So far, TR-CARM + RF-DARM with 3f for PRCL and MICH up to 50Hz CARM offset
Filter shape adjustment for hand over of TR-CARM to RF-CARM on going
Issues
Beam clipping at IFI ?
IMC spot position on MCo does not look good
ALS noise
Why the fiber noise cancellation performance cannot be better ?
Fringe from non-perfect AR ?
ASC
Modified the optical layout of REFL and AS to accommodate PZT mirrors for the QPD centering servo.
Noticed beam clipping at the REFL port.
It seems to be happening in IFI
VIS
Basic damping
Implemented on all the suspensions
Type-B/Bp filters may introduce too much noise during the observation
Need to implement narrow band low noise damping filters(see below)
Kill individual resonances
Mostly done for all the Type-A
Remaining problems in ETMX, ITMY
Filters need to be readjusted as the payload temperature changes
Need to be implemented on Type-B/Bp
Probably we need to fight against new resonances when we start ASC feedback
Actuator diagonalization
Done for all the cryo-payloads(is this correct ?)
Some L2A decoupling was done for BS before, but may not work properly now.
We need to revisit L2A for Type-B/Bp
Sensor correction
Implemented on ITMY, ETMY and ETMX for IP and BF
ITMX is IP only
Work on going to implement this on Type-B IP
If necessary we can implement it for Type-Bp BF
Calm down mode
Implemented for all the Type-A, but only ETMY is working.
Need to tune the filters for the other Type-A
Once the Type-B suspensions have low-noise damping filters, we probably want to implement a calm down state for them(noisy but powerful damping)
OMC
Mirror alignment jigs arrived
We will test them on Sept. 24 and 25 when Somiya-san comes and remove the OMC from the suspension.
Design work on other modifications is ongoing(about 70% done)
Test of M2052 for damping the OMC breadboard is ongoing in Mitaka by Takahashi-san
PRC-PBS
The plan is to ask LMA to make 3-inch low-loss PBS
The coating run will be in October
Matteo is working on the preparation of the substrate
Most likely to use AQ crystal we have and ask a company to polish
Mounting structure of the PBS needs to be designed
Had some discussion among Akutsu, Matteo and Aso
Akutsu will discuss with Hirata for making more concrete design
CAL
Low latency h(t) and Online h(t) are provided.
Online model development is almost done. We are updating the model to increase the accuracy.
Free Swinging Michelson test is ongoing. We tried to estimate the errors of Response functions with Mich DoF. We will estimate DARM DoF based on current measurement.
DC fluctuation measurement has done. The estimated rms of optical efficiency is about 0.1 %. It meet our requirement.
The test of X-end line injection is ongoing.
We measured the cross correlation between Pcal line and the following channels. We cannot see any coherence between the injected channel and following channels. We are monitoring the long time stability.
We developed ver.4 Camera control scripts. We can read the beam position with new script. At that time, the beam position was defined by the edge of mirror. We will switch the scripts ASAP.
We are preparing the low latency line demodulation code test with Mich DoF.
Real time super event monitor was developed. We plan to apply this system for injection tests.(HWI test → send the dummy signal to super event channel → test of Analysis and Offline calibration)
Offline calibration server“calgst-hl” was developed.
Absolute calibration setup in Toyama university was developed. LIGO will send the power standard in this week. After that, we will start the absolute power calibration of PCal.
We are preparing the injection test in October(DAC is plaining Hardware injection test.)
We are developing the error estimation scripts like DARMpy.
PEM
Basic installation was already completed.
We are investigating the interferometer signal by Bruco
MICH, DARM, SRCL, XYarm
Investigations are posted in klog
Hunting the serious origin of the noise source
44Hz found in the ALS noise curve → 24V power supply placed in the PSL room → Turned off
17.2Hz found in the MICH, SRCL → Come from the FFUs
312.5Hz, 315Hz, 450Hz, 460Hz from vacuum pumps
Investigating about the lightning effect
It sometimes gives the vibration to the suspension
Washimi-san introduced the monitor system at the entrance
Interferometer locking
ASC
VIS
OMC
PRC-PBS
CAL
PEM
Early silent run