Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? | Paper Citation Record

Observation 5db4efd9-8fc3-4feb-8e72-96880e7dc49e · outbound

This paper cites Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang

Reference 1

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Observation dd6a2187-ed57-4304-a082-1655335d3bcc · outbound

This paper cites P., 1988, @doi [ ] 10.1086/166961 , https://ui.adsabs.harvard.edu/abs/1988ApJ...335..720A 335, 720.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? P., 1988, @doi [ ] 10.1086/166961 , https://ui.adsabs.harvard.edu/abs/1988ApJ...335..720A 335, 720

Reference 2

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Observation ca2ff86c-0385-4389-b364-d21592f84eb7 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 3

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Observation 356e7239-a224-4d15-b82c-8039143214f0 · outbound

This paper cites C., Loeb A., 2016, @doi [ ] 10.1093/mnrasl/slw055 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.459L..51A 459, L51.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? C., Loeb A., 2016, @doi [ ] 10.1093/mnrasl/slw055 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.459L..51A 459, L51

Reference 4

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Observation a9c607f7-d9a9-4032-ba96-6e9b43239539 · outbound

This paper cites A., Romanowsky A.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., Romanowsky A

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.759727Z

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Observation cd1e090a-1607-4346-9d31-7233cb3b7bef · outbound

This paper cites A., et al., 2021, @doi [Nature Astronomy] 10.1038/s41550-021-01458-1 , https://ui.adsabs.harvard.edu/abs/2021NatAs...5.1255B 5, 1255.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., et al., 2021, @doi [Nature Astronomy] 10.1038/s41550-021-01458-1 , https://ui.adsabs.harvard.edu/abs/2021NatAs...5.1255B 5, 1255

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.763946Z

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Observation c9c80fad-1950-4486-bad2-21fa4ae3728b · outbound

This paper cites A., 2020, @doi [ ] 10.3847/1538-3881/ab5b0e , https://ui.adsabs.harvard.edu/abs/2020AJ....159...56B 159, 56.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., 2020, @doi [ ] 10.3847/1538-3881/ab5b0e , https://ui.adsabs.harvard.edu/abs/2020AJ....159...56B 159, 56

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.769298Z

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Observation 27714572-b97e-4f8b-8c45-718892e14db4 · outbound

This paper cites L., et al., 2022, @doi [ ] 10.1093/mnras/stac2442 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.517.2231B 517, 2231.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? L., et al., 2022, @doi [ ] 10.1093/mnras/stac2442 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.517.2231B 517, 2231

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.773576Z

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Observation a1ead537-7c5e-46e0-98e9-512c8a49bdd9 · outbound

This paper cites L., et al., 2024, @doi [ ] 10.1093/mnras/stae564 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.529.3210B 529, 3210.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? L., et al., 2024, @doi [ ] 10.1093/mnras/stae564 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.529.3210B 529, 3210

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.777130Z

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Observation 2475e66a-b1a1-477f-a89b-6ca2f60dede0 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.780663Z

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Observation 95755ca8-a1ce-4b8c-9d36-0a042ecbc60b · outbound

This paper cites Y., 2023, @doi [ ] 10.1093/mnras/stad1328 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.522.5638C 522, 5638.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Y., 2023, @doi [ ] 10.1093/mnras/stad1328 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.522.5638C 522, 5638

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.784095Z

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Observation b74800ab-9bbc-47e1-9a86-ec6716e14bd1 · outbound

This paper cites A two-phase model of galaxy formation: III. The formation of globular clusters.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A two-phase model of galaxy formation: III. The formation of globular clusters

Reference 12

Resolution: verified exact; local_arxiv, observed 2026-08-11T20:08:38.376695Z

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

Observation adf82002-0bf8-487f-a731-3d6b41c4865c · outbound

This paper cites V., Afanasiev A.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? V., Afanasiev A

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.791061Z

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Observation 9e1fae24-a33a-465f-b5f5-f2d2e600d946 · outbound

