Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-10T15:33:40.659406Z
Paper Citation Record · LEDGER
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.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-10T15:33:40.659406Z
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-13T04:41:12.165957Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-13T04:49:20.251165Z
100 of 104 outbound references displayed
External citation measurements
No source-named external measurement is stored.
Observation 4a9c8fdc-f875-451f-8193-3a6b771cc175 · outbound
Reference 1
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c666613b-7c73-4f18-9d7c-927ccf8ea0e6 · outbound
Reference 2
Source-reported events for the cited work
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Observation 5e98539d-fad1-4069-aab8-b5cd6603f4f6 · outbound
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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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
Reference 6
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Observation 72100cdc-9804-493b-b7c1-5c2f057a3f58 · outbound
Reference 7
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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 8
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Observation 2ffc0d0a-e5ab-4969-a885-e54327d8f818 · outbound
Reference 9
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Observation 704211aa-2220-4043-9956-17de28272906 · outbound
Reference 10
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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
Reference 12
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Observation 70df6480-b2c3-44cd-999e-2894f85bc457 · outbound
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
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Observation 227857a4-e0d8-427f-add3-5558fcf89586 · outbound
Reference 14
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Observation c5b1decc-0e77-4cf0-a3bc-cc9e503cc93a · outbound
Reference 15
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Observation 3b2865dc-2039-4b07-a911-b021eab0907f · outbound
Reference 16
Source-reported events for the cited work
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Observation a3093248-5fca-494a-89d9-f898a71190a5 · outbound
Reference 17
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Observation dea53888-8b83-4d6c-a1d4-14355f52760e · outbound
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
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Observation db00f0b0-a14b-420d-a009-3696286ac25a · outbound
Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work
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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
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Observation 47a4fd52-8223-48d4-b727-7a2baa11e9b0 · outbound
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
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Source-reported events for the cited work
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Observation 7f8b8163-6365-46e1-8d22-e78dc964c971 · outbound
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
Source-reported events for the cited work
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Observation 90c5556d-e77c-4a45-8fe3-df006f60a83d · outbound
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
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
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Observation b7955cdb-212e-47cc-a7e2-380f63f48956 · outbound
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
Source-reported events for the cited work
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Observation 2d8c1382-2248-44f2-853b-25ee92e0c92b · outbound
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
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
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Observation 0375c6fe-7e1a-4a0c-b0eb-a94a75215ef5 · outbound
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
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Unavailable: canonical work link unavailable.
Observation 47a9c2f2-820b-4d14-b972-67517722a7c4 · outbound
Reference 29
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Observation 1bbc5fb8-3e96-4bca-b2c2-ae2be2dc3a00 · outbound
Reference 30
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Observation 166cd629-6987-43c4-9853-dcfdfa89e176 · outbound
Reference 31
Source-reported events for the cited work
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Observation 71e56e67-36e8-4d72-b956-ad633dae3090 · outbound
Reference 32
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Observation e3509204-dfa3-4c83-935e-67b3a48c1101 · outbound
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
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Observation ea23a647-73c3-4a64-bfbc-f04d4cc99165 · outbound
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
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Observation b2d724b2-15b5-4100-8f11-499d0e6803af · outbound
Reference 35
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Observation d56232bf-7d98-4693-97d4-58d142842ed5 · outbound
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
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Observation 36924826-2709-4b6c-8717-067e845533f8 · outbound
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
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Observation 525338ec-74b0-4cd3-bcfc-fb19ad96fb17 · outbound
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2ff8a452-92ba-4d13-bf7f-2662ce28bdd9 · outbound
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
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Observation 49dae055-a64f-4cdf-9c49-b18718fde237 · outbound
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
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Observation 57252f78-1608-494f-8cf6-b2115e58eb41 · outbound
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 16ddeeb2-cdd1-48c7-90e6-5a380aba5d43 · outbound
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
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Observation 18316d1c-e272-408b-9733-d021c4c40d78 · outbound
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
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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
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Observation 28a3a876-5c3c-4bbc-92be-9f325396099e · outbound
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Observation ba63efc4-0ef3-4db2-9dfb-29f44418959b · outbound
Reference 46
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Observation f73df768-31a5-4df2-bcd2-8121ce364ddc · outbound
Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency Unresolved cited work
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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
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Observation 9ee23b0d-44e7-462b-b4e9-b47f3c394aeb · outbound
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
Source-reported events for the cited work
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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
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Observation eff61d06-e040-49b3-a0ee-55393d84b6a1 · outbound
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
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Observation c1ebd4b1-f80d-4e36-b0cf-f1fda0edf301 · outbound
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
Source-reported events for the cited work
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Observation da680909-6091-41a4-b151-49bf852d6c4c · outbound
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
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Observation c9bbe94d-4977-4b06-b50f-c506a273d156 · outbound
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
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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 57
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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
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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 59
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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 60
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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
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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 62
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Observation 5b45ed88-8cbe-4e5b-bc53-1eb71c1a8138 · outbound
Reference 63
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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 64
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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
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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
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Observation 9120402c-cee5-4ee1-9263-befb36f45647 · outbound
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
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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 68
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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 69
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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
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Observation 71c2ebb1-d9e5-4249-a484-b34c55d733b6 · outbound
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
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Reference 72
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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
Source-reported events for the cited work
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Observation 4309a072-7b96-4836-8f26-2e38fa5ce514 · outbound
Reference 74
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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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Observation 19b3b2f3-1f89-436c-82bd-e7e7c01c88e8 · outbound
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
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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 77
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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 78
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Observation 8eaed80f-c9cb-4cab-ab71-1e39c9e5e10c · outbound
Reference 79
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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 80
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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 81
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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 82
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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 83
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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
Source-reported events for the cited work
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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
Source-reported events for the cited work
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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 86
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