SPIM is an optical imaging instrument covering wavelengths ranging from 350 to 1000nm. It employs a 4096 X 4108 CCD camera with a pixel scale of about 0.1 arcsec on the telescope and it covers a field of view of 6.5 x 6.5 arcmin. Currently, Bessel U,B,V,R,I and SDSS u,g,r,i,z filters are available. Stellar images with FWHM less than an arcsec in V-band have been recorded in November 2023. The instrument is available at one of the side-port of the telescope.
Parameters | Value |
Type | Imaging |
Mount position | Side port 2 |
Wavelength range | 350-1000 nm |
Array size | 4096 X 4096 pixel2 |
Pixel size | 15 μm |
Pixel scale | 0″.1 |
Field of view | 6′.5 X 6′.5 |
Readout noise in electron (speed) | 3.8 (100 kHz), 8.5 (1 MHz), 12 (2 MHz ), 23 (4 MHz) |
Readout time | 20s |
Gain | 5.3, 3.4 and 1.5 e-/ADU |
Minimum exposure time | 1 ms |
Available filters | Bessel: U, B, V, R, I and SDSS: u, g, r, i, z |
Limiting magnitude | 23.5, 22 mag in V, I bands with an exposure time of 1 hour |