Displaying reports 81-100 of 81714.Go to page 1 2 3 4 5 6 7 8 9 10 End
Reports until 12:00, Tuesday 22 April 2025
H1 CDS
david.barker@LIGO.ORG - posted 12:00, Tuesday 22 April 2025 (84055)
New JAC EPICS channels, will defer adding these to the DAQ

Daniel, Dave:

Daniel has added JAC channels to the ISC-CS slow controls Beckhoff PLC. H1EPICS_ECATISCCS.ini has new H1:JAC channels, these are listed below.

We have decided at this stage to not add these to the DAQ today, we will defer this until the next maintenance period.

+[H1:JAC-ERROR_CODE]
+[H1:JAC-ERROR_FLAG]
+[H1:JAC-REFL_A_DEMOD_DEMODULATORTYPE]
+[H1:JAC-REFL_A_DEMOD_ERROR_CODE]
+[H1:JAC-REFL_A_DEMOD_ERROR_FLAG]
+[H1:JAC-REFL_A_DEMOD_LOMON]
+[H1:JAC-REFL_A_DEMOD_LONOM]
+[H1:JAC-REFL_A_DEMOD_POWEROK]
+[H1:JAC-REFL_A_DEMOD_RFMAX]
+[H1:JAC-REFL_A_DEMOD_RFMON]
+[H1:JAC-REFL_A_DEMOD_SIGN]
+[H1:JAC-REFL_A_DEMOD_SIGNNOM]
+[H1:JAC-REFL_A_ERROR_CODE]
+[H1:JAC-REFL_A_ERROR_FLAG]
+[H1:JAC-REFL_A_PHASE_DELAYNS]
+[H1:JAC-REFL_A_PHASE_DELAYSTEP]
+[H1:JAC-REFL_A_PHASE_ERROR_CODE]
+[H1:JAC-REFL_A_PHASE_ERROR_FLAG]
+[H1:JAC-REFL_A_PHASE_FREQMHZ]
+[H1:JAC-REFL_A_PHASE_PHASEDEG]
 

LHO FMCS
eric.otterman@LIGO.ORG - posted 11:55, Tuesday 22 April 2025 (84054)
Air handler bearing lubrication and alternation
We lubricated the fan bearings in all the air handlers and switched the lead/lag units. 
H1 CDS (AOS)
david.barker@LIGO.ORG - posted 11:41, Tuesday 22 April 2025 (84052)
Stray light ETMX baffle photodetectors back online following 6th April power outage

WP12479 Fil, Dave:

Fil has fixed the missing slow controls Beckhoff terminals at EX which were lost after the site power outage Sun 6th April 2025 18:05 PDT.

Attached 18 day trend of the baffle PD signals show the loss and restoration of signal.

The CDS overview had been expecting only 125 of 127 terminals, and was displaying the degraded DEV4 in dark green, turning to red now all 127 terminals are back. I have removed this exception, DEV4 is now nominal green when new overviews are opened.

Tagging AOS.

Images attached to this report
H1 DAQ
daniel.sigg@LIGO.ORG - posted 11:35, Tuesday 22 April 2025 (84051)
Slow Controls Update

The TwinCAT slow controls software was updated to incorporate LSC-REFL_B. This includes controls and readbacks for a new demod chassis and a new delay line.

H1 AOS (SEI)
jason.oberling@LIGO.ORG - posted 11:29, Tuesday 22 April 2025 (84049)
Another Look at WHAM1 ISI Alignment

J. Oberling, J. Warner

After letting things settle overnight we took another look at the WHAM1 ISI alignment this morning.  Jim found that a few of the HEPI stops had become engaged (likely during the final moves yesterday afternoon), so he backed those off and I took a look at ISI alignment.  Again, the ISI position is reported as deviation from its nominal LHO global coordinates of [-22726.7, 0.0, -201.9] mm.

Jim said this was good enough to begin attaching HEPI actuators, so that work has begun.  We'll take another look at ISI alignment once the actuators are attached.

Data

Data for the above alignment deviations.  Method described in alog 84057.

