- Astronomers and the AAO
- What do we do?
- AAO Honours Scholarships
- Honours projects
- AAO PhD Scholarship - Deadline 15 March
- PhD projects
- Contact Us
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.
The Australian Astronomical Observatory now offers a $5000 scholarship for Honours students enrolled at any Australian university, for a research project substantially co-supervised with an AAO staff-member. You can apply using this application form in Word format or this application form in pdf format. The deadline for applications is 1 March. Any questions about the AAO Honours Scholarships or the application process can be directed to the Head of AAT Science at the AAO, Andrew Hopkins (ahopkins -@- aao.gov.au).
In addition, we also support jointly-funded Honours scholarships with Monash University (details on the Monash website) and jointly-funded Masters scholarships with Macquarie University (for details contact Quentin Parker, qap -@- aao.gov.au). Students wishing to apply for these scholarships should use the relevant application form from the host university, and follow the instructions on their web pages.
The Australian Astronomical Observatory manages 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 on the AAO PhD Scholarship Scheme webpage. The deadline
for PhD scholarship scheme applications is 15 March.
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.
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 on their personal
web pages, linked from the AAO Science page,
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
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.
Some potential honours projects are described 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 the AAO's Head of Instrumentation, or Jon Lawrence for Instrument Science group. Quentin Parker (AAO/Macquarie Lecturer, qap -@- ics.mq.edu.au) and Dan Zucker (AAO/Macquarie Lecturer, zucker -@- ics.mq.edu.au) can also be contacted for information on Honours Projects through Macquarie University. PhD students who undertake brief (3 month) research projects in their first year, prior to starting their main thesis project can be co-supervised by AAO astronomers in such projects, and some of the Honours projects below may be suitable for this.
Project: 2D spectroscopic analysis of local dwarf star-forming galaxiesSupervisor: Angel Lopez-Sanchez and Heath Jones (Monash)
The new observational technique of 2D spectroscopy using Integrated Field Units (IFU) is providing amazing new results about the kinematics and the chemical composition of galaxies. In particular, Blue Compact Dwarf Galaxies (BCDGs) are excellent targets to perform such studies, because their modest sizes allow that all the galaxy can be observed in just some few pointings. During the last year we have collected some 2D spectroscopy data of a sample of BCDGs using the new WiFeS instrument available at the 2.3m ANU telescope at Siding Spring Observatory, and the preliminary results are quite promising. We are offering the opportunity of study one or two of the BCDGs for which we already have good-quality data. In particular, this project will give to the Honours student an introduction to 2D spectroscopy techniques (we expect to continue the observations using both WiFeS @ 2.3m ANU and SPIRAL @ 3.9m AAT) and to gain some expertise in the reduction and analysis of this kind of data. The aims of this project is to perform an analysis of the physical (mass, star-formation rate, extinction, electron temperature and density, excitation), chemical (ionic and total abundances of helium, oxygen, nitrogen, sulphur, neon, argon...) and kinematical properties of the ionized gas within these galaxies, which may be compared with the properties of the neutral gas from our own ATCA observations. Finally, the student will also learn to write up the results not only for his/her Honours Thesis but for a subsequent publication. As an example of this project, please consult the 2D spectroscopical analysis of the brightest star-forming region of the local BCDG IC10, López-Sánchez et al. (2011) and this research image.
Project: The nature of the extraordinary supernova SNLS-06D4euSupervisor: Chris Lidman
With the advent of wide field patrol surveys, such as the Palomar Transit Factory and SkyMapper, we are entering an exciting era of discovering new types of transient phenomena. Hints of what might be discovered in the not too distant future are emerging from the analysis of data from much smaller surveys, such as the Supernova Legacy Survey or SNLS for short. SNLS-06D4eu is one such discovery. It is one of the most luminous and most distant supernova ever discovered. It is not clear what drives the explosion. One possibility is that it is a pulsating pair-instability supernova. Theory suggests that the progenitor of a pulsating pair-instability supernova undergoes two massive mass loss events. The supernova occurs when the mass ejected from the second event catches up to the first one. If SNLS-06D4eu is such a supernova, then there might be evidence of the first mass loss event in data that was taken up to three years before the supernova was discovered. The goal of this project is to analyse data taken before (and after) the SNLS-06D4eu was discovered and to search for evidence of additionally variability in this source.
