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Improving \textsl{Gaia} parallax precision with a data-driven model of stars
Free accessArXiv | 2017| -
The velocity distribution of nearby stars from Hipparcos data I. The significance of the moving groups
Free accessArXiv | 2009| -
Comoving stars in Gaia DR1: An abundance of very wide separation co-moving pairs
Free accessArXiv | 2016| -
An Ultraviolet-Optical Color-Metallicity relation for Red Clump Stars using GALEX and Gaia
Free accessArXiv | 2018| -
A systematic search for massive black hole binaries in SDSS spectroscopic sample
Free accessArXiv | 2011| -
Approximate Bayesian Computation in Large Scale Structure: constraining the galaxy-halo connection
Free accessArXiv | 2016| -
The principle of maximum entropy production in a simple model of a convection cell
Free accessDSpace@MIT | 1992| -
Clumpy Streams from Clumpy Halos: Detecting Missing Satellites with Cold Stellar Structures
Free accessArXiv | 2010| -
Measuring the undetectable: Proper motions and parallaxes of very faint sources
Free accessArXiv | 2008|
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