Displaying reports 81-100 of 86913.Go to page 1 2 3 4 5 6 7 8 9 10 End
Reports until 17:04, Thursday 05 March 2026
H1 SUS (ISC)
elenna.capote@LIGO.ORG - posted 17:04, Thursday 05 March 2026 (89384)
BHSS moved to optics lab

First alog regarding BHSS!

Betsy, Mitch, Corey, and I moved the BHSS platform from the staging building to the optics lab. We wrapped it in foil and ameristat, and rolled it over on a cart.

Previously, Oli, Camilla, and I have prepped all the optic mounts for both BHSS and BHD optics. These mounts are all currently laid out on the optics lab table with cloths and foil. All the BHSS optics have been clocked to their correct angle using the clocking tool.

BHSS is placed directly on the clean optics table, no foil. Oli has staged 4" height optics to direct laser beam to the platform once we are ready for alignment.

Oli, Camilla and I today pulled first contact on some BHSS optics. We have successfully installed both PCX 333 lenses for BHSS platform (QPD-T-A/B-L1), the 7% 20 deg splitters (QPD-T-A/B-R1), one 50% 45 deg splitter (QPD-T-A-R2) and two BHSS HRs, 36-R1 and TRN-T1. All of these optics have labels (except 36-R1) so they can be distinguished. Serial numbers have been noted in the optics BOM.

These optics are currently mounted in a random place in the center of the platform so they can be kept clean.

Oli and I struggled to remove FC from two 50% 45 deg mirrors and several HR mirrors. Other mirrors were still dirty and needed to be recleaned. We will return to these optics later to re-FC to pull the original FC or clean off spots.

OMCs are still in their cases covered in foil on the same optics table. They were previously opened by Camilla, Jenne, Betsy, and I and confirmed by eye to look good. Begum mailed us 4 great DCPDs from the tested batch, these are still wrapped and bagged and in a tote in the optics lab.

OMC cradle prep is on hold while we wait for EP30 glue to arrive. Other to do items include prepping alignment tooling, finishing cable pylons, and removing FC for the remaining mirrors, etc.

Photos to come...

LHO General
corey.gray@LIGO.ORG - posted 16:59, Thursday 05 March 2026 - last comment - 17:47, Thursday 05 March 2026(89374)
Thurs DAY Ops Summary

TITLE: 03/05 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:

The arms were opened up today! 

I got pulled from my shift for a good chunk of the 2nd half of my shift, and so Ryan Short helped me out and will post about afternoon LOG of activities. 

LOG:

Comments related to this report
ryan.short@LIGO.ORG - 17:33, Thursday 05 March 2026 (89386)

Posting the log starting roughly in the afternoon for anything Corey might've missed.

Start Time System Name Location Lazer_Haz Task Time End
20:47 fac randy lvea - elevator arm work in east bay 20:59
21:05 saf corey lvea - putting up laser signs 21:13
21:20 jac daniel lvea - checking jac wfs electronics 22:57
21:24 jac jennie.jason lvea yes iot1 beam alignment 01:17
21:41 ee gerardo.fil lvea - HAM1 relay checks 22:18
21:53 saf richard lvea - checking in w/ fil 21:58
22:00 ee richard cer - testing something for fil 22:13
22:16 saf travis lvea - putting up laser sign on jac table 22:23
22:27 isc jenne.jane.corey lvea yes isct1 alignment 22:57
22:30 isc elenna.oli optics.lab - bhss optics 00:52
23:09 isc camilla optics.lab - bhss optics 01:01
23:49 cds dave mer - ham6 sus chassis work 00:47
00:26 tcs sophie cheta.lab - cheta table work 01:29
00:29 isc jenne lvea yes opening als shutter and checking isct1 00:47
jennifer.wright@LIGO.ORG - 17:47, Thursday 05 March 2026 (89388)

Camilla, Olli, Ryan S and I all checked through and cleared some sdfs before the green ARM locking and JAC alignment wokr started today. LSC and ASC channels for JAC should be good to go. I also updated the SAFE.snap file for ASCIMC as some channels had been removed in the last model change we did.

I have two pics of diffs that I accepted/reverted here and here.

Images attached to this comment
H1 IOO
daniel.sigg@LIGO.ORG - posted 16:18, Thursday 05 March 2026 (89382)
JAC WFS Electronics Tests

Used the test input of the WFS patch panel to check the 45MHz transfer functions of the JAC WFS. Measurement point was at the RF monitor output of the demodulator. The attached plots show:

  1. JAC WFS A segment 1 (all segments very similar)
  2. JAC WFS B segment 1 (all segments very similar)
  3. ASC REFL_A segment 1 (for comparison)
  4. ASC POP_X segment 1 (for comparison)

Observations:

The data sheet confirms these observations including the test input transconductance beeing 10x higher for S1300512.

