Summer Research Programme 2. We anticipate taking about 8 students, and students from the second year and above are welcome to apply. Applications are welcome from institutes outside of Oxford. Unfortunately, due to UK visa regulations, we are only able to accept applications from candidates within the EU. Students will work with a supervisor in the department, usually a postdoctoral researcher or lecturer, on a self- contained research project. There will also be some lectures on current astrophysics topics. Students are encouraged to take part in department life, joining researchers for coffee, discussions and seminars. The projects run for typically 8 weeks, nominally July 4th - August 2. The duration may be adjusted to be shorter or longer, or to accommodate summer travel. Students will be paid via a stipend (provisionally . The project is full- time but hours can be discussed with your supervisor. You should email a one- page- only application, in pdf format, to Ashling Morris (Ashling . Offers will be made in March. On your 1- page application you should tell us why you are interested in the programme and which project(s) most interest you. Also include your contact details, your year and course, any undergraduate exam results so far, and contact details (including email) of your academic referee. Please also mention any computer programming experience and any previous research experience. You are encouraged to informally contact the supervisor(s) to find out more details about the projects that interest you. For any administrative queries, contact Ashling Morris (Ashling . Here are the projects that were available for 2. They span a range of our interests. Most of the research activity involves analytic and computing work. Searching for transients in the VISTA VIDEO survey.
Supervisors: Dr Rebecca Bowler and Prof. Matt Jarvis The VISTA VIDEO survey provides exquisite imaging in the near- infrared of over 1 million galaxies. Active Galactic Nuclei (AGN) have been proposed as candidates. These sources consist of a super- massive black hole surrounded by an accretion disc in the centre of a galaxy, from where bipolar outflows of relativistic plasma are ejected transversely to the disc plane. In some cases, bright radio synchrotron knots (hotspots) are detected at the jet termination region, where particles accelerated by diffusing back a forth the jet reverse shock emit synchrotron radiation. We will use available data with high spatial resolution at different wavelengths (from radio to X- rays) to model the emission in the new framework of magnetic field damping. This project will introduce the student to the AGN phenomenology, and the basic theory of shock particle acceleration and non- thermal emission processes such as synchrotron radiation and inverse Compton scattering, as well as basic ideas of plasma astrophysics. Basic computer skills are required. Exploring models of intrinsic galaxy sizes. Supervisors: Elisa Chisari. Galaxies come in different sizes, and their sizes are connected to their formation history and their environment. Recently, several models have been developed that link galaxy sizes to the statistical distribution of matter in the large- scale structure of the Universe. In this summer project, we will extend those models to account for different galaxy properties. For example, we will construct a model that is different for elliptical and spiral galaxies and that connects their sizes to the underlying large- scale structure of the Universe. Basic skills in cosmology and statistics are desirable. This is mostly a theory project but if time allows, it might be possible to construct model templates using C or Python programming language. Characterisation and classification of dark matter halos. Supervisors: Julian Merten. This project will make use of computer vision and digital image processing techniques to first characterise and then classify dark matter maps of halos ranging from galaxy to galaxy cluster scales. Starting from numerical simulations of such objects, 2. D projections of their matter density fields are created, very similar to the concept of an image. On these images, existing algorithms of digital image processing are applied to extract the most fundamental few numbers that characterise the image. In a final step, pattern recognition classifiers use these numbers to classify and group the images and hence the underlying dark matter halos. Interest and basic knowledge in coding and numerical algorithms. Preferential programming languages are C(++), Python, eventually Matlab. A basic knowledge in cosmology is appreciated but not strictly required. Exploring Galaxy Evolution with Galaxy Zoo. Supervisors: Chris Lintott. The Galaxy Zoo project has provided reliable morphological catalogues of galaxies out to a redshift of z~1. This project will use this data to explore galaxy evolution, for example by investigating our sample of bulgeless galaxies, systems which have grown despite a lack of major mergers. The project requires moderate computing skills (or a willingness to learn) and would suit someone who is also interested in outreach. Velocity reconstruction in cosmology. Home Degree Abroad Astronomy & Astrophysics Degree Programs. Undergraduate Programs; Graduate Programs; Undergraduate. The undergraduate Astrophysics program at IIT is designed as an introduction to the physics behind. Which universities have the most respected astrophysics/astronomy research. Astrophysics programs. Undergraduate research programs in Indian research institutes. Inter-University Centre for Astronomy and Astrophysics. India (IISER TVM) Max. See the top ranked cosmology, relativity. Use the best physics program rankings to find the right astrophysics program for you. Find Graduate Programs. Students searching for Become an Astrophysicist: Education and Career. Astrophysicist: Education and Career Roadmap. Undergraduate