About usThe Department is located on its own campus in the beautiful Surrey Hills, surrounded by woodland, and is the UK's largest university space research group. Space science is a discipline that demands highly innovative technologies and the Department has an international reputation for excellence in this area. UCL was one of the first universities in the world to become involved in making scientific observations in space. Since 1966, the Department has participated in over 40 satellite missions with the European Space Agency, NASA (US), Japan, Russia, China and India, and flown over 230 rocket experiments. At the Department, you will join a diverse team focused on the detection and characterisation of transiting exoplanets, led by Dr. Vincent Van Eylen. The research project will be further co-directed by Dr. James Owen (Imperial) and Dr. Paola Pinilla (MSSL/UCL).The Department is family friendly and applications would be welcome from applicants seeking part-time opportunities. The Department has been awarded the Institute of Physics Juno Practitioner. The aim of Project Juno is to recognise and reward physics departments, schools, institutes and organisations that can demonstrate they have taken action to address gender equality in physics and to encourage better practice for all staff.About the roleAn exciting opportunity has arisen for a Research Fellow to join the Department of Space and Climate Physics (Mullard Space Science Laboratory), University College London (UCL).The post will be for three years to work in the research group led by Dr. Vincent Van Eylen, Associate Professor in Exoplanets.The post is funded under the Grant award from the UKxe2x80x99s Science and Technology Facilities Council (STFC). The funding is awarded to pursue xe2x80x9cUnderstanding the evolution of Neptune-like planets over billions of yearsxe2x80x9d. The successful candidate will address major open questions relating to how exoplanet properties are linked to stellar ages. They will investigate how the properties of planetary systems are related to their age, as the evolution of the galaxy shapes the formation of planetary systems, and as planetary systems evolve over time. This research will make use of state-of-the-art Bayesian techniques to derive reliable ages combining stellar observations from high-resolution spectroscopic observations and Gaia measurements, as well as potentially asteroseismology. Large data sets from the ongoing NASA Transiting Exoplanet Survey Satellite (TESS) and the upcoming ESA Planetary Transits and Oscillations (PLATO) missions are expected to drive this research. A key goal of this project is the determination of accurate and precise stellar ages for a large sample of small extrasolar Earth and Neptune planets, and pairing this stellar characterisation with a detailed study of planet properties, in particular planet occurrence. A key deliverable of this research will be to show for the first time whether Neptunes exhibit significant evolution over main sequence time scales, as Neptunes may turn into Earths due to ongoing atmospheric loss over billion-year timescales, see their sizes change as their atmospheres evolve and shrink, or even have different properties depending on when they form due to galactic chemical evolution. This research will have profound implications for our understanding of small close-in planets, which make up most of all known exoplanets.About youThe post holder will focus on quantifying the population of Neptune-like planets as a function of their host star characteristics. This includes detecting Neptune-like planets using TESS observations and quantifying their occurrence rate, as well as precisely determining stellar properties including stellar ages. Furthermore, the successful applicant is expected to contribute towards preparing for the upcoming PLATO mission. In addition, the candidate is expected to develop and pursue independent research ideas and interact with a wide variety of exoplanet researchers at the Department and the University.Applicants must have (or be about to receive) a PhD degree in astronomy, physics, astrophysics, mathematics, computer science, or a closely related discipline. The ideal candidate will be experienced in one or more of the following areas: exoplanet characterisation, stellar characterisation, exoplanet detection, time series photometry, planet occurrence rate determination, asteroseismology, space photometry related to TESS or PLATO, Bayesian statistics, machine learning, computational methodsCandidates should submit: 1) an application form, 2) a research statement (max. 3 pages), 3) a CV including the names of three references (max. 2 pages), and 4) a list of publications. The research statement should summarise your main research achievements to date and highlight your research interests and fit for the position. Informal inquiries can be directed to Dr. Vincent Van Eylen ( ).What we offerAs well as the exciting opportunities this role presents, we also offer great benefits some of which are below:
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