Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-15T22:15:53.854480Z
Paper Citation Record · LEDGER
Why is the Star Formation Rate Proportional to Dense Gas Mass?
As of 18 August 2026, this Paper Citation Record lists 75 of 75 outbound references and 0 inbound Pith citation observations for arXiv:2505.07764.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
75 of 75 outbound references displayed
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- verified fuzzy33
- unresolved40
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External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 2bcc1752-5c21-481f-a277-019811034f60 · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 1
- Resolution
- unresolved
- raw_fallback, observed 2026-08-15T22:15:54.711809Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation f5b65eb8-faa3-458b-b0bc-7915b78fa1f4 · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 2
- Resolution
- unresolved
- raw_fallback, observed 2026-08-15T22:15:54.699380Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation ee8260f7-d9db-42b8-84d1-d851838e2239 · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 3
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bd845c07-12eb-4ffd-8d95-51100cb9875a · outbound
This paper cites & Arnouts, S.
Why is the Star Formation Rate Proportional to Dense Gas Mass? & Arnouts, S
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.560812Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 154b5aa4-5f0b-442f-9283-347ba3c6f532 · outbound
This paper cites 2024, A&A, 687, A163.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2024, A&A, 687, A163
Reference 5
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.671049Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 22cf56f6-28f4-431a-93ca-de417f2e39e6 · outbound
This paper cites A., Bate, M.
Why is the Star Formation Rate Proportional to Dense Gas Mass? A., Bate, M
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.569091Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b07b0dfe-fc3a-4d6f-88c8-fcf795624cf1 · outbound
This paper cites H.-H., Burkhart, B., Goodman, A., & Collins, D.
Why is the Star Formation Rate Proportional to Dense Gas Mass? H.-H., Burkhart, B., Goodman, A., & Collins, D
Reference 7
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 054009af-8c3a-4a14-af39-f7399298f4f0 · outbound
This paper cites INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function.
Why is the Star Formation Rate Proportional to Dense Gas Mass? INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function
Reference 8
- Resolution
- metadata mismatch
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation ce474820-fba2-4ad4-a4ea-5a4f7c3efb6d · outbound
This paper cites & Povich, M.
Why is the Star Formation Rate Proportional to Dense Gas Mass? & Povich, M
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.583875Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3c83b5d5-aa12-4656-bfa3-22132eee29b2 · outbound
This paper cites R., & Newman, M.
Why is the Star Formation Rate Proportional to Dense Gas Mass? R., & Newman, M
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 2026-08-18T06:34:40.430872+00:00.
Observation 4ae23541-c9df-4b56-bd16-b8fd965b96f1 · outbound
This paper cites ALMAGAL III. Compact source catalog: Fragmentation statistics and physical evolution of the core population.
Why is the Star Formation Rate Proportional to Dense Gas Mass? ALMAGAL III. Compact source catalog: Fragmentation statistics and physical evolution of the core population
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.591308Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ba4145c7-3de7-436c-972d-4f7aee2813f7 · outbound
This paper cites S., et al.
Why is the Star Formation Rate Proportional to Dense Gas Mass? S., et al
Reference 12
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.619658Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation abb4e8d5-f274-43ea-bd67-84eac3b6ba6c · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 13
- Resolution
- unresolved
- raw_fallback, observed 2026-08-15T22:15:54.605563Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 5f4b4748-c0d9-4cd7-998e-8e5cc44a3c6c · outbound
This paper cites 2017, MNRAS, 471, 100.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2017, MNRAS, 471, 100
Reference 14
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6b0627f2-6fc2-4218-9569-c89ed2a6f56d · outbound
This paper cites 2020, ApJ, 894, 103.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2020, ApJ, 894, 103
Reference 15
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.584757Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 094e2154-f1fd-4934-a0e2-901fd49d83e4 · outbound
This paper cites M., Jørgensen, J.
Why is the Star Formation Rate Proportional to Dense Gas Mass? M., Jørgensen, J
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.611864Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6ef5dd0d-af5f-4758-b397-e85e0be5b26d · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 17
- Resolution
- unresolved
- raw_fallback, observed 2026-08-15T22:15:54.563609Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation ba7f2327-9d9e-4f6a-8e96-e334a76fbcea · outbound
This paper cites J., Heiderman, A., & Vutisalchavakul, N.
