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Paper Citation Record · LEDGER

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift

As of 12 August 2026, this Paper Citation Record lists 100 of 167 outbound references and 2 inbound Pith citation observations for arXiv:2510.26877.

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

pith.paper-citation-record.v1
2510.26877 v2

Coverage vector

measured 100 of 167 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-18T02:48:14.635035Z

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One-hop event checks from named stored sources.

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-28T00:44:40.243679Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T12:15:01.137692Z

Reference resolution

100 of 167 outbound references displayed

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External citation measurements

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Outbound references

Observation 5a1ed5b9-c0b3-4b68-b2f4-2574523ce4f7 · outbound

This paper cites R., Federrath, C., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift R., Federrath, C., et al

Reference 1

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Observation d1af4dd9-4bf8-4921-8df7-7c3c0a76effe · outbound

This paper cites Figuring Out Gas & Galaxies In Enzo (FOGGIE) VIII: Complex and Stochastic Metallicity Gradients at z > 2.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Figuring Out Gas & Galaxies In Enzo (FOGGIE) VIII: Complex and Stochastic Metallicity Gradients at z > 2

Reference 2

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Observation e09ea8b1-8688-43b1-998e-5b740145074b · outbound

This paper cites Spatially resolved gas-phase metallicity at z~2-3 with JWST/NIRISS.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Spatially resolved gas-phase metallicity at z~2-3 with JWST/NIRISS

Reference 3

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Observation 26793499-27ed-4713-a864-41a6bd5ba4c8 · outbound

This paper cites J., Reeves J.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift J., Reeves J

Reference 4

Resolution
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Observation e9190aa2-e647-4444-beed-743aaf21b5f3 · outbound

This paper cites 2024, A&A, 688, A146, doi: 10.1051/0004-6361/202348824.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2024, A&A, 688, A146, doi: 10.1051/0004-6361/202348824

Reference 5

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Observation a9687c58-6bc4-46c6-8822-af21f1e609c7 · outbound

This paper cites 2024, MNRAS, 532, L14, doi: 10.1093/mnrasl/slae036.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2024, MNRAS, 532, L14, doi: 10.1093/mnrasl/slae036

Reference 6

Resolution
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Observation abfb2514-5715-4932-bde6-fedb74685efe · outbound

This paper cites 2017, MNRAS, 469, 151, doi: 10.1093/mnras/stx789.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2017, MNRAS, 469, 151, doi: 10.1093/mnras/stx789

Reference 7

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Observation 2262b7dd-2005-480a-aeed-cfecb5ac4664 · outbound

This paper cites A., Wetzel, A., Loebman, S.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift A., Wetzel, A., Loebman, S

Reference 8

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Observation 1a2505bb-7830-41f7-b6d1-68595f1dad36 · outbound

This paper cites keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 9

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Observation 91c19ff6-a743-4080-95cc-fe24c2e9153d · outbound

This paper cites and Shibahashi , H.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift and Shibahashi , H

Reference 10

Resolution
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Observation 3ac6152d-e9f1-4018-b44c-577164510bcf · outbound

This paper cites D., Springel, V., Ostriker, E.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift D., Springel, V., Ostriker, E

Reference 11

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Observation 3dc14eb5-3735-4aed-94e8-913107e65034 · outbound

This paper cites 2018, MNRAS, 478, 4293, doi: 10.1093/mnras/sty1343.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2018, MNRAS, 478, 4293, doi: 10.1093/mnras/sty1343

Reference 12

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Observation 5d55a442-d71d-43b5-9259-eeaf8e4378e0 · outbound

This paper cites 2016, MNRAS, 457, 2605, doi: 10.1093/mnras/stw064.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2016, MNRAS, 457, 2605, doi: 10.1093/mnras/stw064

Reference 13

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Observation 043f5550-fb09-4c0d-961d-f6e4810fbfae · outbound

This paper cites Galactic Stellar and Substellar Initial Mass Function.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Galactic Stellar and Substellar Initial Mass Function

Reference 14

Resolution
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Observation 6f07818c-8d3e-4868-b123-29d4ef578524 · outbound

This paper cites K., Kereˇ s, D., Wetzel, A., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift K., Kereˇ s, D., Wetzel, A., et al

