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Reports until 13:31, Friday 16 May 2025
H1 ISC
daniel.sigg@LIGO.ORG - posted 13:31, Friday 16 May 2025 (84435)
Excess Noise in ISC Whitening Chassis

This alog summarizes the measurements done with an ISC whitening chassis that implements ISC whitening boards D1001530-v7 using a 9V battery at the input.

Several issues were found:

  1. Due to a BOM error resistors R15 and R21 were stuffed with 3kΩ thick film resistors instead of metal film. Plot 1 shows the output referred noise measure at test point TP1. The blue curve was measured with a grounded input, whereas the red curve was measured with a 9V battery at the input. The later clearly shows the flicker noise of a carbon film resistor at roughly 600nV/√ f.
  2. The power supply input of the whitening board eomploys 10µH series inductors. Together with the bypass capacitors this forms a resonant circuit near 10kHz which shows up as a noise peak in the plots. Plot 2 shows the output noise with no whitening engaged for the original board (blue curve), the board with fixed 3kΩ resistors (green), and with the power supply indcutors shorted out (red).
  3. The gain stages will generate excess noise when over driven. The whitening board employs 4 switchable gain stages with 24, 12, 6, and 3dB of gain, respectively. With 9V input both the 24 and 12dB stage are over driven with their ouput voltage limited by the power supply rails. This will in turn lead to a large differential input voltage at the inputs of the OpAmp which then triggers the protection diodes. The current is limited by the 300Ω resistors (R11) in series with the + input. Even so, it is safe to operate like this, it can generate execss noise as seen in Plot 3. The blue curve shows the output noise with the input grounded, whereas the red curve uses a 9V battery at the input. The green curve shows the noise of the SR785 and the battery alone.

Plot 4 shows the 9V input noise using the optional whitening stages. A whitening stage consist of a 1Hz zero and a 10Hz pole.
Plot 5 shows the same plot but with the 300Ω resistors removed, the 3kΩ resistors replaced with metal films, and the inductors at the power supply shorted out.
Plot 6 is an overlay of Plots 4 and 5.

Non-image files attached to this report
H1 ISC
jennifer.wright@LIGO.ORG - posted 10:33, Friday 16 May 2025 - last comment - 11:40, Tuesday 03 June 2025(84432)
OMC scans with SR3 heater on

Jennie W, Sheila, Elenna

 

In order to get data for mode-matching and for Elenna to get data to calibrate sideband heights we ran some mode scans after the SR3 heater was turned on last night.

16:55:24 UTC Carried out single bounce OMC scan at 10W PSL input with sensor correction on HAM6 on, high voltage on for PZT driver in HAM6, sidebands off , SRM mis-aligned, ITMY mis-aligned, DC 3 and 4 on, OMC ASC on.

Excitation freq changed to 0.005 Hz as the top peak of the TM00 mode looked squint so could have been saturating. Lowering this frequency prevented this.

Ref 15-17 corresponds to dcpd data, pzt exc signal, pzt2 dc monitor.

 

Then mis-aligned ITMX and aligned ITMY (Sheila had to re-align SR2 to centre on ASC-AS_C).

Measurement starts at 17:08:18 UTC.

Ref 18-20 corresponds to dcpd data, pzt exc signal, pzt2 dc monitor.

 

Traces saved in 20250516_OMC_scan.xml. The top left plot is the first scan bouncing beam off ITMX, the second scan is the bottom right bouncing off ITMY.

The top right is the two plots of the PZT2 DC voltage monitor. That is, the current voltage applied to the PZT. The bottom left is the plot of the voltage ramp applied to the PZT2 on the OMC for this measurement.

 

The ndscope attached shows the power in mA transmitted through the OMC on the top, then the PZT used for the scan DC voltage underneath, then the input PZT voltage underneath that, then the reflected power from the OMC in mW, then at the bottom the SR3 heater element temperature in degrees.

 

Elenna did two more scans in single bounce with sidebands back on and different modulations depths in each.

Images attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 10:38, Friday 16 May 2025 (84433)

See Elenna's comment on her previous measurement where this saturation happened.

