Difference between revisions of "Triggers:Microlensing"
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| + | == OGLE == | ||
Amplitude: can be many magnitudes, in range 0.1-10 mag. | Amplitude: can be many magnitudes, in range 0.1-10 mag. | ||
Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. | Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. | ||
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OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. | OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. | ||
| − | [[File:plot_ews_te_ampl.png]] | + | [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] |
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| − | [[File:plot_ews_te_baselinemag.png]] | ||
Revision as of 11:09, 28 July 2009
OGLE
Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed.
OGLE Early Warning System (EWS) is detecting in real-time about 600 events per year towards the Galactic bulge.
