CONTENTS
- Introduction
- Astronomers and the AAO
- What do we do?
- Honours projects
- PhD projects
- AAO PhD Scholarship
- Deadline 1 March, applications details available here. - Contact Us
- FAQ
INTRODUCTION
While the AAO's primary role is the provision of world-class facilities for optical/infrared astronomy, the broad range of experience of AAO astronomers allows many opportunities for exciting and varied student research projects. These can be at either Ph.D. or Honours/Masters level.
As the AAO is not a degree-awarding body, these projects will be carried out under the co-supervision of an AAO astronomer and a University supervisor. Therefore in order to embark on one of these projects you are required to be accepted into a higher degree program at a university.
Usually the joint nature of the project will require students to spend some fraction of their time at the AAO's headquarters in Epping, a suburb 25 km north-west of the centre of Sydney, where they will have access to the office and computing facilities of the AAO. For students based outside Sydney temporary accommodation can be arranged at the ATNF Marsfield Lodge.
The first step in considering a graduate level research project at the AAO is to look through the information on potential supervisors and projects on these pages. Selecting a PhD or Honours supervisor and project will be one of the most critical decisions you will make in starting a research project - both student and advisor will be looking for someone they can work closely with, and who is well matched to the project. Talking to several prospective supervisors about a number of projects will greatly help you decide. So the next step after reading about the projects currently on offer will be to contact and discuss matters with both your AAO and University supervisors before coming to a decision.
AAO PhD Scholarships
The Anglo-Australian Observatory has just introduced a scheme of
top-up scholarships for students at Australian universities who are
substantially co-supervised by an AAO staff member. These grants will
be $5000 per annum for 3 years, with a possible further 6-month extension. More details (including an application form) are
available here.
ASTRONOMERS & THE AAO
Staff at the AAO are actively involved in astronomical research and in the development of new instruments to carry out these research projects. Much of this research concentrates on the Anglo-Australian Telescope (AAT) or the UK Schmidt Telescope (UKST), though AAO astronomers also make frequent use of other national and international facilities, such as the Gemini Telescopes in Hawaii and Chile that Australia is a partner in. The AAO has a world-wide reputation in both optical and infrared imaging and spectroscopy. A particular strength of AAT and UKST research is large-scale surveys to identify hundreds of thousands of a certain class of objects; in particular, old stars, galaxies and quasars.
The AAO is engaged in several major ongoing surveys: the WiggleZ project is using the AAOmega instrument on AAT to determine the evolutionary properties of the mysterious Dark Energy, but measuring the clustering of several hundred thousand distant galaxies; GAMA (Galaxy And Mass Assembly) is studying galaxy structures by building a database of a quarter of a million galaxies; the Anglo-Australian Planet Search is surveying almost 300 nearby stars to search for extra-solar planets; and the RAVE survey is using the UK Schmidt Telescope to map the kinematics and chemical abundances of stars in our Galaxy. Two major surveys (now completed) that have had enormous scientific impact were the Two Degree Field Galaxy Redshift Survey, and the Two Degree Field QSO Redshift Survey. The first of these obtained redshifts (distances) for more than 220,000 galaxies out to a redshift of 0.3. The second survey measured redshifts for over 22,000 quasars, at redshifts up to 3. The 6dF Galaxy Survey has recently completed a mammoth survey of over 15000 nearby galaxies over the whole Southern sky. In addition to planets, old stars, galaxies and quasars, AAO astronomers have a wide range of other interests. These include brown dwarfs, supernovae, star formation, starburst and active galaxies, gravitational lensing and cosmology.
The AAO is also home to one of the world's most innovative and vibrant astronomical instrumentation groups - in recent years the AAO has been involved in the construction of instruments for both the AAT and UKST (IRIS2, AAOmega, 6dF) and other telescopes (OzPoz for the FLAMES instrument on the ESO VLT; Echidna/FMOS for Subaru; as well as work for Gemini and DAzLE for VLT). Research projects involving development of new and innovative instrumentation, followed by an observational component, often produce some of the most sought-after astronomy graduates.
What do we do?
We are often asked "What do we do?" Contrary to popular opinion, a typical astronomer will only use telescopes a few weeks a year. Getting time to use a telescope is highly competitive. At the last estimate, there are 13,000 astronomers world-wide although only about a third of these aggressively pursue access to telescopes. AAO astronomers do not restrict themselves to the AAT or UKST. We apply for time on radio and sub-millimetre telescopes, larger optical/infrared telescopes like Gemini and the VLT, and space-borne observatories like the Hubble Space Telescope, Chandra X-ray observatory and so on.
