Inital Email from Mark: Ken woud like us to focus as soon as possible on getting some stray light data on the new MOBY refresh blue spec. We will use the New Blue spec, Shutter mechanism from the shadowing work and the canned software for the new ANDOR camera. The focus is on determining if the performance at 350 nm is usable.
First laser date set collected on 7 Apr 2015 by Mike, Below are some of the more important bits of info from Mikes email
I am running the OTS "Andor SOLIS" acquisition software
Signal scans = s*.fits = lite data.
Dark scans = d*.fits = no Ekspla light to the sphere.
Background scans = b*.fits.
The SOLIS software has a "Background" scan mode,
which I haven't found much description of, but
a Background scan definitely does NOT fire the shutter, so hopefully
it's timing is the same as if the shutter was being used.
I am wondering if Bac == Dark ?
As a test, with all lights off I collected 5x Background scans (b*t1..5.fits)
then collected 5x Dark scans (d*t1..5.fits), all at 10 sec exposure ... to compare.
My quick-look via MATLAB seems to show these differ by ± 200 ADU.
I took sig,dark,bac scans tonight of Ekspla laser lines, at different exposure times,
so it will be interesting to see how dark compares w/ bac. If they are the "same" then it would be much easier to skip darks and only take backgrounds.
Problems seen:
Spec was sent back to Resonon, and the focus and other things where improved - Hawaii-2015-03 shows that data
Good stuff:
Page Number |
Link |
Description |
Date |
1.01 |
All the raw data files and their images , Table of KEYWORDS variable |
April 7, 2015 |
|
1.02 |
All the raw data files and their images , Table of KEYWORDS variable |
April 8, 2015 |
|
1.03 |
All the raw data files and their images , Table of KEYWORDS variable |
April 9, 2015 |
|
1.04 |
All the raw data files and their images , Table of KEYWORDS variable |
April 10, 2015 |
|
Day 1 - Laser data - Collected at PreAmp Gain 1 - Was saturating at ~35,000 ADU. Also low integration time (< 0.1 sec) leading to "pointed" (i.e. not-saddle-shaped) tracks - all tracks on | |||
2.01 |
Compare the dark and background data collected on 7 April |
April 8, 2015 |
|
2.02 |
Track selection using the day 1 laser data |
April 13, 2015 |
|
2.03 |
Cross Track from track 7 laser data |
April 14, 2015 |
|
2.04 |
Day 1 Laser data (all tracks on and track 7 only) |
April 14, 2015 |
|
2.05 | Pointy Tracks | The pointy track shapes at low int times | April 24, 2015 |
Day 2 - Oriel Lamp - Saturation Check - Collected at PreAmp Gain 1 - all tracks on |
|||
3.01 | Saturation Check | Mike check of when data are Saturating | April 14, 2015 |
Day 3 - Oriel Lamp - New Jig - Different Gains - tracks 1,4,7,10 and 13 on | |||
4.01 | Gain Saturation Check | Saturation Check with the different gains | April 15, 2015 - tax day! |
4.02 | Gain and darks | How Gain changes affect the Darks | April 15, 2015 - tax day! |
4.03 | Gain vs int vs signal | Plots of Gain, integration time and signal at pixel 512 | April 15, 2015 - tax day! |
4.04 | SLC lamp data | SLC using the day 4 track 7 gain 4 basic matrix | April 30, 2015 |
4.05 | Gain vs int vs darks | Plots of Gain, integration time and background at pixel 512 | |
Day 4 - Laser data - Gain 4 - New Jig - tracks 1, 7, 13 indv and 1,4,7,10 and 13 together | |||
5.01 | cross track | Cross Track of laser data tracks | April 16, 2015 |
5.02 | saddle shape | Does the shape of the saddle change for different days | April 22, 2015 |
5.03 | Laser data | Day 4 Laser data (indivdual tracks and 5 tracks on) | April 28, 2015 |
5.04 | off ccd light | Off ccd and other out-of-band light at the UV end of the array | April 28, 2015 |
5.05 | wave cal | Wavelength calibration from the 4 day lasers | April 29, 2015 |
Instrument returned to Resonon to correct the shoulder seen on the tracks causing a large amount of cross talk | |||
6.02 | Casey email - 24 Apr | Course alignment of BS01, with a modified slit mount to decrease the distance between the fiber face and the slit. | April 27, 2015 |
6.03 | Kehoe email - 4 May | infrared artifact | May 14, 2015 |
6.04 | Kehoe email - 7 May | Document: Which shows the cause of the infrared artifact has been identified | May 14, 2015 |
Camera details for BS01 and the software used during this experiment
BS01 camera, Andor iKon-M mod. DU934P-BR-DD, S/N: CCD-16346, I was running Andor SOLIS software: SOLIS ver. 4.23.30002.0, SDK ver. 2.95.30002.0, installed via CD no. 2208071, copyright 2010, on a Windows 7 Pro/SP1 PC.