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A list of all the posts and pages found on the site. For you robots out there is an XML version available for digesting as well.

Pages

Posts

Future Blog Post

less than 1 minute read

Published:

This post will show up by default. To disable scheduling of future posts, edit config.yml and set future: false.

Blog Post number 4

less than 1 minute read

Published:

This is a sample blog post. Lorem ipsum I can’t remember the rest of lorem ipsum and don’t have an internet connection right now. Testing testing testing this blog post. Blog posts are cool.

Blog Post number 3

less than 1 minute read

Published:

This is a sample blog post. Lorem ipsum I can’t remember the rest of lorem ipsum and don’t have an internet connection right now. Testing testing testing this blog post. Blog posts are cool.

Blog Post number 2

less than 1 minute read

Published:

This is a sample blog post. Lorem ipsum I can’t remember the rest of lorem ipsum and don’t have an internet connection right now. Testing testing testing this blog post. Blog posts are cool.

Blog Post number 1

less than 1 minute read

Published:

This is a sample blog post. Lorem ipsum I can’t remember the rest of lorem ipsum and don’t have an internet connection right now. Testing testing testing this blog post. Blog posts are cool.

portfolio

AllStarFit

AllStarFit: R package for source detection, PSF and multi-component galaxy fitting

MultiProFit

MultiProFit: A Python package for fast galaxy model fitting using Gaussian mixtures

ProFit

ProFit: An R package for Bayesian galaxy model fitting

publications

Mergers in Galaxy Groups. I. Structure and Properties of Elliptical Remnants

Published in The Astrophysical Journal, 2013

This first paper from my PhD thesis presented novel N-body simulations of mergers of spiral galaxies in groups of three to twenty-five. Analysis of synthetic images and kinematic maps showed that the merger remnants formed in the centers of these groups have very similar properties to nearby elliptical galaxies, showing that multiple, gas-poor and sometimes minor mergers are an alternative formation mechanism to the previously favoured paradigm of a single gas-rich major merger.

Recommended citation: Taranu D.S., Dubinski J.J., Yee H.K.C., 2013, ApJ, 778, 61. https://ui.adsabs.harvard.edu/abs/2013ApJ...778...61T/abstract

Quenching star formation in cluster galaxies

Published in Monthly Notices of the Royal Astronomical Society, 2014

This undergraduate thesis paper presented simplified models for the evolution of star formation in galaxies in rich clusters. Comparioson of model predictions to observations showed that typical galaxies are quenched on longer exponential time-scales of 3-3.5 Gyr, whereas models with very rapid quenching (<1Gyr) are disfavoured as they produce excessively old and red galaxies.

Recommended citation: Taranu D.S., Hudson M.J., Balogh M.L., et al., 2014, MNRAS, 440, 1934. https://ui.adsabs.harvard.edu/abs/2014MNRAS.440.1934T/abstract

Mergers in Galaxy Groups. II. The Fundamental Plane of Elliptical Galaxies

Published in Monthly Notices of the Royal Astronomical Society, 2015

This second paper from my PhD thesis concluded that Paper I’s simulations follow a similar fundamental plane relation to observed ellipticals, but with a shallower slope, implying that some dissipation is likely necessary to form realistic ellipticals.

Recommended citation: Taranu D.S., Dubinski J.J., Yee H.K.C., 2015, MNRAS, 803, 78 https://ui.adsabs.harvard.edu/abs/2015ApJ...803...78T/abstract

talks

teaching

Teaching Assistant

Undergraduate courses, University of Toronto, Department of Astronomy & Astrophysics, 2008

I was a teaching assistant for a variety of courses at the University of Toronto, including: