Telescope
The TIGRE was transferred to its final site at La Luz Observatory near Guanajuato (Mexico) in 2013. Scheduled observations were started there on August 1st.
Manufacturer:
Main contractor and mechanics:
Halfmann Teleskoptechnik
Some subcontractors:
Optics: Carl Zeiss Jena GmbH; picture of the main mirror
Electronics: RS Elektronik GmbH Augsburg
Software: 4PI Systeme GmbH Sonneberg
The basics
Type Cassegrain-Nasmyth with FOV corrector
Alt/Az mounting
Fully robotic
Optics
Primary mirror M1: aperture 1200mm, focal ratio f/3
Cassegrain focal ratio: f/8
FOV: 7' diameter
Spot concentration 80% in 0.5", >90% in 1"
Material: Schott Zerodur
Mechanics
Mounting: Alt/Az
Tube: Serrurier
M1 cell: active M1 support with 18 axial and 12 radial levers
Bearings: hydraulic/rollers in azimuth/elevation
Drives: final direct drives with high-precision absolute encoders
Pointing accuracy: blind 5" or better, seeing-limited with AGU
Tracking accuracy: better than 0.2"/min
Guiding accuracy: seeing-limited
Instruments stages: at two Nasmyth focii possible; FOV derotator
Telescope control
The Telescope Control Software is a subsystem of the control Software.
-- Initialising
-- Encoder absolute referencing
-- Pointing (slewing)
-- Tracking
-- The fibre entrance is embedded in an inclined mirror reflecting the beam on a ST7 camera
-- Guiding with a few percent of light from the target star
-- Seeing limited
-- Focusing
-- Hydraulic engine control
-- FOV derotator control
-- Sensors and limit switch read-out
-- Mirror covers actuating
-- Emergency action