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Reports until 16:44, Thursday 30 April 2026
H1 SUS
oli.patane@LIGO.ORG - posted 16:44, Thursday 30 April 2026 (90082)
BSFM Transfer Functions good on test stand

To check for any rubbing or other issues that the BSFM might be encountering on the test stand, I took some transfer functions today after Betsy plugged the top mass in yesterday (90063). The measurements have really poor coherence because the BSFM isn't covered, but it's decent enough to at least verify that TFs are looking good and we aren't near touching anywhere.

Data
$(sustrunk)/BSFM/H1/BS/SAGM1/Data/2026-04-30_1615_H1SUSBS_M1_WhiteNoise_{L,T,V,R,P,Y}_0p02to50Hz.xml

Images attached to this report
LHO General
ryan.short@LIGO.ORG - posted 16:30, Thursday 30 April 2026 (90080)
Ops Day Shift Summary

TITLE: 04/30 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: Transfer functions were run on the BS, water lines on the TCSX table were replaced, a galled HEPI spring at BSC2 was removed, and a feedthru on HAM3 was swapped out.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:47 EE Fil LVEA - Running VAC cable 18:54
16:01 FAC Kim LVEA - Technical cleaning 17:11
16:17 TCS TJ, Camilla, Madi LVEA - CO2X water line work 18:18
17:11 IAS Ryan C LVEA - Grabbing a laptop 17:28
17:12 SUS Oli CR - BS transfer functions 18:59
17:16 ISC Elenna Opt Lab YES BHSS OMC work 18:18
17:40 FAC Kim LVEA - Technical cleaning 18:21
17:44 SEI Jim, Randy LVEA - BSC2 HEPI spring replacement 18:49
17:48 VAC Gerardo LVEA - Check in w/ Fil 18:49
17:55 VAC Travis LVEA - HAM3 feedthru work 19:15
18:02 VAC Betsy LVEA - HAM3 feedthru work 19:15
18:50 VAC Jordan X-arm BTE - Taking pictures 18:54
19:01 PEM Ryan C LVEA - BSC2 DM tests 19:41
19:26 CDS Marc, Patrick MER - Checking a chassis 19:36
19:31 SEI Jim, Randy LVEA - BSC2 HEPI spring replacement 20:25
20:11 CAL Tony Opt/PCal Labs Local Beam profiling Ongoing
20:31 FAC Randy LVEA - Craning table over X-arm 21:23
20:33 TCS TJ, Madi LVEA - TCSX table water lines 22:01
20:39 AOS Betsy, Anna LVEA - Walkabout 21:45
20:39 SUS Tom, Oli LVEA - QOSEM testing 21:54
20:57 SUS Fil LVEA - QOSEM testing 21:52
21:12 SAF Richard LVEA - Checks 21:30
21:13 CAL Dripta PCal Lab Local Beam profiling Ongoing
21:32 IAS Ryan C LVEA - Power cycling FARO 21:48
21:38 TCS Camilla LVEA - TCSX table water lines 21:57
21:58 SUS Oli CR - BS transfer functions 23:03
22:24 VAC Jordan, Gerardo LVEA - CP1 work 23:13
22:39 SUS Tom LVEA - QOSEM electronics Ongoing
H1 TCS
thomas.shaffer@LIGO.ORG - posted 15:47, Thursday 30 April 2026 (90078)
TCSX table water lines all swapped and tested, but left off over the weekend

Camilla C, Madi S., TJ S

We finsihed swapping out all of the flex lines on the TCSX table, and have tested the lines at full flow. We will leave the chiller off over the weekend.

We left off last week (alog89976) with the 1/2"OD lines that were spec'd on the BOM not fitting in the Kentek beam dump. I looked it up and the push fittings on the beam dump actually take 10mm OD lines. Ordered those, and we finally were able to install them today. We first plugged in the table lines to the rest of the systme lines but with the chiller off, to get a bit of water on the table, and immediately noticed a leak at one of the beam dump fittings. We tried cutting and reseating the line, but it still had a drip. We replaced the dump with a spare and that seemed to do the trick.

In an effort to put water back in all of the table lines in a lower pressure manner, we hooked one end of the table lines to a wet vac and dipped one in a bucket of lab water. This pulled enough water through the lines and then we capped both lines and let it sit over lunch. There were no drips or evidence of drips when we returned, so we connected the table lines back into the system lines. Madi and I were on the phone while I turned the chiller on with the back 3way valve turned to recirculate (down). I then very slowly moved it up and Madi observed water starting to flow through the system. We kept slowly increasing the flow and watching for leaks until we were at our full 4.0gpm as read from the chiller. 

We decided to keep the chiller off over the weekend, but will turn it back on Monday and will keep a close eye on it since I'm a bit paranoid.

Images attached to this report
H1 DAQ
jonathan.hanks@LIGO.ORG - posted 15:41, Thursday 30 April 2026 (90077)
WP 12469 updated the experimental framewriter

I updated and restarted the frame writer on h1daqfw2 yesterday at 1:37pm and today at 3:04pm localtime.

LHO VE
travis.sadecki@LIGO.ORG - posted 15:14, Thursday 30 April 2026 (90076)
HAM3 D6 flange feedthru swapped

The D6 feedthru on HAM3 was swapped from the 3-port version with 3x Dual DB25 feedthrus to the single piece 12x DB25 connector feedthru.  We re-attached both the in-vac and in-air cables that were originally in that port so that the SUSes can be controlled.

H1 SPI (CDS)
jeffrey.kissel@LIGO.ORG - posted 14:59, Thursday 30 April 2026 (90022)
SPI Fundamentals: DEMOD Filter Digital Signal Processing Trade Study
J. Kissel, S. Koehlenbeck

Executive Summary: as an initial guess -- we chose DEMOD parameters as follows:
    . SIG Bank = NO pre-demodulation filtering (just frequency-independent calibration)
    . I & Q Banks = a comb of notch filters at 4096 Hz (the 1f DEMOD frequency), and 8192 Hz (the 2f DEMOD frequency) and a super simple single-pole 200 Hz low-pass.
as the DEMOD filters for the demodulation of signals from the SPI pathfinder's IFO PDs.

I now have a user interface (LHO:90006) to the SPI pathfinder front-end model infrastructure (LHO:89777), so we're now thinking about filling in that infrastructure with real science (or at least real digital signal processing). 

SIG filters
One of the core principles of the SPI pathfinder's longitudinal degree of freedom is demodulating the 4096 Hz between note between the MEAS and REF beam. We only expect to use the SPI up to ~10-50 Hz, as the demodulated interferometer PDs noise floor begin to be limited by ADC noise ~5 Hz -- see LHO:83412 and detailed noise budget in Figure 1bii.1 in T2400145. Of course, it remains to be seen how much displacement signal we see above this noise floor.

Traditionally when demodulating nowadays, we're looking for the amplitude and phase of the excitation line we inject among surrounding noise that we don't want (think ADS lines, calibration lines, violin mode and PI damping, etc). In that case it makes sense to band-pass the raw signal pre-demodulation -- this is why you see narrow band-passes in many SIG banks. However, in the case of the SPI IFOs and other heterodyne IFOs, we're actually quite interested in the "noise" -- the "excitation line" is instead the carrier frequency, and the "noise" is the phase signal that we then interpret as differential displacement. As such, the design of the SIG, I and Q filters has an entirely different mentality:
    - in the "find the amplitude and phase" mentality, you want a tight band pass on the excitation frequency in the SIG bank, and then as low-a-frequency low-pass filter that you're patience allows.
    - in the "measure the sideband noise out to 100 Hz or so" mentality, you want as little filtering magnitude / phase distortion as possible from any filtering while sill removing any noise above the band of interest from the signal, post demodulation -- which is typically down-conversion from the 2f signal.

So -- we want *no* filtering in the SIG bank prior to demodulation, and a low-pass that has minimal in-band magnitude ripple and minimal in-band phase loss.

Attached is a trade study of filters that show the magnitude, phase, and step response for several options. All these options are installed in the MEAS A and B and REF A and B I and Q filters, but we've turned only the comb and single pole.
Images attached to this report
H1 SEI
jim.warner@LIGO.ORG - posted 14:59, Thursday 30 April 2026 (90075)
HEPI spring galled 2012~ish replaced on BSC2

Since we removed the cartridge from BSC2, I took the opportunity to try to remove a spring that had galled when we first installed the BS & ISI stack for Advanced LIGO. I initially tried coaxing the preload nut on the end of the spring free with alcohol and a couple of long wrenches, but eventually that wasn't enough. With Randy's help, we pulled the two cap pieces off the end of the HEPI house spring tube and lifted the cap, load cell and spring out. This spring was taken to the high bay where Randy used a porta-band to cut the galled nut off, allowing us to retrieve the other hardware off the spring. Was suprised to hear Randy say the kind of dull looking blade on the portaband had no difficulty with steel cap on the spring.