Turn off the sidebands - instructions in this alog.

elenna.capote@LIGO.ORG - 16:51, Friday 16 May 2025 (84441)

Sheila and I ran one more OMC scan with sidebands off after OM2 heated up. Attached is the screenshot with scans off both ITMX and ITMY, data is saved in [userapp]/omc/h1/templates/OMC_scan_single_bounce_sidebands_off.xml

 

Images attached to this comment
elenna.capote@LIGO.ORG - 17:02, Friday 16 May 2025 (84442)

I also ran two OMC scans, single bounce off ITMY, 10 W input, with the sidebands ON. One measurement I ran with the sidebands set to 23 dBm and 27 dBm (9 and 45 MHz) and another set to 20 dBm and 21 dBm (9 and 45 MHz). I will use these measurements to calibrate the modulation depth. Data saved in /opt/rtcds/userapps/release/omc/h1/templates/OMC_scan_single_bounce_RF_cal.xml

SR3 heater was on for this measurement but it should have little effect on my results.

camilla.compton@LIGO.ORG - 11:40, Tuesday 03 June 2025 (84749)

Looked closer at these HWS signals during SR3 heater heat up and cool down. In all these plots, the two t-cursors are used as the reference and shown HWS live image.

  • Heat up plot attached
  • Cool down plot attached (ITMX was misaligned so there's no HWS data)

Some strange things:

  • ITMX heat up ndscope spherical power looks the opposite direction of ITMY, this isn't physical. Looking at the HWS Live plot, this isn't really want's happening, it appears that the SR3 signal just appears if the edge of ITMX is heating up so the center that the calculations are made from isn't correct, making the calculated spherical power wrong.
  • In both the heat up and cool down of the ITMY signal, there appears to be two steps with a flat region in the middle. Looking at the the flat region only, attached, it appears that the spherical power is continuing to change in the expected direction, unsure why this change isn't shown in the calculated spherical power.
Images attached to this comment
LHO VE
david.barker@LIGO.ORG - posted 10:11, Friday 16 May 2025 (84431)
Fri CP1 Fill

Fri May 16 10:06:36 2025 INFO: Fill completed in 6min 33secs

Jordan confirmed a good fill curbside.

Images attached to this report
H1 SEI
oli.patane@LIGO.ORG - posted 09:47, Friday 16 May 2025 (84428)
HEPI Pump Trends Monthly FAMIS

Closes FAMIS#37205, last checked 83981
 
HEPI pump trends looking as expected (ndscope).

Images attached to this report
LHO VE
jordan.vanosky@LIGO.ORG - posted 09:00, Friday 16 May 2025 (84425)
Morning Purge Air Checks 5-16-25

Dry air skid checks, water pump, kobelco, drying towers all nominal.

Dew point measurement at HAM1 -42.1 °C.

Images attached to this report
H1 General
oli.patane@LIGO.ORG - posted 07:39, Friday 16 May 2025 - last comment - 09:30, Friday 16 May 2025(84424)
Ops Day Shift Start

TITLE: 05/16 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: 6mph Gusts, 3mph 3min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.09 μm/s
QUICK SUMMARY:

Most of the work for today involves final checks for HAM1

 

Comments related to this report
oli.patane@LIGO.ORG - 09:30, Friday 16 May 2025 (84427)SUS

Last night RM2 was left in DAMPED with the damping loops on, whereas RM1 asnd PM1 were also in DAMPED but their damping loops had been turned off. The loops on RM2 excited the suspension until it was causing overflows. This continued all night. It seems strange that the loops that were damping well two days ago are now not damping (ndscope1). I noticed that turning off only the L damping solved the issue of the MASTER_OUTs slowly increasing.

Doing some tests (starting in SAFE and then going to DAMPED), it looks like damping is fine for the first few minutes, after which it very quickly starts exciting instead of damping (ndscope2, ndscope3), and the voltmons start going crazy. I did this test a few times with the same result every time.

Doing the same test but immediately switching L damping off as soon as it turns on, we stay just damping P and Y and have no issues with oscillations or saturations (ndscope4).

I am not sure if this means that the issue is specifically with the Length damping? I am putting RM2 in SAFE for now and I'm going to try the same tests on RM1 and PM1 to see if the same issue exists there.

Images attached to this comment
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 02:45, Friday 16 May 2025 (84423)
HAM1 Vacuum Work, Installation Of A New Gauge and Turbo Pump

(Jordan V., Travis S., Gerardo M.)
Today we installed a new gauge on the 16.5" conflat on top of HAM1, installed on the top central port, D1.  A single gauge replaces a gauge pair combo, pirani and cold cathode, this gauge will be used for the high voltage interlock system for HAM1.  The gauge still needs the installation a couple of cables for it to work.

