The SunyaevβZeldovich (SZ) effect is a distortion of the cosmic microwave background radiation caused by inverseβCompton scattering of CMB photons off hot electrons in the intracluster medium of galaxy clusters.
By measuring the integrated Comptonβy parameter, Y_SZ, and combining it with the angularβdiameter distance to the cluster, astronomers can estimate the total mass of the cluster within a given overdensity radius (e.g., M_500).
The calculator below lets you input the observed Y_SZ, the cluster redshift, and the assumed cosmology to obtain an estimate of M_500, useful for comparing with Xβray or lensing mass measurements.
What is the Sunyaev-Zeldovich effect?
How does this calculator estimate cluster mass?
What is M_500 in this context?
What units are used for Y_SZ and D_A?
Can this calculator be used for any galaxy cluster?
What is the significance of the constant C in the formula?
How accurate are these mass estimates?
Results are for informational purposes only and do not constitute professional advice.
