Table 1.

Top: The galaxy properties used to train the decision tree. In the second column, the aperture within which this quantity is calculated is noted. Here, total refers to the total bound mass to this subhalo. In this column, half-mass radius refers to the stellar half-mass radius. Bottom: The cluster properties associated with each galaxy. These are the properties of the cluster that the galaxy has backsplashed from or is falling into. The final column for both shows whether or not the value is pre-scaled logarithmically before its use in the decision tree. Note that this does not affect results, as the decision tree simply performs a set of bisections, but it does aid in the inspection of the results.

Galaxy propertyApertureLog?
Total black hole massTotal|$\checkmark$|
Total black hole mass accretion rateTotal|$\checkmark$|
Magnetic field strength in discTotal|$\checkmark$|
Magnetic field strength in haloTotal|$\checkmark$|
Centre of massTotal×
Gas metal mass fractions for each speciesTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Gas total metallicityTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Galaxy half-mass radius (per species)Total|$\checkmark$|
Galaxy half-mass radius (total)Total|$\checkmark$|
Number of particles (per species)Total|$\checkmark$|
Number of particles (total)Total|$\checkmark$|
Total massTotal, half-mass radius (per species, total), twice half-mass radius, max radius|$\checkmark$|
Subhalo position in boxTotal|$\checkmark$|
Subhalo instantaneous SFRTotal, twice half-mass radius, max radius|$\checkmark$|
Subhalo spin parameter κTotal|$\checkmark$|
Star metal mass fractions for each speciesTwice half-mass radius, half-mass radius, max radius|$\checkmark$|
Star total metallicityTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Magnitude in U, B, V, K, g, r, i, z bandsTotal×
Total mass within K-band half-light radiusTotal|$\checkmark$|
Half-light radius in K bandTotal|$\checkmark$|
1D velocity dispersion of all member particlesTotal|$\checkmark$|
Maximum value of the spherically averaged rotation curve VmaxTotal|$\checkmark$|
Radius at which Vmax is achieved.Total|$\checkmark$|
Total mass currently decoupled as windsTotal|$\checkmark$|
UV and gr colourTotal×
Cluster propertyApertureLog?
Group centre of massTotal×
Group gas metal mass fractions for each speciesTotal|$\checkmark$|
Group gas metallicityTotal|$\checkmark$|
Group star metal mass fractions for each speciesTotal|$\checkmark$|
Group star metallicityTotal|$\checkmark$|
Group aperture massesR500,crit, R500,mean, R200,crit, R200,mean, R200,tophat|$\checkmark$|
Group aperture radiiR500,crit, R500,mean, R200,crit, R200,mean, R200,tophat|$\checkmark$|
Galaxy propertyApertureLog?
Total black hole massTotal|$\checkmark$|
Total black hole mass accretion rateTotal|$\checkmark$|
Magnetic field strength in discTotal|$\checkmark$|
Magnetic field strength in haloTotal|$\checkmark$|
Centre of massTotal×
Gas metal mass fractions for each speciesTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Gas total metallicityTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Galaxy half-mass radius (per species)Total|$\checkmark$|
Galaxy half-mass radius (total)Total|$\checkmark$|
Number of particles (per species)Total|$\checkmark$|
Number of particles (total)Total|$\checkmark$|
Total massTotal, half-mass radius (per species, total), twice half-mass radius, max radius|$\checkmark$|
Subhalo position in boxTotal|$\checkmark$|
Subhalo instantaneous SFRTotal, twice half-mass radius, max radius|$\checkmark$|
Subhalo spin parameter κTotal|$\checkmark$|
Star metal mass fractions for each speciesTwice half-mass radius, half-mass radius, max radius|$\checkmark$|
Star total metallicityTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Magnitude in U, B, V, K, g, r, i, z bandsTotal×
Total mass within K-band half-light radiusTotal|$\checkmark$|
Half-light radius in K bandTotal|$\checkmark$|
1D velocity dispersion of all member particlesTotal|$\checkmark$|
Maximum value of the spherically averaged rotation curve VmaxTotal|$\checkmark$|
Radius at which Vmax is achieved.Total|$\checkmark$|
Total mass currently decoupled as windsTotal|$\checkmark$|
UV and gr colourTotal×
Cluster propertyApertureLog?
Group centre of massTotal×
Group gas metal mass fractions for each speciesTotal|$\checkmark$|
Group gas metallicityTotal|$\checkmark$|
Group star metal mass fractions for each speciesTotal|$\checkmark$|
Group star metallicityTotal|$\checkmark$|
Group aperture massesR500,crit, R500,mean, R200,crit, R200,mean, R200,tophat|$\checkmark$|
Group aperture radiiR500,crit, R500,mean, R200,crit, R200,mean, R200,tophat|$\checkmark$|
Table 1.

