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Paper Citation Record · LEDGER

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency

As of 23 August 2026, this Paper Citation Record lists 100 of 104 outbound references and 1 inbound Pith citation observation for arXiv:2501.14031.

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

pith.paper-citation-record.v1
2501.14031 v1

Coverage vector

measured 100 of 104 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T15:33:40.659406Z

measured 101 of 101 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-13T04:41:12.165957Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-13T04:49:20.251165Z

Reference resolution

100 of 104 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 4a9c8fdc-f875-451f-8193-3a6b771cc175 · outbound

This paper cites write newline.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency write newline

Reference 1

Resolution
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation c666613b-7c73-4f18-9d7c-927ccf8ea0e6 · outbound

This paper cites write newline.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency write newline

Reference 2

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 5e98539d-fad1-4069-aab8-b5cd6603f4f6 · outbound

This paper cites N., et al., 2009, @doi [ ] 10.1088/0067-0049/182/2/543 , https://ui.adsabs.harvard.edu/abs/2009ApJS..182..543A 182, 543.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency N., et al., 2009, @doi [ ] 10.1088/0067-0049/182/2/543 , https://ui.adsabs.harvard.edu/abs/2009ApJS..182..543A 182, 543

Reference 3

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Observation 1a7f866b-217c-44b3-a064-aae2f432bbea · outbound

This paper cites K., et al., 2015, @doi [ ] 10.1051/0004-6361/201425397 , https://ui.adsabs.harvard.edu/abs/2015A&A...579A..45B 579, A45.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency K., et al., 2015, @doi [ ] 10.1051/0004-6361/201425397 , https://ui.adsabs.harvard.edu/abs/2015A&A...579A..45B 579, A45

Reference 5

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Observation d8c4401f-39cb-43f7-a56d-bcd0dd594ad7 · outbound

This paper cites J., Geller M.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency J., Geller M

Reference 6

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 72100cdc-9804-493b-b7c1-5c2f057a3f58 · outbound

This paper cites J., Arnold J.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency J., Arnold J

Reference 7

Resolution
verified exact
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Source-reported events for the cited work

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Observation a17d755f-8b2d-4c04-8c6a-f65b005719bc · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 8

Resolution
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Observation 2ffc0d0a-e5ab-4969-a885-e54327d8f818 · outbound

This paper cites W., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency W., Ellison S

Reference 9

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 704211aa-2220-4043-9956-17de28272906 · outbound

This paper cites W., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency W., Ellison S

Reference 10

Resolution
unresolved
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Source-reported events for the cited work

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Observation eacde06f-b502-49c6-ba8f-eee954574b9c · outbound

This paper cites W., et al., 2024, @doi [ ] 10.1093/mnras/stae1951 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.533.3068B 533, 3068.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency W., et al., 2024, @doi [ ] 10.1093/mnras/stae1951 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.533.3068B 533, 3068

Reference 11

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Observation b6f341c2-c668-434c-87a9-22be5fe768ce · outbound

This paper cites A., Barnes J.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency A., Barnes J

Reference 12

Resolution
unresolved
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Source-reported events for the cited work

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Observation 70df6480-b2c3-44cd-999e-2894f85bc457 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 13

Resolution
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Source-reported events for the cited work

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Observation 227857a4-e0d8-427f-add3-5558fcf89586 · outbound

This paper cites R., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency R., Ellison S

Reference 14

Resolution
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Source-reported events for the cited work

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Observation c5b1decc-0e77-4cf0-a3bc-cc9e503cc93a · outbound

This paper cites L., Patton D.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Patton D

Reference 15

Resolution
unresolved
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Observation 3b2865dc-2039-4b07-a911-b021eab0907f · outbound

This paper cites H., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency H., Ellison S

Reference 16

Resolution
unresolved
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Observation a3093248-5fca-494a-89d9-f898a71190a5 · outbound

This paper cites R., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency R., Ellison S

Reference 17

Resolution
unresolved
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Observation dea53888-8b83-4d6c-a1d4-14355f52760e · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 18

Resolution
unresolved
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Source-reported events for the cited work

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Observation db00f0b0-a14b-420d-a009-3696286ac25a · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 19

Resolution
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Observation f835d38d-c536-451f-9321-d05dec3851c4 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 20

