Dissecting a miniature universe: A multi-wavelength view of galaxy quenching in the Shapley supercluster

Open Access

Table 1

Spearman correlation coefficients relating the Compton y to SFR (upper part of the Table (Fig. 9)) and the Compton y to galaxy number density (lower part of the Table (Fig. 10)) for the full range of y-values and for ŷ_q < log y < ŷ_inner (with ŷ_q = log y_q = −5.46 and ŷ_inner = log y_inner = −4.96).

log y versus SFR
y range	Star-forming	Transitioning	Passive
log y > −7	0.08	−0.06	−0.07
ŷ_q < log y < ŷ_inner	0.25	−0.12	−0.3

log y versus number density
y range	Star-forming	Transitioning	Passive

log y > −7	−0.37	0.23	0.36
ŷ_q < log y < ŷ_inner	−0.45	0.21	0.48

Notes. All p values were found to be smaller than 10⁻⁶.

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