Why is the Star Formation Rate Proportional to Dense Gas Mass? J., Heiderman, A., & Vutisalchavakul, N
Reference 18
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.550897Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 719a9e48-7d3f-4065-a70c-64869b98f18b · outbound
This paper cites ALMA-IMF XIV: Free-Free Templates Derived from H$41\alpha$ and Ionized Gas Content in Fifteen Massive Protoclusters.
Why is the Star Formation Rate Proportional to Dense Gas Mass? ALMA-IMF XIV: Free-Free Templates Derived from H$41\alpha$ and Ionized Gas Content in Fifteen Massive Protoclusters
Reference 19
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation d1ffb443-f2d2-4d9d-b634-aaa8bf4ef6c1 · outbound
This paper cites & Solomon, P.
Why is the Star Formation Rate Proportional to Dense Gas Mass? & Solomon, P
Reference 20
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.538356Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 2a6bca1f-f209-4875-85f0-7c8c1a5c22b0 · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 21
- Resolution
- unresolved
- raw_fallback, observed 2026-08-15T22:15:54.525389Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 37124a7b-6da3-430c-9a84-887595918f66 · outbound
This paper cites 2022, A&A, 662, A9.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2022, A&A, 662, A9
Reference 22
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.512862Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 431ceb9c-a005-44f4-81d1-65921cfe309e · outbound
This paper cites R., Lique, F., & Santa-Maria, M.
Why is the Star Formation Rate Proportional to Dense Gas Mass? R., Lique, F., & Santa-Maria, M
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.640513Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 703faa04-79da-447b-aebd-02d9e7eb8ec2 · outbound
This paper cites F., Heyer, M., Narayanan, G., et al.
Why is the Star Formation Rate Proportional to Dense Gas Mass? F., Heyer, M., Narayanan, G., et al
Reference 24
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.492586Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation e51f71b3-196a-414c-8472-ab81e56abf4b · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 25
- Resolution
- unresolved
- raw_fallback, observed 2026-08-15T22:15:54.478292Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 7f20426e-a2e9-49a3-9427-6ce563b0d4cf · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 26
- Resolution
- unresolved
- raw_fallback, observed 2026-08-15T22:15:54.465356Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 9c86be78-ba9f-4c06-b9aa-5c8727335444 · outbound
This paper cites E., Huard, T., & Heyer, M.
Why is the Star Formation Rate Proportional to Dense Gas Mass? E., Huard, T., & Heyer, M
Reference 27
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.450333Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation de804313-3818-4d05-b7e3-df357f288b1b · outbound
This paper cites 2022b, Research in Astronomy and Astrophysics, 22, 075016 Jim´ enez-Serra, I., B´ aez-Rubio, A., Rivilla, V.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2022b, Research in Astronomy and Astrophysics, 22, 075016 Jim´ enez-Serra, I., B´ aez-Rubio, A., Rivilla, V
Reference 28
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.436528Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 2b638f8d-06cd-47ad-a651-86bb1a54624b · outbound
This paper cites H., Clark, P.
Why is the Star Formation Rate Proportional to Dense Gas Mass? H., Clark, P
Reference 29
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.421994Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 148b8d6f-e9af-4139-84c0-c95d7faaedc0 · outbound
This paper cites & Tan, J.
Why is the Star Formation Rate Proportional to Dense Gas Mass? & Tan, J
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.669639Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d3d21e5f-7a30-4fae-b8a3-939940839e0b · outbound
This paper cites L., Evans, N.
Why is the Star Formation Rate Proportional to Dense Gas Mass? L., Evans, N
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.673311Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 19c71301-dddb-403c-ade7-ccc17a2d9197 · outbound
This paper cites 2017, A&A, 603, A89.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2017, A&A, 603, A89
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.677051Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d46b63af-f0ec-4c27-9d77-6f00bd7d546c · outbound
This paper cites 1998, ApJ, 498, 541.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 1998, ApJ, 498, 541
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.681250Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0a45019a-1a7e-4423-9770-77a6ed18cf15 · outbound
This paper cites 2006, MNRAS, 365, 590.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2006, MNRAS, 365, 590
Reference 34
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.379504Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 8c682489-c388-4eec-b858-fa7975811afb · outbound
This paper cites 2019, ApJ, 873, 31 K¨ onyves, V., Andr´ e, P., Men’shchikov, A., et al.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2019, ApJ, 873, 31 K¨ onyves, V., Andr´ e, P., Men’shchikov, A., et al
Reference 35
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.365912Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation c6a1bd72-918b-432b-bffe-ee38e33e23ef · outbound
This paper cites 2001, MNRAS, 322, 231.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2001, MNRAS, 322, 231
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.693165Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 29f301b3-cfae-4d89-9456-ce5d7fa0af61 · outbound
This paper cites & Weidner, C.