X axis position and yaw:

Y axis position:

Z axis position and level:

 

H1 CDS
david.barker@LIGO.ORG - posted 11:24, Tuesday 22 April 2025 (84050)
Alarms configured to expect GV2 to be open

Gerardo, Dave:

GV2 was transitioned from closed to open. I have reconfigured alarms to expect this gatevalve to be fully open and alarm if not.

H1 ISC
camilla.compton@LIGO.ORG - posted 10:55, Tuesday 22 April 2025 - last comment - 15:33, Tuesday 22 April 2025(84048)
All ISC components ready to go back onto HAM1

Camilla, Jennie W

Finished getting all the ISC components ready to go back onto HAM1, previous alogs 839458387583858.

Last steps were to replace all remaining black glass v-shaped beam dumps with DLC coated SS (Alena sent us more D1800140-v1-01/02). This was 6 beamdumps: BD1, BD6a, BD11, BD13, BD14 and BD16. The glass was very tightly wedged into BD6a, so I removed the hole v-holder and swapped with a new one. 

Both the lower and upper periscope mirror were dusty, the LPM in particular (photo), so we pulled those out, top-gunned and first contacted. Both were labeled E1000425-v3.
When we went to replace them, we noticed v. small shards of black glass by the UPM. I decided to replace the black glass with the piece removed from M15 to avoid any shards dropping onto the LPM. When I removed the black glass beam dump you could see it was broken at the bottom with a piece still in the clip holder (photo), maybe from over-tightened metal screws.

Now everything is ready, on the rack in the HAM3 cleanroom.

Images attached to this report
Comments related to this report
oli.patane@LIGO.ORG - 15:33, Tuesday 22 April 2025 (84066)EPO

tagging EPO

H1 CDS
erik.vonreis@LIGO.ORG - posted 10:37, Tuesday 22 April 2025 - last comment - 12:07, Tuesday 22 April 2025(84047)
Bootserver puppet update to re-order models.

I ran the bootserver puppet on h1vmboot1 to reorder the models on h1seih16.  The puppet module was updated to the latest from gitlab.

Comments related to this report
david.barker@LIGO.ORG - 12:07, Tuesday 22 April 2025 (84056)

The model ordering for seih16 was inconsistent with seih23 and seih45. The the latter the order is both-HEPI followed by both-ISI. h1seih16 on the other hand was using a HAM1 (HEPI+ISI) followed by HAM6 (HEPI+ISI) scheme. These are both good schemes, but for consistency we have made h16 the same as the others.

Note that the order of the models on the CDS overview is the order in which the models are started when the front end is restarted. If you are interested, the order is defined in /opt/rtcds/lho/h1/cds/H1.yaml

Images attached to this comment
LHO VE
david.barker@LIGO.ORG - posted 10:20, Tuesday 22 April 2025 (84046)
Tue CP1 Fill

Tue Apr 22 10:07:18 2025 INFO: Fill completed in 7min 14secs

 

Images attached to this report
H1 CDS (PSL)
filiberto.clara@LIGO.ORG - posted 10:18, Tuesday 22 April 2025 - last comment - 13:53, Tuesday 22 April 2025(84045)
PSL Picomotors Controls

WP 12480
FRS 6499

The PSL picomotor controls have been moved from the ISC Driver to the PSL Driver installed in the PSL-R2 Rack (alog 63613, alog 62830). The new DB25 cable is routed from behind the PSL field rack into the enclosure. The old controls cable was pulled out of the enclosure and will be reused for HAM1/JAC. Ryan Short is testing picomotors are operational through MEDM.

F. Clara, R. McCarthy, R. Short

Comments related to this report
ryan.short@LIGO.ORG - 13:53, Tuesday 22 April 2025 (84062)PSL

I moved the picomotor breakout box (D1101691-v1) from its previous location on top of the water pipes between the PSL table and the north wall of the enclosure (first picture) to underneath the center of the table (second picture) to accommodate the new DB25 cable coming from the west wall out to the PSL racks. New cable was routed through the floor cable manager and DB9 cables up to the table were coiled under the table to account for extra length. Cable routing from the breakout box up to and on the PSL table are unchanged.

I also tested all eight picomotors (four for the two mirrors for PMC steering, four for the two mirrors for RefCav steering) and all are working well and as expected.

