Lucky imaging (LI) will be used mainly to study gravitational micro-lensing events towards the galactic center. The LI CCD model in use is an Andor iXON...

The primary use of the spectrograph is to determine radial velocities of stellar surfaces for asteroseismic analysis. The spectrograph is s a high resolution...

Format: 4Kx4K 15-micron FOV (arcmin): 10.5 Pixel size (1x1 binning, arcsec): 0.152 Pixel size (2x2 binning, arcsec): 0.304 Normal Binning: 2 x 2 Cycle time...

SPRAT (SPectrograph for the Rapid Acquisition of Transients) is a low resolution, high throughput spectrograph. It employs a VPH grating and prism ("grism")...

The SES is a modern white-pupil spectrograph with a moderately high spectral resolution of about 55,000 and a fixed wavelength format of 390 to 870nm. The...