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Table 1

Photometry of Nova Del 2013 from Pan-STARRS 1.

Magnitude (AB) psf_qf Filter JD
17.569 ± 0.029 0.998 i P1 2 456 138.973
17.583 ± 0.033 0.999 i P1 2 456 138.984
16.914 ± 0.029 0.998 g P1 2 456 149.811
16.940 ± 0.024 0.998 g P1 2 456 149.821
16.986 ± 0.041 0.999 r P1 2 456 150.783
16.999 ± 0.047 0.998 r P1 2 456 150.794
17.733 ± 0.027 0.998 z P1 2 456 228.763
17.770 ± 0.029 0.999 z P1 2 456 228.774
17.576 ± 0.027 0.999 z P1 2 456 406.089
17.603 ± 0.022 0.999 z P1 2 456 406.101
17.297 ± 0.024 0.998 y P1 2 456 409.103
17.331 ± 0.022 0.999 y P1 2 456 409.115
17.474 ± 0.029 0.999 y P1 2 456 464.123
17.349 ± 0.022 0.997 y P1 2 456 466.984
18.325 ± 0.022 0.998 r P1 2 456 475.070
18.278 ± 0.020 0.998 r P1 2 456 475.080
17.206 ± 0.031 0.998 i P1 2 456 477.076
17.236 ± 0.046 0.997 i P1 2 456 477.087
17.040 ± 0.042 0.999 g P1 2 456 481.046
17.020 ± 0.026 0.997 g P1 2 456 481.056
17.414 ± 0.030 0.999 g P1 2 456 486.869
17.451 ± 0.034 0.998 g P1 2 456 486.879
17.244 ± 0.031 0.998 i P1 2 456 499.872
17.287 ± 0.026 0.998 i P1 2 456 499.879
12.831 ± 0.020 † 0.886 y P1 2 456 565.704

Notes. The psf_qf parameter describes the fraction of pixels from the object PSF, which were not saturated and did not fall on bad pixels or chip-gaps.

(†)

This post-outburst datapoint has a slightly low psf_qf and is close to the saturation limit in the yP1 band. Hence it should be considered potentially unreliable.

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