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Models and Simulations for the Photometric LSST Astronomical Time Series Classification Challenge (PLAsTiCC)

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Academic year: 2021

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Figure

Fig. 1.— Each row shows model light curves in the ugrizy passbands for the extragalactic models (Table 1) shown on the right
Fig. 3.— For models not included in the training set (class >990 in Table 1), each row shows light curves in the ugrizy passbands for the model shown on the right
Fig. 4.— Peak g and z band magnitude distributions in rest-frame (luminosity function) for extragalactic models
Fig. 5.— For extragalacticmodels, two-dimensional histograms of peak i-band magnitude (rest-frame) vs
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