1 code implementation • 5 Jan 2022 • Mohammad Mohammadi, Jarvin Mutatiina, Teymoor Saifollahi, Kerstin Bunte
Both methods are able to identify UCDs/GCs with a precision and a recall of >93 percent and provide relevances that reflect the importance of each feature dimension %(colors and angular sizes) for the classification.
1 code implementation • 16 Jul 2020 • Job Formsma, Teymoor Saifollahi
We find that both unsupervised methods extract important features from the data and can be used to find many different types of outliers.
no code implementations • 25 Jun 2020 • Teymoor Saifollahi, Ignacio Trujillo, Michael A. Beasley, Reynier F. Peletier, Johan H. Knapen
We conclude that the number of GCs around DF44 is as expected for regular dwarf galaxies of similar stellar mass and DF44 is not extraordinary in this respect.
Astrophysics of Galaxies