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Case Study 3

Beecroft Institute of Particle Astrophysics

and Cosmology University of Oxford

and Department of Physics and Astronomy

and Space Physics at the University of Uppsala

d a r k   m a t t e r  

c o s m o l o g y


by Artemi-Maria Gioti

at DA TA rush, Vienna 2015

A transposition of galaxy clusters into “arpeggiated” piano clusters where the pitch range and duration are determined by their mass. The luminosity of the galaxy clusters is mapped to the maximum velocity with which the piano keys are hit, while their distance from the earth is used to determine the register of the piano clusters.