2012/01/25 by S. Calchi Novati
Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy #Astrophysics #Brown dwarf #Dark matter #Galactic halo #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gravitational lens #Gravitational microlensing #Halo #Large Magellanic Cloud #Massive compact halo object #Milky Way #Physics #Stars #Stellar, planetary, and galactic studies #astro-ph.GA
paper · pdf · doi:10.1088/1742-6596/354/1/012001
published as J.Phys.Conf.Ser. 354 (2012) 012001 · 8 pages, no figures; to appear in the Proceedings of the 3rd Italian-Pakistani Workshop on Relativistic Astrophysics, Lecce 20-22 June 2011, published in Journal of Physics: Conference Series (JPCS)
arxiv created 2012/01/25 · openalex publication_date 2012/03/14 · arxiv updated 2015/06/03 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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 towards an agreement in excluding dark matter MACHOs of less than about 10 −1 M ⊙ ; it remains however an ongoing debate for values in the mass range (0.1 – 1) M ⊙ . The more robust constraints, though not all in agreement, come from the observational campaigns towards the Magellanic Clouds (the LMC and the SMC). The analyses towards the nearby galaxy of M31, in the so called "pixel lensing" regime, have expanded the perspectives in this field of research. In this contribution first we draw a critical view on recent results and then we focus on the pixel lensing analysis towards M31 of the PLAN collaboration.