Resolution
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Source-reported events for the cited work

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Observation 47a4fd52-8223-48d4-b727-7a2baa11e9b0 · outbound

This paper cites J., Jonsson P., Primack J.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency J., Jonsson P., Primack J

Reference 21

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7f8b8163-6365-46e1-8d22-e78dc964c971 · outbound

This paper cites J., Jonsson P., Somerville R.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency J., Jonsson P., Somerville R

Reference 22

Resolution
unresolved
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Observation 90c5556d-e77c-4a45-8fe3-df006f60a83d · outbound

This paper cites H., Appleby S., 2019, @doi [ ] 10.1093/mnras/stz937 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2827D 486, 2827.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency H., Appleby S., 2019, @doi [ ] 10.1093/mnras/stz937 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2827D 486, 2827

Reference 23

Resolution
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Source-reported events for the cited work

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Observation e67af40d-e695-47e9-bae5-c706b68b20fb · outbound

This paper cites J., Liske J., Driver S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency J., Liske J., Driver S

Reference 24

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b7955cdb-212e-47cc-a7e2-380f63f48956 · outbound

This paper cites L., Semelin B., 2007, @doi [ ] 10.1051/0004-6361:20066959 , https://ui.adsabs.harvard.edu/abs/2007A&A...468...61D 468, 61.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Semelin B., 2007, @doi [ ] 10.1051/0004-6361:20066959 , https://ui.adsabs.harvard.edu/abs/2007A&A...468...61D 468, 61

Reference 25

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Observation 2d8c1382-2248-44f2-853b-25ee92e0c92b · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 26

Resolution
unresolved
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Source-reported events for the cited work

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Observation 806f6616-da67-4d1a-80e1-3966de6be2be · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 27

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 0375c6fe-7e1a-4a0c-b0eb-a94a75215ef5 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.439063Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 47a9c2f2-820b-4d14-b972-67517722a7c4 · outbound

This paper cites L., Patton D.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Patton D

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.441697Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 1bbc5fb8-3e96-4bca-b2c2-ae2be2dc3a00 · outbound

This paper cites L., Patton D.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Patton D

Reference 30

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 166cd629-6987-43c4-9853-dcfdfa89e176 · outbound

This paper cites L., Patton D.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Patton D

Reference 31

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 71e56e67-36e8-4d72-b956-ad633dae3090 · outbound

This paper cites L., Mendel J.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Mendel J

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.449141Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation e3509204-dfa3-4c83-935e-67b3a48c1101 · outbound

This paper cites L., Catinella B., Cortese L., 2018, @doi [ ] 10.1093/mnras/sty1247 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.478.3447E 478, 3447.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Catinella B., Cortese L., 2018, @doi [ ] 10.1093/mnras/sty1247 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.478.3447E 478, 3447

Reference 33

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation ea23a647-73c3-4a64-bfbc-f04d4cc99165 · outbound

This paper cites L., Viswanathan A., Patton D.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Viswanathan A., Patton D

Reference 34

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b2d724b2-15b5-4100-8f11-499d0e6803af · outbound

This paper cites L., Thorp M.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Thorp M

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.458056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation d56232bf-7d98-4693-97d4-58d142842ed5 · outbound

This paper cites L., et al., 2020b, @doi [ ] 10.1093/mnrasl/slz179 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.493L..39E 493, L39.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., et al., 2020b, @doi [ ] 10.1093/mnrasl/slz179 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.493L..39E 493, L39

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.461149Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.461149Z digest=sha256:7a67fd66aa73c377b535f48809654c5ca9b9eb6c0746449a75b24366c828c5b3

Observation 36924826-2709-4b6c-8717-067e845533f8 · outbound

This paper cites L., et al., 2022, @doi [ ] 10.1093/mnrasl/slac109 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.517L..92E 517, L92.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., et al., 2022, @doi [ ] 10.1093/mnrasl/slac109 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.517L..92E 517, L92

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.463884Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.463884Z digest=sha256:73b2971a3921705253cdd59f3e4796ec7b52125fb600c6a23e39bf7fb2ac6be3

Observation 525338ec-74b0-4cd3-bcfc-fb19ad96fb17 · outbound

This paper cites Galaxy evolution in the post-merger regime. II -- Post-merger quenching peaks within 500 Myr of coalescence.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Galaxy evolution in the post-merger regime. II -- Post-merger quenching peaks within 500 Myr of coalescence

