Before starting measuring Pitch to Pitch on ITMY, I realized the oplev signal was oscillating at high frequencies. I took a spectra and compared with other oplevs, and the noise floor from 1000Hz is ~2 orders of magnitude higher compared to ITMX. Thomas pointed out that this oplev doesn't have an analog whitening filter yet, so we should double check when it will be installed.
dtt template was saved under SusSVN/sus/trunk/QUAD/H1/ITMY/SAGL2/Data/2014-02-28_Oplev_Spectra.xml

Evan, Yuta

We redid the Michelson noise budget using the NB simulink tool.
The data we used was taken from the long strech MICH lock on Feb 17 (see alog #10127).
The noise budget agrees well with we have done by hand (see alog #10221, #10217).
NB model works pretty nicely.

[Result]
NB_MICH_1076736130.png: Michelson noise budget plot. "Measured" curve shows the sensitivity curve calibrated from H1:LSC-MICH_OUT. Seismic noise is copied from LLO measurement, so seismic noise curve is not real.

sensorNB_MICH_1076736130.png: Noise budget for sensor noises. Low frequency noise mainly comes from the demodulator board noise. Compared with the one we did by hand (alog #10221), there is a factor of 5 difference in ADC noise. This is because we forget to put the PD filter bank gain (H1:LSC-REFLAIR_A_RF45_(I|Q)_GAIN) in the previous one.

[Note on NbNoiseSink]
If you put NbNoiseSink block into your model, noise at the sink will be calibrated by taking out the model loop gain. If you specify a DAQ channel to that sink and if you run 'nbAcquireData' function, it gets the actual data from a NDS server (using Matlab "get_data" function). So, NB tool automatically calculates the sensitivity curve for given GPS time.

Also, note that LiveParts and data fetching fail if you specify GPS time more than ~7 days ago. I'm not sure why, but it is a limitation from "get_data" function.

H1fw1 and the LDAS gateway were rebooted at 14:42 PST to correct problems with keeping the frame writer process running.  On examination of the LDAS gateway for frame writer 0, it was determined that significant problems existed that required a reboot of that as well.  This interrupted the h1nds0 NDS server and the h1dmt data stream.  

Stefan, Kiwamu,

We could not close the oplev damping loops today. It turned out that the oplev servo gains had been wrong since the model reboot on the last Tuesday. In fact, the signs were wrong in safe.snap file. We updated the safe file. Now they are 0.03 and -0.03 for pitch and yaw loops respectively.

After the BSC-ISI passed a coarse alignment check, went out to work on Post-Cartridge tasks for the TMS.  Basically we want to remove excess mass from the TMS & get it ready for fine balancing of the ISI.

Restraint Tooling/Table Cover Removed & TMS Upper Mass Released

Went ahead and removed the TMS Restraint Tooling (turnbuckles, chains, & eyebolts).  Then I went upstairs and released the Upper Mass.  I then removed the Metal Table Cover.  Some thing I missed were some questionable eyebolts attached to the Upper Structure.  We we want to know whether these eyebolts (most likely) & an aluminum part (not sure) stay on the structure or get pulled off.  Will probably have to address this on Monday BEFORE fine ISI balancing.

Safety Stop Structure (Disassembled & Assembled) & Installed

I then went about installing the Safety Stop Structure (D1001781) to the BSC10.  First thing I noticed was this assembly was built for H2! (see photo #1)  So I had to take the assembly apart and then rebuild it for H1.  I then attached it to the ribbing of the BSC chamber.  After some manhandling, I was able to get this structure up and needled through the eyebolts on the TMS Table.  Other than the possible parts above, the TMS is pretty much ready for ISI balancing.

Note:  will keep the TMS Upper Structure "free" (vs. locked).

After the coarse IAS checks were finished this morning, Travis and I fully unlocked the ETMy QUAD which repositioned all of the masses into their pre-aligned posistions.  This also removed alot of extra locking bracket payload.  We then pulled all of the shield and optic cap payload and added the witness plate mount such that the total payload of the QUAD was within ~a lbs of being correct.  We then reclamped some of the masses lightly such that SEI can load masses around upstairs on top of the ISI in order to continue their work.

Kyle investigated.

Cyrus and Dave

around noon the /ligo file system became unavailable, causing the workstations to freeze up. We rebooted cdsfs0 and restored the file system. We are in the process of restarting the workstations to give them a clean NFS mount.

(Doug, Jason, Hugh, Betsy and CO)
First look at the ETMy in chamber measurements are very encouraging. 
Results:
Longitudinal was short by 0.5mm from absolute, tolerance is +/- 3.0mm,
Lateral position is 0.35mm to the south, +/- 1.00mm
Elevation position is high by 0.35mm, tolerance is +/- 1.0mm

Optic is set lightly on EQ stops, but for a first look to identify any need to move the ISI or SUS this is very reasonable results.

The arm cavity baffle was rough positioned to accommodate the line of sight from the spool and currently rests unattached on its installation table so use caution when working around it.

When fully pay loaded, cabled with the ETM suspended we will do the the fine alignments of the positions and optic angles

J. Kissel, for F. Matichard,

As mentioned in LHO aLOG 10397, Fabrice has installed a clean set of three blend filters on ETMX, ITMX, and BS. (I loaded ITMX filters this morning). Here're plots of the new blend filters for ST1 BSC-ISIs. 
"TCrappy" is exactly the same -- a version virtually identical to Ryan DeRosa's very-low-blend filters, 
"Start" are an improved "750mHz" that *actually* rolls off at high-frequency and does not include the T240s. 
"TStart" has the same displacement sensor / inertial sensor 750mHz crossover, but includes the T240s to get rid of L4C noise at low frequency.

The plan is to use "TCrappy" when possible, and "TStart" under high wind conditions.

7:00 pm PT EDIT:
I've now added the filters for both stages in all degrees of freedom for a BSC-ISI. I've done this using a newly committed version of
/ligo/svncommon/SeiSVN/seismic/Common/MatlabTools/plot_current_blends.m
Use it. All the time. When ever you install a new set of blends.

Jason and I are ready for the lateral and longitudinal ETMy position measurements in the AM. We won't know whether we will need to tweak the ACB position for any line of sight issues until the first look. Thanks Betsy and Travis for setting the ACB for us (temporary setup). We will not release the optic suspension for the fine positioning until we are satisfied that no large moves are needed.

The readback channels for the corner station ring heaters seem to not have been working properly since last Friday.  I've attached a graph that shows that the ring heaters seem to have turned off at 02-21-2014 22:5:32 UTC.  Judging from the ALOG around that time, there were a lot of reboots going on in software, I'm not sure about hardware reboots.  However, Kiwamu says that the PRC power level is looking like the ring heaters are on just based off of the amount of loss he measured.  He also advised that since the system is working well, I should hold off on trying to power cycle the TCS chassis until a later time but at the first chance I get, we should try to resolve this issue.

The ITMX ring heater is also displaying similar weirdness, which is expected since they share the same chassis and PLC.

We thought it prudent to have a spare PUM in-hand for the upcoming monolithic builds, so yesterday we started bonding ears to the PUM ITM03.  Gerardo sucessfully placed an ear on the S4 surface with an error of under 0.01mm misplacement (0.1mm is the tolerance, so well done Gerardo!).  On to the S3 ear...