21 years of Astronomy at Warwick: celebrating the legacy of Prof. Tom Marsh
arXiv:2504.20954 · doi:10.1093/astrogeo/ataf009
Abstract
Between the 4th and 6th of September 2024, the Astronomy & Astrophysics group at the University of Warwick held a meeting to celebrate 21 years of astronomy at Warwick and the scientific legacy of the late Prof. Tom Marsh, the group founder. More than a hundred people attended the meeting, with about half of the attendees being external delegates and coming from as far afield as the USA and South Africa. Tom Marsh moved to the University of Warwick from Southampton in 2003, after the Department of Physics decided to expand the scope of its research. From its humble beginnings with only two staff members, Tom himself and Boris Gänsicke, one postdoc and a couple of PhD students, the group has now grown to more than 95 members, including 25 staff. Tom pioneered the development of Doppler tomography, led key discoveries in the field of double-degenerate binary systems and made extensive contributions to instrumentation, primarily to developing the high-speed imaging photometers ULTRACAM, ULTRASPEC and HiPERCAM. This article provides a summary of Tom's legacy and Warwick's history as presented in the 21 years of Astronomy at Warwick meeting.
This is the authors' version of an article featured in Astronomy & Geophysics, Published by Oxford University Press
References in corpus (18)
- ULTRACAM: an ultra-fast, triple-beam CCD camera for high-speed astrophysics
- A radio pulsing white dwarf binary star
- A radio transient with unusually slow periodic emission
- A long-period radio transient active for three decades
- HiPERCAM: a quintuple-beam, high-speed optical imager on the 10.4-m Gran Telescopio Canarias
- Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii
- ULTRASPEC: a high-speed imaging photometer on the 2.4-m Thai National Telescope
- Space Telescope and Optical Reverberation Mapping Project. IX. Velocity-Delay Maps for Broad Emission Lines in NGC 5548
- Coping with loss: Stability of mass transfer from post-main sequence donor stars
- An emission state switching radio transient with a 54 minute period
- A Model for AR~Scorpii: Emission from Relativistic Electrons Trapped by Closed Magnetic Field Lines of Magnetic White Dwarfs
- A transiting brown dwarf in a 2 hour orbit
- Minutes-duration Optical Flares with Supernova Luminosities
- Driving the Beat: Time-Resolved Spectra of the White Dwarf Pulsar AR Scorpii
- Roche tomography of cataclysmic variables - VI. Differential rotation of AE Aqr - Not tidally locked!
- X-ray properties of the white dwarf pulsar eRASSU J191213.9-441044
- Long-term photometric monitoring and spectroscopy of the white dwarf pulsar AR Scorpii
- Nodal Precession of WASP-33b for Eleven Years by Doppler Tomographic and Transit Photometric Observations