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.466525Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.466525Z digest=sha256:d6c8afd9a5ac524c90032b8c6078476275a8708ad9c4d74db245dec38ca0032a

Observation 2ff8a452-92ba-4d13-bf7f-2662ce28bdd9 · outbound

This paper cites E., Lara-L \'o pez M.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency E., Lara-L \'o pez M

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.469699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.469699Z digest=sha256:1ed78f37f90986fda01ec06f4144b8fbc0daad40fdeb10d3497b7d244b1e20fd

Observation 49dae055-a64f-4cdf-9c49-b18718fde237 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.472166Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.472166Z digest=sha256:15b73d48393dc624b7a5b6904d575db36ac29ce4147ea5ffa070878ecca6fbd7

Observation 57252f78-1608-494f-8cf6-b2115e58eb41 · outbound

This paper cites H., Gosain H., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency H., Gosain H., Ellison S

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.475230Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.475230Z digest=sha256:43b24f0c1e9b0f76190a1a6b6880547c8e96dbe8e316ec92db6bea2d7a59d80e

Observation 16ddeeb2-cdd1-48c7-90e6-5a380aba5d43 · outbound

This paper cites M., Avila-Reese V., Conselice C.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency M., Avila-Reese V., Conselice C

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.478229Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.478229Z digest=sha256:aa4592d5921131c87d414094c96fcecdfd180425f5f0a479acfdf71211931351

Observation 18316d1c-e272-408b-9733-d021c4c40d78 · outbound

This paper cites T., Kudritzki R.-P., Kewley L.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency T., Kudritzki R.-P., Kewley L

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.481028Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.481028Z digest=sha256:5dfe8d0c882268f714545258029e969a3e3a8935bcca36933a2c68795a1dcdd9

Observation a4a8f3f9-0b59-4c6b-a207-3bca0e9a1f51 · outbound

This paper cites F., Hernquist L., Cox T.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency F., Hernquist L., Cox T

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.484445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.484445Z digest=sha256:54507a8a351deb0fdc6f51c31c1bf44437f31d0d74e400ad1b0cf9f8471295a5

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.487867Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.487867Z digest=sha256:952ab5f04d1bbf5934327ff5e93f9bf69f6bb924e715fe600ea348647f36f2a8

Observation ba63efc4-0ef3-4db2-9dfb-29f44418959b · outbound

This paper cites S., Mihos J.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency S., Mihos J

Reference 46

Resolution
verified exact
doi, observed 2026-08-10T15:33:41.006806Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.490888Z digest=sha256:b126be2d89e47a5e1b7255c9c1ebb6123bf96b8751ab948e5555a87e9b63bafb

Observation f73df768-31a5-4df2-bcd2-8121ce364ddc · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 47

Resolution
verified exact
doi, observed 2026-08-10T15:33:40.998273Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.493819Z digest=sha256:9c09b97bf61a99af2c0c0f898ca6845e7054f6b87125514696d5eee289f9d129

Observation 59cc7952-fd68-4f18-8163-a211d14e2403 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 48

Resolution
verified exact
doi, observed 2026-08-10T15:33:40.990435Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.496653Z digest=sha256:731183cc881dccda73ff50db9818b4286898901d604a32a67496e53ec7489e80

Observation 9ee23b0d-44e7-462b-b4e9-b47f3c394aeb · outbound

This paper cites J., 1998, @doi [ ] 10.1086/305588 , https://ui.adsabs.harvard.edu/abs/1998ApJ...498..541K 498, 541.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency J., 1998, @doi [ ] 10.1086/305588 , https://ui.adsabs.harvard.edu/abs/1998ApJ...498..541K 498, 541

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.499568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.499568Z digest=sha256:5697b6ee264c84518f4330135dac1aafb772361c907c893cea9bb440e7b8be5c

Observation 9998ff4e-7169-4f16-b3d7-1ff005eba7c7 · outbound

This paper cites J., Rupke D., Zahid H.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency J., Rupke D., Zahid H

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.502774Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.502774Z digest=sha256:bc0887e1e0ca49c7fb8c5404cdd256ab2611fd69e5c3e2eb85cb4a1e4d6037e8

