Name |
Kiso Schmidt telescope |
Observatory |
|
Organization |
|
Location |
Kiso, Nagano, Japan |
Coordinates |
|
Altitude |
1,132 m |
Observatory code |
381 / Tokyo-Kiso |
Effective aperture |
1,050 mm diameter |
Focal length |
3,300 mm |
Focal ratio |
3.1 |
Field of View |
9 degree diameter |
Name |
Tomo-e Gozen camera (Sako et al. 2018) |
Image sensor |
Canon 35MMFHDXM |
Sensor type |
35-mm front-side-illuminated CMOS image sensor with microlens array and AR coated cover glass |
Sensor format |
2,160 x 1,200 pix/chip (whole area) |
Sensor chips |
84 chips |
Pixel size |
19 μm/pix |
Pixel scale |
1.189 arcsec/pix |
Field of view |
39.7 arcmin x 22.4 arcmin x 84 chips = 20.8 degree2 |
Photoelectric conversion efficiency |
0.72 at a peak wavelength of 500 nm |
Beam efficiency |
Degraded at fields outer than 2 deg from the FoV center |
Filter |
Transparent window |
Inverse gain factor |
0.23 e-/count in High-gain |
Read noise |
2.0 e- in High-gain |
Well depth |
6,000 e- in High-gain |
Dark current |
0.5 e-/sec/pix at 290 K |
Thermal design |
Passive cooling (no temperature control) |
Readout overhead |
Zero overhead owing to rolling shutter read out |
Frame rate (max) |
2 fps in full-frame read |
Raw image file |
16-bit cube FITS |
Data production rate (max) |
830 MByte/sec = 30 TByte/night (full-frame, 2 fps, 10 hours) |
Sky background light |
50 e-/sec/pix in dark night |
3 - 4 arcsec (typ.) |
|
Limiting mag in High-gain |
15.9 mag in 0.1 sec exposure |
Photometric stability |
4 to 30 milli-mag (time scale < 5 sec) |
Absolute time accuracy of timestamps |
±0.2 msec |
Stability of frame read time |
10-5 |
The number of frames acquired in each area |
18 frames at 2 fps |
Depth reached in each area |
17.8 mag (stacked of 18 frames, median value in all lunar phases) |
Moving time between areas |
10 sec in dithering of 40 arcmin |
Survey scan rate |
2,500 deg2/hour |
Data production rate |
10 TByte/night |