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Reports until 22:00, Tuesday 18 March 2025
H1 General
ryan.crouch@LIGO.ORG - posted 22:00, Tuesday 18 March 2025 (83443)
OPS Tuesday EVE shift summary

TITLE: 03/19 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 143Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY:The low range coherence check yielded, CHARD_Y and PRCL at low frequency. The range has been in the mid 140s, we've been locked for 5.5 hours.

02:06 low frequency glitch, EX and DCPD saturation

LOG:                                                                                                                          

Start Time System Name Location Lazer_Haz Task Time End
14:34 Electrical Ken LVEA No Finding lift for work Above HAM1 18:59
14:56 Vent Prep TJ near HAM1 N Taking down laser Curtains. 15:28
15:09 VAC Rogers Mech room N Working on kobelco units 20:39
15:11 PCAL Rick,  Francisco EX, EY Yes Beam Spot movment on EX. 16:44
15:23 VAC Gerardo West bay LVEA No Vac work, ION pumps into FCT 18:03
15:25 FAC Kim & Nelly EY, HAM SHAQ, EX N Technical cleaning. 18:05
15:27 VAC? Travis EX, EY Yes Taking Measurements 20:54
15:27 EE Fil LVEA, CER N Pulling cables. 19:48
15:29 IAS Jason Input - West LVEA N Doing some FARO work. 21:05
15:47 EE Marc LVEA N helping Fil 19:48
15:48 Site Safety McCarthy LVEA N Checking roll up door. 16:01
15:49 VAC Norco Y arm N Filling N2 tanks. 18:44
16:07 PEM Robert LVEA N Accel, cable clean up 16:13
16:20 FAC Chris Out Side West bay N Moving Big Green Harvester 19:41
16:48 Faro Jim HAM1, HAM SHAQ N Helping Jason 18:36
17:07 PCAL Francisco PCAL Lab Yes Putting away tools 18:59
17:14 FAC Christina Receiving N Picking up batteries , driving truck 17:59
17:28 SUS Rahul Remote/ EY & EX N SUS measurements on EY 19:14
17:49 TCS Camilla & TJ EX Yes opening laser table and adjusting TCS system 17:49
18:03 IAS Ryan C LVEA input- west N FARO-ing with Jason 21:05
18:06 FAC Kim, Nelly LVEA n Tech clean 19:30
18:23 SEI Jim LVEA, HAM ShAQ N Looking for Install hardware 19:01
18:49 Exercise Mayank & Shiva Overpass N Enjoying the noon view 19:19
19:25 TCS Camilla ITMY n Checking CO2 laser 19:32
19:42 LASER Transition Oli LVEA YES LASER Transition & LVEA Sweep. 19:56
19:53 CPy Sheila, Robert , Betsy ITMY Yes Centering CPy using Oplevs 21:21
19:57 LASER HAZ LASER HAZARD LVEA  (\u2310\u25a0_\u25a0) YES LVEA IS LASER HAZARD  (\u2310\u25a0_\u25a0) 06:36
21:07 ISC Rahul & Camilla, Shiva , Mayank Optics Lab Local Working on ISS, Rahul  Out early 23:37
21:55 ISS Camilla HAM6 Yes Getting parts 21:58
22:32 walk Ryan C Y-arm N Jogging the Y-arm 23:02
23:40 ISC Camilla OSB Receiving N Drove to OSB rec 23:50
01:35 FIT Matt, Francisco, Mayank Yarm N Going for a run 02:09
Images attached to this report
H1 CAL
francisco.llamas@LIGO.ORG - posted 19:19, Tuesday 18 March 2025 (83428)
Pcal XY comparison investigation - Second move at an angle

FranciscoL, RickS

On Tuesday, March 18, we moved the PCALX lower beam by r = 2.5mm, \theta = +237 deg from its nominal center. We expect to see a change of 20 HOPs in \chi_XY -- returning to the value it was a week ago.


