The OGLE view of microlensing towards the Magellanic Clouds – I. A trickle of events in the OGLE‐II LMC data★

@article{Wyrzykowski2009TheOV,
  title={The OGLE view of microlensing towards the Magellanic Clouds – I. A trickle of events in the OGLE‐II LMC data★},
  author={Lukasz Wyrzykowski and Szymon Kozłowski and Jan Skowron and Vasily A Belokurov and M. Clare Smith and Andrzej Udalski and Michał K. Szymański and Marcin Kubiak and Grzegorz Pietrzyński and Igor Soszyński and Olaf Szewczyk and K. Żebruń},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2009},
  volume={397},
  pages={1228-1242}
}
We present the results from the Optical Gravitational Lensing Experiment II (OGLE-II) survey (1996–2000) towards the Large Magellanic Cloud (LMC), which has the aim of detecting the microlensing phenomena caused by dark matter compact objects in the Galactic halo [massive compact halo objects (MACHOs)]. We use high-resolution Hubble Space Telescope images of the OGLE fields and derive the correction for the number of monitored stars in each field. This also yields blending distributions… 
The OGLE view of microlensing towards the Magellanic Clouds – III. Ruling out subsolar MACHOs with the OGLE‐III LMC data★
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Large Magellanic Cloud self-lensing for OGLE-II microlensing observations
In the framework of microlensing searches towards the Large Magellanic Cloud (LMC), we discuss the results presented by the OGLE collaboration for their OGLE-II campaign (Wyrzykowski et al. 2009). We
The origin of the microlensing events observed towards the LMC and the stellar counterpart of the Magellanic stream
We introduce a novel theoretical model to explain the long-standing puzzle of the nature of the microlensing events reported towards the Large Magellanic Cloud (LMC) by the MACHO and OGLE
New Self-lensing Models of the Small Magellanic Cloud: Can Gravitational Microlensing Detect Extragalactic Exoplanets?
We use three-dimensional distributions of classical Cepheids and RR~Lyrae stars in the Small Magellanic Cloud (SMC) to model the stellar density distribution of a young and old stellar population in
OGLE-III MICROLENSING EVENTS AND THE STRUCTURE OF THE GALACTIC BULGE*
We present and study the largest and most comprehensive catalog of microlensing events ever constructed. The sample of standard microlensing events comprises 3718 unique events from 2001-2009 with
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Microlensing is the tool of choice for the search and the analysis of compact halo objects ("MACHOs"), a still viable class of dark matter candidates at the galactic scale. Different analyses point
Microlensing towards the SMC: a new analysis of OGLE and EROS results
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