Reference 15

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Observation 129cebb2-85d1-49ad-a152-374c0ae8e021 · outbound

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Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 16

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Observation 82c73ce5-12de-4de2-970c-f4ebcb8ad5e9 · outbound

This paper cites keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 17

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Observation 26b09bf4-025b-4511-9130-72c35b8a54fd · outbound

This paper cites 2010, Nature, 467, 811, doi: 10.1038/nature09451.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2010, Nature, 467, 811, doi: 10.1038/nature09451

Reference 18

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Observation 08297657-05e1-4326-a2ae-3c825d4c5a13 · outbound

This paper cites 2020, MNRAS, 492, 821, doi: 10.1093/mnras/stz3379.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2020, MNRAS, 492, 821, doi: 10.1093/mnras/stz3379

Reference 19

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Observation 45f12876-71b9-4ef4-9011-7874dc6cf9e0 · outbound

This paper cites A., okas E.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift A., okas E

Reference 20

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Observation 716e79c4-1bec-4624-b1e0-8a0695e6a380 · outbound

This paper cites L., Tacchella, S., \”Ubler, H., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift L., Tacchella, S., \”Ubler, H., et al

Reference 21

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Observation 4c97f25a-963b-436e-859c-f8f5be5b5514 · outbound

This paper cites L., Gil-Pons, P., Lau, H.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift L., Gil-Pons, P., Lau, H

Reference 22

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Observation fb3d83cc-b5a2-4934-a310-4a031449653d · outbound

This paper cites 2016, ApJ, 820, 131, doi: 10.3847/0004-637X/820/2/131.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2016, ApJ, 820, 131, doi: 10.3847/0004-637X/820/2/131

Reference 23

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Observation dcc7327b-2f0d-40de-9abb-d2d92b73338d · outbound

This paper cites 2018a, MNRAS, 473, 1930, doi: 10.1093/mnras/stx2482.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2018a, MNRAS, 473, 1930, doi: 10.1093/mnras/stx2482

Reference 24

Resolution
verified exact
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Observation e0ac51db-ade3-4e34-b7cf-416d543b4fa8 · outbound

This paper cites N., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift N., et al

Reference 25

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Observation faae10ae-51b2-47ae-8c6f-dd515eb5c99f · outbound

This paper cites M., Jørgensen, J.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift M., Jørgensen, J

Reference 26

Resolution
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Observation 3cd8e4f5-e974-4c4c-9ecb-de61e9da248f · outbound

This paper cites Li PS, Klein RI, McKee CF.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Li PS, Klein RI, McKee CF

Reference 27

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Source-reported events for the cited work

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Observation a0740f98-8a6a-4076-87bc-d91b71497558 · outbound

This paper cites 2023, MNRAS, 522, 3831, 10.1093/mnras/stad1205.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2023, MNRAS, 522, 3831, 10.1093/mnras/stad1205

Reference 28

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Observation 1b34e146-9e86-4f77-87ee-65092deae125 · outbound

This paper cites F., Abadi, M.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift F., Abadi, M

Reference 29

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Source-reported events for the cited work

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Observation 62967833-58d6-48e7-92f3-fb297ddda9d3 · outbound

This paper cites K., Karakas, A.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift K., Karakas, A

Reference 30

Resolution
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Source-reported events for the cited work

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Observation 31b23b78-4c82-47b9-b7bc-750c66c37d6e · outbound

This paper cites GASP and MaNGA surveys shed light on the enigma of the gas metallicity gradients in disk galaxies.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift GASP and MaNGA surveys shed light on the enigma of the gas metallicity gradients in disk galaxies

Reference 31

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Observation 79560f4b-b440-4b27-8050-34536ba7a52f · outbound

This paper cites 1995, A&A, 301, 649.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 1995, A&A, 301, 649

Reference 32

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation bccaa8f2-b068-429a-91c4-701c5065fd13 · outbound

This paper cites 1994, ApJL, 430, L105, doi: 10.1086/187449.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 1994, ApJL, 430, L105, doi: 10.1086/187449

