Table 1.
Estimated unbudgeted uncertainties in the ZTF photometric dataset.
Photometric filter | σXCorr | σX |
---|---|---|
(centimag) | (centimag) | |
ZTF g | 4.6 | 1.3 |
ZTF r | 4.9 | 1.8 |
ZTF i | 8.4 | 2.2 |
Notes. Right column shows the portion of the residuals from SALT2 light-curve fits attributed unbudgeted photometric error (σX). The left column shows variation assumed to be physical variation in the light curves, and correlated at a timescale of 5 days (σXCorr).
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