This paper cites Y., 2019, @doi [ ] 10.1093/mnras/stz2097 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.5409C 488, 5409.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Y., 2019, @doi [ ] 10.1093/mnras/stz2097 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.5409C 488, 5409

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.794170Z

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Observation b947b738-090f-4ef2-a39e-dfcd059ae076 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.804111Z

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Observation 800d9f04-231f-4677-9d74-81e06cd60c42 · outbound

This paper cites J., 2019, @doi [ApJL] 10.3847/2041-8213/ab0e8c , https://ui.adsabs.harvard.edu/abs/2019ApJ...874L..12D 874, L12.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? J., 2019, @doi [ApJL] 10.3847/2041-8213/ab0e8c , https://ui.adsabs.harvard.edu/abs/2019ApJ...874L..12D 874, L12

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.808388Z

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Observation 661cf5b5-a984-40fc-9b81-501c6e416b03 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.811976Z

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Observation 7eff273c-789b-44df-a7a8-a60c375981d4 · outbound

This paper cites B., Dutton A.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? B., Dutton A

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.815832Z

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Observation 498e0a7b-2ea2-4921-8006-c69c32b1e205 · outbound

This paper cites E., et al., 2023, @doi [ ] 10.1093/mnras/stac2818 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.2453D 518, 2453.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? E., et al., 2023, @doi [ ] 10.1093/mnras/stac2818 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.2453D 518, 2453

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.819403Z

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Observation c856eeb4-c482-493a-9398-6ab58710d83e · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.823198Z

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Observation 99dd77f8-58ca-431b-b7fc-0489482f6f58 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.826868Z

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Observation c42d6738-f96e-4ce7-a0d5-4c6c8e7e489d · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.830808Z

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Observation 6a324403-a595-4f5f-bccd-5155c5ae5e4b · outbound

This paper cites S., Forbes D.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? S., Forbes D

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.834145Z

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Observation 70c1c393-ea4d-43a3-8b1c-ab1224244ae7 · outbound

This paper cites E., Jones M.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? E., Jones M

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.838734Z

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Observation dedb0409-936a-464b-a52a-3ff659aa842f · outbound

This paper cites A., 2017, @doi [ ] 10.1093/mnrasl/slx148 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.472L.104F 472, L104.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., 2017, @doi [ ] 10.1093/mnrasl/slx148 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.472L.104F 472, L104

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.842408Z

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Observation 6d687a54-7170-49a7-a6ca-10319b333404 · outbound

This paper cites A., Gannon J., 2024, @doi [ ] 10.1093/mnras/stad4004 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.528..608F 528, 608.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., Gannon J., 2024, @doi [ ] 10.1093/mnras/stad4004 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.528..608F 528, 608

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.845944Z

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Observation f4927205-3917-464e-a6f1-a15b94805b6c · outbound

This paper cites A., et al., 2018a, @doi [Proceedings of the Royal Society of London Series A] 10.1098/rspa.2017.0616 , https://ui.adsabs.harvard.edu/abs/2018RSPSA.47470616F 474, 20170616.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., et al., 2018a, @doi [Proceedings of the Royal Society of London Series A] 10.1098/rspa.2017.0616 , https://ui.adsabs.harvard.edu/abs/2018RSPSA.47470616F 474, 20170616

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.849414Z

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Observation fd0c3277-f32c-4021-9a3d-550868cbd30b · outbound

This paper cites A., Read J.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., Read J

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.852986Z

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Observation 8a6828ae-32ee-4b2a-a2de-46adda8ad8f2 · outbound

This paper cites A., Alabi A., Romanowsky A.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., Alabi A., Romanowsky A

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.856411Z

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Observation 10d3f105-385a-490a-bae8-6ddfd7d4828d · outbound

This paper cites A., Gannon J.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., Gannon J

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.860450Z

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Observation 09c6ef7e-b68d-416d-a09e-d8c3817dc83a · outbound

This paper cites A., et al., 2023, @doi [ ] 10.1093/mnrasl/slad101 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.525L..93F 525, L93.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., et al., 2023, @doi [ ] 10.1093/mnrasl/slad101 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.525L..93F 525, L93

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.864492Z

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Observation d8cc13a7-5950-4736-81c2-32236b3fd31a · outbound

This paper cites Keck/KCWI Spectroscopy of Globular Clusters in Local Volume Dwarf Galaxies.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Keck/KCWI Spectroscopy of Globular Clusters in Local Volume Dwarf Galaxies

Reference 33

Resolution: metadata mismatch; local_arxiv, observed 2026-08-11T20:03:52.200431Z

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.

