2009A&A...494..707K -
Astronomy and Astrophysics, volume 494707-717 (2009/2-1)
Investigating the potential of the Pan-Planets project using Monte Carlo simulations.
KOPPENHOEFER J., AFONSO C., SAGLIA R.P. and HENNING T.
Abstract (from CDS):
Using Monte Carlo simulations we analyze the potential of the upcoming transit survey Pan-Planets. The analysis covers the simulation of realistic light curves (including the effects of ingress/egress and limb-darkening) with both correlated and uncorrelated noise as well as the application of a box-fitting-least-squares detection algorithm. In this work we show how simulations can be a powerful tool in defining and optimizing the survey strategy of a transiting planet survey. We find the Pan-Planets project to be competitive with all other existing and planned transit surveys with the main power being the large 7 square degree field of view. In the first year we expect to find up to 25 Jupiter-sized planets with periods below 5 days around stars brighter than V=16.5mag. The survey will also be sensitive to planets with longer periods and planets with smaller radii. After the second year of the survey, we expect to find up to 9 Warm Jupiters with periods between 5 and 9 days and 7 Very Hot Saturns around stars brighter than V=16.5mag as well as 9 Very Hot Neptunes with periods from 1 to 3 days around stars brighter than i'=18.0mag.
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Journal keyword(s):
stars: planetary systems - methods: statistical - techniques: photometric
Simbad objects:
1
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