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Resolution
verified exact
doi, observed 2026-05-18T02:50:47.858586Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation d661943b-6e30-4068-80a6-64ee8e8abb1f · outbound

This paper cites L., Tsujita, A., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift L., Tsujita, A., et al

Reference 34

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:48.389606Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation ce506c59-c86f-4de8-b96b-e47a7a8cf81b · outbound

This paper cites keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 35

Resolution
metadata mismatch
doi, observed 2026-05-18T02:50:48.148308Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 65e4b5d5-b1e5-4ef1-9e40-949cab4135e0 · outbound

This paper cites M., Torrey, P., Hemler, Z.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift M., Torrey, P., Hemler, Z

Reference 36

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.531043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 4243f0ca-cdbb-4141-aca8-9cdb8e0bea60 · outbound

This paper cites M., Torrey, P., Grasha, K., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift M., Torrey, P., Grasha, K., et al

Reference 37

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.026736Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 879393dc-e19b-4c29-8416-2b6169d5f711 · outbound

This paper cites M., Torrey, P., Ellison, S., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift M., Torrey, P., Ellison, S., et al

Reference 38

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.953890Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 94451d2b-9867-4455-adcb-355445763b69 · outbound

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

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift M., Torrey, P., Ellison, S

Reference 39

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.740338Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation af597918-abbd-4ff7-95c7-9ff9f6d7f545 · outbound

This paper cites M., Torrey, P., Bhagwat, A., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift M., Torrey, P., Bhagwat, A., et al

Reference 40

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.060284Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation a10395d1-1444-4b17-977f-7931ba93f769 · outbound

This paper cites S., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift S., et al

Reference 41

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.735181Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:6ca9aa9c379f5fac1437769b50463bb506cc268ef1a3996c3c587a9f6b0843e6

Observation 5d30e09c-4e42-4151-bde6-bbc54437ab29 · outbound

This paper cites F., Wetzel, A., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift F., Wetzel, A., et al

Reference 42

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.895408Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:20b0ef7cd63d03ac28c560fc2e9272b865f26b50cc08e6016359f0307607d65b

Observation daae4745-0e38-44f6-a72d-3001e04b5401 · outbound

This paper cites 2014 , month = sep, publisher =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2014 , month = sep, publisher =

Reference 43

Resolution
metadata mismatch
doi, observed 2026-05-18T02:50:48.050844Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:f2008686df3bd37243058f65e552a4e6571081c1e64a2e829d9a883fe33c7ed2

Observation a657ac52-6402-4c39-b745-6b6500604cfd · outbound

This paper cites K., Pilkington , K., Brook , C.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift K., Pilkington , K., Brook , C

Reference 44

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.128303Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation bf45bed2-7e2b-4c4b-81f4-cbe9a76fe5ed · outbound

This paper cites Inside-out versus Upside-down: The Origin and Evolution of Metallicity Radial Gradients in FIRE Simulations of Milky Way-mass Galaxies and the Essential Role of Gas Mixing.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Inside-out versus Upside-down: The Origin and Evolution of Metallicity Radial Gradients in FIRE Simulations of Milky Way-mass Galaxies and the Essential Role of Gas Mixing

Reference 45

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:47.891965Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:47dd4cee943b368205a1d72e25ba2a5d6b4e5a04c367a89f23360942aff6634d

Observation ebeb80a3-7686-4cc7-8ffb-6ad47455d24e · outbound

This paper cites H., Battisti, A.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift H., Battisti, A

Reference 46

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.803727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:12c31f599a107e8968823d14263b3afa9a44d178ed8984272a345e2d83afa437

Observation 5659a7ee-3252-4620-bfa6-c7d409b0cee1 · outbound

This paper cites 2020, MNRAS, 498, 1939, doi: 10.1093/mnras/staa2382.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2020, MNRAS, 498, 1939, doi: 10.1093/mnras/staa2382

Reference 47

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.843528Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:ced016f2b481f680c92cd2b118937ddd252352901d525199e643d78f7a15d25e

Observation c98bc72d-48f8-4d7a-a93d-31e1a4e5411f · outbound

This paper cites S., Torrey, P., Qi, J., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift S., Torrey, P., Qi, J., et al

