Paper Citation Record · LEDGER

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars

As of 20 August 2026, this Paper Citation Record lists 48 of 48 outbound references and 1 inbound Pith citation observation for arXiv:2505.16458.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2505.16458 v1

Coverage vector

measured 48 of 48 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:07:57.732283Z

measured 49 of 49 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:32:32.053351Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-08T16:32:32.591786Z

Reference resolution

48 of 48 outbound references displayed

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External citation measurements

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Outbound references

Observation 759033f3-239b-4c4f-953b-043d1c59e2ce · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 1

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Observation 626d9578-e123-4a91-9424-80e1259c152a · outbound

This paper cites J., & Scott, P.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars J., & Scott, P

Reference 2

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Observation 6bf23488-96ce-4330-bff1-7080b54d3af7 · outbound

This paper cites I., Abbott, D.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars I., Abbott, D

Reference 3

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This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 4

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Observation d83ed359-9b14-45e8-97d6-2a7ad465db49 · outbound

This paper cites O., Moens, N., et al.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars O., Moens, N., et al

Reference 5

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Observation 87a2bfeb-339c-4af3-926a-451e65e4d5cd · outbound

This paper cites 2020, A&A, 641, A26.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars 2020, A&A, 641, A26

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:08:03.877334Z

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Observation 58bf8cd5-0230-4f83-b807-3afb2d5445eb · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 7

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:08:03.761455Z

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Observation 2f9e888a-8aee-491d-af84-cdfac2d66821 · outbound

This paper cites & Noels, A.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars & Noels, A

Reference 8

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Observation 34a515c9-4ac1-467d-a63a-4e9ca2ef8ca8 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 9

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Observation f060563a-9b08-4fa4-bdc4-a1ab374aa7e9 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:54.131353Z

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Observation ce804928-63b8-4143-aaa5-50de3e96e8ff · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:54.217278Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 24be8995-95db-41ae-acd8-aaa826a263a9 · outbound

This paper cites R., Gräfener, G., & Liermann, A.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars R., Gräfener, G., & Liermann, A

Reference 12

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Observation ff0551b2-696f-4898-969a-7908f782e0ca · outbound

This paper cites R., Gräfener, G., Oskinova, L., & Liermann, A.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars R., Gräfener, G., Oskinova, L., & Liermann, A

Reference 13

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Observation 1f56577e-83e7-40a5-b17f-e6d0076080fe · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 14

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:08:02.698119Z

Source-reported events for the cited work

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Observation bda43300-a995-4322-9d90-7dcf6c40c8a5 · outbound

This paper cites R., Schmutz, W., & Wessolowski, U.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars R., Schmutz, W., & Wessolowski, U

Reference 15

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Observation d4d80b82-9478-4f17-b933-b5e0629bf516 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 16

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:08:02.090590Z

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Observation b5edb69b-469d-497e-bfb4-8121c0fa4ce8 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 17

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Observation 84f1ef73-5dd8-4d5f-9e13-66c072dcb684 · outbound

This paper cites J., Lanz, T., Heap, S.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars J., Lanz, T., Heap, S

Reference 18

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This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 19

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Observation e069375d-53be-4450-8672-017d73267bf0 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 20

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:08:01.644684Z

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Observation 98c6a365-28bc-4788-8041-f7e2562976c5 · outbound

This paper cites & Lanz, T.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars & Lanz, T

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:08:01.475952Z

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Observation 1275e7b4-e4a0-436f-b80a-406682ddd751 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 22

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Observation 2c5f9ca2-5972-416c-96b2-be6288b30ccc · outbound

This paper cites R., Sander, A.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars R., Sander, A

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:08:01.144051Z

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Observation fb4c4c31-fea0-48cf-8014-4851c6696571 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 24

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:08:00.924832Z

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Observation 5754e67e-433d-414b-903c-5fde8115ec15 · outbound

This paper cites & Lamers, H.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars & Lamers, H

Reference 25

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:08:00.618358Z

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Observation ab0ec5d8-d6c8-4b6c-a905-02df4310c5c5 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 26

