ULTRACAM: an ultrafast, triple-beam CCD camera for high-speed astrophysics
By V. Dhillon, Thomas R. Marsh, M. Stevenson, D. Atkinson, P. Kerry, P. Peacocke, A. Vick, S. Beard, D. Ives, D. Lunney and 8 more. 2007
245 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics
View Paper: https://www.semanticscholar.org/paper/e255c6301218dbc3505a8a975e8d65b974a593aa
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In Astronomy and Astrophysics
- James R. A. Davenport
- M. Zorotovic
- B. Gänsicke
- E. Hilton
- M. Schreiber
- S. Schmidt
- A. Kowalski
- J. Greiner
In Atomic and Molecular Physics, and Optics
Citations in the corpus
- Rapid optical and X-ray timing observations of GX 339-4: multi-component optical variability in the low/hard state (2010, methodology): “Our optical observations were carried out with ULTRACAM, which is a fast imaging camera employing frame-transfer CCDs (Dhillon et al. 2007).”
- Post common envelope binaries from SDSS - XI. The white dwarf mass distributions of CVs and pre-CVs (2011, methodology): “The advent of ULTRACAM on large aperture telescopes (Dhillon et al. 2007), and an increasing sample of eclipsing CVs, predominantly from the SDSS (Szkody et al. 2009), led to a significant increase in the number of CVs with published high-precision WD masses (e.g. Feline et al. 2004a; Littlefair et…”
- TIME-RESOLVED PROPERTIES AND GLOBAL TRENDS IN dMe FLARES FROM SIMULTANEOUS PHOTOMETRY AND SPECTRA (2013, methodology): “The χflare and Hγ/C4170 measures indicate the relative importance of each emission component – Hydrogen Balmer vs. blackbody emission – while also giving information about the flare morphology. χflare is a measurement that can made without spectra, for example at very high time resolution and high s”
- GROND—a 7-Channel Imager (2008, methodology): “…Cassegrain foci of the KPNO 2.1-m and 4-m telescopes (Ellis et al. 1992)), ULTRACAM (ULTRAfast, triple-beam CCD CAMera for highspeed astrophysics (Dhillon et al. 2007); portable instrument which has been used, among others, at the Very Large Telescopes at ESO, or the William Herschel Telescope,…”