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

Poss 1 blue 1955

Poss 2 blue 1997

ARIES Images Poss 2 blue

ARIES Images Poss 2 blue 1997

Y position x position

1 2 D = arcsec T = 2/1/2012 Y position x position

Te = 141 days Te1 = 60 days Te2 = 120 days I mag = 15.9 HJD Amplitude 1 HJD

Te1 = 90 days Te2 = 74 days I mag = 14.9 Te = 207 days Amplitude HJD

Te1 = 40 days Te2 = 35 days I mag = 17.6 Possible Black Holes? Amplitude HJD

Te1 = 8 days Te2 = 12 days Te3 = 20 days I mag = 17.8 Three body systems Amplitude HJD

Te = 139 days Te1 = 26 days Te2 = 26 days Te3 = 15 days I mag = 15.6 Amplitude HJD

Te1 = 22 days Te2 = 1 days I mag = Te1 = 15 days Te2 = 20 days I mag = 16.8 Some do not fit well Amplitude HJD Amplitude 1 HJD