Modelling baryonic feedback for survey cosmology
Observational cosmology in the next decade will rely on probes of the distribution of matter in the redshift range between 0<z<3 to elucidate the nature of dark matter and dark energy. In this redshift range, galaxy formation is known to have a significant impact on observables such as two-poi...
Հիմնական հեղինակներ: | , , , , , , , , , , , , |
---|---|
Ձևաչափ: | Հոդված |
Լեզու: | English |
Հրապարակվել է: |
Maynooth Academic Publishing
2019-06-01
|
Շարք: | The Open Journal of Astrophysics |
Առցանց հասանելիություն: | https://doi.org/10.21105/astro.1905.06082 |