Displaying reports 1-20 of 86615.Go to page 1 2 3 4 5 6 7 8 9 10 End
Reports until 11:10, Saturday 14 February 2026
LHO VE
david.barker@LIGO.ORG - posted 11:10, Saturday 14 February 2026 (89160)
Sat CP1 fill

Sat Feb 14 10:14:53 2026 INFO: Fill completed in 14min 49secs

 

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 10:04, Saturday 14 February 2026 (89159)
FW0 spontaneous restart Friday evening

FW0 spontaneously restarted itself at 17:49 Friday 13th February 2026.

The DAQ was last restarted 16:05 Thursday 12th February, and FW0 had been running 1day 1hour 44minutes at the time it restarted. There have been no further restarts.

LHO General
ryan.short@LIGO.ORG - posted 16:54, Friday 13 February 2026 - last comment - 17:12, Friday 13 February 2026(89152)
Ops Day Shift Summary

TITLE: 02/14 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: Productive day with the HAM1 EOM being adjusted to recover IMC alignment, which locked easily and has a good REFL demod phase. Sounds like the EOM needs to be moved again slightly next week, but that's been prepped for this afternoon. A few AUX carts were disconnected in the LVEA as well today.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
22:49 SAF LVEA is Laser SAFE LVEA NO* LVEA is Laser SAFE *BIFURCATED HAM1/2 Ongoing
16:31 FAC Kim LVEA N Technical cleaning 17:46
17:27 CDS Fil, Marc LVEA - Cable pulling (HAMs 3/5 HEPI offline) 20:16
17:55 JAC Keita, Jason LVEA Y JAC EOM alignment 20:25
18:21 FAC Randy LVEA N Working on test stand (W-bay craning possible) 20:40
18:51 VAC Gerardo LVEA N Checking on pumps 19:16
20:11 SEI Jeff Opt Lab Local SPI work 23:59
21:20 CDS Fil, Marc LVEA - Cable pulling (HAMs 3/5 HEPI offline) 22:46
22:43 JAC Jason, Tony LVEA Y JAC REFL alignment 00:25
22:49 VAC Gerardo LVEA N Disconnecting AUX carts 00:05
23:21 PEM Robert EX N Grounding work 00:45
23:57 JAC Keita Opt Lab, LVEA Y JAC EOM alignment prep Ongoing
Comments related to this report
anthony.sanchez@LIGO.ORG - 17:12, Friday 13 February 2026 (89157)

Keita has come back from the LVEA, Light Pipe is closed for the weekend.
JAC Guardian has been taken to down.

LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 16:54, Friday 13 February 2026 - last comment - 17:27, Friday 13 February 2026(89155)
HAM4 Annulus Ion Pump Replacement

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

Late entry-

Late Wednesday we vented the annulus system for HAM4 using nitrogen.  On Thursday, we removed and replaced the ion pump, a very uncomfortable location for this pump, it is surrounded by cable trays, see photos.

We have not been able to fasten the mounting bolts that hold the ion pump body in place, we have noticed that the pipes for the annulus system leading up to the mounting flange are not parallel to the ion pump flange they are |/ and they should be ||.  So, we have to twist the pipe to be able get it parallel to the pump.  We have a mechanical block supporting the pump as a temporary support, we'll replace it as soon as possible.

Comments related to this report
gerardo.moreno@LIGO.ORG - 17:27, Friday 13 February 2026 (89156)VE

Today, I visited HAM4 ion pump and turned the controller on, it railed at first, and a few minutes later it was at nominal value, and after it reaching a bit below 2 milliamps I closed the isolation valve for the annulus system, an hour or so later the aux-cart, can turbo and hoses were removed.  Ion pump pressure signal has turned around and getting lower, nice!  Good job, Jordan and Travis.

Images attached to this comment
H1 IOO (INS)
jason.oberling@LIGO.ORG - posted 16:37, Friday 13 February 2026 (89154)
JAC REFL Path Work

T. Sanchez, J. Oberling

This afternoon we took a look at the JAC Refl path and positioning of IOT1.  We ended up pushing IOT1 in the +X direction by ~1"; new marks were made on the floor to represent this position.

From here we used JACR-M1 and JACR-M2 to align the beam through the viewport simulator and onto the top periscope mirror of IOT1.  This only took a couple of iterations before things looked mostly OK.  The beam is currently a little low in the viewport simulator, maybe 0.5" to 1" (rough measurement by eye) and is hitting the top periscope mirror.  We finished by measuring the beam height at 2 places on the ISI table roughly 28" apart, to give us an idea of how the beam is pitched.

