Displaying reports 1-20 of 84233.Go to page 1 2 3 4 5 6 7 8 9 10 End
Reports until 22:03, Tuesday 02 September 2025
LHO General
ryan.short@LIGO.ORG - posted 22:03, Tuesday 02 September 2025 (86705)
Ops Eve Shift Summary

TITLE: 09/03 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 152Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY: Very quiet shift with H1 locked and observing throughout; lock stretch is currently up to 8 hours. A M5.3 EQ out of Japan rolled through about an hour ago but didn't even put us into EQ mode.

H1 ISC
anthony.sanchez@LIGO.ORG - posted 17:47, Tuesday 02 September 2025 (86703)
Bi-Weekly Locking Histograms

Bi-weekly Histograms of Locking statew times.

Histogram of time spent at NLN or higher:
Length of data 22
max Duration 2613 Min
Average 770.5 Min
% below 5 minutes : 0.0
Between 2025-08-20 00:27:34  and  2025-09-03 00:27:34
 

PowerUp Histogram
Length of data 30
max Duration 39 Min
Average 24.966666666666665 Min
% above 30 minutes 73.33333333333333
Between 2025-08-20 00:45:04  and  2025-09-03 00:45:04
 

DRMI-Histogram
Length of data 51
max Duration 49 Min
Average 11.647058823529411 Min
% above 5 minutes 54.90196078431373
Between 2025-08-20 00:46:03  and  2025-09-03 00:46:03
 

ALS Histogram
Length of data 53
max Duration 30 Min
Average 5.471698113207547 Min
% above 5 minutes 32.075471698113205
Between 2025-08-20 00:46:40  and  2025-09-03 00:46:40

 

Images attached to this report
LHO General (SQZ)
thomas.shaffer@LIGO.ORG - posted 16:30, Tuesday 02 September 2025 (86691)
Ops Day Shift End

TITLE: 09/02 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 149Mpc
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY: A fair amount of work done even though it was looking to be a slower maintenance day. We managed to stay locked for a few hours into it, while staying in light maintenance mode. We relocked automatically with an initial alignment, then lost lock 39 seconds later from an ETMX glitch. On the way up the second time, Elenna opportunistically tuned up PRMI ASC since it has shown some signs of non-convergence (alog86694). We have now been locked for 2.5 hours while a small dropout when the SQZr unlocked.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:30 CDS Fil, Erik EX n HWWD cable 16:10
15:31 FAC Erik Ends n Chiller alarms 16:03
15:34 FAC Kim, Nelly mids, ends n Mats 15:35
15:34 FAC Randy CS n Forklift from VPW to LSB 16:28
15:35 FAC Tyler vertex n Fire hydrant 15:36
15:35 VAC Norco CP7 (EY) n LN2 delivery 16:54
15:36 VAC Travis MX n Pump work 20:03
15:37 FAC Tyler LVEA n Yellow tape 15:38
15:37 FAC Someone Staging n Rock moving 19:35
15:38 FAC - site n Fire pumps running 19:33
15:43 SQZ Sheila CR n SQZ meas. 16:34
15:55 VAC Janos MX n Joining Travis for pump work 20:03
15:56 SEI Jim EX, EY n Wind fence inspection 17:53
15:58 FAC Kim, Nelly LVEA n Tech clean 17:04
16:12 CDS Fil LVEA n SUS56 racks and near HAM3 racks, cable and chassis prep 17:16
16:15 FAC Randy, Tyler OSB rec., LVEA n Forklift into OSB receiving and then moving into LVEA (craning?) 16:33
16:27 VAC Gerardo, Jordan, Anna LVEA n Taking measurements near HAM6 (Jordan, Anna out 1659) 17:17
16:34 FAC Chris LVEA, Y arm, X arm n Pest control escort 17:52
16:37 PCAL Rick, Tony PCAL lab local PCAL lab meas. 20:23
16:42 ISC Daniel LVEA n AS_C whitening cable 18:32
16:53 PSL Jason CR n Ref cav remote alignment 17:11
17:01 - Richard LVEA n LVEA check 17:26
17:05 FAC Kim, Nelly EY, EX n Tech clean 18:24
17:21 PEM Robert LVEA n Shaker setup 19:35
17:32 CDS Marc MY, EY n Checking on power supplies 18:05
17:51 SYS Betsy LVEA n Grabbing dog clamps 18:08
17:53 FAC Chris LVEA n FAMIS checks 18:26
18:08 SYS Betsy Opt Lab - Parts 18:38
18:24 FAC Kim, Nelly FCES n Tech clean 18:50
18:27 FAC Chris Ends, Mids n FAMIS checks 18:54
18:35 SQZ Camilla, Fil LVEA - SQZT7 LOCAL Noise hunt 19:05
18:42 SYS Mitchell LVEA - W n Parts hunt 18:53
18:47 - Matt LVEA n Sweep 19:05
18:56 VAC Gerardo, Jordan MY n Parts hunt 19:35
19:46 PEM Robert LVEA n Wrapping up 20:03
21:38 PCAL Francisco PCAL lab - Packing up to ship out 22:33
22:12 SYS Betsy Opt Lab n Parts 22:40
22:51 ISC Camilla Opt Lab n Parts hunt 23:17
LHO General
ryan.short@LIGO.ORG - posted 16:11, Tuesday 02 September 2025 (86702)
Ops Eve Shift Start

TITLE: 09/02 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 10mph Gusts, 5mph 3min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.11 μm/s
QUICK SUMMARY: H1 has been locked for 2 hours.