Reference 48

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.057129Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:07fff6cca544bab321be7d4be0e128182a2a3a5fd6a26db82fd9485ab59ccf58

Observation d1e8e79e-6f3f-4467-b91e-2c94f50e9161 · outbound

This paper cites 2011, ApJL, 743, L29, doi: 10.1088/2041-8205/743/2/L29.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2011, ApJL, 743, L29, doi: 10.1088/2041-8205/743/2/L29

Reference 49

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.831710Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:f696236fe5ed21f3d9e6e657a5f4fdc6f5a2b3ac1f2fc3debdfbcdd43c26c51b

Observation 27bd1146-2ba5-4d18-8066-507cf6170914 · outbound

This paper cites F., 2015, @doi [ ] 10.1093/mnras/stv195 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.450...53H 450, 53.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift F., 2015, @doi [ ] 10.1093/mnras/stv195 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.450...53H 450, 53

Reference 50

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.009032Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:9798249e34f7f78be6aa7c4cf831abd75b6cc2f03e2f88aba908a8b6ee820e4b

Observation 33f986be-5212-4e8f-9986-3b0e5839e390 · outbound

This paper cites Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation

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Resolution
metadata mismatch
doi, observed 2026-05-18T02:50:47.724859Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 015dff73-f193-4338-87de-59ce1055fd3e · outbound

This paper cites FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation

Reference 52

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.525152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation f3ce9e9b-a281-4cf2-8f28-679a15e51a95 · outbound

This paper cites R., Scholtz, J., Danhaive, A.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift R., Scholtz, J., Danhaive, A

Reference 53

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:47.965011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 02558da5-ee82-4866-a195-918693293dba · outbound

This paper cites 1999, ApJS, 125, 439, doi: 10.1086/313278.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 1999, ApJS, 125, 439, doi: 10.1086/313278

Reference 54

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.002499Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 27c4cd08-a885-4fee-88b0-874eef45e956 · outbound

This paper cites M., Papadakis I.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift M., Papadakis I

Reference 55

Resolution
metadata mismatch
arxiv_id, observed 2026-05-18T02:50:47.551915Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 723e7a9d-21a0-475a-9453-a9bce23be67d · outbound

This paper cites an unresolved cited work.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Unresolved cited work

Reference 56

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.727565Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation ccef993b-7dfc-476d-a3fa-b87590b067cc · outbound

This paper cites S., Richard J., Jullo E., 2013, @doi [ ] 10.1088/0004-637X/765/1/48 , https://ui.adsabs.harvard.edu/abs/2013ApJ...765...48J 765, 48.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift S., Richard J., Jullo E., 2013, @doi [ ] 10.1088/0004-637X/765/1/48 , https://ui.adsabs.harvard.edu/abs/2013ApJ...765...48J 765, 48

Reference 57

Resolution
metadata mismatch
doi, observed 2026-05-18T02:50:47.715016Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:54cb5df262630e2a25c47cff9acc6141cc2ead0b00d641807fad0c9d3edc6fa5

Observation bce9bf18-3026-4128-880f-8c23464950cc · outbound

This paper cites B., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift B., et al

Reference 58

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.019449Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:29ce7216029e28b8b52728bfc140ffaf6ce233044cfbe66614a3955f41048757

Observation 98d7c2d5-84a4-4c21-80ed-2ac41d95f306 · outbound

This paper cites 2025, ApJL, 978, L39, doi: 10.3847/2041-8213/ada150.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2025, ApJL, 978, L39, doi: 10.3847/2041-8213/ada150

Reference 59

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.824184Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation b63c56ad-2e07-43af-affb-12118f56bde0 · outbound

This paper cites keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 60

Resolution
metadata mismatch
doi, observed 2026-05-18T02:50:47.820431Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:284c964b48587e24b8704a71789b728e0faedbeba012fe1eca62cb9b6024d836

Observation e5be2bad-62cc-4bd7-83ed-f148ee422370 · outbound

This paper cites M., Glover, S.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift M., Glover, S

Reference 61

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.691520Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:cd35fcfaa005fa87e73ff5271ae61bc34d2fe994b74fe2bea064bc2634e4d063