A spare spring from LLO has been installed in it's place, torqued to the crossbeam foot, the old load cell and hardware have been added above.

I didn't get any photos of the work really, but here's a shot of the de-galling method we used. 

Images attached to this report
H1 SUS (SUS)
thomas.roocke@LIGO.ORG - posted 10:26, Thursday 30 April 2026 (90072)
QOSEM Sat Amp CDS Checks

[Tom Roocke, Oli]

Summary: QOSEM Sat Amp installed, run into ADCs and Coil drivers, injected signals into sat amp appearing where the should in CDS.

Yesterday the QOSEM Sat Amp was installed into the SUS-R2 rack (D2300383, LHO:90004), along with the in air DB37 wiring into the ADC. We checked that the signal routing into CDS was good, by injecting a current into the QPD inputs on the front panel. We used the portable calibrator found in the EE shop, to generate a 3.5mA DC current, which is about the expected level of photocurrent during nominal operation of the QOSEM. The negative output of the calibrator is connected to the cathode input for the QPD (pins 16 and 21 on the DB25 QOSEM inputs on the sat amp, see D2500300), and the positive output is connected to the anode inputs (pins 25, 12, 24, 11 and 20, 7, 19, 6). 

We injected current into the anodes for all 6 channels in the sat amp, and all showed up in CDS on the expected channels. Next to check is the QOSEM Duopus cables, which we are waiting on from C&B. After which that should be the full signal chain tested.

LHO VE
david.barker@LIGO.ORG - posted 10:23, Thursday 30 April 2026 (90071)
Thu CP1 Fill

Thu Apr 30 10:06:27 2026 INFO: Fill completed in 6min 24secs

 

Images attached to this report
LHO General
ryan.short@LIGO.ORG - posted 07:42, Thursday 30 April 2026 - last comment - 07:50, Thursday 30 April 2026(90066)
Ops Day Shift Start

TITLE: 04/30 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: 4mph Gusts, 2mph 3min avg
    Primary useism: 0.07 μm/s
    Secondary useism: 0.14 μm/s 
QUICK SUMMARY: Several projects continue today, including surveying of the BS on the test stand and setting up new electronics for the BBSS.

Yesterday, Betsy had turned the HAM3 QPD chassis back on after having it off for replacement of the chamber feedthru, and comparing at least the NSUMs of ASC POP A and B to before the chassis was turned off, the levels are a little lower and a bit noisier (see attached).

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 07:50, Thursday 30 April 2026 (90067)

State of CDS

We are currently running with some RED on the Overview, these are:

1. h1suslo12 (BBSS) has its DACKILL part triggered

2. Removed h1susbs IPC senders are causing some IPC receive errors

3. BSC2 SWWD has SEI tripped

4. Pending SPI filter load

Images attached to this comment
H1 CDS (SEI)
filiberto.clara@LIGO.ORG - posted 17:19, Wednesday 29 April 2026 (90065)
STS-2 Signal Distribution

WP 13216
ECR E1400386

Cables for the STS-2 signal distribution removed. Part of ECR E1400386. The STS-2 interface chassis were left powered off. Part of WP 13149.

H1 CDS (SUS)
filiberto.clara@LIGO.ORG - posted 17:14, Wednesday 29 April 2026 (90064)
Mechanical Test Stand / BSC2 & HAM3 Rack Work

a-Plus O5 SUS BSC2 HAM3 HAM4 (susb2h34) System Wiring Diagrams - D2300383

Electronics and cabling for BSC2 and HAM3 suspensions (BBSS,  LO1, LO2) completed per D2300383. The new HAM-A and Triple Acquisition Drivers were left powered off (BS Bot, LO1, LO2).