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Source-reported events for the cited work

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Observation 4e4b0053-f7fa-4fe7-b1e8-e69a4dc7f7de · outbound

This paper cites G., Kee, N.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars G., Kee, N

Reference 27

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Observation 34515136-8f93-42bb-ac07-2217af24a808 · outbound

This paper cites G., Sundqvist, J.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars G., Sundqvist, J

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:08:00.101038Z

Source-reported events for the cited work

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Observation 1838838c-2d74-4cd9-abf7-d9545d49c106 · outbound

This paper cites 1998, A&A, 334, 505.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars 1998, A&A, 334, 505

Reference 29

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Source-reported events for the cited work

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Observation d8f73fd6-486a-4e5b-b619-457fca5a182b · outbound

This paper cites 2008, in Massive Stars as Cosmic Engines, ed.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars 2008, in Massive Stars as Cosmic Engines, ed

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:07:59.826633Z

Source-reported events for the cited work

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Observation fa46eb1c-c381-476d-9e84-22c8f15f44d5 · outbound

This paper cites A., Venero, R., et al.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars A., Venero, R., et al

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:07:59.603728Z

Source-reported events for the cited work

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Observation 8199b495-dc28-402a-9d3f-97fcf6d1745a · outbound

This paper cites D., Lee, L., Schaefer, G., et al.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars D., Lee, L., Schaefer, G., et al

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:07:59.398160Z

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Observation 7be2ba4b-1384-4f31-a661-85463bcb8588 · outbound

This paper cites 2015, A&A, 577, A13.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars 2015, A&A, 577, A13

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:55.971552Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f7d74918-a8cd-4465-9aa2-e8920df2c2f0 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 34

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:07:59.146103Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation b0697c7e-8c04-4979-85ff-1ebc78e153fa · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 35

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:07:58.932010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 8a222b1f-7ca9-4998-b4ef-c843a91d88f9 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 36

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:07:58.717071Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 9afa4816-1372-449b-93b6-0d44306f15ce · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 37

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Observation 58933916-eb4b-49c2-b228-4f305fc78eb9 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:56.687681Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9e59ff2-eccf-4a8e-a136-35eb9ab272a6 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:56.809842Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33d9eb98-31b7-4f1e-a36b-092b186c3058 · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:56.924646Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09c04050-9412-46ee-b768-4f51407aff6c · outbound

This paper cites an unresolved cited work.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Unresolved cited work

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:57.020748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a24a03f6-9d48-4c5f-9c4f-672360aac952 · outbound

This paper cites R., & Wessolowski, U.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars R., & Wessolowski, U

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:57.131497Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 337e3109-c66d-4c37-9729-a476b93696d4 · outbound

This paper cites Wolf-Rayet stars.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars Wolf-Rayet stars

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:57.267787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d190c562-a46b-49cc-9a37-d34e530a33fa · outbound

This paper cites 2020, A&A, 639, L6.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars 2020, A&A, 639, L6

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:57.379051Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2d7babd0-b62f-4722-8da3-c4e0eb5ab787 · outbound

This paper cites 2014, ARA&A, 52, 487.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars 2014, ARA&A, 52, 487

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-07T15:07:57.474059Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6eeff1e9-2469-4b1b-b534-c7d710cfeb2f · outbound

This paper cites & Conti, P.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars & Conti, P

Reference 46

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:07:58.443157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 427f06de-e989-4bcf-a95d-750a369250f2 · outbound

This paper cites O., Owocki, S.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars O., Owocki, S

Reference 47

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:07:58.200327Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation b5a95d31-21ac-49a0-bfdb-bad0524b86b3 · outbound

This paper cites 2018, ApJS, 234, 30 Article number, page 12 of 16 G.

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars 2018, ApJS, 234, 30 Article number, page 12 of 16 G

Reference 48

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:07:57.980973Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Pith citing papers

Observation 0f53b237-facc-49de-998a-105d92fc6603 · inbound

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind cites this paper.

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars

Reference 180

Resolution: verified exact; local_arxiv, observed 2026-08-08T16:32:32.597159Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.