Construction of the reachability region with regard to the attitude motion of a descent module at reentry with near-circular velocity

2014 ◽  
Vol 53 (1) ◽  
pp. 137-148 ◽  
Author(s):  
S. N. Evdokimov ◽  
S. I. Klimanov ◽  
A. N. Korchagin ◽  
E. A. Mikrin ◽  
Yu. G. Sikharulidze
2020 ◽  
Vol 499 (4) ◽  
pp. 4905-4917
Author(s):  
S Contreras ◽  
R E Angulo ◽  
M Zennaro ◽  
G Aricò ◽  
M Pellejero-Ibañez

ABSTRACT Predicting the spatial distribution of objects as a function of cosmology is an essential ingredient for the exploitation of future galaxy surveys. In this paper, we show that a specially designed suite of gravity-only simulations together with cosmology-rescaling algorithms can provide the clustering of dark matter, haloes, and subhaloes with high precision. Specifically, with only three N-body simulations, we obtain the power spectrum of dark matter at z = 0 and 1 to better than 3 per cent precision for essentially all currently viable values of eight cosmological parameters, including massive neutrinos and dynamical dark energy, and over the whole range of scales explored, 0.03 < $k/{h}^{-1}\, {\rm Mpc}^{-1}$ < 5. This precision holds at the same level for mass-selected haloes and for subhaloes selected according to their peak maximum circular velocity. As an initial application of these predictions, we successfully constrain Ωm, σ8, and the scatter in subhalo-abundance-matching employing the projected correlation function of mock SDSS galaxies.


1997 ◽  
Author(s):  
J. Cochran, Jr. ◽  
Y. Cheng ◽  
S. Cho ◽  
S. Yoon ◽  
J. Cochran, Jr. ◽  
...  
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