Table 1.

Summary of the HOSTLIB, WGTMAP, and cadence used for each transient class in our simulation. The first three HOSTLIBs contain CosmoDC2 galaxies that extrapolate distributions of observed hosts in GHOST; the fourth is a representative sample from CosmoDC2. Pclass refers to the probability of each transient class occurring given the properties of a galaxy; these functions are defined in Section 6 and implemented via the WGTMAPs. The cadence refers to the time interval between light-curve samples in the simulation.

HOSTLIBWGTMAPClassCadence (day)
SN Ia HostsPIaSN Ia2.0
SN II HostsPIISN II/IIn/IIP/IIL2.0
H-Poor SN HostsPIbcSN Ib/Ic2.0
RIc-BLSN Ic-BL2.0
PSLSNISLSN-I2.0
PIISN IIb2.0
Rand. DC2 SubsetPAGNAGN0.1, 2.0
RKNKN0.1–2.0
PTDETDE0.1–2.0
HOSTLIBWGTMAPClassCadence (day)
SN Ia HostsPIaSN Ia2.0
SN II HostsPIISN II/IIn/IIP/IIL2.0
H-Poor SN HostsPIbcSN Ib/Ic2.0
RIc-BLSN Ic-BL2.0
PSLSNISLSN-I2.0
PIISN IIb2.0
Rand. DC2 SubsetPAGNAGN0.1, 2.0
RKNKN0.1–2.0
PTDETDE0.1–2.0
Table 1.

Summary of the HOSTLIB, WGTMAP, and cadence used for each transient class in our simulation. The first three HOSTLIBs contain CosmoDC2 galaxies that extrapolate distributions of observed hosts in GHOST; the fourth is a representative sample from CosmoDC2. Pclass refers to the probability of each transient class occurring given the properties of a galaxy; these functions are defined in Section 6 and implemented via the WGTMAPs. The cadence refers to the time interval between light-curve samples in the simulation.

HOSTLIBWGTMAPClassCadence (day)
SN Ia HostsPIaSN Ia2.0
SN II HostsPIISN II/IIn/IIP/IIL2.0
H-Poor SN HostsPIbcSN Ib/Ic2.0
RIc-BLSN Ic-BL2.0
PSLSNISLSN-I2.0
PIISN IIb2.0
Rand. DC2 SubsetPAGNAGN0.1, 2.0
RKNKN0.1–2.0
PTDETDE0.1–2.0
HOSTLIBWGTMAPClassCadence (day)
SN Ia HostsPIaSN Ia2.0
SN II HostsPIISN II/IIn/IIP/IIL2.0
H-Poor SN HostsPIbcSN Ib/Ic2.0
RIc-BLSN Ic-BL2.0
PSLSNISLSN-I2.0
PIISN IIb2.0
Rand. DC2 SubsetPAGNAGN0.1, 2.0
RKNKN0.1–2.0
PTDETDE0.1–2.0
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