The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies (2021)
- Authors:
- Autor USP: DORTA, ANTONIO DAVID MONTERO - IF
- Unidade: IF
- DOI: 10.1093/mnras/stab1571
- Subjects: COSMOLOGIA; GALÁXIAS; ESTRUTURA DO UNIVERSO; MÉTODOS NUMÉRICOS
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 1365-2966
- Volume/Número/Paginação/Ano: v. 505, n. 3, p. 3192-3205, Agosto de 2021
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
RODRIGUEZ, Facundo et al. The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies. Monthly Notices of the Royal Astronomical Society, v. 505, n. 3, p. 3192-3205, 2021Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab1571. Acesso em: 28 fev. 2026. -
APA
Rodriguez, F., Montero-Dorta, A. D., Angulo, R. E., Artale, M. C., & Merchán, M. (2021). The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies. Monthly Notices of the Royal Astronomical Society, 505( 3), 3192-3205. doi:10.1093/mnras/stab1571 -
NLM
Rodriguez F, Montero-Dorta AD, Angulo RE, Artale MC, Merchán M. The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 505( 3): 3192-3205.[citado 2026 fev. 28 ] Available from: https://doi.org/10.1093/mnras/stab1571 -
Vancouver
Rodriguez F, Montero-Dorta AD, Angulo RE, Artale MC, Merchán M. The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 505( 3): 3192-3205.[citado 2026 fev. 28 ] Available from: https://doi.org/10.1093/mnras/stab1571 - Rest-frame UV properties of luminous strong gravitationally lensed Lyαemitters from the BELLS GALLERY Survey
- [O II] emitters in MultiDark-Galaxies and DEEP2
- Subhalo abundance matching through the lens of a hydrodynamical simulation
- The large-scale distribution of ionized metals in IllustrisTNG
- A semi-analytical perspective on massive galaxies at z ∼ 0.55
- Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
- The multi-tracer optimal estimator applied to VIPERS
- The dependence of halo bias on age, concentration, and spin
- On the kinetic Sunyaev–Zel’dovich effect as an observational probe for halo spin bias
- The physical origins of low-mass spin bias
Informações sobre o DOI: 10.1093/mnras/stab1571 (Fonte: oaDOI API)
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