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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 11 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 2026-08-11T06:34:44.6726+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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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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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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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
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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

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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
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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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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
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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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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
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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
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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

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

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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

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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

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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

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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

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

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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
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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
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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
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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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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

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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
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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
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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:ca645a65e11fad5f6bf176af62216aef9cda6ba9e12bf19792c9e2e42e4afea4

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:bcb41025cab303a2f79d05515b8b2b6450183406618eb8fe63c75d3dc9c4ce36

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=sha256:81032d59cc80e031d439f1948e77e4ab4067c97b4bca330432cbe78528036a90

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:e2f3c37473c5048907ace677c61a478634f95366f03c5f6d1b37dbd37ecc843a

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=sha256:68455507a35cd5eebce8cd58422130516b22ccad33639e687fe554058445eb1d

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:b9055c954cd4a59d6b9bf56fd838dcb435168ec1c5280fd397760c292f6e0325

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:fd04c7ac43f21d355fb4bd99ba0f49f8b22129058bbc98e91ddeb01f6951ce4d

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=sha256:29be2c2123f8e6ba5ca188121246467f74e808ec8d2c0fcf2f1b29283ded2388

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:e9e036e64199dded27b8130b5df6a8eda2aba038fcb02dc00319d5a682d8c1da

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=sha256:5674309bda24e5aad51669d75a46fb2845b72ee69a3fe45461a795d65d03acb9

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 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.490888Z digest=sha256:e5dc987c64774974bfd4e91af8d4dc5ee8b144212cc015baf0dbbf834ccb70b4

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 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.493819Z digest=sha256:94798d378efcd9e847ec4e75bbb015631e0a5df022030465e026bd0fe5e5b409

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 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.496653Z digest=sha256:e3569e4895732abe6125df9144750ada94bd1270566a5553fe43bcd4deee3364

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:e8c8eac0dcc9a31e24be5ab05bfadf1721ce73d9741e2b0e254645746c1df15a

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=sha256:7816ef26bec57f81214c4a3a07137d002034f3b16d40769d2f945caad9a6f328

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=sha256:5855a4e335c90e963dd0b37c98f108cb34e63d2d92361a42279763395c7edfc2

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=sha256:125b325bdd04c61c4b98c8da70b80db298d4dc23ccfdd2bf53b3a7aa58c1ffaa

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:ac1dc106b0172db88d1a0ad3fcf2886d65939e40cfacebc2d2c8a830b4615bfb

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:e81981081c5591f75de552e1bd5abc4e8b884499701868eceeb324b2bdef8f93

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=sha256:688f7519f4c49b32e4cbbb68be894efc6f6704945535be719d18df03de7cd44e

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:b0cc817d08fe99f729f2d1b934e742a690e38311b604ce770babbb28cf71af5c

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:cd9e5d69cb1906cdec9ea99460185e7d601a9481a2f53e3fd59d8039ae3f8123

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 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.531060Z digest=sha256:94fad323918b6759e9beb6ac2ac01663f49b342c32f6cf6341a844cb138f780b

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:fe0d674aad3565d9afb0e4d200939248ea9af1fb4fd5ea4e1da1be9704d03e74

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 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.536579Z digest=sha256:c3a1cefe997b8fe710832ecfdd528eb4633f0e9ac76b874658944e1d17149ebe

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=sha256:43cd4b73d673ab6a012070d167b6bca0ba61fb3fc19ff3b411b5f6a4cc8265c7

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=sha256:806e05957afd76ac4f5ebd5e58e23b2b4d5d71c2270473d8e5137fcee962637b

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=sha256:3f80e2adba87978b8a0ff97b295d4cd8cc14cf625c4dc2a9c40faa7304c27a21

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:f19cf3940127f871ce89c0788d5298a97cb80928b9a9ff4d52054af4ab4f805c

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:dc08417c2869c97dd40b2768621b6b6261031a37968a41479d7fc9d0762948ef

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=sha256:3ccaf652af08ead0d2ab2d58fe9a51767e395dd2281c04d8bf3d33885d6c6cbb

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:d9228065214a5402dcf5ad7f97cbd05cf201b76c8800b71cd083c7e703002674

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=sha256:7499793fa1007dfa99b25173856dbba99384fad4d7b4bc8aceb6f66ce17ca8c9

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=sha256:9767346382544c87dc894663d35bf2336e63c35163f1ad040d29bbf63fbd2b1d

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 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-08-10T15:33:40.566061Z digest=sha256:1feb82dc4609ffb03c1e43397c8f319392faf7e3e1663fc906b73c7af50c3e02

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.

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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
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Source-reported events for the cited work

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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

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

Source-reported events for the cited work

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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.

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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.

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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.

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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.

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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:c4a9cd8ba167cec3eaa5fc8aedb8910c605e009d58e2aea1a6df13fab35e3ef0

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.

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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=sha256:7cfb2351b54787e7fa90fff9ecdd1355891c8fdd6bf2aa07c1957d91a41ea1e6

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.

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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 2026-08-11T06:34:44.6726+00:00.

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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.

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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.

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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.

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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.

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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

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Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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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.

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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.

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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.

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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.

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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.

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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.

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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.

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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=sha256:5d027f817304a3ea86f62339ebd4ee32e259c607fbfe4205f193560bb4fac60b

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.

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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.

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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.

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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.

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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.

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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:f91051bfc297d4c9502b6fcc81b32542ec0e551961a728611f0c8a164e9f43c3

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
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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