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Reports until 23:16, Monday 27 April 2026
H1 ISC (CDS, INS, ISC, SYS)
keita.kawabe@LIGO.ORG - posted 23:16, Monday 27 April 2026 - last comment - 23:46, Monday 27 April 2026(90026)
OMCA-QPD1 sense pin is shorted to the suspension platform, causing massive 60Hz problem (Elenna, Keita)

Problem

We started checking the health of QPDs and were puzzled that all four quadrants of the OMCA QPDA are much, much noisier than OMCA QPDB.

Note, there's a naming inconsistency about the QPD numbering between D2200276 wiring diagram and D0981811 (see "cartoon version"). 

D0981811 OMCA QPD-1 OMCA QPD-2 OMCB QPD-1 OMCB QPD-2
D2200276 QPD-2 QPD-1 QPD-8 QPD-7

Cause of the problem

Anyway, the problem was tracked down to short-circuit of common mode noise sensing line for OMCA-QPD1 (pin 11 of DB25 inside the vacuum, pin 3 outside of the vacuum, see attached) to the metal part of the suspension structure (i.e. ISI surface and the chamber) which in turn is grounded to the lab ground.

OMCA QPD-2 as well as both of the QPDs for OMCB are fine.

All QPD segments (incl. OMCA QPD1) responded to the flashlight.

Dark noise test: OMCB QPDs looks OK, not sure about OMCA QPDs

We connected a dual-QPD trans impedance chassis (S1102832, which is the original version of D1002481) to the OMCB QPDs like this:

QPDs-DB25 assy - in-vac cable (DB25F-DB25F)  - feedthrough simulator - DB25F-to-DB25M-cable - S1102832 front panel.

We looked at the output of the TIA with SR785 when there's only ambient light on QPDs (not much), segment by segment. No segment was extra noisy or anything.

OMCA QPDs are a different story because of the 60Hz problem. 

We'll see if the problem could be solved by somehow reassembling the QPD or cutting the noise line. 

Images attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 23:46, Monday 27 April 2026 (90029)

1st attachment shows the connection from the QPD to TIA. ("S1P" "S2N" etc. mean segment 1 positive pin, segment 2 negative pin etc.)

2nd attachment shows how the output of the TIA (all differential) was connected to SR785 or oscilloscope, using QPD1 seg1 as an example.

3rd attachment shows that CH1 (yellow), which is the segment 1 positive pin of the QPD1 for OMCA, was terrible while the segment 1 positive of QPD2 for OMCA (blue) was not. Though there's no picture, the terrible 60Hz noise appeared in the negative pin with the opposite sign (for QPD1) so it's not cancelled.

For OMCB QPDs, DC offset of all segments were smaller than 1mV when there was no light (used a fluke DVM to measure across positive and negative pins). For OMCA QPD2 that was also the case.

OMCB_QPD[12]_SEG[1234].jpg are the noise measurements for OMCB QPDs using SR785. The TIA output (which receives 0.4:40 whitening in the chassis) just shows the TIA noise from 200Hz and higher without any light on QPDs, which looks fine to me. There's no reason to suspect that one or more of these segments/QPDs are broken.

The last attachment (QPD_removed.jpg) shows a measurement of OMCB_QPD2_SEG4 after disconnecting the QPD from the front panel, showing the TIA noise floor. SR785 noise floor is lower than this.

Images attached to this comment
H1 CDS (ISC)
filiberto.clara@LIGO.ORG - posted 17:16, Monday 27 April 2026 (90027)
ISCT1 and JAC Table Enclosures

Cabling to the ISCT1 and JAC table enclosures complete. Use caution when moving the cleanroom, one of the legs is close to the patch panel/cables on ISCT1.

