Morning Shift Summary on 15.08.2023, posted by Teguh Citra Asmara, Eugenio Paris on 17 Aug 2023, 11:00
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Achievements
- Start cooling down the sample
- Align the beamline and deliver the beam into the sample
- Performed knife edge scans and enlarge the beam horizontal size to 350 um
- Tuned the VHM bending by checking the hRIXS resolution
- Performed energy calibration on the 1000 l/mm grating
- Check XAS and RIXS of the NdNiO3 sample at 20 K, normal incidence, and peak A
Problems:
- Nothing of note
Shift Plan:
- Check static RIXS at a few different configuration
- Check damage threshold with x-ray and laser
- Find spatial and temporal overlap between laser and x-ray
- Performed pump-probe XAS and RIXS
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Late Shift Summary on 15.08.2023, posted by Justine Schlappa, Le Phuong on 17 Aug 2023, 11:04
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Achievements:
- Set up PP laser, find spatial and temporal overlap between FEL and PP laser
- Optimize MCP and HAMP settings for good XAS signal
- Find time zero from XAS on sample and optimize for XAS delay scans at 40 deg incidence angle
- Take a fluence series on XAS delay scan from about 0.1 mJ/cm2 up to 2.5 mJ/cm2
Problems:
Nothing of note |
Night Shift Summary on 15.08.2023, posted by Sergii Parchenko, Manuel Harder on 17 Aug 2023, 11:06
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Achievements:
- Replaced focusing lens of PP laser and measured focus with knife edge, focus is about 720 micron vert. & 600 horizontal. Horizontal x-ray spot size is 220 micron
- Adapted fluence calibration for the new spot sizes
- Optimized spatial and temporal overlap with new lens
- Performed optical and x-ray intensity & sample damage tests. We found that up to 15% GATT and up to 50% laser power are okay to use, without altering the sample.
- We started to collect hRIXS data at positive (1ps) and negative (-2ps) delays.
Problems:
- Few beam dumps.
- BAM scene not working
- The new (?) centroiding function produces spectra with different intensity for acquisitions with the same settings. The old algorithm seems to work well.
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Morning Shift Summary on 16.08.2023, posted by Teguh Citra Asmara, Eugenio Paris on 17 Aug 2023, 11:07
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Achievements:
- Performed tr-RIXS on peak A, B, and C at 2.4 mJ/cm^2
- Performed tr-XAS on peak A at 3 fluences
- Performed tr-RIXS on peak A at 4 mJ/cm^2
Problems:
- BAM delay line compensator was not working due to incorrect macro. DOC and LM fixed the issue.
- Delay line scan of hRIXS camera was not working as it was still configured for Viking. MT fixed the issue.
- The new centroiding algorithm (provided natively by the 4137 kernel) is not consistent with integration mode. For the time being, we use an older, manually configured centroiding algorithm developed for a previous user beamtime.
- tR-XAS results show large changes, but these large changes were not reflected in tr-RIXS.
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Afternoon shift summary on 16.08.2023, posted by Teguh Citra Asmara on 17 Aug 2023, 11:08
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Achievements:
- tr-RIXS at 4 mJ/cm2 for energies A, B, C, and D (pre-edge)
- Checked and optimized FEL alignment, t0 and overlap with PP laser after reset of machine synchronization
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Long delay scans for Peak A and C, up to 100 ps
Problems:
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Need to reset machine synchronization by BKR
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Camera scene got stuck, was resolved by DOC
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Night shift summary on 16.08.23, posted by Sergii Parchenko, Manuel Harder on 17 Aug 2023, 11:09
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Achievements
- Acquired tr-RIXS data with 4.0 mJ/cm² laser power for 21 delays between -2 and +10 ps at 853 eV. including static XAS and dark hRIXS runs. Totally collected 210 minutes of data i.e. 10 minutes per delay
- Acquired tr-RIXS data with 4.0 mJ/cm² laser power for 21 delays between -2 and +10 ps at 853.44 eV. including static XAS and dark hRIXS runs. Totally collected 210 minutes of data i.e. 10 minutes per delay
Problems:
- hRIXS camera number of readout ports was set to 1, increasing the readout time. Set it to 2.
