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438 results: 437 articles and 1 books or book chapters

1. 201 Resolved galactic superwinds reconstructed around their host galaxies at z > 3
   M. C. Chen, H. -W. Chen, M. Gronke, M. Rauch, and T. Broadhurst
   Mon. Not. Roy. Astron. Soc. 504, 2629 (2021).
2. 202 Impact of astrophysical binary coalescence time-scales on the rate of lensed gravitational wave events
   S. Mukherjee, T. Broadhurst, J. M. Diego, J. Silk, and G. F. Smoot
   Mon. Not. Roy. Astron. Soc. 506, 3751 (2021).
3. 203 Redshift-space effects in voids and their impact on cosmological tests. Part I: the void size function
   C. M. Correa, D. J. Paz, A. G. Sanchez, A. N. Ruiz, N. D. Padilla, and R. E. Angulo
   Mon. Not. Roy. Astron. Soc. 500, 911 (2021).
4. 204 Predicting halo occupation and galaxy assembly bias with machine learning
   X. Xu, S. Kumar, I. Zehavi, and S. Contreras
   Mon. Not. Roy. Astron. Soc. 507, 4879 (2021).
5. 205 Surrogate modelling the Baryonic Universe II: On forward modelling the colours of individual and populations of galaxies
   J. Chaves-Montero, and A. Hearin
   Mon. Not. Roy. Astron. Soc. 506, 2373 (2021).
6. 206 Tomographic constraints on gravity from angular redshift fluctuations in the late Universe
   C. Hernandez-Monteagudo, J. Chaves-Montero, R. E. Angulo, and G. Arico
   Mon. Not. Roy. Astron. Soc. 503, L62 (2021).
7. 207 Measuring the tidal response of structure formation: anisotropic separate universe simulations using TREEPM
   J. Stucker, A. S. Schmidt, S. D. M. White, F. Schmidt, and O. Hahn
   Mon. Not. Roy. Astron. Soc. 503, 1473 (2021).
8. 208 The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5 (vol 474, pg 4024, 2018)
   V. Gonzalez-Perez, J. Comparat, P. Norberg, C. M. Baugh, S. Contreras, C. Lacey, N. McCullagh, A. Orsi, J. Helly, and J. Humphries
   Mon. Not. Roy. Astron. Soc. 503, 28 (2021).
9. 209 Wave dark matter and ultra-diffuse galaxies
   A. Pozo, T. Broadhurst, I. de Martino, H. N. Luu, G. F. Smoot, J. Lim, and M. Neyrinck
   Mon. Not. Roy. Astron. Soc. 504, 2868 (2021).
10. 210 The galaxy size-halo mass scaling relations and clustering properties of central and satellite galaxies
    F. Rodriguez, A. D. Montero-Dorta, R. E. Angulo, M. Celeste Artale, and M. Merchan
    Mon. Not. Roy. Astron. Soc. 505, 3192 (2021).
11. 211 Exploring the role of binarity in the origin of the bimodal rotational velocity distribution in stellar clusters
    S. Kamann, N. Bastian, C. Usher, I. Cabrera-Ziri, and S. Saracino
    Mon. Not. Roy. Astron. Soc. 508, 2302 (2021).
12. 212 Intergalactic filaments spin
    Q. Xia, M. C. Neyrinck, Y. -C. Cai, and M. A. Aragon-Calvo
    Mon. Not. Roy. Astron. Soc. 506, 1059 (2021).
13. 213 The BACCO simulation project: a baryonification emulator with neural networks
    G. Arico, R. E. Angulo, S. Contreras, L. Ondaro-Mallea, M. Pellejero-Ibanez, and M. Zennaro
    Mon. Not. Roy. Astron. Soc. 506, 4070 (2021).
14. 214 Dissecting and modelling galaxy assembly bias
    X. Xu, I. Zehavi, and S. Contreras
    Mon. Not. Roy. Astron. Soc. 502, 3242 (2021).
15. 215 The BACCO simulation project: exploiting the full power of large-scale structure for cosmology
    R. E. Angulo, M. Zennaro, S. Contreras, G. Arico, M. Pellejero-Ibanez, and J. Stucker
    Mon. Not. Roy. Astron. Soc. 507, 5869 (2021).
16. 216 The boosted potential
    J. Stucker, R. E. Angulo, and P. Busch
    Mon. Not. Roy. Astron. Soc. 508, 5196 (2021).
17. 217 Density weighted angular redshift fluctuations: a new cosmological observable
    C. Hernandez-Monteagudo, J. Chaves-Montero, and R. E. Angulo
    Mon. Not. Roy. Astron. Soc. 503, L56 (2021).
18. 218 A flexible modelling of galaxy assembly bias
    S. Contreras, R. E. Angulo, and M. Zennaro
    Mon. Not. Roy. Astron. Soc. 504, 5205 (2021).
19. 219 A flexible subhalo abundance matching model for galaxy clustering in redshift space
    S. Contreras, R. E. Angulo, and M. Zennaro
    Mon. Not. Roy. Astron. Soc. 508, 175 (2021).
20. 220 The cosmological dependence of halo and galaxy assembly bias
    S. Contreras, J. Chaves-Montero, M. Zennaro, and R. E. Angulo
    Mon. Not. Roy. Astron. Soc. 507, 3412 (2021).