Observation 3d3e240d-ea90-4a24-82c5-8058a492dfc1 · outbound

This paper cites Primordial Rotating Disk Composed of $\geq$15 Dense Star-Forming Clumps at Cosmic Dawn.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Primordial Rotating Disk Composed of $\geq$15 Dense Star-Forming Clumps at Cosmic Dawn

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.872890Z

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Observation b25dc3df-efcc-4faa-a867-63f69b2cc4f6 · outbound

This paper cites S., Forbes D.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? S., Forbes D

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.877403Z

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Observation 9a5725f1-9eba-47bd-b38f-3f64facab50c · outbound

This paper cites S., et al., 2021, @doi [ ] 10.1093/mnras/stab277 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.3144G 502, 3144.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? S., et al., 2021, @doi [ ] 10.1093/mnras/stab277 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.3144G 502, 3144

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.881110Z

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Observation ec8b223c-39c1-4567-9cee-6a14c4203742 · outbound

This paper cites S., et al., 2022b, @doi [MNRAS] 10.1093/mnras/stab3297 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.510..946G 510, 946.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? S., et al., 2022b, @doi [MNRAS] 10.1093/mnras/stab3297 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.510..946G 510, 946

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.888454Z

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Observation a437c584-96eb-4abb-adf3-be021db0f594 · outbound

This paper cites S., Forbes D.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? S., Forbes D

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.891795Z

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Observation 5564f46d-66c5-4b64-8685-31b64a08a488 · outbound

This paper cites S., Ferr \'e -Mateu A., Forbes D.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? S., Ferr \'e -Mateu A., Forbes D

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.895233Z

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Observation 8280c39c-54bd-468c-8114-f866a384c2c9 · outbound

This paper cites Y., Puzia T.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Y., Puzia T

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.898703Z

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Observation 6e1ee900-b2f9-409a-89f7-fd0fcfb385e0 · outbound

This paper cites Y., Ostriker J.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Y., Ostriker J

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.905774Z

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Observation d4371183-eb45-4186-a1ce-1cce16ce0966 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.909313Z

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Observation a892b0d1-3b25-48a2-b1fc-5f098bc5bcfd · outbound

This paper cites E., Harris G.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? E., Harris G

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.912850Z

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Observation 01816e62-3b80-46bb-969e-8865ae81da60 · outbound

This paper cites E., Blakeslee J.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? E., Blakeslee J

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.917011Z

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Observation 4f3aa98f-7c03-4587-a538-ade01a4647e2 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.921641Z

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Observation bee28f98-fbcc-415b-91b6-303dc801b510 · outbound

This paper cites E., 2021, @doi [ ] 10.1093/mnras/staa3297 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.500..986H 500, 986.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? E., 2021, @doi [ ] 10.1093/mnras/staa3297 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.500..986H 500, 986

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.926023Z

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Observation f221188a-8e4a-44b7-9c3f-32982a68cdfe · outbound

This paper cites J., Robison B., 2018, @doi [ ] 10.1093/mnras/sty844 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.3869H 477, 3869.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? J., Robison B., 2018, @doi [ ] 10.1093/mnras/sty844 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.3869H 477, 3869

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.930364Z

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Observation 57cfba2c-7a31-4793-a4b5-bf5bec6e8f6a · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.934282Z

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Observation 976f4a12-1fea-442f-bfed-4197674f094e · outbound

This paper cites Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra-I cluster.I. Project description and preliminary results.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra-I cluster.I. Project description and preliminary results

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-08-11T20:03:52.033031Z

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.