This seems OK for now, but on some reflection while sitting in my office typing this alog we may want to briefly revisit this.  The beam is slightly pitched down and is high on JACR-M2 (~0.5" on a 2" diameter optic), so I think there is some room to improve this, to get the beam closer to center on JACR-M2 while still passing through the viewport simulator and onto the top periscope mirror of IOT1.  More to come.

H1 IOO (ISC)
elenna.capote@LIGO.ORG - posted 15:59, Friday 13 February 2026 (89149)
IMC REFL demod phase is good with new EOM

I checked the IMC REFL demod phase. Locking the IMC was very easy- with 100 mW coming from the PSL, I selected "locked" on the guardian and it locked right away, good work from the team in alog 89106!

I injected a 400 ct line into IMC L at 50 Hz, following similar steps done by the JAC crew here.

I only saw the line in I phase, so I tried taking a no injection reference and also bumping up the injection to 800 ct to see if there is signal in Q phase. There is no visible signal in Q phase. Therefore, I declare that the IMC refl demod phase is just fine at 20.87 deg.

The attached plot shows the injection time in the red and blue live traces in I and Q, and the no injection reference time in pink and blue.

I ran another excitation at 10000 ct to generate the second plot attached.

Images attached to this report
H1 PEM
ryan.short@LIGO.ORG - posted 15:36, Friday 13 February 2026 (89150)
BSC2 Dust Monitor Trend

Richard asked for a one-day trend of the dust monitor at BSC2 since he moved it from the floor up to the dome platform (alog89137); see attached. Heightened counts from today likely from cable pulling activities around/on top of HAM3 nearby.

Images attached to this report
H1 AOS
keita.kawabe@LIGO.ORG - posted 13:33, Friday 13 February 2026 - last comment - 18:14, Friday 13 February 2026(89148)
JAC-EOM work, Friday Feb/13/2026 (Jason, Keita)

Morning report.

Pictured the beam position on the input and the output side plate of the EOM.

We'll see if it's off or not, doesn't look bad but we'll see once I have time to look at the pictures.

We realigned the beam into IMC, mode mismatch < 0.4%.

I just assumed that the MC alignment itself was good. I found MC2 in misaligned state and changed it to aligned.

We had to work both on PIT and YAW, but mostly in PIT (i.e. the difference in horizontal beam deflection between the old batch crystal that we're using and the new batch crystal is smaller than the difference in vertical deflection). 

Good news is that the mode matching is still pretty good. Attached is the MC2 trans VS time while the PSL frequency was ramped. Assuming that the tiny thing pointed by the green arrow is actually 2nd order HOM peak, the mismatch is 0.036/9.4~0.4%. Consider this as an upper limit, because it's hard to tell if the "peak" is actually a peak, could be noise fluctuation.

Images attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 18:14, Friday 13 February 2026 (89158)

Afternoon:

Tony and Jason worked on REFL path: alog 89154.

Elenna confirmed that the demod phase for IMC didn't change: alog 89149.

We'll have to move the EOM again.

Looking at the pictures shot this morning, the beam seemed to be a bit too much in -Y direction relative to the EOM aperture especially on the output plate.

Assuming that the wedge angle is the same (2.85 degrees per surface) and the deflection angle is the same (2.35 degrees per surface) as the new batch, the EOM should move at the input by about 0.7mm and at the output by about 1mm, both in -Y direction.

We'll move the entire structure by marking the +Y edge of the EOM pivot base plate using two dog clamps and then inserting washers between the dog clamps and the base.

I measured the edge thickness of four big slotted washers, they're not uniform in thickness (they're not machined after all) but they're all between 24 and 29 thou (between 0.61 and 0.74mm). Inserting one big slotted washer per dog clamp might be good enough.

Images attached to this comment
LHO VE
david.barker@LIGO.ORG - posted 10:20, Friday 13 February 2026 (89146)
Fri CP1 Fill

Fri Feb 13 10:15:27 2026 INFO: Fill completed in 15min 23secs

Gerardo confirmed a good fill curbside.