Placed target in the same alignemnt as in the previous actuation (TARGET_ON). Both individual beam voltage values, as found, were very similar to the values recorded at the end of the move done last week. We actuated by turning counterclockwise on the pitch adjuster of the outer beam folding mirror, with minor adjustments in yaw. The voltage of the lower beam after the move was higher than last week, it could be from AoI of the optics, but documenting here for future reference.

The following table shows the voltage values as read by the Keithley voltmeter we use during the procedure

Step Comment Readout [V]
1 Both beams - target off 3.377
2 Both beams - target on (as found) (BEFORE_MOVE) 2.896
3 Lower beam after actuation 1.43
4 Both beams - target on (AFTER_MVOE) 2.940
5 Both beams - target off 3.383

We have one more actuationg left in which we move the beam back to nominal center. For the upcoming move, we expect \chi_XY to stay the same.

Images attached to this report
H1 CAL
francisco.llamas@LIGO.ORG - posted 18:25, Tuesday 18 March 2025 (83314)
Pcal XY comparison investigation - Moving beam at an angle

FranciscoL, RickS, SivanandaR

In summary:

On Tuesday, March 11, we moved PCALX lower (outer) beam by r = + 2.5 mm, \theta = - 33 deg (from horizontal) on the ETM. We expect to see a large (~20 HOPs) change in \chi_XY.


From our investigations -- an independent method to estimate IFO beam offset using the Pcal -- we believe that the IFO beam offset, when facing the ETM, is (+ 14.3 mm, -- 09.3 mm) in cartesian coordinates. These coordinates yield an angle of arctan(-- 9.3/14.3) ~ -- 33 deg from the horizontal axis of the ETM center.

The first pdf file (polar_out.pdf) plots the IFO beam offset. The black points represent the measurements of a2l (located at '/opt/rtcds/userapps/trunk/isc/common/scripts/decoup/BeamPosition/a2l_lookup.m'). The green points are what is inferred by Pcal measurements. For the Pcal to estimate the IFO beam offset, we use the scalar product of \vec(c) -- the displacement vector of the Pcal center of force for a given actuation, and \vec(b) -- the IFO center of force, as it is derived in T2400032 equation 11. From the plot, there is a clear disagreement on the horizontal component of the IFO beam from both methods. Following equation 11, a measurement in which an actuation from the Pcal beams results in a parallel displecement of the pcal center of force to the real IFO beam center of force should maximize the change \chi_XY. Conversely, an actuation that is perpendicular would not be seen by \chy_XY (no change). The actuation for today was parallel to what the Pcal estimates is the IFO beam position. We plan to make a second actuation, in which we move perpendicular to our estimate of the IFO beam. Ideally, these measurements would increase our confidence of the IFO offset.

We aligned the target by setting an angle gauge at the calculated 33 deg as seen in the first image (TARGET_ON).

We aligned the Pcal beams to the corresponding apertures by (1) blocking one beam and (2) aligned beam of interest by maximizing the Rx sensor voltage readout from a Keithley digital multimeter (KVM). Since the upper beam has shown inconsistencies in the horizontal displacement (83051), we are actuating on the lower beam. The second image (BOTH_BEAMS) shows both beams after moving the lower beam.

The following table lists the voltage value at each relevant step of the process:

Step Comment Rx Readout [V]
1 Both beams, as found 2.840
2 Upper beam, as found 1.440
3 Upper beam, centered 1.50
4 Lower beam, as found 1.396
5 Lower beam, centered 1.40
6 Lower beam, moved 1.390

Some observations from today's visit to ENDX:

This is the first of three actuations. Additionally, the data processing still needs about a week of data to diagnose results. We will have nominal results in ~3 weeks.

