The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z similar to 5

L. Legrand; H. J. McCracken; I. Davidzon; O. Ilbert; J. Coupon; N. Aghanim; M. Douspis; P. L. Capak; O. Le Fevre; B. Milvang-Jensen

doi:10.1093/mnras/stz1198

The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z similar to 5

L. Legrand, H. J. McCracken, I. Davidzon, O. Ilbert, J. Coupon, N. Aghanim, M. Douspis, P. L. Capak, O. Le Fevre, B. Milvang-Jensen

The Cosmic Dawn Center

12 Citations (Scopus)

Original language	English
Journal	Monthly Notices of the Royal Astronomical Society
Volume	486
Issue number	4
Pages (from-to)	5468-5481
ISSN	0035-8711
DOIs	https://doi.org/10.1093/mnras/stz1198
Publication status	Published - 1 Jul 2019

Keywords

methods: statistical
galaxies: evolution
galaxies: haloes

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Legrand, L., McCracken, H. J., Davidzon, I., Ilbert, O., Coupon, J., Aghanim, N., Douspis, M., Capak, P. L., Le Fevre, O., & Milvang-Jensen, B. (2019). The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z similar to 5. Monthly Notices of the Royal Astronomical Society, 486(4), 5468-5481. https://doi.org/10.1093/mnras/stz1198

Legrand, L, McCracken, HJ, Davidzon, I, Ilbert, O, Coupon, J, Aghanim, N, Douspis, M, Capak, PL, Le Fevre, O & Milvang-Jensen, B 2019, 'The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z similar to 5', Monthly Notices of the Royal Astronomical Society, vol. 486, no. 4, pp. 5468-5481. https://doi.org/10.1093/mnras/stz1198

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author = "L. Legrand and McCracken, {H. J.} and I. Davidzon and O. Ilbert and J. Coupon and N. Aghanim and M. Douspis and Capak, {P. L.} and {Le Fevre}, O. and B. Milvang-Jensen",

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AU - McCracken, H. J.

AU - Davidzon, I.

AU - Ilbert, O.

AU - Coupon, J.

AU - Aghanim, N.

AU - Douspis, M.

AU - Capak, P. L.

AU - Le Fevre, O.

AU - Milvang-Jensen, B.

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The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z similar to 5

Keywords

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