programs in astrophysics. Top Undergraduate Programs in Physics. Supervisors: David Alonso. The interplay between the density and velocity fields in the Universe holds an enormous amount of information to understand the nature of gravity on cosmological scales. However, measuring velocities in astronomy is challenging, and it is of vital importance for future galaxy surveys and CMB experiments to have robust methods to recover it from astronomical datasets. The idea for this summer project is to design and test different algorithms to reconstruct the velocity field in cosmological surveys, and to quantify the impact of these methods on future experiments. A reasonable level of programming (preferentially C or Fortran, and Python) would be desirable. Some experience with Fourier methods could also come in handy, but is not indispensable. Standard Big Bang Nucleosynthesis (SBBN)Supervisors: Khalil Chamcham. Big Bang (primordial) nucleosynthesis is one of the robust components of the standard model of cosmology – the others being the discovery of Hubble expansion and the CMB. Observations of primordial elements abundances of D, 3. He, 4. He and 7. Li set robust constraints on the standard (or base) Lambda. CDM model, particularly by constraining the baryon fraction which is strongly correlated to the D abundance. The recent Planck data (as well as WMAP data) measured the standard LCDM and BBN parameters to such a high precision, making SBBN a parameter free model. The aim of this summer project is to map the parameter space of SBBN within the base LCDM model as constrained by Planck and WMAP data and to analyse the sensitivity of SBBN output to their variations (and to the variation of the fundamental constants) as well as their implications on further production of heavier elements such as C, N and O. One of the possible questions to discuss is whether there is a case for fine- tuning of the parameters of SBBN and LCDM and whether the currently observed abundances are heavily constrained by these fine- tuned parameters. Programming in C++/Python and Java script, familiarity with web programming. The student is expected to review and compile the major ingredients of both SBBN and LCDM models and to develop a comprehensive picture of the formalism involved. KIDSPEC development. Supervisors: Sumedh Mahashabde & Kieran O’Brien. KIDSpec is a concept of a Ultraviolet/Visible/Infrared spectrograph based on superconducting Microwave Kinetic Inductance Detectors (MKIDs). These detectors are capable of detecting the arrival time of individual photons and are also energy sensitive. Thus each MKID pixel is capable of obtaining the spectrum of light falling on it. MKIDs are potential candidates for replacing CCD based photodetectors in the future. We are currently designing a lab- based demonstration of the system and are looking for a student to aid in the assembly and testing phases of the project. This summer project will involve aiding with the assembly of the spectrograph and its associated readout electronics and optics. The MKID array and microwave circuit components will be mounted in a cryostat that will be cooled to < 1. K. The readout system which is based on the Reconfigurable Open Architecture Computer Hardware (ROACH) board will be rolled out. The optical system will use a grating linked to a fiber- optic illumination system. The student has the opportunity to gain practical, hands- on experience in a range of areas in this cutting- edge Astronomical Instrumentation project. The exact project will be tailored to the student's interests, but they could participate in the cryogenic assembly of the system, the testing of the MKID readout or the optical calibration system. Prior experience of data analysis with Matlab/Simulink or Python is a bonus but not mandatory. The Apparent Fine- Tuning of the Cosmological Constant. Supervisors: Rafael Alves Batista. Observational cosmology is at its golden age with high precision experiments such as the Planck satellite measuring the cosmic microwave background with unprecedented precision. In the cosmological model in vogue, the Lambda- CDM model, the universe is flat (or very close to it), with a conspicuous component accounting for the majority of the energy density of the universe, which can be the dark energy or cosmological constant, and a smaller contribution from baryonic and dark matter. The cosmological constant has a very small value which cannot be explained by fundamental physics. A consequence of this apparent fine- tuning is that changes in the value of this constant may affect the growth of structures such as galaxies, rendering life impossible. Although the underlying theoretical framework of Lambda- CDM is well understood, it is interesting to study alternative models to explore the consequences of ``untuning'' the cosmological constant. Best Astronomy Undergraduate Programs? I have recently been in contact with a high school student who wants to pursue Astronomy and he’s got me thinking: What are the best undergraduate programs for budding astronomers? And the places with top- notch Ph. D programs are probably also gonna have top- notch undergrad programs. But some of those top- notch departments don’t actually offer very many astro courses at the undergraduate level. What are the places that actually have really outstanding undergrad programs? Northern Arizona University, Villanova, and Swarthmore come to my mind. None have Ph. D programs, but they do a lot of astro and clearly put an emphasis on undergraduate education. Thomas Arny put together a compilation of all the undergrad programs, but that page hasn’t been updated since 2. I’m more interested to know which programs you think are notable. What are the institutions you know of that offer both research opportunities for undergrads and an array of astro courses at the undergrad level?
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