OGLE-2008-BLG-513Lb: The Orbital Solution for a Microlensing Planet

J. C. Yee; A. Udalski; Subo Dong; J. Greenhill; Y. Tsapras; I. A. Bond; A. Gould; S. Kozlowski; P. Fouque; M. D. Albrow; C. Han; L. A. G. Monard; J. McCormick; A. Williams; N. Kains; J. An; M. Dominik

OGLE-2008-BLG-513Lb: The Orbital Solution for a Microlensing Planet

Earth and Planetary Astrophysics 2011-07-12 v2

Authors: J. C. Yee , A. Udalski , Subo Dong , J. Greenhill , Y. Tsapras , I. A. Bond , A. Gould , S. Kozlowski , P. Fouque , M. D. Albrow , C. Han , L. A. G. Monard , J. McCormick , A. Williams , N. Kains , J. An , M. Dominik

View on arXiv ↗ PDF ↗

Abstract

A static binary star solution for OGLE-2008-BLG-513 has been found. The mass ratio and separation for this solution are q~0.28, s~0.86. This model has a chi^2 comparable to the chi^2 of the model with a planetary mass ratio and orbital motion that was presented in this paper. Because the model with a static, binary star lens is simpler than the model originally presented in this paper, Occam's Razor says it is likely to be the correct solution. Consequently, this paper has been withdrawn from ApJ.

Cite

@article{arxiv.1106.4013,
  title  = {OGLE-2008-BLG-513Lb: The Orbital Solution for a Microlensing Planet},
  author = {J. C. Yee and A. Udalski and Subo Dong and J. Greenhill and Y. Tsapras and I. A. Bond and A. Gould and S. Kozlowski and P. Fouque and M. D. Albrow and C. Han and L. A. G. Monard and J. McCormick and A. Williams and N. Kains and J. An and M. Dominik},
  journal= {arXiv preprint arXiv:1106.4013},
  year   = {2011}
}

Comments

This paper has been withdrawn

OGLE-2008-BLG-513Lb: The Orbital Solution for a Microlensing Planet

Abstract

Cite

Comments

Related papers