Why is the Star Formation Rate Proportional to Dense Gas Mass? & Weidner, C
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.696962Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f8b9c8b5-b77e-4c48-a634-9bd2413c7382 · outbound
This paper cites 2013, in Planets, Stars and Stellar Systems.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2013, in Planets, Stars and Stellar Systems
Reference 38
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.337176Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 6aca1048-bf4c-4eb8-91f4-77b98bbf8ad7 · outbound
This paper cites J., Forbrich, J., Lombardi, M., & Alves, J.
Why is the Star Formation Rate Proportional to Dense Gas Mass? J., Forbrich, J., Lombardi, M., & Alves, J
Reference 39
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.324252Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation a2103d8d-0220-443c-b107-20021430be28 · outbound
This paper cites 2019, A&A, 631, A72.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2019, A&A, 631, A72
Reference 40
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.311826Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation b152c39e-716f-4a6b-a600-d9e9536991f1 · outbound
This paper cites B., Li, D., et al.
Why is the Star Formation Rate Proportional to Dense Gas Mass? B., Li, D., et al
Reference 41
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.299389Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation b59865c1-2610-4c4d-9c1c-c9cd104c01ac · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.716237Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ddbf1e83-1c61-4460-8120-d577a1d1ce6c · outbound
This paper cites C., Cheng, Y., & Kong, S.
Why is the Star Formation Rate Proportional to Dense Gas Mass? C., Cheng, Y., & Kong, S
Reference 43
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.278805Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 1a00d9b0-005f-409e-b76e-80dee72686f9 · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.725025Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3fb4b7a5-cd78-4499-b7c0-f4454852508e · outbound
This paper cites 2024, A&A, 690, A33.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2024, A&A, 690, A33
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.729696Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7b3f94f2-1e1e-4c5f-b83b-8f5ae46940a7 · outbound
This paper cites 1989, A&A, 215, L13.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 1989, A&A, 215, L13
Reference 46
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.253016Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 68e7e169-4eea-4d09-a96f-59d35a6f913b · outbound
This paper cites M., Reid, M.
Why is the Star Formation Rate Proportional to Dense Gas Mass? M., Reid, M
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.737911Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3c1fc8a0-9e3f-429c-b600-881204ed875f · outbound
This paper cites 2010, PASP, 122, 314.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2010, PASP, 122, 314
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.741846Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f5583581-64b9-4687-9176-3ee495a242ac · outbound
This paper cites 2016, A&A, 591, A149.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2016, A&A, 591, A149
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.745818Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bb80e814-9f10-45c7-a133-ba388b024fc9 · outbound
This paper cites ALMAGAL I. The ALMA evolutionary study of high-mass protocluster formation in the Galaxy. Presentation of the survey and early results.
Why is the Star Formation Rate Proportional to Dense Gas Mass? ALMAGAL I. The ALMA evolutionary study of high-mass protocluster formation in the Galaxy. Presentation of the survey and early results
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.750091Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 28ff4d4c-2751-40de-9ce8-a72aebbeaad9 · outbound
This paper cites 1998, A&A, 336, 150.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 1998, A&A, 336, 150
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.754465Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b63ca175-84a4-48d1-9f50-ecc025f0937d · outbound
This paper cites 2022, A&A, 662, A8.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2022, A&A, 662, A8
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.758584Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3d7b2805-c54b-4fcf-aa09-282790c92081 · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 53
- Resolution
- unresolved
- raw_fallback, observed 2026-08-15T22:15:54.206123Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 0ba8aaa6-f4a6-4500-ac56-f8e34723eae4 · outbound
This paper cites & Henning, T.
Why is the Star Formation Rate Proportional to Dense Gas Mass? & Henning, T
Reference 54
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.194121Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation f1316b98-fc1d-4c73-8ef7-d9673ea6af34 · outbound
This paper cites V., Orkisz, J.
Why is the Star Formation Rate Proportional to Dense Gas Mass? V., Orkisz, J
Reference 55
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.181928Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation d959d36f-2613-4855-9f9b-4026772b2a45 · outbound
This paper cites 2010, in Astronomy and Astrophysics, Vol.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2010, in Astronomy and Astrophysics, Vol
Reference 56
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.169942Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 3e09d0ce-1660-442b-87b0-431e610f821b · outbound
This paper cites K., Ginsburg, A., et al.