Project: From Red Giants to Planetary NebulaeSupervisor: David Frew (MQ) and Quentin Parker (MQ/AAO)
A planetary nebula is a short-lived, glowing shroud around a dying low-mass star. It is formed when a bloated red giant star ejects its outer layers, revealing a very hot, contracting stellar core. A high velocity wind and intense ultraviolet radiation from this stellar remnant can sculpt and ionize the shed layers of gas, as the core becomes a white dwarf. However, the transition between the end of the red giant phase and the onset of nebular ionization is still poorly understood. Current images of the ejecta of stars going through this so-called pre-planetary nebula (PPN) phase are strikingly heterogeneous. This suggests there may be a range of physical mechanisms that govern the bizarre and differing morphologies of these objects, making it a highly topical area for study. In this project, the student will begin by determining new distances to a large sample of PPNs by modeling their spectral energy distributions. This is via established techniques and will use extensive published and unpublished multi-wavelength data across a broad range of the electromagnetic spectrum. This new distance information will allow the student, for the first time, to generate a robust volume-limited sample of PPNs in order to facilitate a powerful statistical study based on a careful evaluation of the derived energy distributions and other properties such as morphology and location. The results from this important study will provide fresh insights into this intriguing astrophysical phenomenon.
Project: Celestial wheat from chaff: Identifying Planetary Nebulae contaminantsSupervisor: Quentin Parker (AAO/MQ) and David Frew (MQ)
Planetary nebulae (PN) are the mysterious glowing shrouds of dying low mass stars. PN play a major role in the ecology and evolution of our Galaxy, they are of key importance in understanding late-stage stellar evolution, have considerable power as kinematic tracers (shedding light on dark matter), are unrivalled laboratories of plasma physics and provide potent cosmological distance indicators. This significant astrophysical potential of PN is currently seriously undermined by the presence of PN mimics that contaminate earlier samples and bias any scientific analysis and interpretation. Indeed, we have recently shown that ~20% of objects accepted as nearby PN are actually ionised regions in the interstellar medium around unrelated hot white dwarf or sub-dwarf stars while we have also shown via mid infra-red and radio comparisons that 47% of known pre-MASH PN at very low Galactic latitudes are actually compact HII regions. We have tested and adopted a range of criteria to eliminate such contaminants. Only the recent on-line availability of imaging surveys and other multi-wavelength data has enabled these clear discrimination tools to be developed. In this project the student will undertake a careful multi-wavelength study of the ~1000 PN in the ESO Catalogue of Galactic Planetary Nebulae using newly developed diagnostic photometric and spectroscopic criteria and via recent availability of large-scale multi-wavelength data. The work involves spectroscopic and line ratio measurement and analysis (including determination of temperature, density and where possible crude abundances) and multi-photometric comparison across optical, infrared and radio data. The very latest data from the WISE space telescope will also be incorporated. The results will be the robust multi-wavelength identification of PN contaminants and separation into their interesting classes that will be a legacy of considerable value to the astronomical community.
Project: Focal Ratio Degradation and Loss in Fibers for new AAO instrumentationSupervisor: Mike Ireland The Australian Astronomical Observatory is a world leader in fiber-fed spectrographs for astronomy. These are the workhorses for measuring the redshift of distant galaxies, the elemental abundances of stars throughout our galaxy and form the core of the next generation of hyperspectral imaging instruments. The greatest problem with these instruments is a spreading of the range of angles due to a variety of effects in the fiber, known as focal-ratio degradation (FRD). In this project, you will build on previous work at the AAO to form a comprehensive model of FRD based on laboratory measurements, to inform decisions such as the optimal fiber type for the next generation of AAO instruments.
