Paper Citation Record · LEDGER

Galaxy Morphology Classification: Are Stellar Circularities Enough?

As of 10 August 2026, this Paper Citation Record lists 37 of 37 outbound references and 0 inbound Pith citation observations for arXiv:2506.20002.

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

pith.paper-citation-record.v1
2506.20002 v1

Coverage vector

measured 37 of 37 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-06T23:03:44.134131Z

measured 37 of 37 standing notices

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

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

37 of 37 outbound references displayed

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External citation measurements

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Outbound references

Observation 7a689109-5ce1-459a-a184-d50e7cb3fb4e · outbound

This paper cites an unresolved cited work.

Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 1

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This paper cites an unresolved cited work.

Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 2

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This paper cites an unresolved cited work.

Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 3

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Observation 734a47d2-a2f1-4706-a849-217e6211cb76 · outbound

This paper cites C., Debattista, V.

Galaxy Morphology Classification: Are Stellar Circularities Enough? C., Debattista, V

Reference 4

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Observation 3688143c-f45e-4670-95fe-665b893903aa · outbound

This paper cites C., Zhao, D., et al.

Galaxy Morphology Classification: Are Stellar Circularities Enough? C., Zhao, D., et al

Reference 5

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Observation f792cd9a-49b4-4e04-a2fd-d6f4b718ca62 · outbound

This paper cites A statistical study of lopsided galaxies using random forest.

Galaxy Morphology Classification: Are Stellar Circularities Enough? A statistical study of lopsided galaxies using random forest

Reference 6

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Observation 2c0d8843-68e2-41c4-a879-0ee49fffcf32 · outbound

This paper cites M., Hernquist, L., et al.

Galaxy Morphology Classification: Are Stellar Circularities Enough? M., Hernquist, L., et al

Reference 7

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Observation d3721e91-09b6-4cf4-ba90-d249246615b9 · outbound

This paper cites Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations.

Galaxy Morphology Classification: Are Stellar Circularities Enough? Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations

Reference 8

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This paper cites R., Millman, K.

Galaxy Morphology Classification: Are Stellar Circularities Enough? R., Millman, K

Reference 9

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This paper cites an unresolved cited work.

Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 10

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Observation a3f3d8e0-8fc8-447b-ade6-e1ba601544ee · outbound

This paper cites 2019, MNRAS, 489, 1859.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2019, MNRAS, 489, 1859

Reference 11

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Observation 5e892eee-b4e9-4f80-9398-bae564ab1cb2 · outbound

This paper cites an unresolved cited work.

Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 12

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Observation 61d2e09f-0bb1-4336-b5ca-707ef0db3388 · outbound

This paper cites D., Pillepich, A., Nelson, D., et al.

Galaxy Morphology Classification: Are Stellar Circularities Enough? D., Pillepich, A., Nelson, D., et al

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T23:03:49.574095Z

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Observation 03ef7fd1-0261-450c-802d-6b176d5d6e43 · outbound

This paper cites and Kennicutt, Robert C., J.

Galaxy Morphology Classification: Are Stellar Circularities Enough? and Kennicutt, Robert C., J

Reference 14

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Observation 574fc651-4fdb-473d-9a49-4a19f4ecf063 · outbound

This paper cites 2018, MNRAS, 480, 5113.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2018, MNRAS, 480, 5113

Reference 15

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Observation a26d0288-0833-4baa-b9cd-bf5928344cb4 · outbound

This paper cites A., Morgan, W.

Galaxy Morphology Classification: Are Stellar Circularities Enough? A., Morgan, W

Reference 16

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Observation 4575852e-9cf3-44c4-bb27-e26d50481740 · outbound

This paper cites C., and White, S.

Galaxy Morphology Classification: Are Stellar Circularities Enough? C., and White, S

Reference 17

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Observation 352ee3f1-b9de-47d4-bb9d-262e76cd51c7 · outbound

This paper cites V., Dalal, N., and Gottl¨ ober, S.

Galaxy Morphology Classification: Are Stellar Circularities Enough? V., Dalal, N., and Gottl¨ ober, S

Reference 18

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Observation 822d3f34-434e-497b-98d7-6264d4a94a7b · outbound

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Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 19

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Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 20

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This paper cites P., Pillepich, A., Springel, V., et al.

Galaxy Morphology Classification: Are Stellar Circularities Enough? P., Pillepich, A., Springel, V., et al

Reference 21

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Observation 4879c654-9f54-4973-b32c-eb7a43315e6d · outbound

This paper cites 2018, MN- RAS, 475, 624.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2018, MN- RAS, 475, 624

Reference 22

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Observation 1365a34a-f0f2-45f2-85d8-44d02ef650ba · outbound

This paper cites J., et al.

Galaxy Morphology Classification: Are Stellar Circularities Enough? J., et al

Reference 23

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Observation 8c691795-bd6c-4c15-ad2a-993f95115408 · outbound

This paper cites S., Gupta, P., and Kumar, H.

Galaxy Morphology Classification: Are Stellar Circularities Enough? S., Gupta, P., and Kumar, H

Reference 24

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This paper cites K., Bekki, K., et al.

Galaxy Morphology Classification: Are Stellar Circularities Enough? K., Bekki, K., et al

Reference 25

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Observation d8d79528-a483-48c4-98d8-adc722a6a505 · outbound

This paper cites 2019, MN- RAS, 490, 3196.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2019, MN- RAS, 490, 3196

Reference 26

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Observation ec30fa20-3cca-45d6-9343-18a4ca335a5e · outbound

This paper cites 2018b, MN- RAS, 473, 4077 Planck Collaboration, Ade, P.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2018b, MN- RAS, 473, 4077 Planck Collaboration, Ade, P

Reference 27

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Observation 504ba18e-8fe2-45c8-a918-853905dfe8ae · outbound

This paper cites F., Lotz, J.

Galaxy Morphology Classification: Are Stellar Circularities Enough? F., Lotz, J

Reference 28

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Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 29

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Observation 5d64f6ed-8036-45c9-9fe1-e2ba867bab02 · outbound

This paper cites 2010, MNRAS, 401, 791.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2010, MNRAS, 401, 791

Reference 30

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This paper cites and Hernquist, L.

Galaxy Morphology Classification: Are Stellar Circularities Enough? and Hernquist, L

Reference 31

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Observation 332c39d3-3331-40e5-b3d5-31a1acd53b9b · outbound

This paper cites 2018, MN- RAS, 475, 676.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2018, MN- RAS, 475, 676

Reference 32

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This paper cites 2022, MNRAS, 509, 2654.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2022, MNRAS, 509, 2654

Reference 33

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This paper cites 2020, Nature Reviews Physics, 2, 42.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2020, Nature Reviews Physics, 2, 42

Reference 34

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Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 35

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Observation b178c5dd-89f1-407c-b4b2-7b45611ba41b · outbound

This paper cites 2017, MNRAS, 465, 3291 Wes McKinney.

Galaxy Morphology Classification: Are Stellar Circularities Enough? 2017, MNRAS, 465, 3291 Wes McKinney

Reference 36

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This paper cites an unresolved cited work.

Galaxy Morphology Classification: Are Stellar Circularities Enough? Unresolved cited work

Reference 37

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Pith citing papers

No inbound Pith citation observations are available.