Transpositions [TP]:
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
XMM_Newton
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.