- Elastic line drifted about 40 meV over 3 hours (first and last trRIXS run at 853)
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Afternoon Shift Summary on 17.08.2023, posted by Justine Schlappa on 17 Aug 2023, 23:54
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Achievements:
1. Finalized tr-RIXS series at 1.74 mJ/cm2
2. Checked FEL alignment
3. Started fluence series for tr-RIXS on peak C, completed: 1, 1.5 and 2 mJ/cm2
Problems:
1. We noticed that calculator for PP laser fluence was not giving a correct value. The formula was corrected and the older logbook entries need to be checked. We start to use the "new values" from now on.
2. XAS processor get stuck and was restarted
3. left PC (pcx30525) got stuck and had to be restarted
4. hRIXS camera scene got stuck, so that it would not operate the PP laser delay stage. Help from DOC.
--> Solution: shutdown and reinstatiate device: SCS_HRIXS_DET/MDL/CAMERA_SHUTTER
Shift Plan:
Continue fluence series for: 0.5, 2.5, 3 mJ/cm2. Decide about further data points. |
Noght shift sammary 18.08.2023, posted by Sergii, Manuel on 19 Aug 2023, 07:16
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Night shift summary on 18.03.2023
- Finished XAS series at 1.5 mJ/mm² for different delays
- Performed XAS at 6 mJ/mm²
- Tested tr-RIXS signal at 1mj/mm² with 29 different delays, signal too weak to continue
- Took 5 hours of tr-RIXS signal at 1.2 mj/mm² with 29 different delays
Problems:
- Something in the cryo line froze, cleaned the line by going into the hutch and moving the needle valve a bit. This only helped short-term, as it kept freezing after short time.
- Temperature sensor at the sample stopped working, started to work again during the heating
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Giuseppe, Justine, posted by Giuseppe Mercurio on 06 Sep 2023, 06:35
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achievements:
- we found optimum hRIXS settings for 1020 eV but moving the detector arm
- we found optimum hRIXS settings for 920 eV but moving the detector arm, and then grating pitch and detect arm
- energy calbibration for 920 eV
problems:
- lost internect connection around 6 am
- PI-MTE3 camera claims an exposure of 30 sec but in reakity it"d more lik r13 sec.
- if FEL intensity goes to 0 i spikes, the jupyter notebook give errors, referring to objecests ofdifferent sie.
plans:
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Shift Summary, posted by Ben, Andreas on 06 Sep 2023, 23:33
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Achievements
- Determined temporal overlap between the X-ray and laser
- measured Ti L-edge XAS and RIXS on samples for Asamara beamtime
Problems
Plan for Next Shift
- Confirm spectrometer resolution at the O K-edge following spectrometer rotation
- Transfer user samples into XRD Chamber
- Check X-ray damage on user samples and begin user program
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Shift summary, September 7 after nightshift, posted by Justine Schlappa, Guiseppe Mercurio on 07 Sep 2023, 07:24
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Achievements:
- Optimized hRIXS settings for OK edge at 145 deg scattering angle, resolution of about 50 meV
- Transferred the user sample
- Prepared for delay scans on fluorescence signal from YBCO
Problems:
- There was no internet connection at XFEL and DESY for some time
- hRIXS camera goes frequently into error
- XRD motors (STY) go frequently into error
Next steps:
- Find time zero on fluoresce signal from YBCO, test the same for the samples
- Test PP laser damage threshold |
Shift summary, posted by Andreas Scherz on 07 Sep 2023, 23:46
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Shift summary 07.09.2023
Achievements:
1. found t0 on LSCO x=0.15 at pre-peak O K edge
2. fluence dependence at dt = 130fs, laser-on-off XAS => laser power at 50%
3. static XAS on the three samples x=0,.15, .4 aorund the pre-peak
4. setting for pump-probe: 1.1 MHz 520 pulses at 100% Transmission, PPL at 50%
Problems:
10:10pm loss of optical sync on PP laser. realized before starting time-resolved experiments. coarse timing requried !
Program for the night shift:
reestablished timing
resume experimetns, i.e. time-resolved signal on sample (XAS) then start time-resolved RIXS.