Who are we?
The research interests of staff at the AAO are extensive. You can find
a list of the AAO astronomers and PhD students on the AAO Science page. Additional descriptions of
the research interests of several AAO staff can be found here,
and some recent science highlights from the AAO can be found in the AAO Annual Report,
as well as the AAO's Newsletter and Press
Release pages.
HONOURS YEAR PROJECTS
Honours projects are smaller in scale than PhD projects, and aim to provide final year undergraduate students with a research project they can undertake at a level of ~50% of their time over the course of 1-2 semesters (usually starting in January/February, though some schools offer Honours years starting in July). Honours students will be expected to write a thesis for their University describing this work, and are often also able to write up results for publication in a refereed scientific journal.
AAO/Macquarie University $5000 Honours Scholarships
Two scholarships are available, worth $5,000 each, to students undertaking a one year program for an honours degree in science and technology (particularly in astronomical instrumentation) at the Anglo Australian Observatory. They will be awarded on the basis of academic merit and suitability in this area. They would particularly suit good students studying physics, opto-electronics, computing, astrophysics and/or mathematics. For application forms, etc. click HERE to go to the Scholarship page at Macquarie University.
Some potential honours projects are described HERE as well as being listed below. The nature of research is that some of these projects could be extended and grow into PhD projects. Similarly members of staff may have other projects waiting in the wings. Astronomy is a subject in which developments move rapidly - so the hot topics by the time an honours project starts could have changed. All projects are worked out by discussion between you and your prospective supervisor, so treat this list as a source of ideas and a starting point. If you're interested in subject areas not covered below, you are encouraged to contact relevant AAO astronomers directly. Students who are interested in projects in astronomical instrumentation should contact Sam Barden, the AAO's Head of Instrumentation, or Roger Haynes for Instrument Science group. Quentin Parker, the AAO/Macquarie Lecturer (qap -@- ics.mq.edu.au) also has a page with several more Honours Projects through Macquarie University. PhD students at the ANU undertake two 3 month research projects in their first year, prior to starting their main thesis project. AAO astronomers are able to jointly supervise such students in these projects, and some of the Honours projects below may be suitable for this.

Project: Sequence structure emission in the Red Rectangle bands
Supervisors: Rob SharpWorking with the laser spectroscopy group at the University of Sydney, we have been attempting to identify the interstellar molecules, with a view to understanding the Diffuse Interstellar Bands. The work involves comparing observations from interstellar space with the debris found in the vacuum chamber in the lab here on earth after we've shot the sample up a bit with a few lasers. We have a suite of IFS observations of the Red rectangle Nebula made with the ESO-VLT and the AAT-SPIRAL system.
More projects with Rob Sharp are described here.
Project: Brightest Cluster Galaxies
Supervisors: Heath Jones and Matthew Colless
Most of the brightest and largest galaxies in the universe are found dominating the centres of galaxy clusters. These massive objects, referred to as Brightest Cluster Galaxies (BCGs), are typically large elliptical galaxies sitting at the very centre of the cluster potential. They often show signs of galaxy merging, such as double cores and extended halos, and are thought to have formed due to processes operating in these special, dense environments that are not found in more typical environments. The aim of this Honours project is to understand the properties of these objects, how they are formed, and why they are special. To this end, we have compiled a catalogue of the 1400 most luminous galaxies from the 6dF Galaxy Survey. This survey has mapped the positions and redshifts of over 120,000 galaxies in the nearby universe over nearly all the southern sky, and is one of the largest of its kind. The first step in the project is finding which of these luminous galaxies actually reside in clusters (or groups) and so fit the classical BCG definition. If environment plays a central role in their formation, then the existence of equally-massive galaxies {\em not} resident in clusters is all the more interesting. By comparing properties (such as mass, luminosity, colour, mass-to-light ratio and average surface brightness) for the cluster galaxies to those in a non-cluster control sample, we expect to uncover new insights into the formation and evolution of BCGs. This work could perhaps extend into modelling the formation of BCGs and carrying out follow-up observations of their stellar populations. This Honours project is suited to a student with interests in galaxy formation and optical observations. It will provide a good grounding in a broad range of skills and astronomical knowledge. Some background in statistics and computer modelling would be an asset. There is scope for publishing papers and travelling to conference to disseminate the results of this study.