Observation eff61d06-e040-49b3-a0ee-55393d84b6a1 · outbound

This paper cites G., Alonso S., Mesa V., O'Mill A.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency G., Alonso S., Mesa V., O'Mill A

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.507889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.507889Z digest=sha256:8e01ba6ecca9d14d94064dc59f4be36e8fdcd6a6ead6b8244c6013ff0c002f82

Observation c1ebd4b1-f80d-4e36-b0cf-f1fda0edf301 · outbound

This paper cites L., et al., 2016, @doi [ ] 10.3847/0004-637X/825/2/128 , https://ui.adsabs.harvard.edu/abs/2016ApJ...825..128L 825, 128.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., et al., 2016, @doi [ ] 10.3847/0004-637X/825/2/128 , https://ui.adsabs.harvard.edu/abs/2016ApJ...825..128L 825, 128

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.511199Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.511199Z digest=sha256:cc1402abbc7f09f7008266875ba98dc0d7eb68d1d15dc60de4471a81850b1107

Observation da680909-6091-41a4-b151-49bf852d6c4c · outbound

This paper cites K., Walter F., Brinks E., Bigiel F., de Blok W.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency K., Walter F., Brinks E., Bigiel F., de Blok W

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.514792Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.514792Z digest=sha256:05b39f5298b943d3420f3e4458d0fbb0440e5889831650285d036fb7d92d0fe2

Observation c9bbe94d-4977-4b06-b50f-c506a273d156 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.520530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.520530Z digest=sha256:0a954cf3ca72898122feb0dda1f58fe8175c2f1096e7a8bc561aa0662d7c9b82

Observation b9ddc412-a4e6-4c6d-9b9b-088a17617e20 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.522874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.522874Z digest=sha256:8be42e8806badf4b18f3e150819ce26479ba034cc537e460e4e191ac6cdd7e54

Observation 8382032e-de7e-4d5e-9999-2e5ce158005e · outbound

This paper cites M., Jonsson P., Cox T.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency M., Jonsson P., Cox T

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.525627Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.525627Z digest=sha256:6ed1c414a1a939e136901a6320b448d2f2181dea424968c25fa02cfe91b26400

Observation 744d096f-12a2-4640-8afe-445bddca57c4 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.528530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.528530Z digest=sha256:4cc0b079ae9a3d72e0f3b586b873d65f718d635e34c440f83ae53501d594a307

Observation dad35701-6720-4ad2-a1a1-2a35fbabc18f · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 60

Resolution
verified exact
doi, observed 2026-08-10T15:33:40.942021Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.531060Z digest=sha256:0c6d64d0e3f65c48964c7a4e086dea9833c5a4e2cc18a25d5744c15869817d8b

Observation 79f9965d-52f6-4a0d-80bb-180c2b694646 · outbound

This paper cites C., Hernquist L., 1996, @doi [ ] 10.1086/177353 , https://ui.adsabs.harvard.edu/abs/1996ApJ...464..641M 464, 641.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency C., Hernquist L., 1996, @doi [ ] 10.1086/177353 , https://ui.adsabs.harvard.edu/abs/1996ApJ...464..641M 464, 641

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.533722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.533722Z digest=sha256:d5e24c8c3a050be6719e22723d7d5f3e05615da29ee283da0213d9cd058872dd

Observation 0d408604-9948-48ac-8433-ffa258f82549 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 62

Resolution
verified exact
doi, observed 2026-08-10T15:33:40.927826Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.536579Z digest=sha256:3c779a874c262c6528494dc012f91abbd5b4f7af7e9776b1d448a826ca49fb8e

Observation 5b45ed88-8cbe-4e5b-bc53-1eb71c1a8138 · outbound

This paper cites L., Patton D.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Patton D

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.539085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.539085Z digest=sha256:67c40ac8456344e97de3d04e4fa7cde19c84b0c43bb80099cde0de892350f9d3

Observation 528f34bd-2577-492c-b318-3afa8cd84436 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.541520Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.541520Z digest=sha256:114ff1db91f542822bdd36b59cafd522f080b6e52de5e0785a2418b3b81a16f2

Observation 63a53e7e-0e5b-424f-a2e8-3db1d3a700dc · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.544180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.544180Z digest=sha256:16230d136766f41e2885e000e1cfb37fd3dd85f230be17990e5e92605f37e492

