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

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Table 1:

Dimensionless relative amplitudes A_i' and timescales $\tau _i$ of our different red noise models. Models 1 to 3 are fixed parameter models whereas for the others we draw random values within a given range for each single light curve individually. The timescales are chosen to cover the range of expected transit durations.
Model number	A₁'	A₂'	A₃'	A₄'	$\tau_1$ [min]	$\tau_2$ [min]	$\tau_3$ [min]	$\tau_4$ [min]
1	1	2	3	4	355	169	111	48
2	2	3	4	1	169	131	111	88
3	3	4	1	2	131	99	61	27
4	random [1-4]	random [1-4]	random [1-4]	random [1-4]	random [300-400]	random [200-300]	random [100-200]	random [0-100]
5	random [1-4]	random [1-4]	random [1-4]	random [1-4]	random [250-300]	random [200-250]	random [150-200]	random [100-150]
6	random [1-4]	random [1-4]	random [1-4]	random [1-4]	random [250-300]	random [200-250]	random [150-200]	-
7	random [1-4]	random [1-4]	random [1-4]	random [1-4]	random [250-300]	random [200-250]	-	random [100-150]
8	random [1-4]	random [1-4]	random [1-4]	random [1-4]	random [250-300]	-	random [150-200]	random [100-150]
9	random [1-4]	random [1-4]	random [1-4]	random [1-4]	-	random [200-250]	random [150-200]	random [100-150]

Source LaTeX | All tables | In the text

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