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APM Professional Telescopes

APM Professional Telescopes

1m F/8 Ritchey Chrétien with dual Nasmyth Foci, Cape Town (South Africa)

Another large telescope for the South African Astronomical Observatory (SAAO). An 1m F/8 Alt-Az mounted Ritchey Chrétien for robotic use. It has dual Nasmyth Foci. The main telescopes used for research are located at the SAAO observing station (32°22.795’S 20°48,657’E) near Sutherland in the Northern Cape, a 4-hour drive from Cape Town.

Astronomy is our job

Observatory Telescopes

Big prime focus telescopes for private or public observatories including installation and full service.

Robotic / Remote

Robotic instruments for automatic imaging or telescopes for remote observation.

UVEX Spectrograph

Uvex Spectrograph

The UVEX is a “crossed” Czerny-Turner spectroscope optimized for wavelengths from near UV (<350nm) to near IR (1µm).

Diffraction Limited CCD Kameras

Aluma CCD 695 a

Our most popular camera, the SBIG Aluma AC4040 is a large format Scientific CMOS camera, featuring a 16.8 megapixel sensor with 9 micron pixels.  The camera is compatible with the StarChaser SC-4 Guider and optional AO-X Adaptive Optics accessories.

Diffraction Limited Overview

Astroshell Dome 4.25 m

Astroshell Dome 4.25m

CLAMSHELL DOMES provide an unparalleled 360/180 degree field of view for an absolutely breathtaking nighttime experience. When this observatory dome opens, you are truly among the stars!

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Please make your enquiries about the products you require here. We will contact you as soon as possible with a customised quote.

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Learn about the unique OptAcquire interface

Learn about the unique OptAcquire interface

OptAcquire is a unique control interface, whereby a user can conveniently choose from a pre-determined list of set-up configurations, each designed to optimize the camera for different experimental acquisition types, thus removing complexity from the extremely adaptable control architecture of the iXon.

The control architecture of the iXon is extremely tunable, meaning the camera can be adapted and optimized for a wide variety of quantitative experimental requirements. They range from fast single photon counting through to slower scan, 16-bit dynamic range measurements. However, successfully optimizing EMCCD technology is not a trivial exercise, with various set-up parameters directly influencing different camera performance characteristics. OptAcquire has been designed as a unique interface whereby a user can choose from a pre-determined list of nine camera set-up configurations. A variety of set-up parameters are balanced behind the scenes through the OptAcquire menu. Furthermore, advanced users may wish to create their own additional OptAcquire modes to aid future set-up convenience.

iXon control parameters include:

  • EM gain - this parameter has a direct bearing on both sensitivity and dynamic range.
  • Vertical clock speed - flexibility in this parameter is critical to optimizing the camera for lowest noise, fastest speed, minimal frame transfer smear or maximum pixel well depth.
  • Vertical Clock Amplitude - can be employed to help 'over-clock' the sensor to achieve faster frame rates and can also be used to reduce charge leakage into the image area when there is saturated signal in the frame transfer storage area (e.g. when combining very short exposure with a slow readout speed).
  • Horizontal readout speed - ranging between faster frame rates and best dynamic range.
  • Pre-amplifier gain - trading off reduced digitization noise versus accessing full pixel well depth.
  • EM / Conventional amplifier - to choose between ultrasensitive EMCCD operation or traditional high dynamic range CCD operation, the latter recommended for relatively 'brighter' signals or when it is possible to apply long exposures to overcome read noise floor.
  • Frame Transfer (overlap) - overlap readout is used to achieve 100% duty cycle, ideal for fastest frame rate measurements without switching exposure time between frames. This mode should be deselected for time-lapse experiments
Pre-defined OptAcquire modes include:
Sensitivity and Speed (EM Amplifier) Optimized for capturing weak signal at fast frame rates, with single
photon sensitivity. Suited to the majority of EMCCD applications.
Dynamic Range and Speed (EM Amplifier) Configured to deliver optimal dynamic range at fast frame rates.
Moderate EM gain applied.
Fastest Frame Rate (EM Amplifier) For when it's all about speed. Optimized for absolute fastest frame
rates of the camera. Especially effective when combined with
sub-array/binning selections.
Time Lapse (EM Amplifier) Configured to capture low light images with time intervals between
exposures. Overlap ('frame transfer') readout is deactivated.
Time Lapse and Short Exposures (EM Amplifier) Configured to minimize vertical smear when using exposure
times < 3 ms.
EMCCD Highest Dynamic Range (EM Amplifier) Combines EMCCD low light detection with the absolute highest
dynamic range that the camera can deliver. Since this requires slower
readout, frame rate is sacrificed.
CCD Highest Dynamic Range (Conventional Amplifier) Optimized for slow scan CCD detection with highest available
dynamic range. Recommended for brighter signals or when it is
possible to apply long exposures to overcome noise floor.
Photon Counting Configuration recommended for photon counting with individual
exposures <; 10 sec.
Photon Counting with Long Exposures (> 10 sec) Configuration recommended for photon counting with individual
exposures > 10 sec.

APM Professional Telescopes

1m F/8 Ritchey Chrétien with dual Nasmyth Foci, Cape Town (South Africa)

Another large telescope for the South African Astronomical Observatory (SAAO). An 1m F/8 Alt-Az mounted Ritchey Chrétien for robotic use. It has dual Nasmyth Foci. The main telescopes used for research are located at the SAAO observing station (32°22.795’S 20°48,657’E) near Sutherland in the Northern Cape, a 4-hour drive from Cape Town.

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