Observation f1ffb513-dc86-4bd2-9c2e-a87527959840 · outbound

This paper cites P., et al., 2018, @doi [ ] 10.1093/mnras/sty618 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.1206N 477, 1206.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency P., et al., 2018, @doi [ ] 10.1093/mnras/sty618 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.1206N 477, 1206

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.547954Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.547954Z digest=sha256:0db0fdf78542106d5e61bd5db50cc2e8b9110bf8690aed8d9c39e8716b50e9c5

Observation 9120402c-cee5-4ee1-9263-befb36f45647 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.551535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.551535Z digest=sha256:1691b2c9a7bd9719ca69837564aa19a9918363ba8eeb9e4553e8595d1d85dfa2

Observation 1efb598d-474c-4575-af7b-4227a9de230b · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.554983Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.554983Z digest=sha256:48830b0dcef44188a72a4a40a2ef12e5ebc8793900a9e38fa061d7c89f363164

Observation d82fea3e-08b4-4ebc-8f7b-f5b3e90ced9a · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.557635Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.557635Z digest=sha256:49f0165c3fd853c940253d223e6fb5b0c94f86000a733678d3a67982d05e99d1

Observation b951d9aa-93a8-44d6-bfc1-b8274c4b7096 · outbound

This paper cites Richard I., Choi Y.-Y., 2008, @doi [ ] 10.1086/524192 , https://ui.adsabs.harvard.edu/abs/2008ApJ...674..784P 674, 784.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Richard I., Choi Y.-Y., 2008, @doi [ ] 10.1086/524192 , https://ui.adsabs.harvard.edu/abs/2008ApJ...674..784P 674, 784

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.560486Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.560486Z digest=sha256:5e4cd958db1a0498729bf59c8445812d9c36bff3b51a1e80b5546bb74d1021f4

Observation 71c2ebb1-d9e5-4249-a484-b34c55d733b6 · outbound

This paper cites R., et al., 2002, @doi [ ] 10.1086/324543 , https://ui.adsabs.harvard.edu/abs/2002ApJ...565..208P 565, 208.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency R., et al., 2002, @doi [ ] 10.1086/324543 , https://ui.adsabs.harvard.edu/abs/2002ApJ...565..208P 565, 208

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.563140Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.563140Z digest=sha256:31c8d97728f27404be907d9f3822ff7acd07550e9a8326362325a6d4c45e0086

Observation 86e530b3-d052-415e-b69b-731f1eb6954a · outbound

This paper cites R., Grant J.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency R., Grant J

Reference 72

Resolution
verified exact
doi, observed 2026-08-10T15:33:40.873788Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.566061Z digest=sha256:523406e800f83045b33d829a7613cae2fd3707c76c4abb4b4d42d3493a2d9a2d

Observation ce71c9c6-2091-4495-9eec-f32b99e2a02b · outbound

This paper cites R., Torrey P., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency R., Torrey P., Ellison S

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.569096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.569096Z digest=sha256:c37192f2cfa0bf25d45cb0bf883bd3a3bc9fc2949bdc5ae393f96ef81fd59240

Observation 4309a072-7b96-4836-8f26-2e38fa5ce514 · outbound

This paper cites R., Qamar F.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency R., Qamar F

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.572198Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.572198Z digest=sha256:3cfe5854d7fd48491532ea80e8f597932f44d0aca585c7349380f7f0fb672493

Observation d8363cad-4c4d-423c-8078-3c4dd64a86c3 · outbound

This paper cites R., et al., 2020, @doi [ ] 10.1093/mnras/staa913 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.4969P 494, 4969.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency R., et al., 2020, @doi [ ] 10.1093/mnras/staa913 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.4969P 494, 4969

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.575178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.575178Z digest=sha256:5a4d032d43144ef740fae1e157b7693def2a1ad42993c779d3109028f517ce39

Observation 19b3b2f3-1f89-436c-82bd-e7e7c01c88e8 · outbound

This paper cites R., Faria L., Hani M.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency R., Faria L., Hani M

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.578244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.578244Z digest=sha256:757eb0a650a0edd2f6b8c6b8d153d01dbb5320ebe1a3486a903da2c45d4c43d5

Observation 403c75f8-8550-4f20-91a4-8d70aad04de0 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.581822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.581822Z digest=sha256:63320943ffb6ab3ffff35eb25c7d198b6cb7a3813bf793634f594a7c4ef11ce5

