Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-06T17:52:01.336643Z
Paper Citation Record · LEDGER
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations
As of 14 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 2 inbound Pith citation observations for arXiv:2507.09936.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T07:32:04.538630Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
54 of 54 outbound references displayed
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External citation measurements
No source-named external measurement is stored.
Outbound references
Observation eea98eb5-0dda-486d-8090-4cda82cc33f5 · outbound
This paper cites 2024, A&A, 687, A90.
Reference 1
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 1b7d293a-f20e-42bd-9f82-adc66530ea7a · outbound
This paper cites an unresolved cited work.
Reference 2
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation acafc2fd-e1e8-497f-aaa5-106fe3592ad4 · outbound
This paper cites 2014, ApJ, 786, 116.
Reference 3
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 60428326-48a5-4064-b99b-940b5aab0579 · outbound
This paper cites an unresolved cited work.
Reference 4
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation be62b921-853d-4bbd-be6c-f33b708d933b · outbound
This paper cites & Teyssier, R.
Reference 5
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d5798fd8-9b47-465b-8f6e-5f30b77b338c · outbound
This paper cites A., Bate, M.
Reference 6
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 0bb17843-8aff-46ad-8410-d311ed2b2885 · outbound
This paper cites J., Noriega-Crespo, A., Mizuno, D.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations J., Noriega-Crespo, A., Mizuno, D
Reference 7
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 611ce85f-b545-43f2-b00e-53dd45fae0e8 · outbound
This paper cites 2015, A&A, 579, A71.
Reference 8
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 35257a3a-8dfe-4d87-8210-56d1d37f90da · outbound
This paper cites C., Glover, S.
Reference 9
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T17:52:02.041845Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation f18f8be1-f47e-4532-b730-0688d81acdf9 · outbound
This paper cites 2025, A&A, 696, A151 Di Mascia, F., Pallottini, A., Sommovigo, L., & Decataldo, D.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations 2025, A&A, 696, A151 Di Mascia, F., Pallottini, A., Sommovigo, L., & Decataldo, D
Reference 10
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation dfd64aaf-f3a4-49be-a0fe-0ab7984b8fbb · outbound
This paper cites 2021, OpTool: Command-line driven tool for creating complex dust opacities, Astrophysics Source Code Library, record ascl:2104.010.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations 2021, OpTool: Command-line driven tool for creating complex dust opacities, Astrophysics Source Code Library, record ascl:2104.010
Reference 11
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2485cb9a-d135-4a2d-a5df-7eabb07b62c3 · outbound
This paper cites 2013, A&A, 558, A125.
Reference 12
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T17:52:01.998764Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation a7c67225-b6ad-453f-80ad-cdf45cd668bb · outbound
This paper cites P., Juhasz, A., Pohl, A., et al.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations P., Juhasz, A., Pohl, A., et al
Reference 13
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6e22b3de-ec77-44f6-9bc2-8440cf5f30c1 · outbound
This paper cites K., Robitaille, T.
Reference 14
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation dbf0ef24-fd74-4072-b613-c76ea77657f7 · outbound
This paper cites 2017, MNRAS, 471, 100.
Reference 15
- Resolution
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Source-reported events for the cited work
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Observation 8ec975a4-495d-4169-ad3f-3f5d1d95fa4e · outbound
This paper cites & Pezzuto, S.
Reference 16
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 965eac3a-6bd0-40a5-81f0-5e4b243c50a4 · outbound
This paper cites 2018, A&A, 615, A94.
Reference 17
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation b67a5dab-7ee1-43ad-bb4c-a9ec545d9b3f · outbound
This paper cites 2006, A&A, 457, 371.
Reference 18
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation a3e66bd4-e9fe-4846-b8f9-4ff1ef1e07f2 · outbound
This paper cites J., Abergel, A., Abreu, A., & et al.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations J., Abergel, A., Abreu, A., & et al
Reference 19
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 4f3ad86e-528b-465c-a0ee-2a0625187f3b · outbound
This paper cites D., Devriendt, J.
Reference 20
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation ec620b45-1109-4c37-afd3-8471878a6c33 · outbound
This paper cites S., & Audit, E.
Reference 21
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation d1ae0ec0-b74d-456a-b979-45747f3bac9f · outbound
This paper cites an unresolved cited work.
Reference 22
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation b1c93f0e-1b55-41cf-b475-f04d1878635e · outbound
This paper cites an unresolved cited work.
Reference 23
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fa80ba06-6831-40a4-aab8-e56020fe1555 · outbound
This paper cites 1941, Akademiia Nauk SSSR Doklady, 30, 301.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations 1941, Akademiia Nauk SSSR Doklady, 30, 301
Reference 24
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a6ea2ace-f957-47fa-899d-8f4810d8321f · outbound
This paper cites & Yorke, H.
Reference 25
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 2f3bd826-f94a-493c-b64e-6c71e81f57ae · outbound
This paper cites S., Mezger, P.