The turbo pump was the second item that was replaced on HAM1, an outdated and noisy turbo pump was removed and replaced with a new turbo pump.  No issues were encountered during the removal or installation of the new pump.

All of the affected conflats will need to be checked for leaks.

Images attached to this report
H1 CAL
michael.ross@LIGO.ORG - posted 17:18, Thursday 15 May 2025 - last comment - 17:18, Thursday 15 May 2025(84413)
Spun NCal

Shoshana, Michael, Jeff, Tony

We spun the NCal as a life check while we were on site. At first the NCal wouldn't turn on and threw a 'NCal power' error. Power-cycling the motor power by replugging the AC cable running to the Beckhoff motor controller (black cable coming from the left in attached picture) fixed the error. We spun the rotor up to 10 Hz for a few minutes before spinning it down.

NCal Settings:

Motor Frequency Request: 1040 ct

Motor Ramp Gain: 0.01

Motor Low Pass Time Constant: 5

Images attached to this report
Comments related to this report
anthony.sanchez@LIGO.ORG - 14:37, Thursday 15 May 2025 (84414)

If the Bechhoff error presents it's self hit the system reset button.

Images attached to this comment
H1 General
anthony.sanchez@LIGO.ORG - posted 16:39, Thursday 15 May 2025 (84421)
Thursday Ops shift closing report.

TITLE: 05/15 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:

Vac Folks are still in the LVEA working on the Top VAC Flange Guage.

The TCS SLEDs were swapped.

The Ground checks were done on HAM1

The Ring Heater for SR3 is being left on all night.

BRS team has been pumping down the BRS, seems like perhaps they are mostly done and may go back to EY clean up some wiring.

HAM1 Suspentions seem to be saturating a lot today , but there was a lot of activities on ther ISI and ontop of the HAM1 chamber.

There was some Wind fence work done today at EX, where another Bee hive was spotted on a tumble weed. So please Bee aware, of the TumbleBees.


LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:57 Sys Corey LVEA HAM1 N Taking Pictures of inside HAM1 16:44
15:05 FAC Chris EX N Getting parts 15:05
15:34 VAC Jordan LVEA N Purge Air checks. 15:48
16:17 FAC Kim & Nellie LVEA N Technical cleaning 16:17
16:31 EE Fil LVEA HAM1 N Ground loop checks 19:03
16:35 PEM Carlos, Keit, Robert X-arm Vault N Magnatometer calibration 19:18
16:36 SEI Micheal R. & Shoshana EY N Closing up BRS 18:41
16:51 FAC Kim & Nellie EX N Technical cleaning. 17:45
17:10 SUS Rahul LVEA N Ground loop checks with Fil 19:03
17:31 VAC Jordan & Gerardo LVEA N Vacuum system tests 18:15
17:31 EE Daniel LVEA N Helping Fil do ground loop checks. 19:03
17:58 VAC Janos LVEA n Vacuum Test 18:14
17:59 TCS TJ & Camilla LVEA HAM4 N Replacing Hartman SLED 18:53
18:16 VAC Jordan & Gerardo MY & EY n Vacuum tests. 19:53
19:32 SEI Jim LVEA HAM1 N Setting up measurements. 21:32
19:36 NCAL Micheal R & Shoshana EX N Pluging in NCAL to spin off the cobb webs 20:34
19:45 SEI Randy, Corey, Mitchel EX N Wind fence work 22:34
19:54 VAC Travis & Gerardo MX & EX N vacuum tests 20:34
20:35 VAC Jordan, Travis, Gerardo LVEA HAM1 N Testing Vac equipment & helping Jim 23:40

 

Images attached to this report
H1 TCS
thomas.shaffer@LIGO.ORG - posted 16:16, Thursday 15 May 2025 (84417)
HWS ITM SLEDs swapped

Camilla C, TJ S

The two corner station HWS SLEDs were last swapped back in October 2023 (alog73371), going a bit long than our usual ~1 year before swapping. Today we swapped them with fresh SLEDs following the T1500193 procedure, calibrated their power channels, and started the code back up with fresh references.

