activity
20022021
most citedMultidimensional Data Driven Classification of Emission-line Galaxies

24 citations · 43 across the 6 of their papers we have counts for

collaborators

6 papers

stat.AP2021

Identification of high-energy astrophysical point sources via hierarchical Bayesian nonparametric clustering

Andrea Sottosanti, Mauro Bernardi, Alessandra R. Brazzale +4

The light we receive from distant astrophysical objects carries information about their origins and the physical mechanisms that power them. The study of these signals, however, is…

astro-ph.SR2018★ 11 cited

Bayesian Hierarchical Modelling of Initial-Final Mass Relations Across Star Clusters

Shijing Si, Ted von Hippel, Elliot Robinson +3

The initial-final mass relation (IFMR) of white dwarfs (WDs) plays an important role in stellar evolution. To derive precise estimates of IFMRs and explore how they may vary among…

astro-ph.GA2018★ 24 cited

Multidimensional Data Driven Classification of Emission-line Galaxies

Vasileios Stampoulis, David A. van Dyk, Vinay L. Kashyap +1

We propose a new soft clustering scheme for classifying galaxies in different activity classes using simultaneously 4 emission-line ratios; log([NII ]/Ha), log([SII]/Ha), log([OI]/…

astro-ph.SR2016★ 4 cited

The Power of Principled Bayesian Methods in the Study of Stellar Evolution

Ted von Hippel, David A. van Dyk, David C. Stenning +5

It takes years of effort employing the best telescopes and instruments to obtain high-quality stellar photometry, astrometry, and spectroscopy. Stellar evolution models contain the…

stat.CO2015★ 4 cited

A Corrected and More Efficient Suite of MCMC Samplers for the Multinomal Probit Model

Xiyun Jiao, David A. van Dyk

The multinomial probit (MNP) model is a useful tool for describing discrete-choice data and there are a variety of methods for fitting the model. Among them, the algorithms provide…

astro-ph2002

Bayesian Spectral Analysis of Metal Abandance Deficient Stars

Epaminondas Sourlas, David van Dyk, Vinay Kashyap +2

Metallicity can be measured by analyzing the spectra in the X-ray region and comparing the flux in spectral lines to the flux in the underlying Bremsstrahlung continuum. In this pa…