Table 4: Parameters of the statistical tests applied to our sample galaxies in comparison with normal ones (see text). Columns labeled P() represents the probability that the observed differences are statistically significants.
Tracer Type $\chi^2$ k P( $\chi^2$ ) P(T-test) P(F-test)

Dust
Early 13.39 5 98.0% 95.9% 24.2%

Dust Late 8.29 9 49.5% 94.9% 93.4%

Dust Sab-Sd - - - 84.6% 95.6%

HI Early 16.58 5 99.5% 98.7% 54.6%

HI Late 5.25 9 18.8% 49.3% 67.5%

mol Early 19.47 4 99.9% 2.7% 65.4%

mol Late 21.34 9 98.9% 94.5% 29.2%

X-ray Early 14.95 5 99.0% 97.6% 37.3%

X-ray Late 47.26 9 100.0% 99.5% 63.3%

**Table 4:** Parameters of the statistical tests applied to our sample galaxies in comparison with normal ones (see text). Columns labeled P() represents the probability that the observed differences are statistically significants.
Tracer	Type	$\chi^2$	k	P( $\chi^2$ )	P(T-test)	P(F-test)
Dust	Early	13.39	5	98.0%	95.9%	24.2%
Dust	Late	8.29	9	49.5%	94.9%	93.4%
Dust	Sab-Sd	-	-	-	84.6%	95.6%
HI	Early	16.58	5	99.5%	98.7%	54.6%
HI	Late	5.25	9	18.8%	49.3%	67.5%
mol	Early	19.47	4	99.9%	2.7%	65.4%
mol	Late	21.34	9	98.9%	94.5%	29.2%
X-ray	Early	14.95	5	99.0%	97.6%	37.3%
X-ray	Late	47.26	9	100.0%	99.5%	63.3%

Source LaTeX | All tables | In the text