HWS starting values

Power as measured from fiber launcher: IX 480uW   IY 180uW

Power reported into epics: IX: 1.88   IY: 0.36

SLEDs removed:

X - https://ics.ligo-la.caltech.edu/JIRA/browse/QSDM-790-5--00-11.21.380

Y - https://ics.ligo-la.caltech.edu/JIRA/browse/QSDM-840-5--00-03.20.479

 

HWS ending values

SLEDs installed:

X - https://ics.ligo-la.caltech.edu/JIRA/browse/QSDM-790-5--00-11.21.382 2.5mW = 165mA = 660mV (on TP with 250mA/V) Max current set to 155mA

Y - https://ics.ligo-la.caltech.edu/JIRA/browse/QSDM-840-5-0-00-06.18.005 2.5mV = 100mA = 400mV (on TP with 250mA/V) Max current set to 95mA

Power measured at fiber launcher: 2.2mW for both

To calibrate the H1:TCS-ITM{X,Y}_HWS_SLEDPOWERMON channel, we turned off the SLEDs, found the dark offset, turned the SLED back on, and then changed the gain. These values are in the SDF screenshots attached.

Images attached to this report
H1 AWC
sheila.dwyer@LIGO.ORG - posted 15:58, Thursday 15 May 2025 - last comment - 16:44, Tuesday 03 June 2025(84419)
SR3 heater on overnight

TJ, Camilla, Sheila

TJ and Camilla got the HWSs working, and now we turned on the SR3 heater at 15:54 UTC, 2W requested power.  This is to do a check of the SR3 heater calibration and range similar to 27262

Comments related to this report
camilla.compton@LIGO.ORG - 10:53, Tuesday 20 May 2025 (84481)

SR3 heating up can be seen on the HWS signals but is not particulatly clear, see attached.

Images attached to this comment
jennifer.wright@LIGO.ORG - 10:12, Tuesday 03 June 2025 (84744)

Looking at when this test was done at LLO, the lens changing happened over a period of three hours and the lens power increased in the same direction on both HWS, so its possible our HWS are not a good witness for the SR3 curvature change.

jennifer.wright@LIGO.ORG - 10:25, Tuesday 03 June 2025 (84746)

Aidan calculated 2.45 uD/W at LLO, and we get 9.44 uD/W (from the H1:TCS-ITM{Y,X}_HWS_PROBE_SPHERICAL_POWER  trends with an estimated noise of 4.48e-12uD/W.

camilla.compton@LIGO.ORG - 11:43, Tuesday 03 June 2025 (84751)

Looked closer at these HWS signals during SR3 heater heat up and cool down. In all these plots, the two t-cursors are used as the reference and shown HWS live image.

  • Heat up plot attached
  • Cool down plot attached (ITMX was misaligned so there's no HWS data)

Some strange things:

  • ITMX heat up ndscope spherical power looks the opposite direction of ITMY, this isn't physical. Looking at the HWS Live plot, this isn't really want's happening, it appears that the SR3 signal just appears if the edge of ITMX is heating up so the center that the calculations are made from isn't correct, making the calculated spherical power wrong.
  • In both the heat up and cool down of the ITMY signal, there appears to be two steps with a flat region in the middle. Looking at the the flat region only, attached, it appears that the spherical power is continuing to change in the expected direction, unsure why this change isn't shown in the calculated spherical power.
Images attached to this comment
jennifer.wright@LIGO.ORG - 11:54, Tuesday 03 June 2025 (84753)

With the numbers from ITMY HWS only, and looking at the 3hr 11 m cooldown in Camilla's photo, the lens change is 6.68e-6 Dioptres/W taking into account that the HWS beam passes twice through SR3.

jennifer.wright@LIGO.ORG - 16:44, Tuesday 03 June 2025 (84768)

After talking with Camilla, she reminded me the change in RoC (delta R) =/= 2/(delta D),

where D is defocus (1/focal length).

but instead delta R = 2/(2/R + delta D) - R

Where R=36.013m is given in https://git.ligo.org/IFOsim/ligo-commissioning-modeling/-/blob/main/LHO/yaml/lho_O4.yaml?ref_type=heads

delta R comes out as 4.3mm +/-  0.18 mm (which is the same order of magnitude as the change Aidan measured in alog #27262 at LLO). 

The error was estimated from looking at the noise on the spherical power and propagating through the calculation of delta R.

H1 CDS (CDS, SUS)
rahul.kumar@LIGO.ORG - posted 14:09, Thursday 15 May 2025 - last comment - 16:54, Thursday 15 May 2025(84412)
HAM1 ground loop checks done

Fil, Rahul

This morning we finished ground loop checks on HAM1 chamber, since Jim was done with final cabling work. The only grounding issues we found were in RM1 and PM1, hence we removed pin1 from the in-air cable (connecting Satamps).