Observation dfce7060-f625-401d-8f7c-4d9bd1c4543a · outbound

This paper cites R., Abraham R., Brodie J., Forbes D.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? R., Abraham R., Brodie J., Forbes D

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.942895Z

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Observation 5febb994-392a-45ed-9955-baf59188dd3b · outbound

This paper cites R., et al., 2022, @doi [ ] 10.1093/mnras/stac2717 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.517..858J 517, 858.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? R., et al., 2022, @doi [ ] 10.1093/mnras/stac2717 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.517..858J 517, 858

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.946754Z

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Observation 74e19ee8-7066-4a7e-a499-e1fbe7b0c1ef · outbound

This paper cites The PIPER Survey. II. The Globular Cluster Systems of Low Surface Brightness Galaxies in the Perseus Cluster.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? The PIPER Survey. II. The Globular Cluster Systems of Low Surface Brightness Galaxies in the Perseus Cluster

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.950498Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39845c04-c95c-489e-b76a-38d1f1406017 · outbound

This paper cites P., et al., 2021, @doi [ ] 10.3847/1538-4357/ac1869 , https://ui.adsabs.harvard.edu/abs/2021ApJ...921...32J 921, 32.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? P., et al., 2021, @doi [ ] 10.3847/1538-4357/ac1869 , https://ui.adsabs.harvard.edu/abs/2021ApJ...921...32J 921, 32

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.955655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02d569a8-0cc3-438b-9e92-edb41333c9e0 · outbound

This paper cites J., Dutton A.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? J., Dutton A

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.959177Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dd3e9b23-7ee4-49bf-9b3e-8a0fb3270265 · outbound

This paper cites G., et al., 2023, @doi [ ] 10.3847/2041-8213/acaaab , https://ui.adsabs.harvard.edu/abs/2023ApJ...942L...5J 942, L5.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? G., et al., 2023, @doi [ ] 10.3847/2041-8213/acaaab , https://ui.adsabs.harvard.edu/abs/2023ApJ...942L...5J 942, L5

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.964248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ca0cc537-db35-418a-bf2b-f3e35f14c501 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.968063Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d10f41ab-3283-4d7f-af95-22c4133c86a9 · outbound

This paper cites D., Makarova L.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? D., Makarova L

Reference 59

Resolution: verified exact; doi, observed 2026-08-11T20:03:51.918889Z

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.

Observation 8aa1b9f4-9c83-4aea-b794-bb63bdc4a7fb · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.976042Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f478705-3ac8-4a44-8254-7fc0011f636c · outbound

This paper cites Blowing out the Candle: How to Quench Galaxies at High Redshift -- an Ensemble of Rapid Starbursts, AGN Feedback and Environment.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Blowing out the Candle: How to Quench Galaxies at High Redshift -- an Ensemble of Rapid Starbursts, AGN Feedback and Environment

Reference 61

Resolution: metadata mismatch; local_arxiv, observed 2026-08-11T20:03:51.894027Z

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.

Observation eb9dcf64-dbb4-4954-bd6e-ece39eb1f0af · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.984213Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df08c1d2-f779-451a-af26-cc81a7fd4cb0 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.987945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4177c763-ba81-42b8-be16-15edb88fe2c7 · outbound

This paper cites S., Strader J., Brodie J.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? S., Strader J., Brodie J

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:50.991836Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 162a39ed-8c99-4aff-8362-7c6bb72c32db · outbound

This paper cites Constraints on mass loss of globular clusters in dwarf galaxies.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Constraints on mass loss of globular clusters in dwarf galaxies

Reference 65

Resolution: metadata mismatch; local_arxiv, observed 2026-08-11T20:03:51.849747Z

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.

Observation ba089a48-b94e-4a79-8727-98a84100407c · outbound

This paper cites Globular Cluster Counts around 700 Nearby Galaxies.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Globular Cluster Counts around 700 Nearby Galaxies

Reference 66

Resolution: verified exact; local_arxiv, observed 2026-08-11T20:03:51.821187Z

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.

