If you've landed here then you probably already know who I am, but if not then checkout the about page.
A brief showcase of my research interests.
The "simplest" model of galaxy formation
In this work we introduce a new, simple model that self-consistently connects the growth of galaxies to the formation history of their host dark matter haloes. This "formation history" model is built using just two simple, phenomenologically motivated equations that depend only on dark matter halo properties. The first describes the rate at which dark matter haloes are fed with fresh baryonic fuel for star formation, whilst the second equation describes the efficiency with which this fuel can be converted into stars. Despite its simplicity, our formation history model is capable of reproducing the observed z=0 red and blue stellar mass functions and can easily be extended to arbitrary levels of complexity to match multiple observations across cosmic time.
Constraining the last 7 billion years of galaxy evolution in semi-analytic models
Semi-analytic galaxy formation models are a commonly used tool in modern astronomy and are particularly well suited to helping us understand the statistical properties of large galaxy samples. Typically these models are "hand tuned" to reproduce fundamental observational relations in the local Universe, with inferences then being made about higher redshifts. However, using Monte-Carlo Markov Chain techniques, we present the first robust statistical calibration of a popular semi-analytic model against observations at multiple redshifts simultaneously. In order for the model to be successful, we find that we are required to push a subset of the implemented physical prescriptions to extreme limits. This suggests that our model may be incomplete, possibly requiring the addition of a mechanism to preferentially bolster star formation in the most massive halos at high redshift.
The midlife crisis of the Milky Way and M31
Both the galaxy in which we live, the Milky Way, and our nearest neighbour, Andromeda (a.k.a. M31), are commonly thought to be "typical" spiral galaxies. Using a combination of the best available observations and a state of the art semi-analytic galaxy formation model, we investigate just how typical these galaxies really are in terms of their masses, colours and star formation rates.
The result: Both galaxies may be undergoing a "mid-life crisis"...
|Melbourne Astro Group||The University of Melbourne Astrophysics Group homepage|
|ADS||NASA Astronomical Data System|
|astro-ph||arXiv astro-ph preprints|
|Git||Distributed version control system|
|Github||Social coding and open source goodness|
|Bitbucket||Unlimited free code hosting|
|Matplotlib||The 2D plotting library for python|
|Markdown||Syntax guide for the amazingly useful markdown formatter|
|HDF5||The most flexible and reliable data format around|
|VimTipsWiki||The Vim tips wiki|
|Astropy||The community python library for astronomers|
|Weather Forecast||The Melbourne weather forecast|
|Current Weather||The current Melbourne weather conditions|