Images attached to this report
LHO General
ryan.short@LIGO.ORG - posted 16:33, Monday 27 April 2026 (90024)
Ops Day Shift Summary

TITLE: 04/27 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: The BSC2 cartridge has been flown over to the test stand in the West bay.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:16 FAC Randy LVEA - Prep for cartridge removal 15:44
15:28 FAC Kim LVEA - Technical cleaning 16:38
15:30 AOS Tony LVEA - Connecting headset 16:13
16:51 FAC Kim LVEA - Technical cleaning 17:58
16:58 IAS Jason LVEA - Grabbing laptop 17:06
17:07 AOS Tony LVEA - BSC2 cartridge removal 20:36
17:07 SEI Jim LVEA - BSC2 cartridge removal 20:36
17:11 FAC Tyler LVEA - BSC2 cartridge removal 20:33
17:13 VAC Jordan LVEA - BSC2 cartridge removal 20:36
17:14 FAC Mitchell LVEA - BSC2 cartridge removal 20:36
17:17 TCS Camilla Opt Lab - Looking for a lens 17:32
17:24 AOS Betsy LVEA - BSC2 cartridge removal 20:36
17:24 VAC Gerardo LVEA - BSC2 cartridge removal 20:36
17:26 VAC Travis LVEA - BSC2 cartridge removal 20:01
17:32 TCS Camilla, Madi, Adrien EX YES ALS/HWS table work 18:39
17:34 EE Fil LVEA - Cabling HAM1 tables 19:07
17:38 AOS TJ LVEA - BSC2 cartridge removal 20:32
17:43 FAC Chris LVEA - FAMIS checks 18:29
17:57 SUS Tom Vac Prep - Cable making prep 18:32
18:03 SUS Rahul FCES - Looking for a table 18:29
20:11 ISC Keita, Elenna Opt Lab - BHD OMC work 21:43
20:18 SUS Oli, Tom Vac Prep - QOSEM cables Ongoing
20:43 EE Fil LVEA - Cabling HAM1 tables 22:18
21:08 PEM Ryan C LVEA - Setting up dust monitor at test stand 21:39
21:09 FAC Randy LVEA - Tidying up 21:18
21:46 TCS Camilla, Madi EX YES ALS/HWS table work Ongoing
22:05 ISC Elenna, Adrien Opt Lab - Tour 22:46
22:58 IAS Jason LVEA - Prepping FARO for tomorrow 23:06
23:04 SEI Jim LVEA - Checking dial indicators on BSC2 23:27
23:06 ISC Keita Opt Lab - BHD OMc work Ongoing
23:17 PEM Ryan C LVEA - Swapping dust monitor fuse Ongoing
H1 PSL
ryan.short@LIGO.ORG - posted 14:30, Monday 27 April 2026 (90023)
PSL 10-Day Trends

FAMIS 31135

The PSL was offline for a bit last Tuesday for chassis work that took down the interlock (alog89965), but came back up with only a few things being different. Most notably, the PMC is at a slightly different temperature, so the transmitted power is a bit lower while the reflected power is a bit higher.

Images attached to this report
H1 SYS
betsy.weaver@LIGO.ORG - posted 14:05, Monday 27 April 2026 - last comment - 20:36, Monday 27 April 2026(90021)
BSC2 Cartridge on the Test Stand
The BSC2 cartridge was removed from the BSC2 chamber today and placed on the Test Stand in the West Bay (+Y bay).  The lift took 3 "test lifts" to make very minor adjustments to the CG prior to lift out of the chamber - on the 4th lift, we were very well balanced so embarked on the flight.
Like LLO, the BS had it's "Stay Leg" assemblies and Vibration Absorber Assemblies removed for the flight.  This means it was probably lighter than the 2013 time (alog 5689) when we did this which had the weight slightly heavier.  The cartridge plus 3-point lift fixture and load cell together all weighed 9380 lbs.  It was rotated 90deg Counterclockwise per the procedures and landed on the threaded rod in the test stand with little issue other than careful craning and spotting.
All went as expected and according to the procedures E1200433-v3, E1200971-v4 and associated docs.

Mitchell, Travis, Tyler, Randy (on crane) all up on the platform
Jim and Tony inside of BSC2
Gerardo, Jordan on the eMod as Support
TJ on the camera
Betsy soaking it all in (support)

A pre-lift meeting was held to go over the teams and maneuver details (again) at 9am prior to work starting.

Particle counts up at the dome level were all 0,0 before starting.
More photos and videos will be posted when those folks have them available.

Covers used - A BS/QUAD SUS tube cover up underneath, an ISI cover up on the ISI, the BSC Cartridge sock which encased the whole thing, dropped down to Jim and Tony once the lift was up a couple feet.  