Reference 26
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation dc8179b9-5dd6-4238-8759-426e46f3e6b2 · outbound
This paper cites S., Rumpl, W., & Nordsieck, K.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations S., Rumpl, W., & Nordsieck, K
Reference 27
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e269dadc-dd7b-4986-bf01-cd1ffb54417e · outbound
This paper cites an unresolved cited work.
Reference 28
- Resolution
- unresolved
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation c67bbd2b-8bb6-4dcc-802e-513b7930a501 · outbound
This paper cites an unresolved cited work.
Reference 29
- Resolution
- unresolved
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 1601062d-dcbf-49a9-85d7-a574c271443d · outbound
This paper cites P., Dominik, C., de Koter, A., & Hovenier, J.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations P., Dominik, C., de Koter, A., & Hovenier, J
Reference 30
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 92cbf1f8-5f32-4e81-9e75-3fbcacf71e5b · outbound
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Reference 31
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Source-reported events for the cited work
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Observation 58d71d68-79ae-45bf-9d3c-637338a5eb23 · outbound
This paper cites 2025, A&A, 696, A149.
Reference 32
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 959db2a5-5991-47f1-b844-8c29eb61aed3 · outbound
This paper cites 2010, PASP, 122, 314.
Reference 33
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 37f4494c-b5fe-4626-aee5-183426f5e1e7 · outbound
This paper cites 2024, ApJ, 966, 171.
Reference 34
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 6a5c0c21-271e-4dd1-a466-cc2aeb57de3c · outbound
This paper cites 2022, A&A, 662, A8.
Reference 35
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation da227716-794d-4091-9103-bdac9827d43f · outbound
This paper cites 2018, AR&A, 56, 41.
Reference 36
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 3980401d-742e-4ffa-b6fd-55a56919348f · outbound
This paper cites 2018, A&A, 618, L5.
Reference 37
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 1ce3e501-9108-4bb0-9d08-46f6c0673203 · outbound
This paper cites an unresolved cited work.
Reference 38
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation e2708a4f-1702-43cd-8719-dc71fb6f09e8 · outbound
This paper cites 2020, MNRAS, 496, 3482.
Reference 39
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 08a55e30-ec82-4a9c-84a8-0a98070807e6 · outbound
This paper cites 2012, A&A, 547, A54.
Reference 40
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation e704496c-6df3-4f9e-a0fc-2ed4f8180d94 · outbound
This paper cites 2010, A&A, 518, L2.
Reference 41
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 06dcbd13-569d-46ea-b409-59c3de4874df · outbound
This paper cites 2022, A&A, 664, A26.
Reference 42
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 102cf2e7-ac74-44bf-a672-c9ecafa8d879 · outbound
This paper cites an unresolved cited work.
Reference 43
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation a929637e-4ae9-42d0-a25a-c40089c4e8bd · outbound
This paper cites E., Shirley, Y.
Reference 44
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 0afb9e2e-3dd6-4d5b-ae37-fefac2ff4350 · outbound
This paper cites E., Shirley, Y.
Reference 45
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation bf78238e-b0b8-4f0e-80ea-3a821258248a · outbound
This paper cites 2002, A&A, 385, 337.
Reference 46
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5d45a0a7-53ef-4118-931a-3705f4664334 · outbound
This paper cites 2011, MNRAS, 416, 2932.
Reference 47
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 92cb2909-4875-493e-9c14-55a65a7956c1 · outbound
This paper cites A., Duarte-Cabral, A., & et al.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations A., Duarte-Cabral, A., & et al
Reference 48
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T17:52:01.465660Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 4b7c9742-a047-432b-abee-1c321e647c7c · outbound
This paper cites M., Avison, A., et al.
Reference 49
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T17:52:01.450529Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation fdac9bcb-7552-45e5-b4a7-412f151a2573 · outbound
This paper cites 2024, A&A, 684, A36.
Reference 50
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation d86d0a10-8ca6-40df-b4a4-f3f5a084f0de · outbound
This paper cites The Turbulent Support (TS) and Global Hierarchical Collapse (GHC) models for molecular clouds compared. Differences, convergence, and myths.
The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations The Turbulent Support (TS) and Global Hierarchical Collapse (GHC) models for molecular clouds compared. Differences, convergence, and myths
Reference 51
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2aa96274-67b1-4687-8921-d05d9d7a633c · outbound
This paper cites A., Kirk, J.
Reference 52
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 9a705247-37db-4244-a08b-9990dfaf7be2 · outbound
This paper cites 2016, A&A, 586, A103.
Reference 53
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bff0e3cc-7581-4adc-8336-363870d27d9b · outbound
This paper cites ground truth.
Reference 54
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Pith citing papers
Observation 3fdb318c-82ab-4cc7-9c20-86d4e333a822 · inbound
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations
Reference 66
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 790449a9-3ac3-4424-8bf7-ec003f93dfc7 · inbound
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations
Reference 66
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.