Top: The galaxy properties used to train the decision tree. In the second column, the aperture within which this quantity is calculated is noted. Here, total refers to the total bound mass to this subhalo. In this column, half-mass radius refers to the stellar half-mass radius. Bottom: The cluster properties associated with each galaxy. These are the properties of the cluster that the galaxy has backsplashed from or is falling into. The final column for both shows whether or not the value is pre-scaled logarithmically before its use in the decision tree. Note that this does not affect results, as the decision tree simply performs a set of bisections, but it does aid in the inspection of the results.

Galaxy propertyApertureLog?
Total black hole massTotal|$\checkmark$|
Total black hole mass accretion rateTotal|$\checkmark$|
Magnetic field strength in discTotal|$\checkmark$|
Magnetic field strength in haloTotal|$\checkmark$|
Centre of massTotal×
Gas metal mass fractions for each speciesTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Gas total metallicityTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Galaxy half-mass radius (per species)Total|$\checkmark$|
Galaxy half-mass radius (total)Total|$\checkmark$|
Number of particles (per species)Total|$\checkmark$|
Number of particles (total)Total|$\checkmark$|
Total massTotal, half-mass radius (per species, total), twice half-mass radius, max radius|$\checkmark$|
Subhalo position in boxTotal|$\checkmark$|
Subhalo instantaneous SFRTotal, twice half-mass radius, max radius|$\checkmark$|
Subhalo spin parameter κTotal|$\checkmark$|
Star metal mass fractions for each speciesTwice half-mass radius, half-mass radius, max radius|$\checkmark$|
Star total metallicityTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Magnitude in U, B, V, K, g, r, i, z bandsTotal×
Total mass within K-band half-light radiusTotal|$\checkmark$|
Half-light radius in K bandTotal|$\checkmark$|
1D velocity dispersion of all member particlesTotal|$\checkmark$|
Maximum value of the spherically averaged rotation curve VmaxTotal|$\checkmark$|
Radius at which Vmax is achieved.Total|$\checkmark$|
Total mass currently decoupled as windsTotal|$\checkmark$|
UV and gr colourTotal×
Cluster propertyApertureLog?
Group centre of massTotal×
Group gas metal mass fractions for each speciesTotal|$\checkmark$|
Group gas metallicityTotal|$\checkmark$|
Group star metal mass fractions for each speciesTotal|$\checkmark$|
Group star metallicityTotal|$\checkmark$|
Group aperture massesR500,crit, R500,mean, R200,crit, R200,mean, R200,tophat|$\checkmark$|
Group aperture radiiR500,crit, R500,mean, R200,crit, R200,mean, R200,tophat|$\checkmark$|
Galaxy propertyApertureLog?
Total black hole massTotal|$\checkmark$|
Total black hole mass accretion rateTotal|$\checkmark$|
Magnetic field strength in discTotal|$\checkmark$|
Magnetic field strength in haloTotal|$\checkmark$|
Centre of massTotal×
Gas metal mass fractions for each speciesTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Gas total metallicityTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Galaxy half-mass radius (per species)Total|$\checkmark$|
Galaxy half-mass radius (total)Total|$\checkmark$|
Number of particles (per species)Total|$\checkmark$|
Number of particles (total)Total|$\checkmark$|
Total massTotal, half-mass radius (per species, total), twice half-mass radius, max radius|$\checkmark$|
Subhalo position in boxTotal|$\checkmark$|
Subhalo instantaneous SFRTotal, twice half-mass radius, max radius|$\checkmark$|
Subhalo spin parameter κTotal|$\checkmark$|
Star metal mass fractions for each speciesTwice half-mass radius, half-mass radius, max radius|$\checkmark$|
Star total metallicityTwice half-mass radius, half-mass radius, max radius, SF gas only|$\checkmark$|
Magnitude in U, B, V, K, g, r, i, z bandsTotal×
Total mass within K-band half-light radiusTotal|$\checkmark$|
Half-light radius in K bandTotal|$\checkmark$|
1D velocity dispersion of all member particlesTotal|$\checkmark$|
Maximum value of the spherically averaged rotation curve VmaxTotal|$\checkmark$|
Radius at which Vmax is achieved.Total|$\checkmark$|
Total mass currently decoupled as windsTotal|$\checkmark$|
UV and gr colourTotal×
Cluster propertyApertureLog?
Group centre of massTotal×
Group gas metal mass fractions for each speciesTotal|$\checkmark$|
Group gas metallicityTotal|$\checkmark$|
Group star metal mass fractions for each speciesTotal|$\checkmark$|
Group star metallicityTotal|$\checkmark$|
Group aperture massesR500,crit, R500,mean, R200,crit, R200,mean, R200,tophat|$\checkmark$|
Group aperture radiiR500,crit, R500,mean, R200,crit, R200,mean, R200,tophat|$\checkmark$|
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