The bulk of the work was from ~10:30am-1pm.  Most of the time before was getting folks in headsets and gear and getting equipment on.


Images attached to this report
Comments related to this report
jenne.driggers@LIGO.ORG - 20:36, Monday 27 April 2026 (90028)

Going over the details during the 9am pre-lift meeting. Congratulations, all, on a smooth operation!

Images attached to this comment
H1 General (OpsInfo, SEI, SUS, VE)
ryan.short@LIGO.ORG - posted 13:13, Monday 27 April 2026 (90020)
BS Cartridge Landed on West Bay Test Stand

As of 20:05 UTC, the cartridge from BSC2 (including the soon-to-be-decommissioned beamsplitter) has been placed on the test stand in the LVEA West bay. The cartridge was first lifted at 19:15 UTC before making its slow procession across the LVEA via the 5-ton overhead crane. More details and documentation to be posted later.

H1 TCS
sheila.dwyer@LIGO.ORG - posted 11:10, Monday 27 April 2026 - last comment - 11:10, Monday 27 April 2026(90004)
thermal actuator summary

I've been trying to understand how to make estimates of actuation strength for thermal actuators, and I wanted to make a summary to make this easier in the future.  With .  

In looking at data from the HWS, the values are divided by 2 to account for double passing (the compensation plates, ITM substrate, and SR3 are all double passed by the HWS beam).  These are then reported in micro diopters of spherical power, which is a measure of the change in wavefront curvature. 

If we are using these values to calculate the focal length of a lens, we would use:  f_new = 1/(1/f_original +spherical power)

If we are talking about a curved mirror, and we want to calculate the radius of curvature we use:  Rc_new = 2/(2/Rc_original + spherical power)   

  ITMX(uD/W) ITMY (uD/W)  
Ring heater (substrate lens) -10uD/W  -10uD/W 90003 (also close to value Matt's thesis from measurement and model, close to -9.9 uD/W value in finesse). Note that this is per Watt of total ring heater power, not per segment power
ETM Ring heater (surface) 

1.63+/- 0.11uD/W (Matt Todd's thesis)

1.53+/- 0.2 uD/W (88148)

Matt defines the "surface defocus" in his thesis, 

Di = 2/Ri , this should be equivalent to spherical power in the equation above.

central CO2 23.7uD/W 26.5uD/W 89999
annular CO2 -5.4uD/W -7.3uD/W 89999
SR3 heater 4.75uD/W spherical power, (2.375 µD/W of ROC change) 88413, agrees with Evan's simulation, T1600095 has 2.9uD/W
OM2 Tsams

1.75m ROC for "cold" (no heater power, thermistors should both be near room temperature)

2.1m ROC for "hot" (Thermistor 2 temperature 73C)

ROC data: 65280

Jennie Wright summary of hot and cold ROCs: 84255

 

Comments related to this report
evan.hall@LIGO.ORG - 16:11, Friday 24 April 2026 (90007)

The measured SR3 RoC change coefficient agrees with the value from 2D axisymmetric finite element simulation in which uniform circular irradiation is applied to the central 6″ diameter of the back of SR3. This code exists as a test function test_back_heat() in finesse-fenicsx. Compare the heater plate design in D1500385. Aidan's Comsol model is T1600096.

Non-image files attached to this comment
LHO VE
david.barker@LIGO.ORG - posted 10:25, Monday 27 April 2026 (90019)
Mon CP1 Fill

Mon Apr 27 10:07:42 2026 INFO: Fill completed in 7min 39secs

 

Images attached to this report
LHO General
ryan.short@LIGO.ORG - posted 07:38, Monday 27 April 2026 - last comment - 10:24, Monday 27 April 2026(90017)
Ops Day Shift Start

TITLE: 04/27 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: 9mph Gusts, 5mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.16 μm/s 
QUICK SUMMARY: The BSC2 (BS) cartridge is planned to be flown out of the chamber and onto the test stand in the LVEA West bay today!

Comments related to this report
david.barker@LIGO.ORG - 10:24, Monday 27 April 2026 (90018)

We have some cell phone alarm bypasses in place this week.