Project: Calibration for Compact Astronomical Spectrographs for Planet SearchSupervisor: Mike Ireland Calibration of astronomical spectrographs is a key part in achieving the meter per second Doppler velocity precision needed to detect planets around other stars. The difficulties in calibration have driven US-based planet search teams to use lossy Iodine absorption cells, and European teams to make very expensive vacuum spectrographs calibrated by complex frequency-comb lasers. In this project, you will trial and model different cost-effective methods for calibrating the single-mode spectrograph to be used for planet search at Macquarie University observatory, nearby to the AAO. These methods will include the traditional Th-Ar reference lamp, temperature-controlled glass cavities and a Fabry-Perot cavity locked to a stabilized laser. Results from this project will have the potential to drive the technology for the next generation of planet searches.
Project: Unveiling the nature of passive galaxies using GAMA and SDSS dataSupervisors: Maritza Lara-Lopez and Angel Lopez-Sanchez The Mass/Star formation rate (SFR) relation in galaxies is a well known relation formed by a main sequence when SFR increases with stellar mass. Using GAMA and SDSS galaxies we have identified a population of passive galaxies in the mass-SFR relation that form a second "main sequence" at very low SFRs. We have catalogued a total of ~100 of these passive SF galaxies for SDSS, and ~300 for GAMA. These galaxies have been classified as SF galaxies, although they show very low SFRs, an elliptical-type morphology, and very low obscuration values. Since that population of galaxies is formed by fainter galaxies with low emission line fluxes, we will perform individual measurements of the fluxes of all detected emission lines using IRAF following the prescriptions given by Lopez-Sanchez & Esteban (2009,2010). Using this method we will get, at the same time, the reddening and the stellar absorption correction to the Balmer lines. With these data, we will get a better characterization of the sample galaxy in the BPT diagrams, as well as measuring SFR and metallicities in a more reliable way for this low emission line population. We will locate the galaxies in a mass-color diagram to unveil their nature as possible galaxies migrating from the blue cloud to the green valley. Although those galaxies have been classified as SF galaxies in the BPT diagram, we suspect that an active nucleus contribution is feasible in some of them.
Project: The Composition of Stars in Clusters - Tracing the Chemical History of the GalaxySupervisors: John Lattanzio, Simon Campbell (Monash), Gayandhi de Silva (AAO), Brad Gibson (U Central Lancashire, UK, visiting Monash in 2012)
Most stars are born in clusters. The oldest and most populous are the globular clusters which orbit our Galaxy. Within the galaxy itself are younger, less populous "open clusters". Recent studies have shown that the stars in globular clusters show chemical element abundance patterns that are unique to the clusters. We do not know why they are not seen in the Galaxy, but only within the globular clusters. Is it possible for similar patterns to appear in open clusters? Preliminary observations suggest that they do not, and that the stars within a given open cluster all have the same abundances. But how does the composition of the open clusters as a population compare to the patterns seen in the globular clusters? Are the open clusters showing a similar chemical enrichment history or a different history? It is proposed to collect data from the literature on the abundances in various open clusters and to compare these to the patterns seen in globular clusters. Do the open clusters show the sort of enrichment history that is seen in the Galaxy overall? Or do they share some of the patterns seen in globular clusters? The project will involve understanding stellar nucleosynthesis as well as the chemical evolution of the Galaxy, and work with a computer codes that calculate these properties. This project will involve travel to the Australian Astronomical Observatory (in Sydney) to visit and work with Dr de Silva.