Images attached to this report
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 13:22, Thursday 05 March 2026 (89381)
Gate Valves are Open

(Travis S., Jordan V., Gerardo M.)

After taking an RGA, HAM7 chamber was joined to the corner vacuum envelope, we opened RV-1, FCV-1, FCV-2, FCV-3, FCV-4 and FCV-5, no issues to report.

Then we opened GV5 and GV7.  GV7 started opening at 45 psi after a double clank noise, left GV7 set at 55 psi.  GV5 took some time to open, we got up to 40 psi and then left it alone, for about 20 minutes, then increased pressure to 45 psi a loud clank and then the valve opened, GV5 was set at 55 psi.

WP13071 is closed now.

H1 SEI
jim.warner@LIGO.ORG - posted 10:32, Thursday 05 March 2026 (89380)
March 2026 Wind Fence Inspection

I did the monthly wind fence inspection yesterday. No new issues. Damage to the one panel at EY seems stable, no damage noted at EX. 

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 10:15, Thursday 05 March 2026 (89379)
Thu CP1 Fill

Thu Mar 05 10:10:28 2026 INFO: Fill completed in 10min 25secs

 

Images attached to this report
H1 PEM
ryan.crouch@LIGO.ORG - posted 10:02, Thursday 05 March 2026 (89378)
H1 dust monitor Month Long Trends FAMIS37262

Closes FAMIS37262, last checked in alog88698.

Everything looks as expected, no new issues. There was an odd dust spike (10 minutes of >1000 cts, so 2 cycles of sampling) from the PSL102 (Anteroom) dust monitor on Sat Feb 7th around 11:30 local.

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 09:32, Thursday 05 March 2026 (89376)
h1sush6 front end computer first boot

Fil, Erik, Dave:

Fil ran the 24V-DC power to the h1sush6 IO Chassis on the MER Wed afternoon and I completed the fiber connections to the rear of the computer in the MSR. Erik and I booted h1sush6 for the first time late Wed afternoon after setting the BIOS and IPMI.

Current hardware status:

computer has Dolphin card installed but not connected to the switch. MTP at the computer end sends 4-Adnaco and 1-timing pairs to the MER via port-3 on the patch.

This is a W2275 14core machine, was cdsproxmox2. Its disks have been removed and it needed a full set of RT BIOS changes.

IO Chassis is "what was left" of h1sush2b after cards were moved over to the new h1sush12 chassis. So it has a mismatch of cards, but each Adnaco has a unique layout which is all that is needed to confirm Adnaco functionality.

A1 [slot1=TC, slot4=18AO8]

A2 [slot1=18AO8,slot2=16AO16]

A3 []

A4 [slot1=BIO]

The computer booted with some difficulty because it was trying to load the non-existent h1iopsush6 model. We were finally able to ssh onto the machine and showcards sees all the cards except A4. 

Also the timing card is not syncing, we will investigate that today.

A minor issue, we had some DNS issues on the workstation-LAN which Erik resolved.

LHO General (PEM)
corey.gray@LIGO.ORG - posted 08:15, Thursday 05 March 2026 (89375)
HVAC Fan Vibrometers FAMIS Check (FAMIS 39857)

For FAMIS #39857: All fan trends look nice and flat.

Images attached to this report
LHO General
corey.gray@LIGO.ORG - posted 07:40, Thursday 05 March 2026 (89373)
Thurs DAY Ops Transition

TITLE: 03/05 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: MAINTENANCE
    Wind: 10mph Gusts, 7mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.24 μm/s 
QUICK SUMMARY:

HAM1 (@4.0e-6) & HAM7 (@2.6e-7) continue to pump down.  There has been mention of opening gate valves (5 & 7), but not sure when.  CEBEX contractors are out and continue to unload pallets of brick.

H1 TCS
sophie.muusse@LIGO.ORG - posted 18:44, Wednesday 04 March 2026 (89372)
CHETA update

S. Muusse


The translation and rotation stage issues have been solved with help from patrick and daniel and now all optomechanics and sensors can be accessed and operated through beckhoff!
Dependent on a delivery, the feed throughs and rack should be constructed tomorrow allowing a full test of the electronics on the completed Y table.


Table 2 (X-arm) is almost fully aligned with only the beam dump and visible laser left to install. 

H1 CDS (AWC)
filiberto.clara@LIGO.ORG - posted 17:18, Wednesday 04 March 2026 (89371)
CHETA Field Cabling

WP 13063

CHETA field cables have been pulled. This includes the picomotor, analog readback, and laser interlock cables.