Images attached to this report
Non-image files attached to this report
X1 DTS
joshua.freed@LIGO.ORG - posted 17:04, Tuesday 18 March 2025 - last comment - 20:31, Tuesday 18 March 2025(83439)
Double Mixer Focus on the 8kHz Sideband

J. Freed

Today I collected 2 phase noises, first phase noise is of the 80 MHz OCXO after it has gone through an RF distributer. The reference was the SRS SG382 at 80MHz

The second is of the Double Mixer again but with an extra focus on the 8192Hz sideband.The reference was agian the SRS SG382 at 80MHz-4096Hz

These tests was done with the direct plug in method without using a PLL. This requires both the device under test and the reference device to be at quadrature. Normally a PLL is required to keep them there, however since both devices are connected to the LIGO timing system in some way,  a PLL is unnecessary to keep them locked in quadrature. To put them in quadrature I just lined them up on an oscilloscope best I could then added 90 deg by adjusting the phase on the SRS.  I bypassed the internal amp of the BluePhase1000 for all tests.

DM_vs_RF.pdf Is a plot of the two phase noises, as seen, the low frequency noise (<2Hz) has these humps. I now attribute these to the RF distributer causeing a shape change in the pure sin wave signal. 

RF_Distributer_Signal.jpg Shows how the RF distributer has a not exact sin wave (Yellow) compared to the SRS Pure tone (Blue)

DM8kSideband.pdf Shows a close up on the 8k sideband that will also couple into our SPI output 

Images attached to this report
Non-image files attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 20:31, Tuesday 18 March 2025 (83446)

The measured curve looks very similar to the SRS SG382 spec at 100MHz. There is no reason to believe the SG382 is better than the OCXO.

H1 General
anthony.sanchez@LIGO.ORG - posted 16:49, Tuesday 18 March 2025 (83444)
Tuesday afternoon Maintenance Recovery

TITLE: 03/18 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
INCOMING OPERATOR: Ryan C
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 10mph Gusts, 6mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.22 μm/s
SHIFT SUMMARY:
H1 has almost recovered from Maintenance day changes, We are currently in Nominal_Low_Noise but not Observing as the Cameras need to be reverted back to the old server.
NLN reached at 23:27 UTC.

Sheilas CPy measurements were completed.
 

LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:34 Electrical Ken LVEA No Finding lift for work Above HAM1 18:59
14:56 Vent Prep TJ near HAM1 N Taking down laser Curtains. 15:28
15:09 VAC Rogers Mech room N Working on kobelco units 20:39
15:11 PCAL Rick,  Francisco EX, EY Yes Beam Spot movment on EX. 16:44
15:23 VAC Gerardo West bay LVEA No Vac work, ION pumps into FCT 18:03
15:25 FAC Kim & Nelly EY, HAM SHAQ, EX N Technical cleaning. 18:05
15:27 VAC? Travis EX, EY Yes Taking Measurements 20:54
15:27 EE Fil LVEA, CER N Pulling cables. 19:48
15:29 IAS Jason Input - West LVEA N Doing some FARO work. 21:05
15:47 EE Marc LVEA N helping Fil 19:48
15:48 Site Safety McCarthy LVEA N Checking roll up door. 16:01
15:49 VAC Norco Y arm N Filling N2 tanks. 18:44
16:07 PEM Robert LVEA N Accel, cable clean up 16:13
16:20 FAC Chris Out Side West bay N Moving Big Green Harvester 19:41
16:48 Faro Jim HAM1, HAM SHAQ N Helping Jason 18:36
17:07 PCAL Francisco PCAL Lab Yes Putting away tools 18:59
17:14 FAC Christina Receiving N Picking up batteries , driving truck 17:59
17:28 SUS Rahul Remote/ EY & EX N SUS measurements on EY 19:14
17:49 TCS Camilla & TJ EX Yes opening laser table and adjusting TCS system 17:49
18:03 IAS Ryan C LVEA input- west N FARO-ing with Jason 21:05
18:06 FAC Kim, Nelly LVEA n Tech clean 19:30
18:23 SEI Jim LVEA, HAM ShAQ N Looking for Install hardware 19:01
18:49 Exercise Mayank & Shiva Overpass N Enjoying the noon view 19:19
19:25 TCS Camilla ITMY n Checking CO2 laser 19:32
19:42 LASER Transition Oli LVEA YES LASER Transition & LVEA Sweep. 19:56
19:53 CPy Sheila, Robert , Betsy ITMY Yes Centering CPy using Oplevs 21:21
19:57 LASER HAZ LASER HAZARD LVEA  (\u2310\u25a0_\u25a0) YES LVEA IS LASER HAZARD  (\u2310\u25a0_\u25a0) 06:36
21:07 ISC Rahul & Camilla, Shiva , Mayank Optics Lab Local Working on ISS, Rahul  Out early 23:49
21:55 ISS Camilla HAM6 Yes Getting parts 21:58
22:32 walk Ryan C Y-arm N Jogging the Y-arm 23:02

