the open cluster M67","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.11008","snapshot_observed_at":"2026-08-05T10:57:04.816136Z","title":"627:A117","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-05T10:57:04.816136Z"},"links":{"cited_paper":"/paper/1902.11008","citing_paper":"/paper/2509.03435"},"observation_digest":"sha256:f6584b1258eaca305b98aac47356b1afc37ed44225bb22f87430edf83e3e10ae","observation_id":"ace9b7c4-a5fa-4637-8b8f-00397fd32dda","resolution":{"observed_at":"2026-08-05T10:57:04.816136Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2509.03435","last_updated":"2025-09-03T16:06:30Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-18T01:17:22.385387Z","submitted_at":"2025-09-03T16:06:30Z","title":"Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":90,"verified_exact":9,"verified_fuzzy":0},"total_outbound_references":184},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 100 of 184 outbound references and 0 inbound Pith citation observations for arXiv:2509.03435."}