Project: New light on a dark galaxy
Supervisors: Dr Stuart Ryder and Dr Baerbel Koribalski (ATNF)The HI Parkes All-Sky Survey (HIPASS) conducted in the late 1990s revealed surprisingly few "proto-galaxies", containing hydrogen gas but no stars. One of these, HIPASS J0731-69 (Ryder et al. 2001, ApJ, 555, 232) was found to be associated with the lopsided spiral galaxy NGC 2442. In an effort to understand how this object came to be, and why it has yet to form stars at the same rate as other galaxies, we have collected observational data including deep optical imaging, high-resolution atomic hydrogen maps, and measures of the molecular gas content. While analysing these data and writing up the results for their thesis and subsequent publication, the student will gain experience in both optical and radio astronomy techniques.
PhD PROJECTS
PhD projects are programs which target significant new bodies of research over a ~3 year timescale. As an astronomy PhD student you will be involved in developing (with your supervisors) a program of research designed to attack some set of key questions. You will have to write observing proposals, take data, analyse it and prepare it for publication, as well as writing up your results in thesis form. The AAO can offer co-supervision of students in PhD projects together with a University-based supervisor at your home institution.
The following are a few potential projects for PhD students. Astronomy is a subject in which developments move rapidly - so the hot topics by the time a project starts could have changed. All projects are worked out by discussion between you and your prospective supervisor, so treat this list as a source of ideas and a starting point. Members of staff may have other projects waiting in the wings. Students who are interested in subject areas not covered below are encouraged to contact relevant AAO astronomers directly. Students who are interested in projects in astronomical instrumentation should contact Sam Barden, the AAO's Head of Instrumentation.
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Project: The Star Formation History of the Universe
Supervisors: Andy Bunker and Rob Sharp
A key question in astrophysics is: When did most of the stars in the Universe actually form? By studying very distant galaxies, whose light is redshifted by the expansion of the Universe, we are able to look back in time to earlier stages of evolution. We can measure the rate at which stars are being born by measuring the UV and blue light from the most massive stars (which are the hottest, bluest and shortest-lived). The indications are that there was much more star formation activity when the Universe was about half its current age, but the picture is confused - the UV is heavily extinguished by astrophysical dust in these distant galaxies (formed by dying stars); we can look at the various longer-wavelength recombination lines of hydrogen, excited by the UV from young stars but less obscured by dust.
But at the high redshifts we are working at, these longer wavelengths are redshifted from the optical to the near-infrared. Only recently have instruments on large telescopes arrived that can do spectroscopy of many galaxies simultaneously. The aim of this project is to determine the star formation history of the Universe by taking spectra of a large sample of galaxies at redshift one and greater and measuring the H-alpha Balmer line of hydrogen. This can then be compared with similar nearby samples to determine how the Universe has evolved - specifically, how is star formation distributed among the galaxies. We can also compare with other star formation indicators, and assess the impact of dust absorption of the light. The spectra also contain emission lines from heavier elements made in the cores of stars, and from this we can chart the chemical enrichment history. We already have data from the Anglo-Australian Telescope IRIS2 instrument, and the MOIRCS spectrograph on the large Subaru telescope in Hawaii. We intend to expand this with the forthcoming FMOS spectrograph, which can study many hundred galaxies simultaneously and should revolutionize our understanding of galaxy evolution and the history of star formation.
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Project: Quasar Host Galaxies
Supervisors: Rob Sharp
We are using the new breed of Integral Field Spectrograph (IFS) systems, at a number of telescopes, in order to study the galaxies that host Active Galactic Nuclei (AGN).
Quasars and other AGN are thought to be powered by Black Holes in the center of galaxies, but due to the brightness of the AGN emission it has been difficult in the past to study the properties of the galaxies that host the AGN, which has hampered our understanding of how they form. IFS instruments allow one to look at these host galaxies in 3D to disentangle the problems of subtracting off the AGN in order to study the galaxy below.
More projects with Rob Sharp are described here.
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Project: Mass and Motions in the Local Universe
Supervisors: Heath Jones and Matthew Colless
Galaxies have two components to their motions: the dominant component is usually their Hubble `recession velocity', arising from the expansion of the universe; however all galaxies also have a `peculiar velocity' component that is their motion in response to the gravity field of the surrounding matter distribution. We can separate a galaxy's peculiar velocity from its recession velocity if we can measure both the redshift of the galaxy (which is the sum of the recession and peculiar velocities) and the distance of the galaxy (which gives the recession velocity via the Hubble Law). Because the peculiar velocities of galaxies are a direct reaction to the total mass distribution (i.e. both the ordinary `baryonic' matter and the dominant dark matter), they provide a clean probe of the dark matter that is largely unaffected by any bias that may exist between the galaxy distribution and the dark matter distribution. Thus measuring both the galaxy distribution and the velocity field can substantially improve our estimate of the overall mean mass density in the universe and reveal correlations and differences between the distributions of baryonic matter and dark matter.