Project: Spectroscopy and the Composition of Stars in Globular ClustersSupervisors: John Lattanzio, Simon Campbell (Monash), Gayandhi de Silva (AAO)
Globular clusters are the oldest and most populous stellar aggregates in existence. Recent studies have shown that the stars in globular clusters show abundance patterns that are unique to the clusters. We do not know why they are not seen in the Galaxy, but only within the globular clusters. They may even be the remnants of collisions between dwarf Galaxies and our Milky Way. A fuller understanding requires us to determine the abundances of many stars in many clusters and to compare with theoretical models so we can see what stars produced the existing patterns. Project: We will source original data form the world's largest telescopes and then analyse this to determine the abundances of key species in globular cluster stars: perhaps Li, C, N, O, Mg, Al, Fe as well as the heavy elements made by neutron capture, such as Sr, Y, Zr, Ba, La. Stellar models that can produce these species will be compared with the abundances we measure. This project will involve travel to the Australian Astronomical Observatory (in Sydney) to visit and work with Dr de Silva. There is also the opportunity to visit and observe with the 4m Anglo-Australian Telescope in Coonabarabran, NSW.
Project: The Rate of Deep Mixing in Red Giants as a Function of Stellar MetallicitySupervisors: Sarah Martell
It is well established that red giants experience continuous mixing between their atmospheres and their hydrogen-burning shells: one consequence of this is a constant removal of carbon from the atmosphere due to the CNO-cycle fusion occurring in the hydrogen-burning shell. The exact process responsible for the mixing is unknown, though it is a subject of ongoing research and simulation. Models by Charbonnel, Denissenkov, and Lattanzio are all qualitatively consistent but different in the details, predicting more vigorous mixing in lower-metallicity stars because of a less compact internal structure. In Martell & Smith 2009, I determined carbon abundances for red giants in globular clusters across a wide range of metallicity and found that the carbon depletion rate is twice as large in the lowest-metallicity cluster in the data set as in the highest-metallicity cluster in the data set. I have additional, analogous spectra at the high- and low-metallicity ends of that data set, and would like to analyze them in a similar fashion, to confirm the result. IDL and FORTRAN programs exist for generating large grids of synthetic spectra and using them to derive carbon abundances and depletion rates from the observed spectra. The student is free to use existing programs, to adapt them, or to develop a new analysis method, depending on their level of experience with programming.
Project: Katabatic Weir PoolsSupervisors: Will Saunders and Jon Lawrence
The Antarctic Plateau contains the driest, coldest and clearest astronomical sites on Earth. However, the katabatic winds flowing down off the Plateau create a turbulent surface boundary layer, tens of metres thick, within which the seeing is degraded. Various terraforming methods have been proposed to modify this boundary layer, including the creation of a 'weir pool' where the flow is temporarily deepened and slowed as it flows around the telescope. Such weir pools occur naturally, and are associated with the coldest temperatures ever recorded on Earth. A series of models will be devised and tested, to find suitable geometries. The project requires a strongly motivated student with some existing knowledge of FEA (Finite Element Analysis) or CFD (computational fluid dynamics) modelling.
Project: Starbugs Robotic Fibre Positioners - Characterization and OptimizationSupervisors: James Gilbert (Engineer), Michael Goodwin (Instrument Scientist)
The AAO is a world leader in multi-object fibre spectroscopy, which uses optical fibres to observe hundreds of objects in the sky at once. When an astronomer wants to observe a new set of objects, these fibres must be repositioned within the telescope's field of view - a task typically performed by a 'pick-and-place' robotic arm. The problem with pick-and-place fibre positioning is that it takes a long time to reconfigure what can be hundreds of individual fibres. The process can also be cumbersome due to the way in which delicate fibres have to pass over one another.
Starbugs are miniature 'walking' robots that are being developed at the AAO to enable fast and accurate parallel positioning of optical fibres. This is achieved by giving each fibre its own robotic 'legs' made from piezoelectric actuators; it means that instead of a field reconfiguration taking up to an hour to complete, it can be achieved in just a few minutes. Starbugs present huge gains for future astronomical instrumentation.
In this project you will play a direct part in the development of Starbug technology, helping to characterise and optimise the way Starbugs move and the way they are controlled. This may include analysis and modelling of piezoelectric actuator performance, use of nanometrology devices to identify inefficiencies in the way Starbugs move, investigating better ways to drive Starbugs through waveform shaping, or looking at how changing the geometry of a Starbug affects its performance. This project would suit a science or engineering student. No prior knowledge of astronomy is required.
