activity
20052012
most citedK-corrections and filter transformations in the ultraviolet, optical, and near infrared

1.7k citations · 3.3k across the 10 of their papers we have counts for

collaborators

10 papers

cs.LG2012★ 55 cited

On the Convergence of Bound Optimization Algorithms

Ruslan R Salakhutdinov, Sam T Roweis, Zoubin Ghahramani

Many practitioners who use the EM algorithm complain that it is sometimes slow. When does this happen, and what can be done about it? In this paper, we study the general class of b…

cs.LG2012★ 186 cited

Collaborative Filtering and the Missing at Random Assumption

Benjamin Marlin, Richard S. Zemel, Sam Roweis +1

Rating prediction is an important application, and a popular research topic in collaborative filtering. However, both the validity of learning algorithms, and the validity of stand…

astro-ph.IM2009★ 1.1k cited

Astrometry.net: Blind astrometric calibration of arbitrary astronomical images

Dustin Lang, David W. Hogg, Keir Mierle +2

We have built a reliable and robust system that takes as input an astronomical image, and returns as output the pointing, scale, and orientation of that image (the astrometric cali…

astro-ph.GA2009★ 63 cited

The velocity distribution of nearby stars from Hipparcos data I. The significance of the moving groups

Jo Bovy, David W. Hogg, Sam T. Roweis

We present a three-dimensional reconstruction of the velocity distribution of nearby stars (<~ 100 pc) using a maximum likelihood density estimation technique applied to the two-di…

stat.ME2009★ 159 cited

Extreme deconvolution: Inferring complete distribution functions from noisy, heterogeneous and incomplete observations

Jo Bovy, David W. Hogg, Sam T. Roweis

We generalize the well-known mixtures of Gaussians approach to density estimation and the accompanying Expectation--Maximization technique for finding the maximum likelihood parame…

astro-ph2008★ 4 cited

Blind Date: Using proper motions to determine the ages of historical images

Jonathan T. Barron, David W. Hogg, Dustin Lang +1

Astrometric calibration is based on patterns of cataloged stars and therefore effectively assumes a particular epoch, which can be substantially incorrect for historical images. Wi…