Comments related to this report
filiberto.clara@LIGO.ORG - 16:54, Thursday 15 May 2025 (84422)

D0902810 aLIGO SUS HAM 1-2 System Wiring
T1200131 Grounding and Shielding at LIGO
D1900511 ISC/SQZ Wiring Diagram

The following were checked for ground loops:

  1. REFL_A LSC DC, cable ISC_221
  2. REFL_B LSC DC, cable ISC_226
  3. POP_A LSC DC, cable ISC_222
  4. REFL_A WFS DC, cable ISC_223
  5. REFL_B WFS DC, cable ISC_224
  6. POP_X WFS DC, cable ISC_225
  7. Picomotors, cable ISC_227
  8. REFL Beam Diverter, cable ISC_314
  9. POP Beam Diverter, cable ISC_315
  10. RM1 Tip Tilt, cable ISC_HAM1_228
  11. RM2 Tip Tilt, cable ISC_HAM1_229
  12. PM1 Tip Tilt, cable ISC_HAM1_311

To get a good chamber ground connection, testing was done at the feedthroughs. Normally done at the ISC racks. Shorts found on RM1, PM1, and both beam diverters.

  1. Beam diverters issue known, see alog 63589. No effort made to repair.
  2. Rahul had tried adding Kapton on the RM1 OSEM. This method repaired the short last vent, alog 63589. Short still present. Pin 13 removed from connector at the SUS field rack
  3. No attempt to remove short inside chamber for PM1. Rahul mentioned in-vacuum cables are dressed/tied down. Pin 13 removed from connector at the SUS field rack.

With suspensions in safe mode, the termination shielding was repaired on the following PM1 cables:

  1. ISC_HAM1_315
  2. ISC_HAM1_319

F. Clara, R. Kumar

H1 SEI
jim.warner@LIGO.ORG - posted 17:03, Wednesday 14 May 2025 - last comment - 16:11, Thursday 15 May 2025(84403)
HAM1 ISI testing so far

Now that ISC is done with their alignment, I have been working on testing the ISI. Last night TJ and I unlocked and balanced the ISI, I did some quick tests to make sure the actuators were pushing where I expected them and found the horizontal and vertical actuator for each corner was swapped, so I switched the cables at the chamber. This morning I did some tests like range of motion and CPS linearity and some quick spectra to check that all of the sensors looked more or less the same and a quick set of tfs to look for rubbing. Now starting my long overnight tfs, so hopefully there are no big eqs overnight. If those go well, I hope to have everything for the testing report by the afternoon tomorrow.

Attached images are some of the tests I did today. First image is CPS linearity, which looks kind of ratty because I think the purge was too high, but otherwise looks okay. Second image shows unlocked asds for the CPS, GS13s and L4Cs. No glaring issues, but the kind of noisy V2 GS13 and CPS made me think some rubbing or high purge was happening. Last image is a set of tfs I used for chamber closeout comparing the measurements on HAM8 from last year to HAM1 today. Looks okay for a quick measurement.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 09:24, Thursday 15 May 2025 (84407)

L2L tfs look good. Still have some other information to collect.

Images attached to this comment
jim.warner@LIGO.ORG - 16:11, Thursday 15 May 2025 (84420)

My testing is done. Testing report is uploaded to E2500128. Payload was light by a lot during testing, it did not get better in chamber and there were a lot of beam dumps that got added that I don't have weights for, so the payload section of the report should be taken with a grain of salt.

H1 SEI (SEI)
shoshana.apple@LIGO.ORG - posted 15:54, Monday 12 May 2025 - last comment - 15:04, Friday 16 May 2025(84366)
BRS ETMY Mass Adjuster Install
[Shoshana, Michael]

We've started preparing to install the BRS mass adjuster to the End-Y BRS. The plan is to follow the same procedure/same parts as the End-X install outlined in LIGO-T2400043 and SEI log 1886 (https://alog.ligo-la.caltech.edu/SEI/index.php?callRep=1886).
 We've taken apart the BRS and discovered that doesn't match the designs on the DCC. How the parts are arranged blocks access to where the pico-motor mount should attach, but we think we have a work around that should work.
The electronics/wiring of the BRS is as expected and we've finished all the wiring for the pico-motor so that it should attach to the feed through.
Assuming all goes well we plan on installing the mass adjuster parts and begin testin.
Images attached to this report
Comments related to this report
shoshana.apple@LIGO.ORG - 16:51, Tuesday 13 May 2025 (84379)SEI
[Shoshana, Michael]