F. Clara, M. Pirello

LHO VE
jordan.vanosky@LIGO.ORG - posted 16:48, Wednesday 04 March 2026 (89370)
HAM 1 Leak Checking

Travis, Jordan

We were able to leak check the new JAC viewport on the -Y door of HAM1 today. Since this is an o-ring sealed viewport we bagged the viewport leaving the conflat seal exposed before spraying helium, in an attempt to reduce helium diffusion through the o-ring.

With the helium leak detector backing the main turbopump, the helium background was ~4E-10 Torr-l/s. While spraying the flange/leak check ports, the helium signal slowly rose (30-60 seconds) to maximum of ~1E-9 Torr-l/s, typical of permeation through an o-ring, see attached picture. 

Once, leak checking was completed, we disconnected the leak detector from the main turbo pump cart, isolated the turbopump from the chamber, and moved the SS500 cart closer to HAM2 to allow room for the new JAC table to be moved into place. 

HAM1 continues to be pumped via turbopump, while the annulus volume is still pumping with both the aux carts and the annulus ion pumps.

Images attached to this report
LHO General
corey.gray@LIGO.ORG - posted 16:33, Wednesday 04 March 2026 (89352)
Wed DAY Ops Summary

TITLE: 03/04 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:

HAM1 continues to pump down, but we are getting closer to opening gate valves.  CEBEX work near MY had several truck loads of bricks (on pallets) put in lay-down areas.  Had a couple of tours on-site.  HAM1 ISCT1 & new small JAC in-air tables were rolled into place.
LOG:

H1 ISC
camilla.compton@LIGO.ORG - posted 15:39, Wednesday 04 March 2026 - last comment - 09:41, Thursday 05 March 2026(89369)
ISCT1 and new JAC table IOT2R in place and bellows attached

Randy, Mitch, Betsy, Camilla, Jenne, Jennie, Richard

ISCT1 was forklifted into place by Randy and the table height checked. The new JAC table, IOT2R, was pushed into place and lifted off it's of it's wheels, height may need to be further adjusted once we start alignment. Bellows were attached. Photos of JAC table attached. 

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 09:41, Thursday 05 March 2026 (89377)EPO

tagging EPO

LHO EPO
tyler.guidry@LIGO.ORG - posted 15:36, Wednesday 04 March 2026 (89368)
CEBEX Progress pt1
Surveying for building footprint and water tie-in/routing actuals have been placed, and the masonry sub has begun staging CMU block while we await our grading permit.

B. Gateley M. Link T. Guidry
Images attached to this report
H1 SEI
jim.warner@LIGO.ORG - posted 12:08, Wednesday 04 March 2026 - last comment - 15:24, Wednesday 04 March 2026(89360)
HAM1 long tfs after JAC and periscope stiffener install

I took the .5-800hz tfs last night on HAM1 ISI, to see if the 70hz feature was improved by the periscope brace. Short version, it has been and I now see the ~170hz that I measure here. There's also a feature at ~102hz that could be a number of things, but I didn't see that in the B&K measurement of the periscope+stiffener. 

First attached image are the L2L gs13 tfs I took last night. Data below .5hz is from measurements I took last year, I don't expect those to have changed. Above .5hz is new data. These new measurements were taken with HEPI locked, so features around the pier modes at 15hz might not be permanent. I might also get better resolution above 200hz when the pumpdown is done and it's a little quieter at the chamber.

Second image are the data from last year, after adding the viton to the periscope dog clamps. That viton is still in place, but we now also have the stiffener added, so the sharp feature at 70hz is now moved to 170hz.

Third and fourth images are the CPS tfs. These are harder to compare because HEPI was unlocked for the fourth image (june 2025 tf) and locked for the third (last night). 

I will post C2C tfs when I get there. Hope to see if I can increase the loop gain on HAM1 with the 70hz feature gone, we'll see.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 12:25, Wednesday 04 March 2026 (89361)

These are the gs13 c2c tfs. First image is the data from last night, second image is the data from last year. Similar story, the new tfs look a little easier to wrap loops around, but the 170hz feature will require some notching. There is also still some feature at 75hz in the X and Z dofs. Hmm.

Images attached to this comment
jim.warner@LIGO.ORG - 15:24, Wednesday 04 March 2026 (89367)

I've touched up the isolation loops, removing the 70hz notches where I could and increased ugfs to more normal levels, from 22hz before to 25-30 hz. This should mostly help below 10hz. 

