Summary Repeated noise measurements were performed making changes in our setup. Two surces of 1/f noise were identified, * The strongest is the fast servo with...
1/f Servo plots for different pid configurations. Open loop PID at 50%Rn Open Loop PID 0% Rn Closed loop slow servo at 50%Rn Closed loop slow servo at 0%Rn ...
We used the 3D printed ABS plastic horn with the smooth transition in one end and the Pasternack Horn on the receiving end. Results A summary of the results for ...
AdvACT Masurements in the Field * Determination of the gain %$\frac{I_{TES}}{DAC_{fb}}$% * Aliasing measurements June 2019 * Aliasing measurements May 20...
Typical spectrum: Absolute Aliasing: Low Pct Rn tend to have lower noise There seems to be little trend between alias fraction and Pbias for varying L f See every...
Aliasing measurements 03 29 2019 Log: Start with MCE1 ./config_wo_syncbox.sh ./take_IV.sh Wait for 5 minutes ./takeData.sh vim /usr/mce/config/array_AR4.cfg and e...
Aliasing measurements at the site in 2017 Aliasing data is taken using takeData.sh which is in /home/mce/pato/AliasingData_2017. This script calls the script alia...
IR Camera Results from the first bonding run. It is found that the silicon wafer behaves like a transparent material on the wavelenth of the camera ~8um. Also the...
Determination of the gain %$\frac{I_{TES}}{DAC_{fb}}$% Here I followed the procedure presented here and here. I also inferred the %$R_{cable}$% value from the col...
Accessing the MCE data using code from Cornell at the site. Follow the following steps: 1 Make a directory to work in 1 In this folder, run: code/NoisePlots...
List of tod files varying the Number of Rows Data taken on 11/22/2016 To plot data, first create an out file, so you can use Shawn and Pato's plotting scripts. D...
Use this page to store fiduciary designs for different studies ACTPol v24 Zemax from Simon D. Complete telescope design, only camera shown in the picture Simons_...