ULTRACAM operations

Lead Research Organisation: University of Sheffield
Department Name: Physics and Astronomy

Abstract

ULTRACAM is a digital camera capable of taking (and storing) up to 500 red, green and blue images per second. The instrument was built in just under 3 years by a consortium from the Universities of Sheffield, Warwick and the UK Astronomy Technology Centre in Edinburgh, using a £300,000 grant awarded by PPARC. ULTRACAM saw 'first light' on 16 May 2002 on the 4.2-m William Herschel Telescope (WHT) on La Palma, and first light on the 8.2-m Very Large Telescope (VLT) in Chile on 4 May 2005. To date, ULTRACAM has been awarded a total of 92 nights of time on these telescopes for projects as varied as white dwarfs, brown dwarfs, asteroseismology, pulsars, black-hole/neutron-star X-ray binaries, eclipsing binary stars, gamma-ray bursts, cataclysmic variables, extrasolar planets, active galactic nuclei, Kuiper Belt objects and Saturn's moon Titan. This grant proposal requests funding for the proper maintenance and operation of ULTRACAM, as well as a modest programme of minor upgrades, thereby ensuring that ULTRACAM maintains its position as the world's premier instrument for high-speed optical astrophysics. As well as maximising the return on PPARC's original investment, this money will also allow us to continue to offer ULTRACAM to others in the UK and astronomical community who wish to use it.

Publications

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Copperwheat C (2010) Physical properties of IP Pegasi: an eclipsing dwarf nova with an unusually cool white dwarf in Monthly Notices of the Royal Astronomical Society

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Copperwheat C (2011) The photometric period in ES Ceti

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Copperwheat C (2013) Transmission photometry of WASP-12b: simultaneous measurement of the planetary radius in three bands in Monthly Notices of the Royal Astronomical Society

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Bento J (2014) Optical transmission photometry of the highly inflated exoplanet WASP-17b? in Monthly Notices of the Royal Astronomical Society

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Gandhi P (2016) Furiously fast and red: sub-second optical flaring in V404 Cyg during the 2015 outburst peak in Monthly Notices of the Royal Astronomical Society

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Föhring D (2019) Atmospheric scintillation noise in ground-based exoplanet photometry in Monthly Notices of the Royal Astronomical Society

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Wang L (2019) The Pre-He White Dwarf in the Post-mass Transfer Binary EL CVn in The Astronomical Journal

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Hynes R (2019) Optical and X-ray correlations during the 2015 outburst of the black hole V404 Cyg in Monthly Notices of the Royal Astronomical Society

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McAllister M (2019) The evolutionary status of Cataclysmic Variables: eclipse modelling of 15 systems in Monthly Notices of the Royal Astronomical Society

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Pala A (2019) Evidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73-033933.0 in Monthly Notices of the Royal Astronomical Society

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Casewell S (2020) WD1032 + 011, an inflated brown dwarf in an old eclipsing binary with a white dwarf in Monthly Notices of the Royal Astronomical Society

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Marsh T (2020) Optical, X-ray, and ?-ray observations of the candidate transitional millisecond pulsar 4FGL J0427.8-6704 in Monthly Notices of the Royal Astronomical Society

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Nieder L (2020) Discovery of a Gamma-Ray Black Widow Pulsar by GPU-accelerated Einstein@Home in The Astrophysical Journal Letters

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Wild J (2020) Spectroscopic and photometric periods of six ultracompact accreting binaries in Monthly Notices of the Royal Astronomical Society

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Schaffenroth V (2021) A quantitative in-depth analysis of the prototype sdB+BD system SDSS J08205+0008 revisited in the Gaia era in Monthly Notices of the Royal Astronomical Society