We've managed to get all of the hardware/parts installed in and we've closed up the BRS chamber. We had to add an inch of shims beneath to motor mount in order to get it to fit/align properly, but otherwise there were only minor complications during installation. We've tested the pico-motor and the mass adjuster using the pico-motor driver that we brought from UW and both seem to work fine. 
For in air balancing, we left the new mass adjuster centered to increase range for future adjustments for when the BRS is pumped down and running, and tried to just stick to moving masses that are inaccessible when the BRS chamber is pumped down. We unfortunately reached the maximum range with the internal masses and had to slightly move the manual mass adjustment system (what is currently used to adjust the center of mass) from center, but that might be returned to center after we re-balance it when it's pumped down. Right now the resonance frequency looks to be around ~7mHz (around 130 second period) which is about the same as it was before Mass Adjuster installation, but we'll check again after the chamber has been pumped down.
Tomorrow we'll finish all of the wiring and electronics to hook up the pico-motor to the LIGO system. The plan is to pump down the BRS chamber tomorrow and re-balance and test the pico-motor some more.

The reference pattern has a higher intensity than expected and we aren't sure why. Right now our best guess is that the light source drifted slightly, and we'll look into it more tomorrow.


Images attached to this comment
jennifer.wright@LIGO.ORG - 13:36, Wednesday 14 May 2025 (84391)EPO

EPO tag for BRS pics

shoshana.apple@LIGO.ORG - 16:05, Thursday 15 May 2025 (84411)SEI
[Shoshana, Michael]

Pumped down the BRS chamber overnight and started the ion pump this morning and got it down to 1.9e-6 Torr before we left end End-X. We also wired up the picomotor to the LIGO picomotor controller system. It is hooked up to the 7th channel X-direction and we tested it out and were able to hear it spinning for both directions. The BRS's thermal insulation was reapplied the box closed and the temperature sensors and heating plate were all re-attached and plugged back in. The reference beam's intensity has gone down to be closer to normal somehow, so it doesn't seem to be anything to worry about
We might go back to End-Y one more time tomorrow to clean up the wiring and do a final check of the vacuum pressure.
We waited for the temperature to equilibrate a bit before balancing  because we were hoping that as the temperature rises it would drift back to center, but we ended up using the mass adjuster to try and balance it.
It looks like the + - wires for the damping were switched, meaning when the damping was on it would ring up the BRS. Fixed by changing a line in the BRS code[IF H1_ISI_GND_BRS_ETMY_CAPDRIVE>=0] by switching the [>=0] to [<=0] and switching [H1_ISI_GND_BRS_ETMY_CAPOUTL] and [H1_ISI_GND_BRS_ETMY_CAPOUTR], and [H1_ISI_GND_BRS_ETMY_RELAYL] and [H1_ISI_GND_BRS_ETMY_RELAYR]


FROM THE END-X INSTALL:
Coupling/decoupling move: 1.25k steps
Maximum: +-140k steps
Be careful: +-100k steps

NOTE: MOVING PICOMOTOR +(POSITIVE) DIRECTION TRANSLATES TO MOVING THE BRS UP

TOTAL MOVEMENT TODAY:+21k steps
shoshana.apple@LIGO.ORG - 11:49, Friday 16 May 2025 (84434)
Centered both ETMY and ETMX BRSs.
For ETMX net movement was +2200 steps, for ETMY net movement was -3200 steps.
For ETMX we saw that the DRIFTMON was moved by about ~3.27 counts per step, and ~2.3 counts per step for ETMY
shoshana.apple@LIGO.ORG - 13:55, Friday 16 May 2025 (84437)
Cleaned everything up for the ETMY BRS and relabeled all the wires. The final reading that we saw for the ion pump was 9.9e-7 Torr (186uA, 6950V) which seems about right. We left some extra mass adjuster parts with Jim just in case. 
michael.ross@LIGO.ORG - 15:04, Friday 16 May 2025 (84438)

Shoshana, Michael

We took tilt subtraction spectra as a final life check of the BRSs. Both BRSs appear to be in good working order and doing their jobs well.