EY Chiller supply temp is above nominal, a contractor will work on this during the week.

Fire pumps are running intermittently to supply water for construction. These are only bypassed during construction hours.

Bypass will expire:
Sat May  2 07:05:16 AM PDT 2026
For channel(s):
    H0:FMC-EX_CY_H2O_SUP_DEGF
    H0:FMC-CS_FIRE_PUMP_1
    H0:FMC-CS_FIRE_PUMP_2
 

H1 SEI
mitchell.robinson@LIGO.ORG - posted 07:28, Monday 27 April 2026 (90016)
BSC2 Lifting pad install

Friaday Jim and I installed the lifting pads onto BSC2. Jim also secured disconnected cables, while I assisted Ibrahim with suspension gusset removal.

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:40, Sunday 26 April 2026 (90015)
Sun CP1 Fill

Sun Apr 26 10:08:57 2026 INFO: Fill completed in 8min 54secs

 

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:17, Saturday 25 April 2026 (90014)
Fri & Sat CP1 Fill

Sat Apr 25 10:09:51 2026 INFO: Fill completed in 9min 48secs

Fri Apr 24 10:11:05 2026 INFO: Fill completed in 11min 1secs

 

 

Images attached to this report
H1 General
anthony.sanchez@LIGO.ORG - posted 16:39, Friday 24 April 2026 (90010)
Friday Ops shift report.

TITLE: 04/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:

CDS Frame Write restarts @ 15:21 UTC

Lots BSC2 work was done today.
Beam splitter Stays were removed and in between BSC2 and HAM4. Pictures of the Beam Splitter cover and more details can be found here: alog link. 
The Beam splitter cartridge is closer than ever to fly out of the BSC2 Chamber. 

LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:56 FAC Kim & Nellie LVEA N Technical Cleaning & resupply Nellie out first 15:49
15:45 CDS Jonathan Remote N FW restarts. 15:50
16:11 FAC TJ, Randy LVEA N Moving IOT2 table. 16:35
16:24 IAS Jason & Ryan C LVEA West bay N Faro surveying. 19:24
16:33 EE Marc LVEA N Pulling sat amps 17:13
16:39 FAC Randy LVEA N Working on MEGA CleanRoom 21:32
16:53 SEI Jim CER N Checking AA chassis for inputs 17:08
19:24 SUS Ibriham & Betsy LVEA BSC2 N Putting a sheild around the BS. 20:45
19:31 SPI Jeff Optics lab N Dropping part off 19:31
20:21 SEI Jim LVEA BSC2 N Helping prep for flying a Beam splitter 22:42
20:33 SUS Mitch LVEA N Helping Jim/Betsy 21:32
20:43 IAS Jason & Ryan C LVEA West bay N Faro surveying 22:44
21:32 SUS Ibrahim LVEA BSC2 N Takeing BS stays 22:42
21:58 BHSS Keita & Disha & Elenna Optics lab yes? Working on Manta Ray 22:44
H1 SUS
ibrahim.abouelfettouh@LIGO.ORG - posted 16:11, Friday 24 April 2026 (90009)
BS stays removed + SEI cables removed and bundled

Ibrahim, Jim, Mitchell

Mitchell and I removed the BS stays from the beamsplitter and placed them in the tube between BSC2 and HAM4. Then, Mitchell and I put the cover over the BS.

Jim and Mitchell were working on removing and bundling SEI cables from inside BSC2 for storage by ISI. Jim (on ISI) and I (in BSC2) then removed cable clamps from the bottom of the ISI/ceiling of BSC2.

Picture provided.

Images attached to this report
H1 SPI (CDS, CSWG, OpsInfo, SEI, SPI)
jeffrey.kissel@LIGO.ORG - posted 16:06, Friday 24 April 2026 - last comment - 16:39, Friday 24 April 2026(90006)
SPI MEDM Screen Initial Release
J. Kissel

After the install of front-end software (LHO:89777 and LHO:89919) the next step for SPI is MEDM screens -- the UI/UX for the SPI L interferometers and PY one-way optical levers.

Here, I post screenshots and corresponding userapps svn file and location.
Sub-screens and their future purpose will come in the comments, but make sure to also check out G2402138.

