Characterizing the SPT cluster selection function ...
Sunyaev-Zel'dovich Effect (SZE) experiments such as the South Pole Telescope (SPT) are currently surveying a large area of sky searching for clusters via their imprint on the CMB. In order to use the resulting cluster catalogues for cosmology, it is necessary to know the mass- and redshift-depe...
Format: | Article in Journal/Newspaper |
---|---|
Language: | English |
Published: |
Perimeter Institute
2009
|
Subjects: | |
Online Access: | https://dx.doi.org/10.48660/09040040 https://pirsa.org/09040040 |
Summary: | Sunyaev-Zel'dovich Effect (SZE) experiments such as the South Pole Telescope (SPT) are currently surveying a large area of sky searching for clusters via their imprint on the CMB. In order to use the resulting cluster catalogues for cosmology, it is necessary to know the mass- and redshift-dependent cluster selection function. I will describe ongoing work to understand and characterize the current SPT cluster yield, using synthetic SZ sky maps constructed from cosmological simulations and noise models calibrated against SPT data. ... |
---|