Non-image files attached to this comment
H1 ISC (SUS)
camilla.compton@LIGO.ORG - posted 07:42, Thursday 08 May 2025 - last comment - 08:54, Friday 16 May 2025(84314)
ISC Alignment Work, Day 6 in HAM1 (May 7th): 20W now into IMC, POP beam profiles done.

Oli, Keita, Elenna, Jennie, Sheila, Ryan S, Rahul, Betsy, Camilla

Day 1: 84193, Day 2: 84228, Day 3: 84230 and 84239, Day 4: 84274, Day 5: 84292

In the morning Keita and Jennie aligned the POP flashes on the periscope mirrors and M10 dichroic. The height of this beam is 3.75" on these mirrors to account for the ALS green beam being 13mm above the POP beam. Keita was a little concerned about the height of the top periscope mirror so we'll need to check the green ALS beam carefully on this and if it 's near clipping we may need some in-vac pico-ing.

Rahul then moved PM1 to it's final position. Elenna and Rahul checked that the signed of the PIT and YAW sliders were correct. 

Shiela, Rahul and I then worked on centering the beam on PM1 and L2 without the 90/10 M12 in place, so that we could later have enough power to beam profile the POP single bounce beam. To get the beam height back up to 4" at PM1, Rahul needed to pitch PM1 mechanically. 

Oli then increased PSL input power to 20W, we aligned to POP single bounce and Sheila and I took beam profile measurements before PM1 and after L2, details in 84307.

Elenna, Rahul and I then replaced the 90/10 M12 and recentered the beam on PM1 and L2. We started aligning the POP air path but aren't happy with it, dumped the beam and will continue to work on. 

Betsy let in the PSL ALS beam into HAM1 by opening the light pipe and I dumped it straight away. See 84312.

Today we plan to: align the POP, REFL and PSL ALS beams out of the chamber, open the X-arm check the green ALS beam alignment on the shared optics and off the table, including rolling up ISCT1 and adding the VP simulator. The POP LSC/ASC diodes and all beam dumps still need to be aligned and checked. 

Comments related to this report
camilla.compton@LIGO.ORG - 14:48, Friday 09 May 2025 (84340)

Keita and Jennie's log on the work done in the morning is 84308.

elenna.capote@LIGO.ORG - 08:54, Friday 16 May 2025 (84426)

Just adding a clarification. "Elenna and Rahul checked that the signed of the PIT and YAW sliders were correct. "

We confirmed that adding a positive pitch offset in the alignment slider of PM1 results in PM1 pitching downward, as expect in a right handed coordinate system, and verified by watching the beam reflecting off PM1 shifting down. We also confirmed that a positive yaw offset results in the optic rotating left (as seen from behind the optic), again as expected from the right handed coordinate system, and verified by watching the beam reflected off PM1 shifting left.

I went back and forth a few times with the offsets while Rahul held an indicator card in front of the optic to watch the beam move to see the response of PM1.

H1 ISC
elenna.capote@LIGO.ORG - posted 14:04, Tuesday 18 March 2025 - last comment - 10:05, Friday 16 May 2025(83437)
Single Bounce OMC scans taken - process notes

I took two single bounce OMC scans today with the help of TJ and Tony. Here are some notes to future me and others to reference if we want to do single bounce scans:

Edit to add: unfortunately the scan results from today look pretty bad. In short, the peaks look "lopsided" somehow, and so I'm not sure the results are usable. Looking back at Jennie W's previous scans, it looks like she had to slow them down to 200 second scans. I only did a 100 second scan with amplitude 105 so maybe I scanned too fast. I'm not sure what the correct resolution of this is, because the scans I did in 2022 were 100 second scans and the results were fine. Adding this note here for reference in the future to think about the appropriate scan length and amplitude.

Comments related to this report
elenna.capote@LIGO.ORG - 10:00, Friday 16 May 2025 (84429)

Jennie, Sheila, and I ran OMC scans this morning and realized that the proper way to slow down the scan to avoid weird saturation effects is to reduce the excitation frequency in the template. The nominal templates have excitation frequencies of 0.01 Hz, so sweeping over 200 seconds just sweeps at the same speed twice. To sweep once, slower, you have to increase the sweep time to 200 seconds AND reduce the sweep frequency to 0.005 Hz.

elenna.capote@LIGO.ORG - 10:05, Friday 16 May 2025 (84430)

Sheila and I want to note some things that are "obvious" but easily forgotten:

  • high voltage must be on
  • sensor correction must be on
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