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Shift summary, posted by Benjamin van Kuiken on 22 Sep 2023, 06:51
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Achievemnets
- Characterized the X-ray and laser danage on the STO2LNO2
Problems
- Cound not find fine timeing from XAS measurements performed on the sample
- MCP sees 266 nm PP laser
- SiN mesaurement not successful so far. It is possible that there is an issue with the SN membranes on the sample holder
Plan for next shift
- Find fine timing
- conclude damad sutdy of sample.
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summary of 23.09, posted by Natalia, Justina, Giacomo, Sergey, Ben, Eugenio, Teguh on 24 Sep 2023, 07:49
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Around 6:55 there was a power glitch. Power in the experimental hutch and rack room went down in SASE3, error message in Xray interlock system and no power for PP laser.
During morning TS turned the power on and interlock issues were solved by DESY. SCS could restart large part of SCS systems, however got help of DOC only after 2:30p.m. Similarily, PP laser was needed help of DOC and got this help only around 2p.m. The afternoon shift was mainly bringing the instrument in operation with helps of DOC. Around 9p.m. we realized that PP laser is not in operational state because of large fluctuations, this was not communicated to SCS at all. After calling the Laser group, SCS was told that the laser group will work on recover of the laser on Sunday morning. Without laser we could not continue user program, therefore at least 24h of user operation were lost.
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SCS Night Shift Summary, posted by Benjamin van Kuiken on 27 Sep 2023, 07:51
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Achievements
- Characterized optical laser spot at sample
Problems
- FEL beam had very unstable intensity and spectrum. As a result no useful data could be collected during the night
- FEL pointing seemed to be stable on all tunnel imagers. The issue was communicated to BKR, and they said that things looked fine from there perspective.
- Large fluctuations in spectral distrubtion at SCS spectrometer were observed. See video at https://syncandshare.xfel.eu/index.php/s/emtwonCsQJJqpz6
- Oth-order beam on SCS pop-in showed large intensity fluctuations with ~50% of the time showing no beam at all
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Shift summary, posted by Laurent Mercadier on 29 Sep 2023, 22:59
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# Late shift summary 29.09.2023
Laurent, Phuong
## Achievements
- Continue tr-RIXS
- Laser fluence scan
- Check PPL 266 nm power
- Setup DAMNIT
## Problems:
- online analysis not displayed on gui1 server fixed by DOC
## Plan for the night:
- continue tr-RIXS
- monitor energy and position drifts |
Morning shift summary, posted by Giuseppe Mercurio on 01 Oct 2023, 14:48
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# Morning shift summary
Giuseppe, Martin
* achievements
- continued tr-RIXS measurements
- good beam conditions
- added new alarms to give warning if parameters are wrong for certain measurement type
- created new karabo device to calculate the fluence and train-averaged pulse energy in nJ from pulse-resolved HAMP values (see new scene in Main)
* problems
- none |
Morning Shift Summary, posted by Benjamin van Kuiken on 20 Oct 2023, 15:22
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Achievements
- Tested MCPs and APD for XAS
- Both MCPs give a good XAS spectrum with no amplification, but small MCP requires higher bias voltage
- No fluorescence signal observed on the APD
- Measured XAS of both samples
- Measured static RIXS of under-doped sample
Problems
Plan for next shift
- Sample alignment (half clip+diffraction)
- Switch AFS laser to burst mode and find timing
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Late Shift Summary on 20.10.2023, posted by Sergii, Giacomo on 20 Oct 2023, 23:22
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Late shift summary 20.10.2023
Achievements
-Switched AFS to burst mode
-Characterized PPL beam size
-Found coarse timing
-Working on fine timing with TR_XAS
Problems
-SCS_XGM data recorded with some mismatch that the run could not be loaded for an offline analysis with XGM. Other channels are fine.
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Night shift summary 21.10.2023, posted by Laurent, Phuong on 21 Oct 2023, 06:30
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Night shift summary 21.10.2023
Achievements
- Found T0 on SiN, but the response is very slow (~10 ps).
- Azimuth (phi) scan
- Start of theta scan with optimized phi
Problems
- Even after finding T0 on SiN, still could not find T0 on sample with XAS
- Beam down at 5:25
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