Observation 956e7405-6e41-4504-8dee-d014c235fe89 · outbound

This paper cites K., Koch A., 2010, @doi [ ] 10.1051/0004-6361/200913364 , https://ui.adsabs.harvard.edu/abs/2010A&A...521A..43L 521, A43.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? K., Koch A., 2010, @doi [ ] 10.1051/0004-6361/200913364 , https://ui.adsabs.harvard.edu/abs/2010A&A...521A..43L 521, A43

Reference 67

Resolution: verified exact; doi, observed 2026-08-11T20:03:51.802968Z

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.

Observation 9128410d-77c4-47c9-aef0-ec1481dcc76a · outbound

This paper cites W., C \^o t \'e P., Sales L.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? W., C \^o t \'e P., Sales L

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.007463Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b9fa053-ca99-4c93-b7c8-87c47efe4c5b · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.010671Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2c233485-6cbb-4cba-884e-451462599da0 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.014132Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a9c66466-3327-4546-9307-68b92d787631 · outbound

This paper cites F., et al., 2016, @doi [ApJ] 10.3847/1538-4357/833/2/167 , https://ui.adsabs.harvard.edu/abs/2016ApJ...833..167M 833, 167.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? F., et al., 2016, @doi [ApJ] 10.3847/1538-4357/833/2/167 , https://ui.adsabs.harvard.edu/abs/2016ApJ...833..167M 833, 167

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.017620Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 99768fc4-f1fa-4132-ba08-766dd3cc9bb1 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.020909Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 60d8afc7-5b86-4468-a10a-54d269c17465 · outbound

This paper cites W., 2012, @doi [AJ] 10.1088/0004-6256/144/1/4 , https://ui.adsabs.harvard.edu/abs/2012AJ....144....4M 144, 4.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? W., 2012, @doi [AJ] 10.1088/0004-6256/144/1/4 , https://ui.adsabs.harvard.edu/abs/2012AJ....144....4M 144, 4

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.024833Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c620205c-4ea6-46b9-96e0-a17fab9b1155 · outbound

This paper cites C., et al., 2022, @doi [ApJ] 10.3847/1538-4357/ac35d9 , https://ui.adsabs.harvard.edu/abs/2022ApJ...924...87M 924, 87.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? C., et al., 2022, @doi [ApJ] 10.3847/1538-4357/ac35d9 , https://ui.adsabs.harvard.edu/abs/2022ApJ...924...87M 924, 87

Reference 74

Resolution: verified exact; doi, observed 2026-08-11T20:03:51.717736Z

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.

Observation ffc61bfb-d785-48b4-b61e-87f0c8ac29be · outbound

This paper cites A., et al., 2016, @doi [ ] 10.1093/mnras/stv2435 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.455.2323M 455, 2323.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., et al., 2016, @doi [ ] 10.1093/mnras/stv2435 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.455.2323M 455, 2323

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.033739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d21e437d-6bab-4151-88da-80155075a836 · outbound

This paper cites A., Li H., Souza S.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., Li H., Souza S

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.038877Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3d108304-a9c2-40ae-ba26-8eed748846c1 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.043067Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3c7721d-6be4-49bf-9196-2ff259f146a5 · outbound

This paper cites The Firefly Sparkle: The Earliest Stages of the Assembly of A Milky Way-type Galaxy in a 600 Myr Old Universe.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? The Firefly Sparkle: The Earliest Stages of the Assembly of A Milky Way-type Galaxy in a 600 Myr Old Universe

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.048044Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f0a7690e-ad74-438c-afee-8027d331080a · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.052687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e91d9f00-bcfa-45b1-830d-10f7a653905e · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.056089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f57d1a38-ab92-4090-8e59-f2f713e96664 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.059386Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 99d97fea-f8fb-4f1f-a139-0c47594ee66e · outbound

This paper cites C., Springel V., van de Voort F., 2023, @doi [ ] 10.1093/mnras/stac3776 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.520.2692P 520, 2692.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? C., Springel V., van de Voort F., 2023, @doi [ ] 10.1093/mnras/stac3776 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.520.2692P 520, 2692

