REVISION DATE: 17-Nov-2016 17:42:29

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 

Diver cal lamp LuBot data and the darks taken before and after the data set (if there is before and after).

Figure 1

Diver cal lamp LuBot data and the darks taken before and after the data set (if there is before and after).

Figure 2

Diver cal lamp LuMid data and the darks taken before and after the data set (if there is before and after).

Figure 3

Diver cal lamp LuMid data and the darks taken before and after the data set (if there is before and after).

Figure 4

Diver cal lamp LuTop data and the darks taken before and after the data set (if there is before and after).

Figure 5

Diver cal lamp LuTop data and the darks taken before and after the data set (if there is before and after).

Figure 6

Net signal for each Lu. By net I mean an average of the 5 lites for data set 1 and the darks taken before and after the lites. These where each meaned and then subtracted from each other and divided by int time.

Figure 7

Logged version of the Net data.

Figure 8