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Gravitational Microlensing Events. Diane Feuillet Kailash Sahu. Tracking High Proper Motion Stars to Predict Possible Microlensing Events Fitting Light Curves of Long-Duration Binary Events Derived the Mass Function of Observed Events From the Timescales. ARIES Images-240 2009 .
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Gravitational Microlensing Events Diane Feuillet Kailash Sahu
Tracking High Proper Motion Stars to Predict Possible Microlensing Events Fitting Light Curves of Long-Duration Binary Events Derived the Mass Function of Observed Events From the Timescales
Poss 2 blue 1997 5 3 4 6 2 1 7
Poss 2 blue 1997 5 ARIES Images-240 2009 3 6 4 2 1 5 7 4 3 2 1 6 7
Poss 2 blue 1997 5 ARIES Images-240 2009 3 6 4 2 1 7 6 5 3 4 2 1 7
6 600 Y position 5 4 3 2 1 7 400 600 400 x position
515 Y position 510 2 D = 0.400 arcsec T = 2/1/2012 1 505 445 450 440 x position
Te = 141 days 1 Amplitude 1999-19 Te1 = 60 days Te2 = 120 days I mag = 15.9 1300 1700 HJD - 2450000 HJD - 2450000
Te = 207 days 0.5 Amplitude 2006-393 Te1 = 90 days Te2 = 74 days I mag = 14.9 0 3900 4200 HJD - 2450000
1 Possible Black Holes? 2008-143 Te1 = 40 days Te2 = 35 days I mag = 17.6 Amplitude 0.5 4500 4800 HJD - 2450000
4 Three body systems 3 Amplitude 2002-051 Te1 = 8 days Te2 = 12 days Te3 = 20 days I mag = 17.8 2 1 0 2250 2400 HJD - 2450000
Te = 139 days 1 Amplitude 0.5 2003-095 Te1 = 26 days Te2 = 26 days Te3 = 15 days I mag = 15.6 0 2800 3200 HJD - 2450000
2 2004-039 Te1 = 22 days Te2 = 1 days I mag = 17.3 Amplitude 1 Some do not fit well 0 3060 3100 HJD - 2450000 2003-056 Te1 = 15 days Te2 = 20 days I mag = 16.8 Amplitude 1 0 2800 2650 HJD - 2450000