Observation 078347ee-6df6-4b86-a5e1-dfc711c8fa9a · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.585232Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.585232Z digest=sha256:a335d4742232a4306c80d475e90b566507329b67a87535ac75f04b1518555bd6

Observation 8eaed80f-c9cb-4cab-ab71-1e39c9e5e10c · outbound

This paper cites H., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency H., Ellison S

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.588282Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.588282Z digest=sha256:837f035670db323c7eda4fad06c6a1881f3c137904f63b4c8be0aaaaedfa5dae

Observation b7621c28-aa6e-44b3-8d10-ba85a81b30ec · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.591245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.591245Z digest=sha256:fe800868919e6dc18622232cdfb02255bd97fbc8f6261cecb0c00542e8127cba

Observation 4131a367-cdce-490f-a4d0-0be71511e0db · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.594381Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.594381Z digest=sha256:cbf5f144edb5500fceaa483de42a70bca5a1d61397268697e69f7e56dad8b1e9

Observation 3b35f636-024b-4273-91a9-8bb5b1fd738a · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.597238Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.597238Z digest=sha256:a4543455b263289130cd0d2ff2e2246210eed3eb6f89433a4a95d33262498ae2

Observation d348399f-c559-4987-bf74-08d5a5401b4c · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.600839Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.600839Z digest=sha256:c33ddb990762c38b4fbf5304959fde34b2027888afc5b1575c2cabbc0bbc01f7

Observation 0172510b-159d-4d63-9d74-37b60ae0bf33 · outbound

This paper cites The molecular gas content throughout the low-z merger sequence.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency The molecular gas content throughout the low-z merger sequence

Reference 84

Resolution
verified exact
local_arxiv, observed 2026-08-10T15:33:40.810090Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.603379Z digest=sha256:5f4f04e73ba303d776354a7b95da6488c9502d53ef5188717bc26dc32cc56bc5

Observation 01c1091a-2e10-40f9-a20e-78441fb41c6f · outbound

This paper cites L., McAlpine W., Hickox R.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., McAlpine W., Hickox R

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.605976Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.605976Z digest=sha256:eb59b92b0e2d2c5ef2a21ad7851aaeaa830d67b093692087972d1ca2aeb3e148

Observation 246bf0fd-952c-46df-8e19-e95208f68e95 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.608635Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.608635Z digest=sha256:e7c4d4f74f1c7448bd36a5da974dc6d955fbcd7ac7056ba30c6a011f7c6fa1f3

Observation 2845fcfa-5dd8-4038-ba8f-4157c9da8edf · outbound

This paper cites M., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency M., Ellison S

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.614918Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.614918Z digest=sha256:8fc0c98c2a1087a15edc4a353b709e4c1586206e5ec2bee304e6b25c2041606f

Observation e672277b-a962-4e4c-9f17-5b768bd0561a · outbound

This paper cites M., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency M., Ellison S

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.618551Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.618551Z digest=sha256:5c80d99f82a77536be13e6fa26b49fbab33e3ca9fb64798780354fed0726430f

Observation 7b6b9a81-c93d-4eeb-8739-2bb82ddd002a · outbound

This paper cites D., et al., 2018, @doi [ ] 10.3847/1538-4357/aae25e , https://ui.adsabs.harvard.edu/abs/2018ApJ...867...92S 867, 92.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency D., et al., 2018, @doi [ ] 10.3847/1538-4357/aae25e , https://ui.adsabs.harvard.edu/abs/2018ApJ...867...92S 867, 92

Reference 90

Resolution
verified exact
doi, observed 2026-08-10T15:33:40.783113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.621529Z digest=sha256:da6a6a9fdb2166f902d026257b9d67c8165a7c6850fc4d3ba5bc32d86c12f11b

Observation 9c81cc8b-e7d6-4e14-b473-0da8692cb5e4 · outbound

This paper cites H., Richter P., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency H., Richter P., Ellison S

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.624821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.624821Z digest=sha256:707bab66408970c12d065e61e240c723b0a11cd693306e7b41db6a90e07be158

Observation d9019573-b0cc-4994-a536-00cd2184d133 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.627609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.627609Z digest=sha256:7df81d12d796b8eb30d205c20b9b68ef08b5856f68e8107040f09bedf6ef4e51