Images attached to this comment
LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 07:32, Tuesday 22 April 2025 (84043)
OPS Day Shift Start

TITLE: 04/22 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: MAINTENANCE
    Wind: 7mph Gusts, 5mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.20 μm/s
QUICK SUMMARY:

IFO is in PLANNED ENGINEERING for the vent.

Some of today's planned maintenance:

Work safe!

LHO VE
janos.csizmazia@LIGO.ORG - posted 18:31, Monday 21 April 2025 - last comment - 08:10, Wednesday 23 April 2025(84042)
2025 April vent - VAC diary
4-21 (Monday) activities:

- The aux carts from the annuli of GV5 and HAM4 were valved out; after a little hesitation, both IPs turned over, so now all AIPs are in good shape, without external support
- The pumpdown of the corner continues, with the corner being at 1.51E-6 Torr, and HAM6 is at 1.49E-6 Torr. There is a ~17% increase in pumping speed relatively to the last pumpdown in 2024 August. The details will be summarized soon.
- The pressure in the soft-closed GV7's actuator was increased from 10 to 15 psig, in preparation of opening GV2 tomorrow
- The flanges of the recently installed HAM6 turbo and HAM6 gauge was leak checked, no leaks were found, with the background of <1.0E-10 He
- All the welding seams on the X-manifold have been leak checked, no leaks were found, with the background changing between 2.6-3.0E-10 He. The welds have been individually bagged, see attached pic
Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 08:10, Wednesday 23 April 2025 (84079)EPO

Tagging this unique photo for EPO since these sorts of leak checks (on welds) you don't see everyday.  :)

H1 SUS (SEI, SUS)
edgard.bonilla@LIGO.ORG - posted 18:20, Monday 21 April 2025 - last comment - 08:39, Thursday 24 April 2025(84041)
SR3 OSEM estimator preliminary fits

Edgard, Brian.

Following up on the fits for the SR3 estimator. I ran the plotall scripts on the transfer functions we took last Friday [see 84003]. Then ran the attached code to fit the transfer functions.

Figure 1 shows the ISI-M1 fitted transfer function. The Q-factors for the fit were tweaked by hand so I could get a decent fit. The exported M1 to M1 transfer function is shown in the second attachment. I decided it should have the same poles as the ISI one, and the gain was fit so the estimator matches the high-frequency behavior of the measured transfer function. The choice to share poles is because the math indicates that it will lead to some potential modeling errors cancelling out.

The pole information for the two filters is:

         Pole              Damping       Frequency      Time Constant  
                                       (rad/seconds)      (seconds)    
                                                                       
 -4.38e-02 + 6.38e+00i     6.86e-03       6.38e+00         2.28e+01    
 -4.38e-02 - 6.38e+00i     6.86e-03       6.38e+00         2.28e+01    
 -7.64e-02 + 1.44e+01i     5.30e-03       1.44e+01         1.31e+01    
 -7.64e-02 - 1.44e+01i     5.30e-03       1.44e+01         1.31e+01    
 -2.97e-02 + 2.13e+01i     1.39e-03       2.13e+01         3.37e+01    
 -2.97e-02 - 2.13e+01i     1.39e-03       2.13e+01         3.37e+01

And the zpk strings (in MATLAB format) are:

ISI to M1:

zpk([-0.068+20.398i,-0.068-20.398i,-0.099+11.454i,-0.099-11.454i,0,0],[-0.03+21.271i,-0.03-21.271i,-0.076+14.435i,-0.076-14.435i,-0.044+6.384i,-0.044-6.384i],-0.75)'

M1 to M1:

zpk([4745.079,-0.089+8.28i,-0.089-8.28i,-0.113+19.058i,-0.113-19.058i],[-0.03+21.271i,-0.03-21.271i,-0.076+14.435i,-0.076-14.435i,-0.044+6.384i,-0.044-6.384i],-0.015)

 

I did the fits by using the spectrumest function in MATLAB (which is sadly not available in 2019a). The long term plan is to switch to one of the many python fitting tools that people like for the fits. The code is attached to this logpost for bookkeeping

Images attached to this report
Non-image files attached to this report
Comments related to this report
edgard.bonilla@LIGO.ORG - 15:23, Wednesday 23 April 2025 (84093)

I added a script to

... SusSVN/sus/trunk/HLTS/Common/FilterDesign/Estimator/

that uses autoquack to add the fits to the Foton file for H1 SR3.