Four Kepco supplies were installed in the CER Mezzanine. Supplies provide power to the SUS-R2 rack. A second junction box was added to SUS-R2. They have been set to ±18V and ±24V, shared between SUS and SPI

Final dressing of the field cables going from the biergarten to the West Bay Mechanical Test Stand completed. They will be used for testing of the old and new BS. Some cable swapping in the CER is required for testing the QOSEMs (some old BS electronics will be reused).

Images attached to this report
H1 AOS
betsy.weaver@LIGO.ORG - posted 16:56, Wednesday 29 April 2026 - last comment - 09:47, Thursday 30 April 2026(90063)
BS on Test Stand - Top Stage is damping again
I connected the temp cables which Fil routed for us to the BS Satellite Boxes in the rack in the biergarten.  I disconnected the "to chamber" cables on the Sat amps and connected our temps to those.  After some resorting of the BS Top Stage BOSEM cabling at the ISI, I was able to get the appropriate signals from the appropriate 6 BOSEMs on the medm.  
I am not sure that we will reuse these cables but for the record (since I couldn't find an old BS alog with this info), the Cable Bracket on the ISI is stuffed with these D1000225 cables:

S1106798 Against ISI (Top floor) - BS F1, F2, F3, LF
S1106797 Middle floor - RT, SD
S1104787 Lowest floor - M2 - medm no longer connected tho, says Oli - not plugged in right now anyways

We have more trending to do tomorrow but the F1, 2, 3 Face BOSEMs seem to be "in deeper" while the LF, RT, SD DOFs all show about nominal OSEM position from when it was in the chamber a few days ago.  Chewing on what this means wrt the structure position and ISI/Test Stand level, etc.
Comments related to this report
oli.patane@LIGO.ORG - 08:48, Thursday 30 April 2026 (90068)

M2 cable is unplugged, but if plugged in, we would see the readbacks for that stage on the BBSS M2 stage. So still would be possible to get some info 

betsy.weaver@LIGO.ORG - 09:47, Thursday 30 April 2026 (90070)
Note, I also had to partially uncover the front of the ISI to get the cables out and pinned in such a way to connect to the mock feedthru and then dirty cables.
Images attached to this comment
H1 General
camilla.compton@LIGO.ORG - posted 16:43, Wednesday 29 April 2026 (90062)
ISCT1 to HAM1 Bellows Re-attached

WP13200 Tony and I reattached the bellows between ISCT1 and HAM1.

LHO General
ryan.short@LIGO.ORG - posted 16:32, Wednesday 29 April 2026 (90060)
Ops Day Shift Summary

TITLE: 04/29 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: More surveying was done on the BS on the test stand, and electronics were connected to that the suspension can be damped.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:37 FAC Kim LVEA - Technical cleaning 17:54
14:37 FAC Randy LVEA - Work on HAM5/6/7 cleanroom 18:30
15:41 AOS Betsy LVEA - Walkabout 15:58
16:08 SUS Fil LVEA/CER - QOSEM susrack work 18:46
16:32 IAS Jason, Ryan C LVEA - BS FARO surveying 19:15
17:00 AOS Mitchell LVEA - Checking totes by HAM6 17:32
17:55 FAC Kim EX - Technical cleaning 19:15
18:25 SEI Jim LVEA - Replacing spring on BSC2 HEPI 19:10
18:29 AOS Mitchell LVEA - Bagging parts for LLO 18:51
18:40 ISC Elenna, Sheila Opt Lab - BHSS build 19:45
19:46 SEI Jim, Randy LVEA - Replacing spring on BSC2 HEPI 20:17
19:59 SUS Oli CER n Checking BS cabling 20:47
20:12 SUS Fil LVEA/CER - QOSEM susrack work 21:41
20:18 FAC Randy FCES - Forklifting a table to hi-bay 21:08
20:30 VAC Travis LVEA - Finishing HAM3 feedthru 21:41
20:42 IAS Jason, Ryan C LVEA - BS FARO surveying Ongoing
21:02 SUS Betsy LVEA - BS surveying 23:05
21:11 SUS Oli LVEA/CER - Check in w/ Fil 21:19
21:18 VAC Jordan LVEA - Staging parts by CP1 21:38
22:04 SUS Tom, Oli LVEA - QOSEM electronics 23:15
22:21 ISC Sheila LVEA/Opt Lab - Looking for laptops 22:33
22:24 AOS Mitchell LVEA -   22:35
22:40 ISC Camilla LVEA - ISCT1 bellows, putting away parts Ongoing
23:00 AOS Travis LVEA - Check in w/ Betsy 23:05
23:02 AOS Mitchell LVEA -   23:06
23:15 ISC Tony LVEA - ISCT1 bellows Ongoing
LHO VE
travis.sadecki@LIGO.ORG - posted 16:12, Tuesday 28 April 2026 - last comment - 16:37, Wednesday 29 April 2026(90042)
HAM3 D3 feedthru swapped

