Investigating the potential of the Pan-Planets project using Monte Carlo simulations

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Table 10:

Number of VHN detections after the first and second year of the Pan-Planets survey for our selected survey strategy for different residual red noise levels (model 4).
RRN level	1 yr	2 yr
1 mmag	$5.7 \pm 2.4$	$16.6 \pm 4.1$
2 mmag	$3.5 \pm 1.9$	$9.7 \pm 3.1$
3 mmag	$2.4 \pm 1.6$	$6.3 \pm 2.5$
4 mmag	$1.7 \pm 1.4$	$4.6 \pm 2.2$

Source LaTeX | All tables | In the text

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