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 07:54, Friday 13 February 2026 - last comment - 08:53, Friday 13 February 2026(89141)
Another round of PEM model changes and DAQ restart

Robert, Dave:

Thursday 12th February 2026

h1pemex was changed, the newly installed AMON subsystem which reads the current to ground signal now drives the 4th channel of the 20bit-DAC via the GDS_3/DACOUTF_3 filter module chain.

h1pemey was modified to fix a typo I had made to the DACOUTF_3 filtermodules, it was missing the underscore.

Both models were restarted at 15:55, followed by a DAQ restart at 16:01-16:06

I created MEDMs for the new DAC drive system. I'll work with Ryan S on integrating this with his "GDS DAC DRIVE" screen, currently I've added buttons to the bottom of Ryan's MEDM to open mine.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 08:53, Friday 13 February 2026 (89145)

I made a slight change to h1pemex to reposition output ports and connect them via goto-tags for the mainsmon channels which are sent via long-range dolphin to h1oaf.

I restarted h1pemex at 08:47 (no DAQ restart needed) and verified the IPC was still good.

LHO General
ryan.short@LIGO.ORG - posted 07:35, Friday 13 February 2026 (89144)
Ops Day Shift Start

TITLE: 02/13 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: 3mph Gusts, 2mph 3min avg
    Primary useism: 0.07 μm/s
    Secondary useism: 0.59 μm/s 
QUICK SUMMARY: Another cold and foggy morning at LHO. Today, the EOM with its new crystal will continue to be aligned in HAM1 while the JAC reflected path is finalized pointing to IOT1. HAM7 continues to pump down as well.

H1 IOO (IOO, ISC)
jennifer.wright@LIGO.ORG - posted 13:58, Thursday 12 February 2026 - last comment - 12:16, Friday 13 February 2026(89139)
JAC work today

Jennie W, Jason O, Keita K, Betsy W, Camilla C

 

Summary: EOM alignment and position captured, moved to opics lab for crystal replacment, JAC-REFL path alignment in progress.

 

This morning Jason, Keita and I checked the centering of the HAM1 irises after the JM3 alignment Olli and I did on Tuesday. We didn't move the irises right after JM3 as this seemed centred. We did reposition the iris right before the HAM2 septum plate in x and y.

This, along with the alignment of the IMC Olli, Jenne and I did on Tuesday, captures where the beam was with the current EOM installed.


Keita marked the EOM base position with a dog clamp and removed it to the optics lab for crystal replacement. The shims for the EOM and the screws that hold it to the table are in a foil packet on the +Y - X HEPI pier.


Betsy, Camilla and I rechecked the REFL path and spent some time moving JACR-M2 to centre it on the incoming and outgoing beams. Then we pitched down this mirror so the outgoing beam hit the upper periscope mirror. After this Betsy had some concerns that we were too close to where the JM3 tip-tilt will sit (we are  currently using a siskiyou mount for this mirror). So we yawed the JACR-M2 mirror so the beam hits the viewport slighly more to the right (as viewed from -Y side). Looking at the placement on the viewport simulator, the beam is low and right on the viewport, whereas it comes to the table, high and right in the bellows hole. This table it almost at the top of its adjustment range, so Jason and I plan to go in this afternoon and see it we can move up the table feet so the beam can move up in the viewport a bit. Betsy and I measured the tilt of the beaM from JACR_M2 off the table. The heigh is 103 mm at the table hole 8 inches from the -X edge and 8 inches from the +Y edge. It tilts up to 113mm at the last hole in this row on the -Y side.


Betsy and I also checked the pitch of the beam entering and leaving JAC after the EOM was removed. The input beam to the JAC was 102 mm above the table, the output beam before the L1 lens was the same height, and the beam height just before JAC_M3 was also 102mm. There is not a large distance between the JAC and JAC_M3 steering mirror so it is hard to get a good measurement of any small pitch in the beam. Pictures for this alog are coming.

Comments related to this report
keita.kawabe@LIGO.ORG - 17:36, Thursday 12 February 2026 (89142)

EOM crystal was swapped, EOM was tuned in the lab and put back in place in HAM1. Tuning is good. First look at the beam looks good, no ghosts.

We extracted the EOM from HAM1 after the position of the EOM base was marked with three dog clamps.

In the lab, the EOM pivot plate was separated from the EOM base (which was a major pain again), then the EOM top structure was separated from the pivot plate.