The aim of this project is measure peculiar velocities for more than 10,000 galaxies throughout a large volume of the nearby universe and extract the cosmological information inherent in a comparison between the galaxy distribution and the peculiar velocity field. The data comes from the 6dF Galaxy Survey (6dFGS), a combined redshift and velocity survey of the whole southern sky outside the Galactic Plane. The 6dFGS observations were completed in 2006 and include redshifts for over 120,000 galaxies selected from the near-infrared Two Micron All-Sky Survey (2MASS). For a subset of about 15,000 bright, early-type galaxies (i.e. galaxies where the pressure-supported buldge component dominates the rotationally-supported disk component), the 6dFGS also provides the internal velocity dispersion (a measure of the galaxy's mass) and the effective size and surface brightness (measures of the galaxy's structure). These quantities are correlated through the Fundamental Plane relation for early-type galaxies, which can be used to estimate distances (since velocity dispersion is distance independent, while size and surface brightness are distance dependent).
The questions we want to address in this project are: What are the motions of galaxies in the local universe? What differences are there between the galaxy distribution and that of dark matter (of which we presently know rather little)? Do the parameters of the current best-fit model of the universe (the `Lamba-CDM concordance cosmology') accommodate the non-Hubble velocities observed locally?
The thesis plan consists of constructing the Fundamental Plane relation for the bright early-type galaxies in the 6dFGS, using it to derive distances and velocities for this sample, and comparing the galaxy density and velocity fields to determine the overall matter density, the relative densities of baryonic matter and dark matter, the overall bias factor between these components and the correlation between their distributions. Because the 6dFGS provides a sample that is 3-5 times larger than previous surveys of peculiar velocities (and has a more homogeneous set of spectroscopic and photometric data), it should significantly extend the current boundaries of our knowledge of the local velocity field. In particular, it will yield the first precise measure of the velocity field power spectrum (as well as the galaxy density field power spectrum), resulting in stronger constraints on a range of fundamental cosmological parameters.
In addition there are many interesting subsidiary topics to be explored along the way, including: Is the Fundamental Plane universal? Does it vary with local environment (i.e. the local density of galaxies or the type of structure-cluster, filament, void-in which the galaxies are found)? Do galaxies of different types, masses or luminosities have different biases relative to the dark matter? What are the origins of any scale-dependent variations found in the correlation between galaxies and dark matter? These questions are generally related to the processes of galaxy formation, and are important in their own right.
The data for this project are already in hand, so the research program will start immediately with analysis and interpretation, allowing several papers to be published in the course of the thesis and opportunities to present results at international conferences. The project requires a student with strong mathematical and computational capabilities
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Project: How Do Elliptical Galaxies Form?
Supervisors: Heath Jones and Matthew Colless
Astronomers already know a lot about elliptical galaxies, as they are relatively common and straightforward to study. The stars in elliptical galaxies are distributed smoothly and, unlike spiral galaxies, they contain almost no new stars. We also know that these stellar populations are dominated by old, low-mass stars that have been around for almost as long as the universe itself. And we know that ellipticals are found more commonly within the rich clusters of galaxies than in more typical regions of the universe. One of the most remarkable characteristics of elliptical galaxies is that they obey a special relationship (called the Fundamental Plane) between galaxy size, brightness and internal stellar velocity - the origin of this relationship remains something of a mystery, but appears to be linked to the way they are formed and the distribution of dark matter.
Given all this, it's easy to see why elliptical galaxies play a central role in guiding our understanding of how galaxies form; the hard part is figuring out how all these facts fit together into a consistent picture of galaxy formation. The aim of this project is to examine the properties of a very large sample of elliptical galaxies from the recently-completed 6dF Galaxy Survey in order to understand how they form and evolve. The 6dFGS is one of the largest existing datasets for studying galaxy properties, including distances and spectra for more than 120000 galaxies, collected using the AAO's UK Schmidt Telescope over the past 7 years.
From these data we can infer several key galaxy properties such as the age, mass and heavy-element fraction (called `metallicity') of the stellar population, and the ratio of luminous matter to dark matter in the galaxy. We can then investigate how age and metallicity affect the Fundamental Plane. And because the thousands of galaxies in the 6dFGS delineate galaxy clusters, voids, filaments, and large-scale structures in general, we can study trends with local environment in the stellar populations and dynamics of elliptical galaxies.