H1 SQZ
camilla.compton@LIGO.ORG - posted 11:18, Thursday 31 July 2025 - last comment - 15:06, Wednesday 04 March 2026(86117)
2W Mid SQZ Data for 5kHz and 10kHz HOM Spacing
Sheila, Camilla
Took data mid sqz only data once Ryan had the IFO locked at 2W on DC READOUT, he paused at CHECK_VOILINS_BEFORE_POWERUP. Aim is to see the HOM spacing at 5kHz and 10kHz to compare to the thermalized 60W data took in 85957. They have definitely shifted: at 2W at 5kHz and 10kHz and at 60W were at around 5.35kHz and 10.5kHz.
 
We saved  H1:OMC-DCPD_524K_A2_IN1 data with the PD sum after I changed the matrix as in 85937. DTTs saved as /ligo/home/camilla.compton/Documents/sqz/templates/dtt/20250731_SQZdata.xml screenshot attached and /ligo/home/sheila.dwyer/Noise_Budget_repos/quantumnoisebudgeting/data_files/higher_order_modes_sqzdataset2W.xml screenshot attached.
 
Starting angle is (-)130, requested SQZ_MANGER to FREQ_DEP_SQZ and once we got there, took SQZ_ANG SERVO to DOWN.
 
Type Time (UTC) Angle DTT Ref in SQZ DTT ref in HOM Notes
No SQZ 15:20:00 -15:25:00 N/A ref 0 ref 0,1  
FDS Mid - SQZ 15:31:00 - 15:34:00 (-)120 ref 1 ref 2,3 Was close to ASQZ so retook below
FDS Mid + SQZ 15:36:00 - 15:39:00 (-) 30 ref 2 ref 4,5  
FDS Mid - SQZ 15:40:00 - 15:43:00 (-)150 ref 3 ref 6,7  
 
Checked the NLG the normal way, checked OPO crystal temp but it was already optimized, unsure why is is so low already, we left it at 15.8 on Tuesday 86067.
OPO Setpoint Amplified Max Amplified Min UnAmp Dark NLG Note
80 0.0533596 0.00250 0.007039 -1.93e-5 7.6 Temp already optimized
Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 16:15, Monday 04 August 2025 (86182)

In this data I only see evidence of one mode at 5kHz, and one mode at 10kHz.  If the astigmatism that caused the X arm second order modes to separate into two in 86107 is due to the point absorbers or some other laser heating, it could make sense that we don't see astigmatism at 2W.  However, the ring heater settings for the two arms are different, so I would have expected the X and Y arm HOMs to be separated even at 2W.  This data was taken with 0.44W on ITMX RH (per segment), 1W per segment on ETMX RH, 0W on ITMY RH, and 1.5W per segment on ETMY RH.

Using a cursor to find the edges of the rotation from the three mid sqz traces that Camilla tok, the 5kHz mode frequency is 4956.5+/- 20 Hz, and the 10kHz mode is at 9981.5 +/- 19.5 Hz.  This suggests that the second order mode is at 99% of 2* first order mode frequency, similar to the ratio that we saw at full power.  86107. In the attached screenshot, the top panel shows where I put the cursor to measure the location of the 5kHz mode, the lime veritcal line in the bottom plots shows twice that frequency, 9913 Hz, which is clearly below the sqz rotation caused by the HOMs.

 

Images attached to this comment
camilla.compton@LIGO.ORG - 13:49, Tuesday 05 August 2025 (86208)

The hour times in my data table are all incorrect, should be starting at 17:20UTC.

When we started the data taking with NO_SQZ at 15:20UTC, the IFO had been down and the CO2 lasers off for 2hours 5mins.

sheila.dwyer@LIGO.ORG - 15:06, Wednesday 04 March 2026 (89362)

At Matt's request I revisited this data.  

We didn't plan on doing subtraction on this data at the time we took it, so we didn't save the high rate individual PD time series to do the cross correlation.  Instead, I made a rough shot noise model (a line in a semilog plot), subtracted that in quadrature from the no squeezing data to estimate the non quantum noise and subtract that from the squeezing measurements. 

Above I wrote that there is only one mode at 5kHz, and one at 10kHz, but after doing the rudimentary subtraction this data does seem to suggest that there are two modes at 10kHz, which we would expect since the ring heater settings are different for the two arms.  The rotation that is partially hidden by quantum noise and is around 9875-9900 Hz, and seems to rotate in the opposite direction from the more visible one at 10kHz.  (This is different from what was seen at full power in 86107 and in the similar ADF measurements in Kevin's comment).

The code used to make these plots is based on 86107 and is available here

Note: The pink trace in this plot is labeled anti-squeeze, but it is not, it is actually a mid squeezing angle that is somewhat close to anti-squeezing.

Non-image files attached to this comment
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