Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments | Paper Citation Record

Observation 75578818-7d8e-4066-889d-d026ca486dd9 · outbound

This paper cites , " * write output.state after.block = add.period write newline.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments , " * write output.state after.block = add.period write newline

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments write newline

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Is Gvwwlx'v[< EQdmmM4M UUʕ+m4HXt: ,8R֭[ ^nuu] 8v]וv-V߮ʵkפV CbJpcVJT[(r s mh4D?F & ih4DUU)Jp 8!

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

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This paper cites M., Lim , P.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments M., Lim , P

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This paper cites M., Lim , S., D'Eugenio , F., et al.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments M., Lim , S., D'Eugenio , F., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments J., Cullen , F., et al

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This paper cites H., Hearin , A.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments H., Hearin , A

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This paper cites S., Conroy, C., & Wechsler, R.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments S., Conroy, C., & Wechsler, R

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This paper cites S., Wechsler , R.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments S., Wechsler , R

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2000, , 545, 6, 10.1086/317788

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments K., Somerville , R

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., McLure , R

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., McLeod , D

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., McLure , R

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., Cullen , F., McLure , R

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2024, , 633, 318, 10.1038/s41586-024-07860-9

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments K., Lin , Y.-T., Ho , S., & Genel , S

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2023, , 944, 207, 10.3847/1538-4357/acb5f3

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments E., & White , M

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

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This paper cites 2011, MNRAS, 413, 2087, 10.1111/j.1365-2966.2011.18286.x.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2011, MNRAS, 413, 2087, 10.1111/j.1365-2966.2011.18286.x

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments J., Brammer , G., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2025 b , , 697, A189, 10.1051/0004-6361/202452186

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This paper cites C., Birnboim , Y., Mandelker , N., & Li , Z.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., Birnboim , Y., Mandelker , N., & Li , Z

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2024, The CANDELS-Area Prism Epoch of Reionization Survey (CAPERS) , JWST Proposal

Reference 26

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This paper cites P., Whitler , L., et al.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments P., Whitler , L., et al

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This paper cites The Case for a James Webb Space Telescope Extragalactic Key Project.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments The Case for a James Webb Space Telescope Extragalactic Key Project

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments L., Song, M., Behroozi, P., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments S., White , S

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2024, , 628, 277, 10.1038/s41586-024-07191-9

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments R., Millman, K

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments E., Watson , D., Brammer , G., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments G., Angeloudi , E., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2024, , 964, 192, 10.3847/1538-4357/ad2512

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2025, , 697, A111, 10.1051/0004-6361/202453211

Reference 39

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments The Spectral Energy Distributions of Galaxies

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments K., Cranmer , M., Melchior , P., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments The Optical and Infrared Are Connected

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments K., Steinhardt , C

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments B., Magdis , G

Reference 45

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2016, in Positioning and Power in Academic Publishing: Players, Agents and Agendas, ed

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., Harrison , I., Harikane , Y., Tacchella , S., & Wilkins , S

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., Thomas , P

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., Vijayan, A

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 1984, The postmodern condition: A report on knowledge, Vol

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments A., Trenti , M., & Treu , T

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2025, , 982, 153, 10.3847/1538-4357/adb30f

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments P., Somerville , R

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2024, Scientific Reports, 14, 3724, 10.1038/s41598-024-52585-4

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments M., Hawkins , E., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Much Ado About Nothing: Galaxy Formation and Galactic Outflows in Cosmic Voids

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments J., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2020, , 641, A6, 10.1051/0004-6361/201833910

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2018, , 618, A85, 10.1051/0004-6361/201833070

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Observation b3a7c8c3-6dba-4202-b0fc-53b8f354c33b · outbound

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments J., Gavazzi , R., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2025, , 695, A20, 10.1051/0004-6361/202452570

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Observation 2711afc2-0ccb-4e8c-9e37-3cd1ad92bc3e · outbound

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments L., Capak, P., Masters, D., & Speagle, J

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This paper cites L., Jespersen , C.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments L., Jespersen , C

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments L., Kokorev , V., Rusakov , V., Garcia , E., & Sneppen , A

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Observation efaafad2-aebb-4272-9f41-12611e3a9f63 · outbound

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments A., Lovell , C

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This paper cites 2008, ApJ, 676, 767, 10.1086/528674.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2008, ApJ, 676, 767, 10.1086/528674

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

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Observation 741cb8cc-60e1-4120-b470-f1a7a21dc9d1 · outbound

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Gas outflows in two recently quenched galaxies at z = 4 and 7

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments E., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2010, , 401, 35, 10.1111/j.1365-2966.2009.15709.x

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Observation d8ea02dc-5711-4e00-821f-02ade2a21a62 · outbound

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments R., Davidzon , I., Toft , S., et al

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments 2010, in P roceedings of the 9th P ython in S cience C onference, ed

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Observation 70b9c43c-d892-4df6-a698-fe83b7b28b85 · outbound

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments C., Oesch , P

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Observation 65da8ad9-05df-4e69-97d8-cfc342fbfe38 · outbound

This paper cites Learning the galaxy-environment connection with graph neural networks.

Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Learning the galaxy-environment connection with graph neural networks

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments F., Jespersen , C

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

Reference 78

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Explaining ultra-massive quiescent galaxies at $3 < z < 5$ in the context of their environments Unresolved cited work

Reference 79

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