The script is named

make_SR3_yaw_model.m

and it uses the fits mentioned in the logpost above, which are contained in the same folder, as

fits_H1SR3_2025-04-21.mat

The changes are current to the sus svn under revision 12277.

oli.patane@LIGO.ORG - 16:36, Wednesday 23 April 2025 (84096)

These filters have been loaded into the SR3_M1_YAW_EST_MODL_SUSP_Y_2GAP and SR3_M1_YAW_EST_MODL_DRV_Y_2GAP.

Attached are the plots that came up when I ran the matlab script that loaded them in, along with the log message that was created and the coeff diffs.

Images attached to this comment
edgard.bonilla@LIGO.ORG - 17:51, Wednesday 23 April 2025 (84098)

Small modification that will not affect the estimator test, so it is here for bookeeping.
I didn't clean up the zpk for the M1 to M1 transfer function, so it has a high frequency zero that is due to floating point errors in my fit.

the real zpks should be:

ST1 to M1

    'zpk([-0.068+20.398i,-0.068-20.398i,-0.099+11.454i,-0.099-11.454i,0,0],[-0.03+21.271i,-0.03-21.271i,-0.076+14.435i,-0.076-14.435i,-0.044+6.384i,-0.044-6.384i],-0.75)'

and M1 to M1

    'zpk([-0.089+8.28i,-0.089-8.28i,-0.113+19.058i,-0.113-19.058i],[-0.03+21.271i,-0.03-21.271i,-0.076+14.435i,-0.076-14.435i,-0.044+6.384i,-0.044-6.384i],71.17)'

I have uploaded the correct ones to the HLTS/Common/FilterDesign/Estimator with today's date (2025-04-23), svn revision 12279.

 

oli.patane@LIGO.ORG - 08:39, Thursday 24 April 2025 (84105)

That filter change has been loaded in

Images attached to this comment
H1 DAQ
jonathan.hanks@LIGO.ORG - posted 18:11, Monday 21 April 2025 (84040)
WP 12469 Installing an experimental frame writer for testing
Today I setup h1daqfw2 as a platform to test a new frame writer for use after O4.

For the fw hardware I repurposed h1digivideo3 which is an older Xeon server with 10 cores and 64GB of ram.  I added 2x2TB old hard disks in a RAID 0 config (to improve the write performance).  At this point I am not looking to do any mid to long term storage of frames.

I did not connect this up to the data stream via dolphin.  Instead I am running a new instance of cps_xmit on h1daqnds0 and using that over a new dedicated 1g link to h1daqfw2.  I've updated the puppet config for h1daqnds0 to make this a persistent change.

At this point I am running the new frame writer on h1daqfw2, and it is producing frames.  I need to do some more configuration (mainly around the run number server) so the frames will be identical to those output from the other frame writers (the difference should be in metadata in the frame headers, not the recorded data).  In simulated data setups I have produced frames that are byte for byte identical to daqd frames so it is fairly likely that after I get that working I will see identical frames.

The point of this frame writer is to move towards a auto-reconfiguring/restartless system that is able to adjust on the fly to channel changes, remove some other limitations in the daqd, and to become the ngdd projects frame writer for downstream derived data products.

The first things I will look at with this is memory and cpu requirements under the H1 load.

This testing will be ongoing.
H1 AOS
jason.oberling@LIGO.ORG - posted 17:49, Monday 21 April 2025 - last comment - 12:09, Tuesday 22 April 2025(84039)
IAS First Look at WHAM1 ISI

R. Crouch, J. Warner, J. Oberling

We took a first look at the alignment of the WHAM1 ISI today.  Quick alog with results, I'll add details as a comment tomorrow.

Nominal position of the WHAM1 ISI is, in LHO global coordinates, [-22726.7, 0.0, -201.9] mm.  I post the results as deviations from these nominal positions.

Initial:

After a few rounds of adjustments, the final measurements for the day:

Will let things settle overnight and take a full round of measurements in the morning, including another look at y-axis position (since we didn't get a final measurement on that).  Will do any further adjustments at that point.

