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des-class-populations

Here are the scripts needed to correct your moving object survey for observational biases. findProb.py will calculate the debiased probability of finding an object on a set of frames. Bias factors include: frame latitude, longitude, size, and tilt angle; object H magnitude, semimajor axis, eccentricity, inclination, and apparent magnitude and distance when discovered.

Example objects and search frames are taken from the Deep Ecliptic Survey search for Kuiper Belt objects. (Note: full DES frame characteristics not available at this time.)

If used in research, please cite: Adams, E. R., A. A. S. Gulbis, J. L. Elliot, S. D. Benecchi, M. W. Buie, D. E. Trilling, and L.H. Wasserman. De-biased Populations of Kuiper Belt Objects from the Deep Ecliptic Survey, submitted to AJ Oct 2013

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