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 every 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 STFC. ULTRACAM saw 'first light' in 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 in May 2005. To date, ULTRACAM has been awarded a total of 147 nights of time on these telescopes to study white dwarfs, brown dwarfs, pulsars, black-hole/neutron-star X-ray binaries, gamma-ray bursts, cataclysmic variables, eclipsing binary stars, extrasolar planets, flare stars, ultra-compact binaries, active galactic nuclei, asteroseismology and occultations by Solar System objects (Titan, Pluto, the moons of Uranus and Kuiper Belt Objects). 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 status as the world's premier instrument for high-speed optical astrophysics. As well as maximising the return on STFC's original investment, this money will also allow us to continue to offer ULTRACAM to others in the astronomical community who wish to use it.
Organisations
Publications
Parsons S
(2012)
A precision study of two eclipsing white dwarf plus M dwarf binaries Precise parameters for SDSS J1212-0123 and GK Vir
in Monthly Notices of the Royal Astronomical Society
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
Dhillon V
(2011)
A search for optical bursts from the rotating radio transient J1819-1458 with ULTRACAM - II. Simultaneous ULTRACAM-Lovell Telescope observations A search for optical bursts from RRAT J1819
in Monthly Notices of the Royal Astronomical Society
Bentley S
(2009)
A stellar flare during the transit of the extrasolar planet OGLE-TR-10b
in Astronomy & Astrophysics
Burdge K
(2020)
A Systematic Search of Zwicky Transient Facility Data for Ultracompact Binary LISA-detectable Gravitational-wave Sources
in The Astrophysical Journal
Ortiz JL
(2012)
Albedo and atmospheric constraints of dwarf planet Makemake from a stellar occultation.
in Nature
Parsons S
(2012)
An accurate mass and radius measurement for an ultracool white dwarf Accurate parameters for an ultracool white dwarf
in Monthly Notices of the Royal Astronomical Society
Föhring D
(2019)
Atmospheric scintillation noise in ground-based exoplanet photometry
in Monthly Notices of the Royal Astronomical Society
Savoury C
(2011)
Cataclysmic variables below the period gap: mass determinations of 14 eclipsing systems Short-period CVs below the period gap
in Monthly Notices of the Royal Astronomical Society
Osborn J
(2011)
Conjugate-plane photometry: reducing scintillation in ground-based photometry Conjugate-plane photometry
in Monthly Notices of the Royal Astronomical Society
Description | We have used this grant to operate ULTRACAM on the 3.5m New Technology Telescope and the 4.2m William Herschel Telescope. ULTRACAM is a high-speed astronomical camera which has helped increase our understanding of the dead remnants of stars: white dwarfs, neutron stars and black holes. |
Exploitation Route | Our findings provide the observational underpinning of theories of the structure and evolution of binary stars containing white dwarf, neutron stars and black holes. |
Sectors | Education |
URL | http://www.vikdhillon.staff.shef.ac.uk/ultracam/ |
Description | Advanced Grant |
Amount | € 3,500,000 (EUR) |
Organisation | European Research Council (ERC) |
Sector | Public |
Country | Belgium |
Start | 01/2014 |
End | 12/2018 |