no code implementations • 4 Jul 2019 • Chirag Modi, Martin White, Anze Slosar, Emanuele Castorina
For redshifts $z=2$ and 4, we are able to reconstruct 21cm field with cross correlation, $r_c > 0. 8$ on all scales for both our optimistic and pessimistic assumptions about foreground contamination and for different levels of thermal noise.
Cosmology and Nongalactic Astrophysics
3 code implementations • 14 Dec 2018 • Nora Elisa Chisari, David Alonso, Elisabeth Krause, C. Danielle Leonard, Philip Bull, Jérémy Neveu, Antonio Villarreal, Sukhdeep Singh, Thomas McClintock, John Ellison, Zilong Du, Joe Zuntz, Alexander Mead, Shahab Joudaki, Christiane S. Lorenz, Tilman Troester, Javier Sanchez, Francois Lanusse, Mustapha Ishak, Renée Hlozek, Jonathan Blazek, Jean-Eric Campagne, Husni Almoubayyed, Tim Eifler, Matthew Kirby, David Kirkby, Stéphane Plaszczynski, Anze Slosar, Michal Vrastil, Erika L. Wagoner
As a result, predictions for correlation functions of galaxy clustering, galaxy-galaxy lensing and cosmic shear are demonstrated to be within a fraction of the expected statistical uncertainty of the observables for the models and in the range of scales of interest to LSST.
Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics