Limits on compact halo objects as dark matter from gravitational microlensing
Microlensing started with the seminal paper by Paczyński in 1986 [1], first with observations towards the Large Magellanic Cloud and the galactic bulge. Since then many other targets have been observed and new applications have been found. In particular, it turned out to be a powerful method to det...
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EDP Sciences
2014-04-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/20147000025 |
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doaj-0601ac384b794e83988ee1752154ee7e2021-08-02T09:35:14ZengEDP SciencesEPJ Web of Conferences2100-014X2014-04-01700002510.1051/epjconf/20147000025epjconf_icfp2012_00025Limits on compact halo objects as dark matter from gravitational microlensingJetzer Philippe0Institute of Theoretical Physics University of Zürich Microlensing started with the seminal paper by Paczyński in 1986 [1], first with observations towards the Large Magellanic Cloud and the galactic bulge. Since then many other targets have been observed and new applications have been found. In particular, it turned out to be a powerful method to detect planets in our galaxy and even in the nearby M31. Here, we will present some results obtained so far by microlensing without being, however, exhaustive. http://dx.doi.org/10.1051/epjconf/20147000025 |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
Jetzer Philippe |
| spellingShingle |
Jetzer Philippe Limits on compact halo objects as dark matter from gravitational microlensing EPJ Web of Conferences |
| author_facet |
Jetzer Philippe |
| author_sort |
Jetzer Philippe |
| title |
Limits on compact halo objects as dark matter from gravitational microlensing |
| title_short |
Limits on compact halo objects as dark matter from gravitational microlensing |
| title_full |
Limits on compact halo objects as dark matter from gravitational microlensing |
| title_fullStr |
Limits on compact halo objects as dark matter from gravitational microlensing |
| title_full_unstemmed |
Limits on compact halo objects as dark matter from gravitational microlensing |
| title_sort |
limits on compact halo objects as dark matter from gravitational microlensing |
| publisher |
EDP Sciences |
| series |
EPJ Web of Conferences |
| issn |
2100-014X |
| publishDate |
2014-04-01 |
| description |
Microlensing started with the seminal paper by Paczyński in 1986 [1], first with observations towards the Large Magellanic Cloud and the galactic bulge. Since then many other targets have been observed and new applications have been found. In particular, it turned out to be a powerful method to detect planets in our galaxy and even in the nearby M31. Here, we will present some results obtained so far by microlensing without being, however, exhaustive.
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| url |
http://dx.doi.org/10.1051/epjconf/20147000025 |
| work_keys_str_mv |
AT jetzerphilippe limitsoncompacthaloobjectsasdarkmatterfromgravitationalmicrolensing |
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