Key questions we want to address are: Exactly how old are the oldest galaxies, and when do they form their heavy elements? How and why does galaxy formation vary with environment? What is the origin of the Fundamental Plane, and how does it relate to the distribution of dark matter around galaxies?
This project is suitable for a student with interests in observational cosmology and galaxy formation. Data are in hand for immediate use, and opportunities exist to be involved in follow-up observing and conference travel to disseminate results.
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Project: Supernovae in Luminous Infrared Galaxies
Supervisor: Stuart Ryder
Stars bigger than 8 times the mass of our Sun are doomed to end their lives in colossal explosions we experience as "supernovae". Measuring the rate at which stars explode today is the key to unlocking the star formation history of our Universe, on which so much of cosmology rests. Despite the dedicated efforts of amateur astronomers and robotic surveys, we know we are missing a substantial fraction of supernovae still.
If you wanted to increase your odds of discovering a supernova, where better to look than the so-called Luminous (or even Ultra-Luminous) Infrared Galaxies ("LIRGs") where short-lived, massive stars are being formed more rapidly than anywhere else in the Universe? The trouble is LIRGs are so dusty that even the largest telescopes can barely see into them at optical wavelengths. By observing at infrared wavelengths, we can see deeper into the LIRGs where supernovae could be hiding. Furthermore, we can use the technique of adaptive optics to overcome the blurring effects of the Earth's atmosphere, and help to reveal the supernovae and the stellar clusters in which they form.
We are about to embark on a campaign to find supernovae in LIRGs, using both the Laser Guide Star adaptive optics system on the 8 metre Gemini North telescope, and the Australian-built Gemini South Adaptive Optics Imager, over the next 2 years. Opportunities exist for a PhD student to play a key role in coordinating this campaign, in image analysis, and following up the supernova discoveries at infrared and radio wavelengths, which can in turn allow us to replay the last days in the life of the star before it exploded.
CONTACT US
There are no hard and fast rules for establishing a joint supervision project - every case is unique. Your University, however, will have guidelines for when you must select a project, and for the approval of projects (and supervisors) by the University.
The process for establishing a joint supervision project will usually go something like this
- Talk to your prospective AAO supervisor (in fact you should talk to several).
- Talk to your prospective University supervisor, or the supervisor of the PhD or Honours program at your University.
- Establish with the supervisor of the PhD or Honours program at your University that they are prepared to allow joint supervision.
- There will now be a phase where all three of you work out how the project will work, what hoops the University will require you all to go through, and when.
In general the earlier you start making contact with supervisors before your research project would be due to actually start, the better. For example, getting the ball rolling and talking to prospective supervisors in the July-November period before an Honours project starts in February (though not essential) would be a good idea (though exact timing seems to vary from University to University, with students in some departments choosing projects as late as the first week of the academic year).
PhD programs are generally organized somewhat earlier, with the Australian Postgraduate Award deadline of October 31 being a hard limit forcing students to at least choose what University they are going to do their degree at, which may also involve getting a feel for the kind of research they'd like to do. Once you are accepted for a PhD programme, if you are co-supervised by someone at the AAO you can then apply for one of the AAO top-up scholarships (worth $5000 per year for 3 years). The deadline for these is 1 March.
Please feel free to contact us here at the AAO to discuss your interests, concerns or problems. You can either contact a prospective supervisor directly, or make contact through Andy Bunker (bunker -@- aao.gov.au), the AAO's Head of Astronomy.
FREQUENTLY ASKED QUESTIONS
Will I get paid?
Most PhD studentships are funded through the Australian Research Coucil (ARC) or through scholarships from individual Universities. The Anglo-Australian Observatory has just introduced a scheme of top-up scholarships for students at Australian universities who are substantially co-supervised by an AAO staff member. These grants will be $5000 per annum for 3 years. More details (including an application form) are available here. For visiting undergraduate students, the AAO offers stipends through our AAO Student Fellowships and the Australian Gemini Undergraduate Summer Studentships. There are also Honours scholarships available to joint AAO/Macquarie students. Access to the AAO's computer facilities, and office space at the AAO's Epping offices are provided to PhD/Honours students jointly supervised by AAO staff.Will I get better access to AAT time?
Observing time on the AAT is awarded purely on the basis of scientific merit in a process of peer review of proposals - so in short, no. Having said that, AAO staff are extremely successful in competing for and winning time on both the AAT and other telescopes, so you will receive the best possible assistance in preparing winning proposals.When should I start organising all this?
The details of arranging a research project are given here.