Project: Starbugs Robotic Fibre Positioners - Routing Algorithms and SimulationsSupervisors: Michael Goodwin (Instrument Scientist), James Gilbert (Engineer)
Starbugs fibre positioning technology is one of the R&D projects here at the AAO and a key technology for the MANIFEST (many instrument fibre system) concept for the Giant Magellan Telescope for 2020. The Starbugs technology for MANIFEST involves miniature piezoelectric robotic devices that simultaneously 'walk' underneath a thin glass field plate to position optical fibre(s) at precise positions. The optical fibres then 'catch' the star light of the telescope to feed astronomical spectrographs. The optical fibres can be placed in parallel with Starbugs to significantly reduce the configuration time to several minutes. Starbugs technology enables the Giant Magellan Telescope to be the most powerful Extremely Large Telescope for survey astronomy. The AAO has successfully demonstrated Starbugs technology in the laboratory as part of the MANIFEST feasibility study, which can be seen in this movie.
In this project you will assist in the development of routing algorithms and simulations to optimize the field configuration. This involves the development of Matlab model to explore the optimal field configuration algorithms and performance for an arbitrary sized field plate and number of Starbugs for the MANIFEST instrument concept. The model can use pre-measured laboratory data that characterizes the performance of the current vacuum 'lift-and-step' Starbugs. The model should explore algorithms to prevent fibre entanglement and other criteria specified by the MANIFEST instrument concept documentation. The model can be functionally tested with actual hardware using the Starbugs test-rig. This project requires no prior knowledge of astronomy.
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 Andrew Sheinis, the AAO's Head of Instrumentation.
Project: Evolution of the most massive galaxies.Supervisor: Sarah Brough
One of the pressing, unanswered questions in astronomy is why the most massive galaxies in the Universe are not observed to have grown in mass as much in more recent times as galaxy models suggest that they should. A possible solution is that the galaxies which models predict to merge with the most massive galaxies may actually be destroyed into diffuse stellar regions from their previously bound states. This solution would also explain the origin of diffuse, stellar haloes observed around some of the most massive galaxies: Brightest Cluster Galaxies (BCGs). BCGs are massive elliptical galaxies found at the centres of groups and clusters of galaxies. Those with diffuse stellar haloes are referred to as cD galaxies.
This project would utilise data from the multi-wavelength imaging and spectroscopic Galaxy And Mass Assembly (GAMA) survey to determine BCGs in the survey, creating one of the largest and certainly widest redshift range samples of BCGs. The surface brightness profiles of these galaxies would then be characterised in order to determine which BCGs have cD haloes and the relative amounts of mass in each component. Utilising the multi-wavelength data it will also be possible to determine colours for these components and therefore a picture of their origins (whether from massive evolved galaxies or those still forming stars). Comparing how the fraction of mass in the halo changes with BCG mass, group mass and time with the models available will tell us whether this is a reasonable solution to the question of how massive galaxies evolve.
Project: Supernovae and Star Formation in Luminous Infrared GalaxiesSupervisor: 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.
Beginning in 2008 we embarked on a campaign to find supernovae in LIRGs, using the Laser Guide Star adaptive optics system on the 8 metre Gemini North telescope, and have already discovered 2 supernovae. From 2012 we will expand the search to southern hemisphere LIRGs using the Australian-built Gemini South Adaptive Optics Imager. Opportunities exist for a PhD student to play a key role in coordinating this campaign, in image analysis, and following up the supernova discoveries they make at infrared and radio wavelengths. In addition to discovering supernovae, the student will use the resulting LIRG images (the sharpest and deepest ever obtained) to work out what drives the extreme star formation in the first place.
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 15 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 Andrew Hopkins (ahopkins -@- aao.gov.au), the AAO's Head of AAT Science.
Will I get paid?
Most PhD studentships are funded through the Australian Research Coucil (ARC) or through scholarships from individual Universities. The Australian Astronomical Observatory manages 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 on our AAO PhD Scholarship Scheme webpage. 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 in the Contact Us section.
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