Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-48327
Ingrosso, G; Calchi Novati, S; De Paolis, F; Jetzer, P; Nucita, A; Zakharov, A (2011). Search for exoplanets in M31 with pixel-lensing and the PA-99-N2 event revisited. General Relativity and Gravitation, 43(4):1047-1060.
Several exoplanets have been detected towards the Galactic bulge with the microlensing technique. We show that exoplanets in M31 may also be detected with the pixel-lensing method, if telescopes making high cadence observations of an ongoing microlensing event are used. Using a Monte Carlo approach we find that the mean mass for detectable planetary systems is about 2 M J. However, even small mass exoplanets () can cause significant deviations, which are observable with large telescopes. We reanalysed the POINT-AGAPE microlensing event PA-99-N2. First, we test the robustness of the binary lens conclusion for this light curve. Second, we show that for such long duration and bright microlensing events, the efficiency for finding planetary-like deviations is strongly enhanced with respect to that evaluated for all planetary detectable events.
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Deposited On:||19 Feb 2012 18:57|
|Last Modified:||16 Jan 2014 06:05|
|ISSN:||0001-7701 (P) 1572-9532 (E)|
|Additional Information:||The original publication is available at www.springerlink.com|
|Citations:||Web of Science®. Times Cited: 5|
Scopus®. Citation Count: 5
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