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.
Organisations
Publications
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
Copperwheat C
(2009)
ULTRACAM observations of two accreting white dwarf pulsators
in Monthly Notices of the Royal Astronomical Society
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
Clark C
(2021)
Einstein@Home discovery of the gamma-ray millisecond pulsar PSR J2039-5617 confirms its predicted redback nature
in Monthly Notices of the Royal Astronomical Society
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
Burleigh M
(2006)
The nature of the close magnetic white dwarf + probable brown dwarf binary SDSS J121209.31+013627.7*
in Monthly Notices of the Royal Astronomical Society
Burdge K
(2020)
A Systematic Search of Zwicky Transient Facility Data for Ultracompact Binary LISA-detectable Gravitational-wave Sources
in The Astrophysical Journal
Bonnet-Bidaud J
(2020)
Fast quasi-periodic oscillations in the eclipsing polar VV Puppis from VLT and XMM-Newton observations
in Astronomy & Astrophysics
Besselaar E
(2007)
DE CVn: A bright, eclipsing red dwarf - white dwarf binary