Observation 872b9c5e-acc0-472f-b820-69872ce693f4 · outbound

This paper cites 2019, MNRAS, 485, 117, doi: 10.1093/mnras/stz287.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2019, MNRAS, 485, 117, doi: 10.1093/mnras/stz287

Reference 62

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.745083Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:1ef10908883628da1ba270d6357a628128a08390bbe38b9ed8757ae6d7697e60

Observation 8d7dd3db-21bb-47f8-8390-815bbf7ea2a2 · outbound

This paper cites 2025, arXiv e-prints.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2025, arXiv e-prints

Reference 63

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:47.985025Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:ff05baaa32023a61bc538c5b3065bb9a5e4383c77c75ac829ce59762544d8bfe

Observation 47000c43-9bcc-4cb0-9bb3-80089128cadb · outbound

This paper cites R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607

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Resolution
metadata mismatch
arxiv_id, observed 2026-05-18T02:50:48.030522Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:6ae2de8b806c1a24aa865993afc1627f128d49179a1bcab7e5fba1b2318a274d

Observation b1a04656-d43d-4c22-b15d-47a3c7a13c5b · outbound

This paper cites Star Formation in Galaxies Along the Hubble Sequence.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Star Formation in Galaxies Along the Hubble Sequence

Reference 65

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.638035Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 8b2266c8-eda3-481f-b63f-05cf7d7dba4a · outbound

This paper cites keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 66

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.947718Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation d41bcfa9-d159-439c-9155-ed1ee3662bdf · outbound

This paper cites R., & Knebe, A.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift R., & Knebe, A

Reference 67

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.868628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation f67bb3d3-8915-4a4a-bb53-6a45b93ac902 · outbound

This paper cites 2006, title Galactic Chemical Evolution: Carbon through Zinc , , 653, 1145, 10.1086/508914.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2006, title Galactic Chemical Evolution: Carbon through Zinc , , 653, 1145, 10.1086/508914

Reference 68

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.141043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 08cf8cdd-6151-4e60-a701-c585277753b4 · outbound

This paper cites 2020, MNRAS, 492, 1385, doi: 10.1093/mnras/stz3495.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2020, MNRAS, 492, 1385, doi: 10.1093/mnras/stz3495

Reference 69

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.758042Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation d327f95b-4bba-47ff-93cf-16cdca622bcc · outbound

This paper cites 2002, Science (80-.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2002, Science (80-

Reference 70

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.615846Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 2033fdec-976b-4bd4-9349-cdb15f294c83 · outbound

This paper cites keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 71

Resolution
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doi, observed 2026-05-18T02:50:47.749934Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation f5343332-7154-4ac1-aa15-7bf24b4860da · outbound

This paper cites A., Ellis, R.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift A., Ellis, R

Reference 72

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.772649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation ef30506d-7313-4306-b677-59000636d62a · outbound

This paper cites 2014, ApJS, 212, 14, doi: 10.1088/0067-0049/212/1/14.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2014, ApJS, 212, 14, doi: 10.1088/0067-0049/212/1/14

Reference 73

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.543453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation b3b548e6-3ce3-4932-a64e-a8ae4c516c92 · outbound

This paper cites Starburst99: Synthesis Models for Galaxies with Active Star Formation.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Starburst99: Synthesis Models for Galaxies with Active Star Formation

Reference 74

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.801040Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 9f8d5b45-d505-4ed3-8d3d-963e7d753da1 · outbound

This paper cites 2022, ApJL, 929, L8, doi: 10.3847/2041-8213/ac626f.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2022, ApJL, 929, L8, doi: 10.3847/2041-8213/ac626f

Reference 75

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.016126Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation c10c8445-561b-4ab3-bf08-6fd5d58ab5a7 · outbound

This paper cites A 13-Billion-Year View of Galaxy Growth: Metallicity Gradient Evolution from the Local Universe to $z=9$ with JWST and Archival Surveys.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift A 13-Billion-Year View of Galaxy Growth: Metallicity Gradient Evolution from the Local Universe to $z=9$ with JWST and Archival Surveys

Reference 76

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:47.557104Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 490657b4-e9f2-4e68-888f-7ca53638074d · outbound

