MIKE – Calibrations

MIKE – Calibrations

Here we provide some reference numbers for calibrations with MIKE

Note: Be aware that every time MIKE is installed the position of the quartz lamp might change slightly leading to 10% fluctuation of the counts. If the counts are a lot less than what reported in the tables below, it means that the lamp is not aligned with the slit. In such case please inform the daytime crew. 

Flats: Internal Quartz lamps – binning 2×2 – speed fast  (updated July 2018)

Slit sizeBlueRed
 exptimecountsexptimecounts
 0.35″15s 27000 4s 28000
 0.5″ 12s 28000 3s 28000
 0.7″ 9s 29000 2s 27000
 1.0″ 6s 28000 2s 36000
 1.5″ 4s 26000 1s 26000
 2.0″ 3s 28000 1s 38000

Milky flats: same configuration as above but with the diffuser inserted (updated July 2018) 

Slit sizeBlueRed
 exptimecountsexptimecounts
 0.35″ 55s28000 25s 32000
 0.5″ 40s27000 20s 34000
 0.7″ 25s25000 12s 29000
 1.0″ 19s25000 9s 31000
 1.5″ 15s28000 7s 34000
 2.0″ 10s27000 4s 28000

Sky flats: to be done in daytime with louvres open at 50% and flat screen in. The following exposure times give between 35000 and 45000counts at peak (2×2 binning, speed fast). This results to ~600counts above background on the less efficient part of the blue side and ~1500counts for the red side. 

Slit sizeBlueRed
 exptimecounts
at peak
exptimecounts
at peak
 0.7″ 100s40000 30s 48000
 1.0″ 90s40000 20s 40000
 1.5″ 45s40000 10s 35000

Blue flats: The internal incandescent lamp is fine on the red side of MIKE, but it does not supply much light for the blue side. For that reason, we STRONGLY suggest that you take some milky flats during twilight using an O or B star. It is a good idea to take half of the flats with the star at one end of the slit, and half with the star at the other end of the slit. The best stars for this purpose are stars with high rotational velocities – high v*sin(i). There is a catalog of such stars with the Telescope Operators (“high_vsini_obscat.cat”). A star with V=4-5 mag gives very good flats in about 25 sec per exposure. For more details please consult the manual.

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