The D3 feedthru on HAM3 was swapped from the 3-port version with 3x Dual DB25 feedthrus to the single piece 12x DB25 connector feedthru.  We re-attached the in-vac cables that were originally in that port and Betsy re-attached the in-air cables so that the SUSes can be controlled overnight. 

Comments related to this report
betsy.weaver@LIGO.ORG - 08:09, Wednesday 29 April 2026 (90050)
Cables were unplugged on both the vac and air sides, so keeping track was a bit tedious.  I have started an AS-BUILT cheatsheet which tracks the serial numbers as we go on the main LHO HAM3 Flange Layout DCC page https://dcc.ligo.org/D1002874-v10, see the google doc.  Attached is a snapshot of the sheet with the D3 work logged so far.  
TBC...
Non-image files attached to this comment
betsy.weaver@LIGO.ORG - 16:37, Wednesday 29 April 2026 (90061)
Note, for the 24hours that this feedthru work and recabling was happening, I turned off the chassis that powers this ISC/IO_245 cable to POPA/POPB at the transimpedence amp  SLot U25 of the ISC_R4 rack near the PSL (Thanks Kissel for the consult to get me there).  Per Fil, the picomotors had already been "turned off" when their plug in was disconnected at the ISCT2 picomotor "box", so I didn't do anything for that one. 
H1 SUS
rahul.kumar@LIGO.ORG - posted 14:22, Tuesday 28 April 2026 - last comment - 09:38, Thursday 30 April 2026(90035)
HAM3 chamber vent work - SLiC, BAFFLE ASSY attached to both PR2 and MC2

Mitchell, Rahul

This morning we entered HAM3 chamber and attached the baffles (for stray light control) to both PR2 (HSTS) and MC2 (HSTS) suspensions. The baffle assembly design is shown D1700257_V5. These baffles were attached (directly mounted on the HSTS structure) on both the sides of the optic, i.e  HR and AR side.

Before attaching the baffles I inspected both the optics and they looked nice and clean, hence didn't needed any First Contact cleaning. 

I am attaching pictures below for reference.

We found that both PR2 and MC2 had two missing 1/4-20 threads on the HR side for attaching the mounting rail (D1700249_v1) of the baffle (Mitchell will attach a picture showing the same). Typically, these rail need four holes on the structure for securing them. However, we used the lower two threaded holes for attaching these mounting rail and they were rigidly secured. On the DCC I found that both PR2 and MC2 have D020023_V3 of the HSTS_Structural Weldment Assembly, latest D020023_V7 has more holes on the frame.

We also noted that one of the Siskiyou mount is very close to the MC2 baffle (AR side) as shown in the picture here. However, I can confirm that they are not touching and there is a decent amount of clearance between them. 

I still need to perform health checks on both the suspensions to rule out any rubbing and will post the results as a comment over here.

Note - counts on dust monitor were in single digit before and after entering/exiting the chamber (Thanks to Ryan C for arranging this). 

Images attached to this report
Comments related to this report
rahul.kumar@LIGO.ORG - 14:25, Tuesday 28 April 2026 (90036)

WP13211 closed. 

mitchell.robinson@LIGO.ORG - 14:27, Tuesday 28 April 2026 (90037)

Pictures of the HR side of PR2. No upper mounting holes for the HRST Baffle rail.

Images attached to this comment
rahul.kumar@LIGO.ORG - 10:51, Wednesday 29 April 2026 (90052)SUS

Note:- All the mounting holes looked centered and they aligned nicely and we found no issues (except the one mentioned above) during installation.

rahul.kumar@LIGO.ORG - 09:38, Thursday 30 April 2026 (90069)

IIET ticket filed - https://services1.ligo-la.caltech.edu/FRS/show_bug.cgi?id=37761

 

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