The IAS survey equipment is still set up on the -Y side of WHAM1 (East if going by crane directions).  Please do not disturb this equipment!

Edit 4/22/2025: Had the wrong yaw direction for the final set of measurements, should be CCW.  Also had the wrong z-axis deviation for the final set of measurements, should be +0.69 mm.

Comments related to this report
jason.oberling@LIGO.ORG - 12:09, Tuesday 22 April 2025 (84057)

Details and Methodology

Since the FARO decided it needed a Florida vacation we have to use the same alignment method employed during aLIGO install.  This is done using a total station for measuring X and Y axis position and ISI yaw, and an autolevel for measuring ISI height and level.

X Axis Position and Yaw

2 sets of crossed scales are used with the total station to make the required measurements.  These scales are mounted in such a way that one edge of the vertical scale lines up with the y-axis centerline of the ISI; a second scale is mounted horizontally to give a reading of the x-axis position of that location.  The 2 sets of scales are mounted to the outermost holes on the +Y and -Y side of the ISI, see the attached picture for an example (the right-most edge of the vertical scales are in line with the ISI y-axis centerline).  The -Y scale mount also has a mounting hole for a corner cube retroreflector, which gives us the ability to used the total station's Electronic Distance Measurement (EDM) function to measure the distance between the total station and the outermost -Y holes of the ISI.

There is a brass monument on the floor to the East of WHAM1 that the total station is set over; this is monument LV25, coordinates [-22726.7, -3050.7] mm.  The total station the sights monument LV26 (cooridnates [-2133.6, -3050.7] mm), which is down by WHAM4, and this line sets our horizontal angle to zero.  The total station is then turned -90° to point at the center of WHAM1.  We then use the total station to read the horizontal scale of each set of crossed scales to get a measurement to calculate x-axis position deviation and ISI yaw; the distance between the outermost holes, 2082.8 mm (taken from the SolidWorks model of the ISI), gives us the needed info to calculate the yaw.  Using the numbers for the final measurements from the above main alog as an example, the calculation looks like this:

  • +Y scale reading: 0.0 mm
  • -Y scale reading: +0.5 mm
  • X axis position deviation: (0.5 + 0.0) / 2 = +0.25 mm
  • Yaw: (0.5 - 0.0) / 2082.8 = 240 µrad CCW

Y Axis Position

A corner cube retroreflector is mounted to the -Y scale mount, designed in such a way so the measurement point of the corner cube lines up with the outermost row of holes.  From the SolidWorks model of the ISI this outermost row of holes is 1041.4 mm from the center of the ISI.  The total station occupies monument LV25, which has a y-axis coordinate of -3050.7 mm.  Since the ISI should be at a y-axis coordinate of 0.0 mm, we then use the total station's EDM function to measure the distance from the total station to the corner cube.  The target distance is the y-axis coordinate of monument LV25 minus the y-axis coordinate of the outermost -Y holes of the ISI, or |-3050.7 - (-1041.4)| = 2009.3 mm.  Using the numbers from the Initial measurements (since we did not take a final look at y-axis position yesterday afternoon) in the above main alog as an example, the calculation is:

  • Total Station EDM: 2009.7 mm
  • Target Distance: 2009.3 mm
  • Y axis position deviation: 2009.7 - 2009.3 = +0.4 mm

Z Axis Position and Level

For the z-axis position deviation and ISI level we use an autolevel and a scale set at various points on the ISI.  The autolevel is set to +100.0 mm above the target ISI height using height mark 600 (on the East wall across from WHAM1).  From T1100187 the LHO local coordinate for this height mark is -249.7 mm.  We set a scale on this height mark, with 10.0 mm on the scale lining up with the height mark.  We can then calculate what scale reading required to set the autolevel at +100.0 mm above the target height of the ISI.  The LHO global z-axis coordinate for the WHAM1 ISI is -201.9 mm, but the height mark is in LHO local so we have to translate between the two coordinate systems.  This means we have to add 14.1 mm1 to the LHO global coordinate to get the LHO local coordinate for the WHAM1 ISI; doing this, the LHO local coordinate for the ISI is -187.8 mm.  Now the delta between the WHAM1 ISI z-axis position and height mark 600 is calculated, then add 100.0 mm to that to set the autolevel 100.0 mm above the target ISI height; we have to also add 10.0 mm since that's where the scale was set on the height mark: |-249.7 - (-187.8)| + 100.0 + 10.0 = 171.9 mm.  So sighting 171.9 mm on the scale we mounted on height mark 600 puts the autolevel 100.0 mm above the target z-axis position of the ISI.

