REVISION DATE: 10-Nov-2016 15:15:35
The darks collected during BS02s first set of diver calibrations while on MOBY261
The files I am calling darks where taken with the camera shutter closed and external shutter open. Backgournd files where collected with the camera shutter open and the external shutters closed. /
File numbers for the data sets collected Lite I1L01 --> s2016111011.fits LuBot Lite I1L02 --> s2016111012.fits LuBot Lite I1L03 --> s2016111013.fits LuBot Lite I1L04 --> s2016111014.fits LuBot Lite I1L05 --> s2016111015.fits LuBot Dark I1D01 --> d2016111001.fits Dark I1D02 --> d2016111002.fits Dark I1D03 --> d2016111003.fits Dark I1D04 --> d2016111004.fits Dark I1D05 --> d2016111005.fits Lite I1L06 --> s2016111016.fits LuBot Lite I1L07 --> s2016111017.fits LuBot Lite I1L08 --> s2016111018.fits LuBot Lite I1L09 --> s2016111019.fits LuBot Lite I1L10 --> s2016111020.fits LuBot Dark I1D06 --> d2016111006.fits Dark I1D07 --> d2016111007.fits Dark I1D08 --> d2016111008.fits Dark I1D09 --> d2016111009.fits Dark I1D10 --> d2016111010.fits Lite I2L01 --> s2016111031.fits LuMid Lite I2L02 --> s2016111032.fits LuMid Lite I2L03 --> s2016111033.fits LuMid Lite I2L04 --> s2016111034.fits LuMid Lite I2L05 --> s2016111035.fits LuMid Dark I2D01 --> d2016111021.fits Dark I2D02 --> d2016111022.fits Dark I2D03 --> d2016111023.fits Dark I2D04 --> d2016111024.fits Dark I2D05 --> d2016111025.fits Lite I2L06 --> s2016111036.fits LuMid Lite I2L07 --> s2016111037.fits LuMid Lite I2L08 --> s2016111038.fits LuMid Lite I2L09 --> s2016111039.fits LuMid Lite I2L10 --> s2016111040.fits LuMid Dark I2D06 --> d2016111026.fits Dark I2D07 --> d2016111027.fits Dark I2D08 --> d2016111028.fits Dark I2D09 --> d2016111029.fits Dark I2D10 --> d2016111030.fits Lite I3L01 --> s2016111051.fits LuTop Lite I3L02 --> s2016111052.fits LuTop Lite I3L03 --> s2016111053.fits LuTop Lite I3L04 --> s2016111054.fits LuTop Lite I3L05 --> s2016111055.fits LuTop Dark I3D01 --> d2016111041.fits Dark I3D02 --> d2016111042.fits Dark I3D03 --> d2016111043.fits Dark I3D04 --> d2016111044.fits Dark I3D05 --> d2016111045.fits Lite I3L06 --> s2016111056.fits LuTop Lite I3L07 --> s2016111057.fits LuTop Lite I3L08 --> s2016111058.fits LuTop Lite I3L09 --> s2016111059.fits LuTop Lite I3L10 --> s2016111060.fits LuTop Dark I3D06 --> d2016111046.fits Dark I3D07 --> d2016111047.fits Dark I3D08 --> d2016111048.fits Dark I3D09 --> d2016111049.fits Dark I3D10 --> d2016111050.fits
Track 7 all the dark files.
Figure 1
Track 7 all the background files.
Figure 2
Darks showing for pixel x in the track and wavelength direction (every third dark file)
Figure 3
Figure 4
Figure 5
Figure 6
track 7 mean for every third file against time
Figure 7
The same data verses int time
Figure 8
The same data divided by int time
Figure 9
Figure 10
Figure 11
Figure 12
Figure 13
Figure 14
Images of the dark and background repeats for this data set. All the darks had the temp control flag on.
Figure 1
Figure 2
Figure 3
Figure 4
Figure 5
Figure 6