Observation 6d363a8c-949f-4957-b0ac-65e77e13feb2 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.630659Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.630659Z digest=sha256:c3862d89036ff33f23e99e9f57a3d4d61bffa16cf48aa2cc78d842b05e7a4aa2

Observation 407465cc-f4c2-4e2e-b5c4-d6b5f5178bf0 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.633343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.633343Z digest=sha256:c0482312ecd07b41b436648d103ab7f2e85e5ab8795ee1a31ebeaa2ce392faf9

Observation 543e000f-c425-4d37-b854-33c75588f2bc · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.635727Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.635727Z digest=sha256:a0b8b473079331f417dfaf153bdd3b8301ebeb128fa240a14251acfd5477444a

Observation f928124f-4d1b-4904-be61-1b4af4d3b213 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.637996Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.637996Z digest=sha256:9809b79978b5fb2cd6ed65245b86c59a9571e914362a8b7f31796b17417a4c2d

Observation d679ebf0-0673-49ce-bee1-9be51b669899 · outbound

This paper cites D., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency D., Ellison S

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.640209Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.640209Z digest=sha256:c5b22a46d5c7c4fd50e2fed838ccde837b4809c8a9a017963d2de1ec6e1fa436

Observation 6085ca4f-fb47-499e-8121-92e90cf9d9e6 · outbound

This paper cites D., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency D., Ellison S

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.642911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.642911Z digest=sha256:580c13b5181dcef3fa265f759be0d827f102608db231ed00717369e0f384d24c

Observation b33d16b6-18e3-4921-a222-575ac45fd091 · outbound

This paper cites D., Ellison S.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency D., Ellison S

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.645992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.645992Z digest=sha256:56448b417f9b11a5b5408ba823b7d2acc9e7360a3794232222abad0ea5147857

Observation 8c19fddb-03a5-4ff2-834e-a259b5c23865 · outbound

This paper cites J., Kewley L., Hernquist L., 2012, @doi [ ] 10.1088/0004-637X/746/1/108 , https://ui.adsabs.harvard.edu/abs/2012ApJ...746..108T 746, 108.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency J., Kewley L., Hernquist L., 2012, @doi [ ] 10.1088/0004-637X/746/1/108 , https://ui.adsabs.harvard.edu/abs/2012ApJ...746..108T 746, 108

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.648866Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.648866Z digest=sha256:bcacaaef8367fe3fad9567bee0ffe77da782c17768c4278c98f5ed8f27402c9e

Observation ee1cbf87-ce65-49ae-aa22-9a3fd7bfee71 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.652303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.652303Z digest=sha256:929d801307a6648686452ff6d5388b4680e76173ea15e5ab23ecbccb946bfd61

Observation c73367a9-9dcb-4395-9d25-15cb32f41d33 · outbound

This paper cites an unresolved cited work.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.654651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.654651Z digest=sha256:3726097e9dd5d293c5ef8a62d6d6678019187a1a08199a0cea4bb19fe81faa68

Observation 81f3b04f-a76a-47e0-8055-2cc838c52975 · outbound

This paper cites W., 2022, @doi [ ] 10.3847/1538-4357/ac4fbc , https://ui.adsabs.harvard.edu/abs/2022ApJ...926..203V 926, 203.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency W., 2022, @doi [ ] 10.3847/1538-4357/ac4fbc , https://ui.adsabs.harvard.edu/abs/2022ApJ...926..203V 926, 203

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.656966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.656966Z digest=sha256:8b261b0a49c64ba6df887d6db78e5101ad0a2bad179ad7670686a04ee0fc042c

Observation c3eb9b92-99bc-4bef-ad40-3eab6124231d · outbound

This paper cites L., Sargent M., Coppin K.

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency L., Sargent M., Coppin K

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-10T15:33:40.659406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:33:40.659406Z digest=sha256:7117b9e7189e708fc37aee39b4b014da4a9767c831adb516994070d5e5015a05

Pith citing papers

Observation 669bfcf8-c618-40dc-8b17-227e9bdd93a3 · inbound

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods cites this paper.

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency

Reference 103

Resolution
verified exact
local_arxiv, observed 2026-07-13T04:49:20.253164Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-13T04:41:12.165957Z digest=sha256:23f3a5a400519849a34940c6efaa2cc1142f42f27f113ec920565d94d45f6c5d