Before unmounting the old crystal, three set scews in the face plate were screwed in to contact the electrode board, and then very slightly backed off. After this, we lifted the board/side assy from the front plate to expose the crystal on top of the face plate, swapped the crystal (in our setup, the distance between the crystal edge and the front plate edge close to the output side was set to ~7.5mm due to 0.5mm shim washer we use between the front plate and the input side plate), and put the board/side assy on. This was much easier than before due to the aforementioned set screws. Elenna will post some pictures.

In the afternoon the EOM was tuned in the lab and put back into HAM1. We didn't bother to tap things around this time.

EOM was transferred to HAM1. Tuning measurement was repeated in chamber, no big change from the lab measurement and they're good (see pictures).

With EOM in place, we locked JAC and confirmed that the wedge orientation of the crystal was correct (because the beam was mostly deflected in YAW toward +Y direction). We also saw that the beam deflection was different from the old EOM in PIT as well as YAW (more difference in PIT according to Jason).

No fine alignment of the EOM was done for today, but we quickly raised the power to 1W and neither Jason nor I were able to find any clear ghost beams, unlike with the old crystal.

Below is a table of RTP crystals at LHO (see alog 89125alog 89115).

RTP crystal S/N, batch Status
10252007, Old Good, in HAM1
10252003, Old Chipped. Probably never used.
B1913109, New Uninstalled, ghost beams
B1913108, New Never used, ghost beams

 

Images attached to this comment
elenna.capote@LIGO.ORG - 12:16, Friday 13 February 2026 (89147)

Here are some further notes and photos of the replacement work:

  • The EOM crystal we chose to use did have pencil markings on one side ("z" for the crystal axis and also a number) which keita attempted to remove with a tex wipe and isopropyl alcohol. He was not able to completely remove the markings. Inspection photo and placement photo
  • When we took the EOM off the base mount, we had to do extensive cleaning of the peg and hole as essentially we are just reaming the hole larger whenever we place the EOM or remove it. We used q tips soaked with isopropyl alcohol to clean the hole until the q tips came out clean, and a tex wipe with alcohol to clean the peg. There were metal shaving and metal dust
  • We did not see any problems by eye with the EOM crystal we removed. Here is a photo where you can see the number on the ruler through the crystal
  • Here is a photo of the EOM in place with the front shims only (back shims placed shortly after)
Images attached to this comment
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 22:02, Tuesday 10 February 2026 - last comment - 17:23, Friday 13 February 2026(89116)
HAM7 Pumpdown Update

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

Pumpdown was restarted this morning around 9:11 am local time.  After pressure inside HAM7 reached 0.5 Torr we switched over to the turbo, we had a very smooth transition.  After the internal pressure of HAM7 reached 5.0x10-05 Torr all O-ring isolation valves were closed (we have one at the turbo pump, another at the chamber and one more at the relay tube).
HAM7 internal pressure after 12+ hours of pumping is 5.2x10-06 Torr.  The attached plot has a small glitch at the 10 hour mark, likely due to the DAQ restart.

Annulus ion pump update.  The ion pump controller was turned on this morning, the ion pump controller struggled for some time as it was railed, but we did noticed that the pressure reading reported by the aux-cart (aux-cart remains connected and pumping on this system) dropped very slow, but after a some minutes the ion pump controller was not railed no more.

Images attached to this report
Comments related to this report
gerardo.moreno@LIGO.ORG - 17:23, Friday 13 February 2026 (89153)VE

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

Update for HAM7 pump down and other accessories.

- Pressure internal to the chamber continues to drop, slow but it is making progress.  Plot attached.  Pressure as of this entry is at 1.27x10-06 Torr.

- HAM7 Annulus system update, the ion pump made some good progress.  The ion pump has settled down to 3 milliamps, good pressure reading, this allowed us to remove the aux-cart, can turbo and hoses from this ion pump.

- HAM7 RGA system, yesterday we connected an aux-cart+can turbo combo to this system, we are pumping it down to get it ready for use, but first we need to leak test the conflats that removed from the +Y door.

Images attached to this comment
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 18:40, Sunday 08 February 2026 - last comment - 17:24, Friday 13 February 2026(89078)
HAM3 Annulus Ion Pump Replacement

(Jordan V., Gerardo M.)