Why is the Star Formation Rate Proportional to Dense Gas Mass? K., Ginsburg, A., et al
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.779446Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bb6965d1-faaf-4cd5-ad12-07c22d8a80cc · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.783509Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed2dbcf6-09b4-49a0-b0a6-a268aa3ca308 · outbound
This paper cites M., Zhang, Q., et al.
Why is the Star Formation Rate Proportional to Dense Gas Mass? M., Zhang, Q., et al
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.787431Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c51381f6-408f-438a-89cd-01ca9890fe92 · outbound
This paper cites G., Goicoechea, J.
Why is the Star Formation Rate Proportional to Dense Gas Mass? G., Goicoechea, J
Reference 60
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.136762Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 113ada7d-31c6-42d5-88dc-308686de20df · outbound
This paper cites Molecular Gas and the Star Formation Process on Cloud Scales in Nearby Galaxies.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Molecular Gas and the Star Formation Process on Cloud Scales in Nearby Galaxies
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.796421Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 52b1cf01-9abe-494d-a13c-2d4951c0d37d · outbound
This paper cites 2015, MNRAS, 453, L41.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2015, MNRAS, 453, L41
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.801003Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e0cb42d8-7d48-4c43-99d4-bbbc5d4c8c29 · outbound
This paper cites 2015, A&A, 582, A93 Su´ arez, G., Galv´ an-Madrid, R., Aguilar, L., et al.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2015, A&A, 582, A93 Su´ arez, G., Galv´ an-Madrid, R., Aguilar, L., et al
Reference 63
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.116619Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 3e82eb3b-df39-4c51-9d63-73db1eb819bd · outbound
This paper cites J., & Andre, P.
Why is the Star Formation Rate Proportional to Dense Gas Mass? J., & Andre, P
Reference 64
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.104629Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 0bc0ebdd-04dc-4e5b-8c4e-e7e04e0b71db · outbound
This paper cites Power-law distributions in binned empirical data.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Power-law distributions in binned empirical data
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.812969Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8e40d5fd-3681-45bd-ac73-eef923867cdd · outbound
This paper cites & Kroupa, P.
Why is the Star Formation Rate Proportional to Dense Gas Mass? & Kroupa, P
Reference 66
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.092490Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 79807540-d995-4bb4-9432-64f1124087cd · outbound
This paper cites 2013, MNRAS, 434, 84.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2013, MNRAS, 434, 84
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.821375Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 85bc4dca-aaa7-449c-b8cb-e0273cbdad20 · outbound
This paper cites P., Blitz, L., & McKee, C.
Why is the Star Formation Rate Proportional to Dense Gas Mass? P., Blitz, L., & McKee, C
Reference 68
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.073423Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 84bb54f0-6c4e-4104-97d7-e51a4cda5f5f · outbound
This paper cites an unresolved cited work.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Unresolved cited work
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:15:53.830566Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d659d802-d6c2-4d75-bd1a-adb41ad769c6 · outbound
This paper cites 2005, ApJL, 635, L173.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2005, ApJL, 635, L173
Reference 70
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.052683Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation f0f0a368-f678-44c7-a5a0-8a04ea3dfae6 · outbound
This paper cites L., & Knez, C.
Why is the Star Formation Rate Proportional to Dense Gas Mass? L., & Knez, C
Reference 71
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.039424Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 486666fd-48bc-4439-b152-af7c388afaa4 · outbound
This paper cites 2023, MNRAS, 520, 3259.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2023, MNRAS, 520, 3259
Reference 72
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.026066Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 51627780-c3ab-4d74-8682-27b9e373ba30 · outbound
This paper cites 2017, A&A, 607, A126.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2017, A&A, 607, A126
Reference 73
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:54.013182Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 72dd73d9-648c-41b7-9a25-a7072fbef7a9 · outbound
This paper cites 2023, A&A, 670, A151.
Why is the Star Formation Rate Proportional to Dense Gas Mass? 2023, A&A, 670, A151
Reference 74
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:53.999674Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 69162a29-5ce4-43ff-bb30-0d58adb9d3f4 · outbound
This paper cites Y., Wang, J.
Why is the Star Formation Rate Proportional to Dense Gas Mass? Y., Wang, J
Reference 75
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-15T22:15:53.985991Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Pith citing papers
No inbound Pith citation observations are available.