This paper cites J., D’Eugenio, F., Maiolino, R., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift J., D’Eugenio, F., Maiolino, R., et al

Reference 77

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.663522Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 70f56341-3d78-45bb-b95e-a846a5245c99 · outbound

This paper cites A., Krumholz, M.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift A., Krumholz, M

Reference 78

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.901611Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation a21bfd24-d313-4668-b41d-e4e4ff44b3c3 · outbound

This paper cites F., Feldmann, R., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift F., Feldmann, R., et al

Reference 79

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.991226Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 66e18cfc-6eed-46cd-9569-afb3b6c9680b · outbound

This paper cites 2020, MNRAS, 498, 2001, doi: 10.1093/mnras/staa2404.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2020, MNRAS, 498, 2001, doi: 10.1093/mnras/staa2404

Reference 80

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.631507Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 86f9d296-be5c-4e7a-9b31-07419608f815 · outbound

This paper cites F., Garrison-Kimmel, S., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift F., Garrison-Kimmel, S., et al

Reference 81

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.634169Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation f7c27b48-389c-4bae-9b9d-ce0ff897ae04 · outbound

This paper cites C., Casey, C.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift C., Casey, C

Reference 82

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.957152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 111756f0-cb96-4b0f-b0da-ad6ee4786311 · outbound

This paper cites 2019, A&A Rv, 27, 3, doi: 10.1007/s00159-018-0112-2.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2019, A&A Rv, 27, 3, doi: 10.1007/s00159-018-0112-2

Reference 83

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.144644Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 4be17d47-fb1b-40f9-8549-921fb287f186 · outbound

This paper cites and Yang , J.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift and Yang , J

Reference 84

Resolution
metadata mismatch
arxiv_id, observed 2026-05-18T02:50:48.103004Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 5a718098-abca-4000-bd31-54a126f3a400 · outbound

This paper cites 2001, A&A, 370, 194, doi: 10.1051/0004-6361:20000247 The Role of Bursty Versus Smooth Feedback on Metallicity Gradients19.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2001, A&A, 370, 194, doi: 10.1051/0004-6361:20000247 The Role of Bursty Versus Smooth Feedback on Metallicity Gradients19

Reference 85

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.980487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation bf6cca66-86c2-4483-9475-333c3d5c9743 · outbound

This paper cites keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 86

Resolution
metadata mismatch
doi, observed 2026-05-18T02:50:47.703115Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 08d6b039-02d1-4f2f-8fa9-9155a2ceb2b6 · outbound

This paper cites 2025, ApJL, 991, L4, doi: 10.3847/2041-8213/adf74b.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2025, ApJL, 991, L4, doi: 10.3847/2041-8213/adf74b

Reference 87

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.534563Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation c9af7b93-9155-48bf-80f4-61d820165fa3 · outbound

This paper cites arXiv e-prints , keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift arXiv e-prints , keywords =

Reference 88

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:47.688301Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:0ec73fc2cdeb8c379c3166db8dc8277c2965b40e141cbfe35c2153d538ad5e21

Observation 3e225787-84cc-4659-9f26-7ac71933c089 · outbound

This paper cites 2016, MNRAS, 457, 3775, doi: 10.1093/mnras/stw253.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2016, MNRAS, 457, 3775, doi: 10.1093/mnras/stw253

Reference 89

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.169666Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation a724639e-109c-4d02-bfd8-3e796e225728 · outbound

This paper cites C., Marinacci F., 2017, @doi [ ] 10.1093/mnras/stx467 , http://cdsads.u-strasbg.fr/abs/2017MNRAS.468.1505M 468.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift C., Marinacci F., 2017, @doi [ ] 10.1093/mnras/stx467 , http://cdsads.u-strasbg.fr/abs/2017MNRAS.468.1505M 468

Reference 90

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.537628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 36bd1f8a-921d-4685-a871-f5d4842ca792 · outbound

This paper cites 2024, arXiv e-prints.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2024, arXiv e-prints

Reference 91

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:48.384781Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 53898f0f-d91d-4987-8ff1-65387a8f9570 · outbound

This paper cites L., Kereˇ s, D., Faucher-Gigu` ere, C.-A., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift L., Kereˇ s, D., Faucher-Gigu` ere, C.-A., et al

