Jan exchanged the Mesytec CFD/shper since it could not be "remote controlled" anymore. The new one has different shaping times and delays.
It is noted the threshold range is rather small. 
With the new  shaper only the x100 signals could meaningfully discriminated etc.
After start of the ESR (magnets etc.) the signals of the 10x channels see quite some noise that makes it more difficult to adjust the thresholds for the low signals.

The simulated frequency is given in simulation_result.out. The yield is calculated by LISE file. The LISE file is attached here also.

The preliminary identification has been thoroughly checked using the RionID software. We have confirmed that the identification is accurate.

Attached can be found the simulation file with each of the expected ions, their revolutions frequencies in the 125th harmonic and expected yield from the LISE file attached.
Also attached are some figures from RionID that highlight the region of interest for the 124th and 125th harmonics. The center frequency of the 245 MHz resonator is closer to the 124th harmonic for 229Th+89 which is located at 244.769 MHz. 

If necessary, we can slightly shift the resonator curve to higher frequencies to fine-tune the signal-to-noise ratio for 229Th+89.

Harmonic: 124.0 , Bp: 7.796046 [Tm]
ion            fre[Hz]                       yield [pps]    
------------------------------------------------------------
237U+92        243732740.7822311819          8.6164e+03     
237Np+92       243732858.1891748905          1.9672e+02     

224Ac+87       243759120.6575988531          1.7025e+03     

229Pa+89       243784072.1343108118          2.5529e+03     
229Th+89       243784111.0000000000          3.3883e+03   
  
234Pa+91       243807737.9699291289          2.4721e+03     
234Np+91       243807852.4158236086          1.7745e+01     

The strongest line is 229Th+89/229Pa+89. The yield and frequency of 229Pa+89 and 229Th+89 are very close to each other.  We needed to 
install Al target to suppress Pa as much as possible. Al gives a better ratio of h-like to he-like than Be. Two peaks at left 
side are 237U+92/237Np+92 and 224Ac+87. One peak at right side is 
234Pa+91/234Np+91. 

Note added 2024-06-14 (Carsten): a) We will not produce Np, this is an artifact of Lise, b) relative intensities are for injection only. Line intensities for  237U/224Ac/234Pa are substantially lower after cooling/HF/deceleration.

data:
(env_OnlineDataAnalysisSystem) litv-exp@lxbk0497:/lustre/astrum/experiment_data/2024-05_E018/OnlineDataAnalysisSystem/data/iq/IQ_2024-06-
12_21-47-54$
The root file is at:
(env_OnlineDataAnalysisSystem) litv-exp@lxbk0497:/lustre/astrum/experiment_data/2024-05_E018/OnlineDataAnalysisSystem/data/iq/IQ_2024-06-
12_21-47-54$ root filtered_spectrum_670_750.root

The figure below shows the interface of the program "combine_injection". You can combine any tdms file with this program. To run this 
program, you need to log in to the server /luster/astrum/, and activate the conda environment. Then type the command "combine_injection" at 
the terminal. You will see the interface. 

Calculation from Helmut Weick (copied from E142)
Distance e-cooler to particle detectors chamber:
“This is half of ESR plus distance target - detector. This even is on the web page”
54.28 m + 21.64 m

attched is more info about the T-scrapers (E-cooler) by Robert Boywitt (Tel: 2067 or 3357)

No beam today.--.