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A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. I Method description
M. Huertas-Company, D. Rouan, L. Tasca +2
We present a new non-parametric method to quantify morphologies of galaxies based on a particular family of learning machines called support vector machines. The method, that can b…
Evolution of the Frequency of Luminous (\geq L_V*) Close Galaxy Pairs at z < 1.2 in the COSMOS Field
J. S. Kartaltepe, D. B. Sanders, N. Z. Scoville +8
We measure the fraction of luminous galaxies in pairs at projected separations of 5-20 kpc out to z=1.2 in the COSMOS field using ACS images and photometric redshifts derived from…
The Multiple Timescales of Optical Variability of the Blazar 3C 279 During the 2001-2002 Outburst
Jeyhan S. Kartaltepe, Thomas J. Balonek
During 2001-2002 the optically violent variable (OVV) blazar 3C 279 un- derwent the most intense outburst seen during the entire fourteen year history that this quasar has been stu…