Reference 92

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.787770Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 5c079a4c-1bc1-4414-aade-9609b3d202ac · outbound

This paper cites The Ultraviolet Slopes of Early Universe Galaxies: The Impact of Bursty Star Formation, Dust, and Nebular Continuum Emission.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift The Ultraviolet Slopes of Early Universe Galaxies: The Impact of Bursty Star Formation, Dust, and Nebular Continuum Emission

Reference 93

Resolution
verified exact
arxiv_id, observed 2026-05-18T02:50:47.698966Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 580b6cf9-9c8b-4a3f-8706-2decc74d09b6 · outbound

This paper cites 2024, ApJ, 961, 73, doi: 10.3847/1538-4357/ad0966.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2024, ApJ, 961, 73, doi: 10.3847/1538-4357/ad0966

Reference 94

Resolution
verified exact
doi, observed 2026-05-18T02:50:47.935027Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation c40c4b98-7798-4781-b78b-31e36d206757 · outbound

This paper cites keywords =.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift keywords =

Reference 95

Resolution
metadata mismatch
doi, observed 2026-05-18T02:50:47.667125Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-18T02:48:14.635035Z digest=sha256:351202584e6baf609c21253d24342e16d1b0eab31067a7554491150c2ed22b48

Observation 78cd96d8-3f9e-418b-9993-6e9ff26212f4 · outbound

This paper cites K., Brachwitz F., Tsujimoto T., Kubo Y., Kishimoto N., 1997, @doi [ ] 10.1016/S0375-9474(97)00291-1 , https://ui.adsabs.harvard.edu/abs/1997NuPhA.621..467N 621, 467.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift K., Brachwitz F., Tsujimoto T., Kubo Y., Kishimoto N., 1997, @doi [ ] 10.1016/S0375-9474(97)00291-1 , https://ui.adsabs.harvard.edu/abs/1997NuPhA.621..467N 621, 467

Reference 96

Resolution
verified exact
doi, observed 2026-05-18T02:50:48.047672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 4848ea5d-fc16-4c75-bdd2-d52a84536baf · outbound

This paper cites 2006, title Nucleosynthesis yields of core-collapse supernovae and hypernovae, and galactic chemical evolution , , 777, 424, 10.1016/j.nuclphysa.2006.05.008.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift 2006, title Nucleosynthesis yields of core-collapse supernovae and hypernovae, and galactic chemical evolution , , 777, 424, 10.1016/j.nuclphysa.2006.05.008

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doi, observed 2026-05-18T02:50:47.742863Z

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Observation a0497f99-e3ab-4854-bb03-d3ba0eae6896 · outbound

This paper cites E., Burkhart, B., Wetzel, A., et al.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift E., Burkhart, B., Wetzel, A., et al

Reference 98

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doi, observed 2026-05-18T02:50:48.159974Z

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Observation 183b0b5a-90a6-402d-ad9d-e8bdd1461234 · outbound

This paper cites Pandya,et al., Characterizing mass, momentum, energy, and metal outflow rates of mul- tiphase galactic winds in the FIRE-2 cosmological simulations.Mon.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift Pandya,et al., Characterizing mass, momentum, energy, and metal outflow rates of mul- tiphase galactic winds in the FIRE-2 cosmological simulations.Mon

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doi, observed 2026-05-18T02:50:48.005803Z

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Observation 935db249-b4ee-4076-b223-57d643e14db4 · outbound

This paper cites and Shibahashi , H.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift and Shibahashi , H

Reference 100

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arxiv_id, observed 2026-05-18T02:50:47.587425Z

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Pith citing papers

Observation 53b29d6f-2b20-4303-beef-b32128e75f73 · inbound

The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles cites this paper.

The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift

Reference 32

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local_arxiv, observed 2026-05-17T01:58:50.960421Z

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Observation a029204e-4b19-454f-8694-6182c674e11f · inbound

Grain-size evolution and rapid dust growth in high-redshift galaxies cites this paper.

Grain-size evolution and rapid dust growth in high-redshift galaxies Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift

Reference 16

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local_arxiv, observed 2026-06-28T00:51:26.992690Z

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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