ULTRACAM is a high-speed, 3-channel CCD camera for astrophysical research. Dichroics split the light up into ultraviolet, visual and red wavelengths which are exactly simultaneously imaged with frame transfer CCDs (1024 by 1024 imaging area). These CCDs use a masked area to shunt exposures rapidly from the imaging area, which can then be read out while the next exposure is running. Timestamps are generated from the GPS.


  1. Tips for observing with ULTRACAM
  2. Data logs
  3. Pipeline installation instructions
  4. Pipeline software
  5. Calibration information
  6. Publications
  7. Vik Dhillon's ULTRACAM web pages


Schematic design of ULTRACAM This picture shows the schematic design of ULTRACAM: light from the telescope is first collimated and then split into different wavelengths with dichroics. Each channel is then re-imaged onto its own CCD. Each CCD is a frame transfer device, which allows a dead-time of only 0.026 seconds in the normal readout mode. A special "drift mode" allows much faster operation, with frame rates of over 100 Hz.

ULTRACAM can produce lots of data, up to 3 MB per second. Over the course of the night, this can stack up to many gigabytes. We have developed software to allow us to look at and reduce the data in near real-time.


Photograph of ULTRACAM mounted on the 4.2m WHT This photograph shows ULTRACAM mounted on the 4.2m WHT in La Palma during the commissioning run in May 2002. The black tube with flanges at the top of the picture is the mounting collar for connecting to the WHT; the telescope focus is located in the middle of the tube at the top of the picture.The large silver box at the bottom houses the SDSU CCD controller which drives the readouts of all three CCDs. One of the CCDs can be seen as a smaller silver box on top of the SDSU controller. ULTRACAM is very approximately 0.5m wide, deep and high.

This 3.6MB animated gif shows an area around an eclipsing white dwarf/M dwarf binary called NN Ser during its eclipse. The right-hand panel shows the light-curve. Only 1 in 5 frames are plotted to keep the file size down. The data were taken with 2 second exposures.

ULTRACAM at the the VLT

Click for full size photo In May 2005 we had our first run with ULTRACAM at the visitor focus of the VLT (UT3, Melipal). We were allocated a block of nights, 4 to 21 May, to undertake some 15 projects. The weather was kind and we obtained some beautiful data, which will appear here at some point in the future.


ULTRACAM was funded by PPARC and is a collaboration between Vik Dhillon (Sheffield), Tom Marsh (Warwick) and the Astronomy Technology Centre (Edinburgh).

Tom Marsh, Warwick