The Astronomy and Astrophysics group at Warwick started in September 2003 with the appointment of Prof Tom Marsh. We are interested in stars and planets, how they live and how they die, and the exotic physical processes that they allow us to explore. We are both an observational and theoretical group, and we make use of a wide range of ground-based telescopes, such as ESO's Very Large Telescope (VLT) in Chile and the Isaac Newton Group of telescopes (ING) in the Canary Islands, as well as space telescopes such as NASA's Chandra and ESA's XMM-Newton X-ray observatories and the Hubble Space Telescope.
The objects we study are dynamic and can change within minutes, seconds and even milli-seconds. We specialise in the high-speed data acquisition and analysis techniques needed to track them. Members of the group have contributed to the development and exploitation of the ULTRACAM high-speed photometer, the Wide Angle Search for Planets project (WASP), the Next Generation Transit Survey (NGTS) and are preparing to deploy the Gravitational Wave Optical Transient Observer (GOTO) . We are also heavily involved in the development of space missions including ESA's Exoplanet missions - PLATO (launch 2024) and CHEOPS (launch 2018).
01 October 2016: The Department of Physics at the University of Warwick, UK, seeks to appoint up to three academic posts in the area of Exoplanets, see the job add on jobs.ac.uk or on the AAS job register.
30 August 2016: The solar system could be thrown into disaster when the sun dies if the mysterious ‘Planet Nine’ exists, according to research from the University of Warwick.Dr Dimitri Veras in the Department of Physics has discovered that the presence of Planet Nine – the hypothetical planet which may exist in the outer Solar System - could cause the elimination of at least one of the giant planets after the sun dies, hurling them out into interstellar space through a sort of ‘pinball’ effect. Read the press release and the paper on arXiv.
27 July 2016: A Warwick-led study published in Nature presents the discovery of a pulsar- like white dwarf binary. The system, which is known as AR Sco, emitts across the whole electromagnetic spectrum, all the while pulsing intensely on a two minute period. Read the press release, the paper on ArXiV or see the movie (and more). Image credit: Mark Garlick/University of Warwick.
25-29 July 2016: EuroWD16. The University of Warwick will host the 20th European White Dwarf Workshop. This meeting cover the structure and evolution of white dwarfs, as well as a wide range of astrophysical problems in which white dwarfs play a central role, such as SN Ia progenitors, the local star formation history, and evolved planetary systems.
7 Jan 2016: Out-of-Town RAS Meeting "The future of Astronomy and Planetary Science in the Ultraviolet". The University of Warwick will host an RAS 'Out of Town' meeting on Thursday 7th January 2016. This meeting will be on current UK research at Ultraviolet wavelengths, covering both planetary science remote sensing and astrophysics topics.
15 Dec 2015: Dr. Pier-Emmanuel Tremblay, Assistant Professor in Warwick, has been awarded a 1.5 million Euro Starting Grant from the European Research Council (ERC). The research project entitled "Evolution of white dwarfs with 3D model atmospheres" will soon recruit 1 PDRA and 3 PhD students to work on theoretical aspects of white dwarf research, in close connection with the observational work currently accomplished within the Warwick astronomy group.
11 Nov 2015: Astronomers from Warwick University have captured for the first time and image of an asteroid being ripped apart by a dead star and forming a glowing debris ring. Read the Warwick press release, and the preprint from ArXiv. Image credit: Mark Garlick/University of Warwick.
25 June 2015: Published in the journal Nature, a team including Warwick astronomer Peter Wheatley has discovered a giant comet-like tail of hydogren gas evaporating from a Neptune-sized exoplanet. The gas is thought to be boiled off by X-rays from the parent star and then swept away by radiation pressure. The tail was revealed in Hubble Space Telescope observations in which 56% of the star is covered by the tail in ultraviolet light. The planet is losing its atmosphere at a rate of 1000 metric tonnes per second, having narrowly escaped total evaporation by the intense X-ray irradiation it suffered when its parent star was young and active. Read the Warwick press release, the full journal article in Nature, or the preprint from ArXiv. Image credit: Mark Garlick/University of Warwick.
See for example coverage by the Washington Post, and the Daily Mail.
24 June 2015: The Warwick astronomy group has been very successful in the latest round of time allocation on the Hubble Space Telescope, and will lead six projects in the forthcoming Cycle 23, including a 67-orbit GO program and a 75-orbit snapshot program: Boris Gänsicke (An HST legacy ultraviolet spectroscopic survey of the 13pc white dwarf sample and The frequency and chemical composition of rocky planetary debris around young white dwarfs: Plugging the last gaps), Mark Hollands (The dawn of rocky planet formation), Andrew Levan (The late time behaviour and environments of the first gravitational wave transients), Chris Manser (A highly dynamical debris disc in an evolved planetary system) and Elizabeth Stanway (Understanding the star formation environment of a very low redshift, low luminosity, long Gamma Ray Burst). These observations were facing an oversubscription of approximately six to one.
7 May 2015: A research team led by Warwick astronomers Roberto Raddi and Boris Gänsicke have found that water delivery via asteroids or comets is likely taking place in many other planetary systems, just as it happened on Earth. Read the Warwick press release and the paper in the Monthly Notices of the Royal Astronomical Society.
14 January 2015: Warwick astronomers have begun searching for small planets around bright stars using an array of twelve robotically-controlled telescopes. The telescopes, which form a wide-field observing system called the Next Generation Transit Survey (NGTS), are designed to detect the slight dimming of a star when a planet passes across its face. The NGTS team aims to find planets the size of Neptune down to twice the size of the Earth. Dr Peter Wheatley, one of the NGTS project leaders, said "The NGTS discoveries, and follow-up observations by telescopes on the ground and in space, will be important steps in our quest to study the atmospheres and composition of small planets such as the Earth.”
Read more in press releases from ESO and Warwick.
See also regional BBC News coverage.
08 August 2014: A research team led by Warwick astronomers Joe Lyman and Andrew Levan have investigated the locations of peculiar 'calcium-rich' supernovae, which are often seen to explode at huge distances from any nearby galaxy. They postulate the merger of white dwarf-neutron star binary systems 'kicked' from their galaxy may explain these remote locations. The Warwick press release can be found here.