-Late entry

On Friday we removed and replaced the ion pump for HAM3.  We replaced the copper gasket twice, the first gasket seal had a bad leak, it was hard to see the mating surfaces due to visibility issues (laser safety goggles and not enough light).
After installing a second gasket, we started pumping down the annulus system and pressure went down fast.  Last pressure reading at the aux-cart was 4.63x10^-05 Torr.
BTW, we have other 4 (four) ion pumps to replace.

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 09:23, Thursday 12 February 2026 (89129)EPO

EPO taggin'.

gerardo.moreno@LIGO.ORG - 17:24, Friday 13 February 2026 (89151)VE

(Jordan V., Gerardo M.)

After a couple of days of "assisted" pumping, the annulus system isolation valve was closed.  After a day of solo pumping the ion pump was able to maintain the annulus pressure at nominal.  Now the aux-cart, can turbo and hoses were removed, pressure looks good.

Images attached to this comment
H1 ISC
sheila.dwyer@LIGO.ORG - posted 16:34, Monday 08 September 2025 - last comment - 06:03, Friday 13 February 2026(86785)
summary of September 4th OM2 heating test

On Sept 4th we had a longer commissioning period to allow us to heat up OM2.  The main goal was to use this to characterize the mode matching of the arm cavities to the OMC, but we also made some other interesting measurements.

Summary:  heating up OM2 now costs us about 1% of optical gain, while it used to cost us 2%.  Heating up OM2 also changed the SRCL offset needed to get flat squeezing significantly, and reduced the amount of squeezing that we could get (without adjusting psams).

The interferometer unlocked (86727) while Jennie Wright was running the DARM offset step script with OM2 cold, to get a measurement of HAM6 throughput and look at OMC refl before heating up OM2.  As that link says, there wasn't an obvious connection between the DARM offset script which was in it's final steps (nearly back to normal) when the lockloss happened. 

We turned on the OM2 heater while relocking after some back and forth, then had an commissioning caused lockloss while trying to recover.  By the time we were relocked, OM2 was heated up according to thermistor 2, which is the thermistor who's timescale matched the timescale of optical gain changes in the past (see screenshot of June 2023 example).  We also had a large earthquake while relocking, so we paused after power up and before going to nominal low noise, so we do not have tracking of the optical gain using pcal in the first 30 minutes of this thermalization. 

The optical gain in this thermalization seemed to be fairly similar to the previous lock where OM2 was cold in the first hour.  The change in optical gain between OM2 hot and cold was much smaller this time around, so we needed to see the full thermalization in order to see what the gain change was.  We set the OM2 heater off 4 hours and 5 minutes after the power up, the attached screenshot shows a trend of optical gain during the previous thermalization while OM2 was cold, with a vertical cursor 4 hours 5 minutes into the lock.  The horizontal cursors show where the optical gain was at 4 hours and once the thermalization was complete, the optical gain continued to increase by 0.2% after the first 4 hours. The next screenshot shows vertical cursors also at the time of power up and 4 hours later, and the horizontal cursors are the same as on the previous screenshot (OM2 cold).   It seems that the optical gain was about 1.1% lower with OM2 hot than cold, although fitting these two thermalizations to an exponential might bring them closer by as much as 0.2%. Our current ring heater settings are 0W on ITMY, 1.5 W/segment on ETMY and 0.44W/segment on ITMX and 1W/segment on ETMX.

Since this is a different result than in the past times of OM2 changes, I've gone back to look at old times when we did this change.  One possible explanation for the difference could be ring heater settings being different. 

Once the OM2 heater was turned back on, the optical gain increased by nearly 1%, but the IFO lost lock before that thermalization finished.  There was a 2% decrease in POP18 during the cool off and a 3 urad shift in SRM top mass. 

While OM2 was hot, we did a few tests.

 

Images attached to this report
Comments related to this report
evan.hall@LIGO.ORG - 06:03, Friday 13 February 2026 (89143)ISC, MDL/SIM, TCS

I crunched this data using Gabriele's calibration of OM2 temperature into RoC (LIGO-T2200274). Actually in both the 2023 and 2025 tests it seems like throwing OM2 from cold to hot reduces optical gain by about 2%. One might eke out a bit more data by allowing a bit more thermalization of OM2, but probably not much. kappa_c is a measure of only relative optical gain against a nominal value, so it's not clear that kappa_c = 1 means the same thing for these two datasets since they're two years apart.

Non-image files attached to this comment
Displaying reports 1-20 of 86615.Go to page 1 2 3 4 5 6 7 8 9 10 End