One of the fastest telescopes of the world!
UWF300 Optical Layout
The UWF300 uses a prime focus configuration. The main mirror is a high order asphere and in the prime focus we use a 5 Lens corrector to correct any field aberrations in a wavelength range from 400nm to 700nm.
With the ultra short focal length and wide field it is the ideal telescope for fast sky surveys searching for brighter objects. The resolution with modern small pixel CMOS is nevertheless surprisingly high even with such a short focal length. It can also be arranged in arrays on our DDM mounts.
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Inquire now Datasheet UWF300_f1.3
Optical performance
As the below image demonstrates, the UWF300 reaches a unprecedented resolution for a telescope in the 400mm focal length range and shows details and first bright stars in M31 even in 10s exposures)
Mechanics
The closed full tube is made of carbon fiber and includes a light shroud. The main mirror can be collimated fully electronic to allow an easy and fast remote collimation. The electronics for the collimation and focusing is attached to the tube. The total weight of the OTA is 31kg.
ASA/APM Services
ASA Accessories
The remote package contains an IP Camera mounted inside the Dome to remotely view the Telescope and an Uninterruptible Power Supply (UPS). The IP Camera allows to always view the telescope orientation to give you situational awareness of the observatory status. The UPS allows the telescope to keep operating during shorter (<30sec) power interruptions and to safely park the telescope in the event of a longer power outage.
This package contains sensors for sky and ambient temperature, rain and humidity and wind speed plus all necessary mounting material.
This package guaranties operational safety of your observatory in case of unsuitable or hazardous weather conditions. It also provides the operator with a web interface to monitor and log weather events.