 

H1 General
ryan.crouch@LIGO.ORG - posted 16:15, Tuesday 18 March 2025 - last comment - 17:03, Tuesday 18 March 2025(83442)
OPS Tuesday EVE shift start

TITLE: 03/18 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 7mph Gusts, 4mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.22 μm/s
QUICK SUMMARY:

Comments related to this report
ryan.crouch@LIGO.ORG - 17:03, Tuesday 18 March 2025 (83445)

00:03 UTC Observing

H1 SUS
brian.lantz@LIGO.ORG - posted 15:41, Tuesday 18 March 2025 (83441)
added new part to SUS SVN

FYI - I've added a new block to the SUS SVN at SUS/common/models/

Adding         SIXOSEM_T_ESTIM_STAGE_MASTER.mdl   - this is simulink R2019a
Adding         SIXOSEM_T_ESTIM_STAGE_MASTER_tmp.mdl  - this was my working file in R2023b
Committed revision 31074.

These are a long way from done. This will be the new piece for the OSEM Estimator part for the HLTS (PR3)

The ECR is https://services1.ligo-la.caltech.edu/FRS/show_bug.cgi?id=32526

H1 AOS
sheila.dwyer@LIGO.ORG - posted 15:00, Tuesday 18 March 2025 (83440)
ITMY optical lever shifted

Robert, Betsy, Sheila

We went to the ITMY optical lever piers to check the CPY alignment, similar to 77557.  We tried to reset the optical lever back to where it was before we started, the optical lever is now slightly shifted though.  The sum dropped from 9060 coutns to 8930 counts, PIT went from -12.7 urad to -19.7 urad and YAW went from 1.3 urad to -4.4 urad.

H1 SEI (CDS)
filiberto.clara@LIGO.ORG - posted 14:25, Tuesday 18 March 2025 (83438)
Field Cabling for HAM1 ISI

WP 12393
ECR E2200105
DCC D2200162
DCC D1002872
T2300221

Started installation of the SEI HAM1 ISI field cables. Cables are now pulled from the CER SEI-C1 rack to the LVEA near HAM2/SUS-R1. Final routing of cables will continue next week. Documents D2200162, D1002872, and T2300221 don’t have the same flange layout. Imagine they will get updated once plans are finalized. Cables will be routed to HAM1 flanges as listed below:

Corner 1: Flange D1
SEI_HAM_15
SEI_HAM_16
SEI_HAM_17
SEI_HAM_18

Corner 2: Flange D5
SEI_HAM_33
SEI_HAM_34
SEI_HAM_35
SEI_HAM_36

Corner 3: Flange D3
SEI_HAM_51
SEI_HAM_52
SEI_HAM_53
SEI_HAM_54

CPS 1&2: Flange D5
SEI_HAM_63
SEI_HAM_64

CPS 3: Flange D3
SEI_HAM_65
SEI_HAM_66

F. Clara, M. Pirello

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
H1 General
anthony.sanchez@LIGO.ORG - posted 13:50, Tuesday 18 March 2025 (83435)
Mid Shift Maintenance Day Update

TITLE: 03/18 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 7mph Gusts, 4mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.24 μm/s
QUICK SUMMARY:

Be careful using the Roll up down between the receiving area and LVEA. It seems to be  in need of maintenance.
SNEWS Test T565015 16:00:15 UTC
HAM7 ISI WD Tripp17:09 UTC
HAM7 CPS Glitch 17:10 UTC
2 Norco trucks went in the Y armdirection from the parking lot.

