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.
ZWO ASI120MM Guider
The new ZWO ASI120MM Mini (mono) with its 3.75 µm pixels is a highly sensitive autoguider for in a 1.25" body
Suitable for the spectrograph ZWO MONO Astro Camera ASI 533MM-PRO cooled, Sensor D= 16 mm, 3.76 µm Pixel Size Cooled USB 3.0 monochrome astro camera with powerful back-illuminated CMOS sensor for astrophotography in square format
The UVEX is the most versatile instrument in the range. Achromatic by design, it can explore far into the ultraviolet and infrared – at the very limits of what today’s cameras can achieve. The interchangeable gratings (in option) allow different resolutions. Combined with its motorization module, it can be operated remotely.
The motorized UVEX is the ultimate version of the UVEX, allowing remote operation. You can remotely control the central wavelength (grating angle) and adjust the spectroscope’s focus.
The motorization integrates the control of the calibration module (equivalent to the SPOX module). So it’s easy to do your dark, flats and calibration images remotely.
The UVEX is now motorized, and can be operated remotely.
The spectrograph slit has 6 positions that can be easily changed using a Phillips screwdriver (supplied with the UVEX). Several slot widths are available: 25µm, 50µm, 100µm, 300µm, a 25µm hole and a 3mm hole. Other slots are available as options, and Alpy slots are UVEX-compatible.
Mototrization : The motorized UVEX allows you to select the central wavelength observed (grating angle) and adjust the spectroscope’s focus.
Remote control of integrated calibration module : The motorization integrates the control of the calibration module (equivalent to the SPOX module). It is therefore easy to make your images of black, flats and calibration, remotely.
DEMETRA remote control Version: The UVEX motorization module is accompanied by a new version of the DEMETRA software: – Calibration “by set line”. We establish once and for all the law of dispersion, and we can readjust it on a well identified line. This is useful for covering all areas from UV to IR, when the reference lines are few. – Motors module control, – Image sequences, to link several series of images, – Consideration of CMOS cameras (by the CMED correction step).
Not a DEMETRA user? Don’t panic, Shelyak has thought of you! We provide you with a small software program, USIS Controller, which allows you to control the UVEX from your computer: USIS-controller And if you want to integrate UVEX control more deeply into your own environment, the communication protocol between the computer and the UVEX motorization module is documented: this is the USIS protocol.
Specifications
Cross Czerny-Turner Spectrograph
Spectral range : 350 nm à 1µm
Spectral resolution with the 600 tr/mm grating R=1700 @ 650nm
Multi position slit : 25µm, 50µm, 100µm, 300µm and a hole of 25µm
Optimal telescope F-ratio : F/8
Compatible with ZWO, QHY et ATIK camera with a backfocus <14mm
Motorized grating: select the central wavelength you want to observe.
Motorized focus: fine tune the UVEX focus position, to get the best optical quality.
Calibration module: control light source, through the (external) calibration module. You can switch between Sky, Dark, Flat and Calibration.
Dimensions (UVEX + Motors module, w/o cameras): 153 x 154 mm Height: 133 mm
Weight: 1.46 Kg (w/o camera)
Communication protocol : USIS
Camera recommendation
The acquisition camera (or “Science” camera) is used to acquire the spectra of the observed object. The criteria for choosing a camera are :
The size of the sensor (the bigger the better) The size of the pixels (which gives the sampling) Reading dynamics (the number of shades the camera can see) Quantum efficiency (the sensitivity of the camera to light) Reading noise (the lower the better) Cooling (for long exposures)
In each product sheet you will find the camera we recommend – but of course other solutions are possible.
The UVEX can be used with additional 150 tr/mm, 300 tr/mm, 1200 tr/mm and 1800 tr/mm gratings, in addition to the 600 tr/mm grating supplied as standard with the UVEX.
Each grating is supplied with:
A grating holder (the grating is delivered mounted and adjusted on the grating holder)
A box for securely storing your grating on its holder
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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