Detection limits for close eclipsing and transiting sub-stellar and planetary companions to white dwarfs in the WASP survey

Details Detection limits for close eclipsing and transiting sub-stellar and planetary companions to white dwarfs in the WASP survey Detection limits for close eclipsing and transiting sub-stellar and planetary companions to white dwarfs in the WASP survey

2010-08-05

arxiv.org/abs/1008.1089v2

Monthly Notices of the Royal Astronomical Society 410, 899-911 2011

Astronomy and Astrophysics

Astrophysics

Earth and Planetary Astrophysics

17 pages, 6 figures, 4 tables - Accepted 2010 August 5, Received 2010 August 3; in original form 2010 July 13

Scientific paper

10.1111/j.1365-2966.2010.17488.x

We have performed extensive simulations to explore the possibility of detecting eclipses and transits of close, sub-stellar and planetary companions to white dwarfs in WASP light-curves. Our simulations cover companions $\sim0.3\Re<{\rm R}_{pl}<12\Re$ and orbital periods $2{\rm h}

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