Mechanical room has fumes in it , doors  have been opened to allow ventilation while Roger Bros

HAM7 CPS glitches 18:03 UTC

Dust alarms have been telling us there is dust.
 

Expected work:
LVEA:
Ham1 Laser Barrier taken down?
Lighting Fixtures above HAM1
Fil HAM1 pulling cables.
Vac roughing pumps & compressor
OMC scans by Elenna


EX:
PCAL ES Beam Mv over by 9am
Laser hazard Camilila & TJ TMS & ALS Return beam
Rahuls OPLEV SUS Charge measurements


EY:
Rahuls OPLEV SUS Charge measurements
Vac EY comp still in progress

CDS:
Dan LDAS maint.
Eric BS camera server testing

 

Still on going:
ITMY CPy adjustments.

H1 ISC
matthewrichard.todd@LIGO.ORG - posted 13:34, Tuesday 18 March 2025 (83432)
EX Beam scan measurements

M. Todd, C. Compton, T.J. Shaffer


We went down to EX with the intention of getting the reflected ALS beam to be a little cleaner, as we've been plagued with this lobey beam seen in alog 82752. If we were to succeed in cleaning up the beam we would have taken beam profile measurements; however, we were unable to make the beam any clearner, and any profile measurements did not make sense.

 

We started off a little cleaner than the previous log (82752) but we still had some weaker lobes that looked like ears (lending a sort-of Mickey Mouse shape).

Measuring the ALS return beam at  ETMX, we misaligned ITMX and ITMY. Starting slider values were:

20250318 - 16:00:00 UTC P Y
ETMX -34.6 -145.1
TMSX -87.0 -90.2

Moved to ETM Y: -2.4, TMSX: 634.8. (seems too big check this number on ndscope??), got worse, now has almost two lobes
Other way in Tat: ETM Y: -346.4, TMSX: -275.2. looks better, similar to original: Mickey Mouse.
Yaw back, not in Pitch: ETM P :204.4, TSMX P 139.0, now worse in Pit than yaw

Images attached to this report
H1 General
oli.patane@LIGO.ORG - posted 12:57, Tuesday 18 March 2025 (83434)
LVEA has been Swept

LVEA has been swept

H1 TCS
camilla.compton@LIGO.ORG - posted 12:34, Tuesday 18 March 2025 (83433)
CO2Y Tripped off 10:26am (17:26UTC) with RTD or IR alarm trip

Plot attached, reset at 19:30UTC.

There has been activity near that TCS rack this AM, both cable pulling and wire racks moved nearby. We've seen this happen before, LLO is currently trying to investigate why. 

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 11:33, Tuesday 18 March 2025 (83431)
Tue CP1 Fill

Tue Mar 18 10:12:51 2025 INFO: Fill completed in 12min 47secs

 

Images attached to this report
H1 AOS
david.barker@LIGO.ORG - posted 11:23, Tuesday 18 March 2025 (83430)
h1caley now using single safe SDF snapfile, no longer has separate observe file

h1caley's OBSERVE.snap is now a sym link to its safe file, bringing it in line with h1calex and the LLO models. h1caley_safe.snap was modified to monitor all of its channels.

lrwxrwxrwx 1 controls   advligorts     62 Mar 18 11:01 h1caley/h1caleyepics/burt/OBSERVE.snap -> /opt/rtcds/userapps/release/cal/h1/burtfiles/h1caley_safe.snap
lrwxrwxrwx 1 controls   advligorts     62 Apr 21  2015 h1caley/h1caleyepics/burt/safe.snap -> /opt/rtcds/userapps/release/cal/h1/burtfiles/h1caley_safe.snap


lrwxrwxrwx 1 controls   advligorts     62 Apr 28  2017 h1calex/h1calexepics/burt/OBSERVE.snap -> /opt/rtcds/userapps/release/cal/h1/burtfiles/h1calex_safe.snap
lrwxrwxrwx 1 controls   advligorts     62 Apr 21  2015 h1calex/h1calexepics/burt/safe.snap -> /opt/rtcds/userapps/release/cal/h1/burtfiles/h1calex_safe.snap