In the main entry, I show off the new place that SPI lives on the LHO sitemap and the overview screen.
The overview screen, and all subordinate screens use a marco file, which I also attach.

All of these files are, of course, properly version controlled in the userapps SVN, here:
OVERVIEW SCREEN
    ${USERAPPS}/spi/common/medm/
        SPI_CUST_OVERVIEW.adl        rev 35102

MACRO FILE
    ${USERAPPS}/spi/h1/medm/
        h1spih23_overview_macro.txt  rev 35106
Images attached to this report
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 16:08, Friday 24 April 2026 (90008)
POWER MONITORING

These cover the on-board power monitor SPDs. Eventually, we'll use these filter banks to calibrate the PDs into [mW] as it lands on the ISIK breadboard.

${USERAPPS}/spi/common/medm/SPI_CUST_FBR_PWRIN.adl     rev 35102
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 16:23, Friday 24 April 2026 (90011)
LOCAL OSCILLATOR

The SPI's longitudinal IFO that measures the differential displacement in the main IFO's X direction release on heterodyne interferometry, with the interference between two beams modulated at 80 MHz and (80 MHz- 4096 Hz) = 79995904 Hz, which creates a beat note at 4096 [Hz]. 80 MHz comes from the site's RF distribution system of 80 MHz. The 4096 Hz is initially digitally generated via CDS, and a copy of that is sent out via DAC to be subtracted from 80 MHz with our homegrown single-sideband mixer, a.k.a "double mixer" (D2400315). This is the screen that controls the parameters of the cds oscillator, as well as some phase rotators and filterbanks to condition the digital LO into an analog signal for the DAC.

Nominally, the cds oscillator clock emits a 1 [count] amplitude wave, and the CLKGAIN, SINGAIN and COSGAIN parameters are set arbitrarily high, since its use as the LO for digital demodulation is usually entire internal to CDS. However, because this LO goes somewhere into real electronics, I've set the calibration of the signal condition filters such that the CLK, SIN, and COS gain are in units of [mV/ct] -- and I've set the LO amplitude at 5000 [mV] = 5 [V], mid-range of the DAC.

Since we don't yet know the right phasing, all the phase rotators are current set to 0 [deg].

${USERAPPS}spi/common/medm/SPI_CUST_LO.adl    rev 35103
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 16:30, Friday 24 April 2026 (90012)
INTERFEROMETERS

Here're the screens (less commissioned) that cover the digital demodulation and conversion to differential displacement.

${USERAPPS}spi/common/medm
    SPI_CUST_IFO.adl
        SPI_CUST_IFO_DEMOD.adl
        SPI_CUST_IFO_DISP.adl
    SPI_CUST_DIFFDISP_MTRX_RAMP.adl
    SPI_CUST_DIFFDISP.adl

all commited to rev 35102
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 16:39, Friday 24 April 2026 (90013)
ONE-WAY OPTICAL LEVERS

Here's the signal chain for the one-way optical levers. There's a good bit of confusing basis changing happening given
- the orientation of the QPD segments w.r.t. to vertical being different on HAM2's ISIJ QPDA and HAM3's ISIK QPDB,
- The usual conversion from QPD segments to pitch and yaw, as the beam flies, then
- Converting from beam pitch and yaw to ISI rotation, given that the HAM2 QPDA measuring HAM3 rotation is on the "front" +X side of HAM2, and the HAM3 QPDB measuring the HAM2 rotation is on the "back" -X side of HAM3.
So I had to make custom SPI screens (rather than use the standard ASC QPD screen) that hopefully clears all this up. Also, the QPD2CART matrix is a ramping matrix, and I've never liked the auto-generated MEDM screen for this, so I pioneered a new one that I think has a better user interface.

${USERAPPS}/spi/common/medm/
    SPI_CUST_QPD.adl
        SPI_CUST_QPD_MTRX.adl
    SPI_CUST_OL_QPD2CART_RAMP.adl
    SPI_CUST_OL_ISIOUTF.adl

all at rev 35103.
Images attached to this comment
Displaying reports 1-20 of 87453.Go to page 1 2 3 4 5 6 7 8 9 10 End