With the autolevel set, we then place a scale at several points on the ISI and use the autolevel to read the scale at each point.  The scale we have for this is in inches, and has tic marks at every 0.01".  Since the autolevel is 100.0 mm above the target ISI height we should be reading 3.94" (100.0 / 25.4 = 3.94) on the scale if the ISI is at the correct height; reading a lower number on the scale means the ISI is too high, and reading a higher number on the scale means the ISI is too low.  The scale is placed at the 4 corners of the ISI, with a reading taken at each point.  These 4 readings are averaged to give the height of the ISI table.  For the table level, the delta between the highest and lowest scale reading is used.  Using the numbers from the final measurements from the above main alog, this calculation looks like:

  • -X/+Y scale reading: 3.905"
  • -X/-Y scale reading: 3.915"
  • +X/+Y scale reading: 3.915"
  • +X/-Y scale reading: 3.915"
  • Average: 3.913"
    • Z axis deviation: 3.94 - 3.913 = 0.027" => +0.69 mm
  • Level: 3.915 - 3.905 = 0.01" => 0.25 mm

1: The 14.1 mm correction comes from removing the global x-axis tilt of -619.5 µrad, done by multiplying the x-axis tilt by the x-axis position of the WHAM1 chamber: -22726.7 * -.0006195 = +14.1 mm.

Images attached to this comment
H1 SEI
jim.warner@LIGO.ORG - posted 17:49, Monday 21 April 2025 - last comment - 13:06, Tuesday 22 April 2025(84038)
HAM1 HEPI floating with most of the payload, progress on intial alignment

Jason, RyanC, Mitch, Randy, Jim

This morning Randy, Mitch and I put initial payload on the HAM1 ISI, 210kg of tabletop mass, stacks of 2 D091075 10kg masses. 3 of these stacks are suspended on viton for damping, these are spread across the table as much as I could, but the drawing I'm working from basically has them all in a row down the middle. This got the payload close enough that we could start thinking about initial alignment. 

After lunch, we went out and squeezed 4 more dial indicators on the north side of the chamber. This was pretty difficult getting 2 under the chamber and then attaching 2 more with magnetic bases to the HAM2 crossbeams. With that, we were able to start putting weight on the HEPI springs. We went to each corner, backed all of the stops off till they were barely touching the foot, except for the 3 stops holding the corner up. We then evenly loaded the springs on one pier until the bottom stops were free, while watching dial indicators to make sure nothing moved too much.

Once all 4 corners were floating on springs, we called Jason and Ryan out to set up and take position shots with the total station. All of us very much missed the Faro for the next 90 minutes. When they were set up and got a measurement, I went around and tweaked the springs until the ISI was within more or less +/- 1mm. Table is level to about 1/4 mm across the 4 points we measured. Table yaw I think was out about 250 urad, but hopefully Jason can put some numbers up later.

Tomorrow, the plan is to lock HEPI again, verify we haven't disturbed the position and start reattaching actuators. When that is done, ISC can start their reinstall.

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 13:06, Tuesday 22 April 2025 (84059)EPO

Tagging for EPO photos.

H1 General
anthony.sanchez@LIGO.ORG - posted 16:42, Monday 21 April 2025 (84036)
Monday Ops Shifts Report

TITLE: 04/21 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:

HAM Team1 has said "We managed to suspend HEPI on HAM1, but are still doing initial alignment so the mechanical stops are disengaged. The whole stack is just on springs, so running into the crossbeams could damage the bellows if done with enough exuberance. Don't do that. "

Norco Contractor arrived at at 17:20 UTC 
Model resart H1ASC H1LSC starting at 19:50 UTC


LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:46 VAC Jordan LVEA N Purge Air Checks. 14:59
14:58 FAC Kim LVEA N Technical Cleaning 16:58
16:17 IAS Jason & Ryan LVEA HAM1 N Setting up for alignment. 17:59
16:19 CDS Johnathan MSR No Installing & Spinning up AUX Frame writer 18:19
16:20 FAC Randy LVEA N Helping HAM1 Alignment work 18:47
16:32 VAC Jordan & Janos LVEA +X N Leak checking 18:32
16:33 Safety McCarthy LVEA N Safety Checks 17:33
16:47 SEI Jim LVEA HAM1 N Aligning HAM1 18:47
16:48 SEI Mitchel LVEA HAM1 N HAM1 Aligning & Installing 18:40
17:13 EE Fil LVEA & Mids N Capitol Inventory 19:12
17:26 FAC Kim HAM Shaq N Technical Cleaning 18:32
17:44 ISC Camilla & Jennie W LVEA N Swapping Beam dumps from glass to metal. 19:32
18:43 PCAL Tony PCAL Lab YES Move Power sensors 18:52
19:11 VAC Jordan LVEA & Ends N Annual inspect of Dewers  Site Wide 17:11
19:13 EE Fil & McCarthy LVEA N Satelite check 19:43
19:32 SEI Randy , Mitchel, Jim LVEA HAM1 N Aligning and installing ISI 22:13
20:51 ISC Camilla LVEA N First contacting optics 21:36
20:53 FAC Tyler Ham Shaq area N De-tumble weeding 22:25
21:14 ISC Ryan LVEA N Helping Camilla 21:21
21:15 Safety McCarthy LVEA N Looking for Fil 22:00
21:22 VAC Janos & Jordan LVEA N Vacuum Work 01:22
22:01 EE Tony, Fil PCAL Lab y(local) Checking if SR95 for Fil is in there 22:57
22:18 IAS RyanC, Jason LVEA n Alignment work 00:18
22:45 ISC Camilla & Jennie LVEA N First contacting 23:05
22:49 VAC Gerardo LVEA & Ends N Capitol eye Inventory 00:49
H1 ISC
elenna.capote@LIGO.ORG - posted 16:45, Tuesday 08 April 2025 - last comment - 16:19, Monday 21 April 2025(83820)
First Half of HAM1 table cleared

[Betsy, Camilla, Elenna, Oli]

We cleared half of the HAM1 table today on the +y side. This cleared optics on the ALS and POP paths, and the first part of the optics on the REFL path. We carefully labeled each component, and Oli logged component and cable names with serial numbers. Betsy laid the components in clean pans lined with cleanroom cloths. The cables are still attached to the feedthroughs and were left lying at the bottom of the chamber.

Attached photos show cleared side of the table.

Before removing components, we reviewed the table layout after Ibrahim and TJ noticed some discrepancies between the solidworks drawing and the optic locations as depicted in Corey's pictures from yesterday. We confirmed that there are some dispcrepancies between the two. TJ has a more detailed report.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 16:48, Tuesday 08 April 2025 (83822)

Before we started, Betsy and I replaced the septum plate VP cover we had removed yesterday 83798

Layout before: D1000313-v15

camilla.compton@LIGO.ORG - 16:19, Monday 21 April 2025 (84035)EPO

Added photo of myself, Betsy, Melina and Elenna before the HAM1 ISC removal work started. 

Images attached to this comment
H1 SQZ
camilla.compton@LIGO.ORG - posted 14:33, Monday 31 March 2025 - last comment - 09:42, Tuesday 22 April 2025(83660)
SQZ with SRCL offset at -306, FC detuing at -28

Sheila, Camilla, Jennie

This morning we changed SRCL offset from -191 to -306 and FC de-tuning from -34 to -28, as discussed in  83570. Took some SQZ data here as we were interested if we could get FIS SQZ lower than No SQZ ~100Hz and below, Sheila's models (e.g. 83572) suggest we should but it looks like there's a low frequeceny noise source (in FIS not FDS) in our data sets preventing us from getting down to the modeled level of SQZ.