H1 ISC (OpsInfo)
sheila.dwyer@LIGO.ORG - posted 11:57, Thursday 13 March 2025 - last comment - 11:22, Tuesday 18 March 2025(83357)
ALS DIFF sped up a bit

We lost lock from the calibration, so we tried to lock ALS without the linearization (some background in this alog: 83278.)  An active measurement of the transfer function from DRIVEALIGN_L to MASTER out was 1 without the linearization, and -0.757 with the linearization on.  So I've changed the DRIVEALIGN gain to -1.3 in the ALS_DIFF guardian when the use_ESD_linearization is set to false.  

We tried this once, and it stayed locked for a DARM gain of 400, but unlocked as the UIM boosts were turning on. We tried this again but it also didn't lock DIFF, so it is now out of the guardian again.

I looked at a few more of the past ALS DIFF locks, both sucsesful and unsucsesful attempts we are saturating the ESD (either the DAC or the limiter in the linearization) in the first steps of locking DIFF.  We do these steps quite slowly, stepping the darm gain to 40 waiting for the DARM1 ramp time, stepping it to 400, then waiting twice the ramp time, then engaging the boosts for offloading to L1.  I reduced the ramp time from 5 seconds to 2 seconds to make this go faster.  This worked on the first locking attempt, but that could be a coincidence. 

We will leave this in for a while, so that we can compare how frequently we loose lock at LOCKING_ALS.  In the last 7 days we've had 48 LOCKING_ALS locklosses, and 19 locklosses from NLN, so roughly 2.5 ALS locklosses per lock stretch. 

Comments related to this report
sheila.dwyer@LIGO.ORG - 10:14, Tuesday 18 March 2025 (83427)

Since the time of this alog, around 19 UTC on March 13th, we've had 68 locking_ALS locklosses and 12 NLN locklosses, so about 6 locklosses per sucsesful lock.   It seem though that the change to 2 seconds was never in place, and the guardian code still said 5 seconds.  So this issue seems to be getting worse without any change. 

Now I've loaded the change to 2 seconds, so this should be sped up after today's maintence window.

sheila.dwyer@LIGO.ORG - 11:22, Tuesday 18 March 2025 (83429)

I've looked at a bunch more of these locklosses, and they mostly happen in the time when the DARM gain is ramping, less often as the boosts are coming on in L1, and 1 I saw happened while COMM was locking.

In all the cases the linearization seems to hit its limiter before anything else goes wrong.

H1 PEM
marc.pirello@LIGO.ORG - posted 10:16, Tuesday 11 March 2025 - last comment - 14:02, Tuesday 18 March 2025(83294)
BSC1 Temperature Sensor Maintenance

We removed the BSC1 temperature sensor to run some testing in the lab.  Will reinstall next week.

Comments related to this report
marc.pirello@LIGO.ORG - 11:59, Tuesday 11 March 2025 (83301)

After testing in the lab, the sensors are working as designed, outputs are clean.  We reinstalled the BSC1 temperature sensor but left it floating (not attached to BSC1). The BSC3 sensor we isolated from BSC3 with a thermal pad, and the power supply was isolated from the pier it is resting on.  This is an effort to remove ground loops on these systems.  Will revisit next week.

M. Pirello, F. Clara

marc.pirello@LIGO.ORG - 14:02, Tuesday 18 March 2025 (83436)

After review of the data over the week, we saw a marked improvement in temprature information so we reapplied the BSC1 sensor to the chamber along with a thermal pad to maintain electrical ground isolation.  We also isolated the power box for both supplies.

M. Pirello, F. Clara, D. Barker

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