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.062448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5b20739b-f28c-4622-9f8f-cac08bf1d8d9 · outbound

This paper cites W., Lim S., 2016, @doi [ ] 10.3847/2041-8205/822/2/L31 , https://ui.adsabs.harvard.edu/abs/2016ApJ...822L..31P 822, L31.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? W., Lim S., 2016, @doi [ ] 10.3847/2041-8205/822/2/L31 , https://ui.adsabs.harvard.edu/abs/2016ApJ...822L..31P 822, L31

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.066071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e468248-1876-448b-a79d-31bbb24f3d0d · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.069304Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bb58a809-a2a6-417a-885e-d0000d04a08c · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.072377Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5b64b43a-f94d-4722-b272-0914294dcde2 · outbound

This paper cites J., van der Burg R.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? J., van der Burg R

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.075606Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0387a489-d2b9-47fe-a176-be5b4b782dad · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.079224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d6e7ee5e-d3b9-4949-b5e4-244b18ec2919 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.082919Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 87f6620a-35c7-4e7c-a80b-60f992642eee · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.086661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f0a1a3e-e600-4b11-be2c-954e8ba89102 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.090310Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3bfbc39e-43dc-4df0-a546-17cee0948f43 · outbound

This paper cites F., Knapen J.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? F., Knapen J

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.094391Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88ec1588-c8c4-4f6c-a3bd-d4381f281360 · outbound

This paper cites P., et al., 2017, @doi [ ] 10.1093/mnras/stw2162 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.465..501S 465, 501.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? P., et al., 2017, @doi [ ] 10.1093/mnras/stw2162 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.465..501S 465, 501

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.098130Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3752658f-2c6f-435e-8b78-8642e530b50a · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.101945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 40844660-aa03-409d-b7ca-99d992f33bfc · outbound

This paper cites Confirmation of an anomalously low dark matter content for the galaxy NGC1052-DF4 from deep, high resolution continuum spectroscopy.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Confirmation of an anomalously low dark matter content for the galaxy NGC1052-DF4 from deep, high resolution continuum spectroscopy

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.106081Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation da8deb34-5831-471e-9e54-18ac876248df · outbound

This paper cites D., 2019, @doi [ ] 10.1146/annurev-astro-091918-104453 , https://ui.adsabs.harvard.edu/abs/2019ARA&A..57..375S 57, 375.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? D., 2019, @doi [ ] 10.1146/annurev-astro-091918-104453 , https://ui.adsabs.harvard.edu/abs/2019ARA&A..57..375S 57, 375

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.109358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e91fa2f7-5d63-459d-b1ef-f75cd1072b5f · outbound

This paper cites R., Forbes D.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? R., Forbes D

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.112479Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c2c898be-4810-48f8-adb7-465f02be986e · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.115542Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c8dc9bb-95f4-41e3-a83f-350629628f1b · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.118743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b5a81e3f-e0be-4793-8e10-8b42374ecca2 · outbound

This paper cites W., et al., 2024, @doi [ ] 10.1093/mnras/stae682 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.529.3301T 529, 3301.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? W., et al., 2024, @doi [ ] 10.1093/mnras/stae682 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.529.3301T 529, 3301

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.122584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e70bf740-a6ae-4842-9299-f852eaab6901 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.125885Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75ea52da-6b2c-4b18-aa0a-f035522a98fc · outbound

This paper cites M., Moster B.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? M., Moster B

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.128914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fcdf3a90-bf31-4b74-ae10-9f61488ddee7 · outbound

This paper cites an unresolved cited work.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Unresolved cited work

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.132577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bc8c9566-76fd-4a74-94d5-961c7bcbd60d · outbound

This paper cites A., et al., 2022, @doi [MNRAS] 10.1093/mnras/stac2417 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.516.3318W 516, 3318.

Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? A., et al., 2022, @doi [MNRAS] 10.1093/mnras/stac2417 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.516.3318W 516, 3318

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-11T20:03:51.136801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Coverage vector

Reference resolution

Outbound references

Pith citing papers