Sheila turned OPO trans setpoint up from 80uW to 95uW to increase NLG from 11 to 19 (similar to what we had earlier in O4). Measured NLG with 76542. OPO gain left at -8. Turned off  SQZ ASC.

opo_grTrans_ setpoint_uW Amplified Max Amplified Min UnAmp Dark NLG (usual) NLG (maxmin) OPO Gain
95  0.0176 0.000279 0.00002 0.00094 19.1 20.0 -8
110 0.03315 0.000269 0.000879 -0.00002 35   -8
 
Starting FC2 misaligned offsets in M1 TEST were 100 and 200, Sheila increased to 200 and 400. So that we know FC2 is really misaligned. Saw no difference at SQZ or ASQZ. So this low fruecny noise in FIS is not due to FC backscatter.
Data attached and saved at camilla.compton/Documents/sqz/templates/dtt/20250331_SRCL_neg306.xml
 
Type Time (UTC) Angle Notes DTT Ref
No SQZ 03/29 N/A   ref 0
FIS SQZ   171 Angle tuned for FDS (maybe thermalized since) ref1
FIS SQZ 17:05:00 154 Ang tuned for FIS ref2
FIS Mid(ish) 17:15:00 101 Little better than no SQZ at 60Hz ref3
FIS Mid(ish)   92   ref4
ASQZ FIS   68   ref5
ASQZ FIS -10deg 17:24:00 58   ref6
ASQZ FIS +10deg   78   ref7
FIS Mid(ish) 17:31:30 115   ref8
FIS Mid(ish) other side 17:43:00 27   ref9
FIS Mid(ish) 17:45:30 82 Check data doesn't include a glitch ref10
 
Then changed the SRCL de-tuning back to -191 (still in FIS so FC de-tuning doesn't matter). Comparison is attached.
This SRCL offset change didn't effect the level of low frequency noise.
 
Type Time (UTC) Angle Notes DTT Ref
FIS ASQZ +10deg 17:53:00 82 Plot seems similar with same ang, different SRCL offset ref 11
FIS ASQZ 17:56:00 72   ref12
FIS ASQZ -10deg   62   ref13
FIS Mid (ish)   104 Can see that rotation is a little different with SRCL de-tuning different but low freq noise level is the same. ref14
 
Kept SRCL de-tuning at -191 but increased NLG to 35. 
This was interesting for mid-SQZ values as the level of the low freq noise increased with the higher NLG but was the same at different SQZ angles (112 and 100deg). Plot attached. Compare grey and pink (NLG 35) to blue and brown (NLG19) <70Hz. So the low frequency FIS noise is NLG dependent.
 
Type Time (UTC) Angle Notes DTT Ref
Mid SQZ   112 Interesting data here. Low freq noise higher than with NLG 19. ref 15
ASQZ 18:20:00 70   ref16
MidSQZ 18:22:30 100   ref17

Sheila turned OPO trans back to 96uW so expect NLG to be 19 going into Observing, larger than normal but closer to the value uses before the last OPO crystal move. SQZ angle servo off and angle set back to 171. ADF left on.

Images attached to this report
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sheila.dwyer@LIGO.ORG - 09:42, Tuesday 22 April 2025 (84032)

I had a brief look at some of this data to put bounds on losses and arm power in 83953:

The first attachment shows a plot of more of this data against models, focusing on the unexplained low frequency noise that we don't see with the filter cavity . The measured NLG matches the NLG infered from anti-squeezing and squeezing for the NLG 19 measurements, but for the NLG 35 measurements the infered NLG is 27.3, so that is what I've used here.  As Camilla wrote above, the NLG 35 measurements were made with a different SRC detuning than NLG19, so that is included in this model.  Squeezing angles are fit to the band from 2100 Hz to 2300 Hz. 

The first plot shows the measured data in solid lines, the quantum noise model in dashed lines, and the dotted lines show the non quantum noise from subtraction added to the quantum noise models.  There is a discrepancy where many of the measurements seem to have extra noise from 20-50 Hz, I've tried to make an easier to read version in the second plot, and finally removed some traces to try to make it easier to see.

In the above alog we thought perhaps that this could be explained as an excess noise that was larger with higher nonlinear gain but consistent with squeezing angle, the last attachment shows the residuals between the model and measurement for the measurements that had clear discrepancies, they all seem to be different, so this excess seems to depend both on squeezing angle and nonlinear gain. 

The script used to make these plots can be found at this repo

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