H1 PSL
ryan.short@LIGO.ORG - posted 16:00, Tuesday 02 September 2025 (86701)
PSL 10-Day Trends

FAMIS 31101

The fire alarm yesterday briefly shut off air handlers, so we see some temperature changes in several places that appear to have all settled back to nominal. Also, Jason's PMC, RefCav, and ISS adjustments this morning are seen clearly. No other major events of note in the past week.

Images attached to this report
H1 PSL
ryan.short@LIGO.ORG - posted 15:47, Tuesday 02 September 2025 (86700)
PSL Cooling Water pH Test - Monthly

FAMIS 26684

pH of PSL chiller water was measured to be between 10.0 and 10.5 according to the color of the test strip.

X1 SEI (SEI)
richard.savage@LIGO.ORG - posted 15:34, Tuesday 02 September 2025 (86699)
Measurement of SPI HR mirror transmissivity and SPI BS AR surface reflectivity

TonyS and RickS

Today, we measured the transmissivity of one of the SPI HR mirrors and the AR surface reflectivity of one of the SPI beamsplitters, as requested by Jeff Kissel.  The reflectivities of the beamsplitters were measured earlier, see this aLog entry.

HR mirror reflectivity:  We used a set of Gentec power meters procured for the Pcal effort.  An SPI HR mirror (see attached photo for details).  Aligned at 45 deg. AOI with s-polarized light, the power transmissivity (P_trans/P_inc) was measured to be 23 e-6 W/ 567 e-3 W or 4.1e-5 (0.004%). 

BS AR surface reflectivity: The reflectivity of the AR surface of a 50/50 beamsplitter was measured in two ways, both after mounting the BS with the AR surface closest to the input beam.

1. Using the PS5 Pcal power sensor and blocking the beam reflected from the 50 % reflectivity surface near the beamsplitter, the output voltage (after zeroing the no-laser-light level) was - 0.387 mV.  With both the main reflected beam (~ 50 % of the incident light) and the beam reflected from the AR surface, the voltage was - 1.3699 V.  Doubling the voltage for what would have been expected with the full incident power, the estimated AR reflectivity is  0.387 e-3 / (2 x 1.3699) = 1.4 e-4 or  0.014 %.

2. Using power meters to measure the power in the beam reflected from the AR surface and the power incident on the BS, we measure 52.6 e-6 W / 564 mW = 9 e-5 or about 0.01 %.

 

Images attached to this report
H1 SQZ
camilla.compton@LIGO.ORG - posted 15:21, Tuesday 02 September 2025 (86692)
SQZ NLG Messurements at Different ISS AOM Setpoints

Tried to measure NLG (following 76542) at different ISS setpoints (by changing the SHG waveplate to adjust how much power is incident on the AOM), with the same OPO TRANS power. Because in 86363 we were confused that the NLG increased significantly when we realigned Pump fiber, with the same OPO Trans setpoint.

This was confusing and I'd like to repeat next week. I initially thought we were getting pump depletion so decreased the seed power, but later noticed the ISS was just unable to keep up and the control voltage was dropping to -5 for the low values of ISS setpoint, see attached, it could hold in LOCKED_CLF_DUAL with 80uW OPO_TRANS fine but not with the SEED beam.

OPO Setpoint ISS Setpoint when locked on Amplified Unamplified NLG Notes
CLF DUAL SEED Max Min UnAmp Dark
80 4.9 3.2 0.192924 0.002389 0.0079612 -2.1e-5 24.2  
80 2.9 2.9 0.045037     -2.2e-5 39 ?(using below unamp) Pump deplation?  Reduced SEED power from 0.7 to 0.3 to keep it locked on SEED (still didn't work first time).
80 6.3 6.3 0.0430464 0.000546 0.0011063 -2.2e-5 38 ? Unamp signal decreased from SEED power change.
80 4.8 4.7 0.0454944 0.0005378 0.0018533 -2.7e-5 24.2  
80 2.9 -5 ?           Noticed ISS Controlmon at -5. 
80 3.5 3.5 0.0452317 0.00054049 0.0018636 -2.4e-5 24.0  
80 4.95   0.04523       24.0 Leaving here.
 
Images attached to this report
H1 SQZ (DetChar)
camilla.compton@LIGO.ORG - posted 14:43, Tuesday 02 September 2025 - last comment - 14:52, Tuesday 02 September 2025(86696)
SQZT7 Pico causing buzzing now disabled and monitored in sdf

Fil, Camilla, Sheila. WP#12784

In 86323 we noticed a high pitched noise in SQZT7. Today we found the SQZT7 picos were enabled. When Sheila disabled them, the noise disappeared. It did not come back when they were re-enabled. 

All picos should be off in Obserivng so I monitored the sdf. However, even when enabled, the picos should not make this noise. Fil suggests we watch this pico controller closely as when used it it might intermittently get stuck trying to drive and start to make this noise again. 

Tagging DetChar:  this pico has been on in Observing from 24th June until 2nd September.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 14:52, Tuesday 02 September 2025 (86698)

TJ and I then checked that all other picos are monitored in sdf.

H1 General
thomas.shaffer@LIGO.ORG - posted 14:16, Tuesday 02 September 2025 (86697)
Back to Observing at 2109UTC

We made it up to NLN at 1941UTC but this only lasted 39 seconds before an ETMX glitch took us out. On the way back up we noticed that it would need to go through PRMI, so Elenna took the time to fix it since we ran into some issues with it last week (alog86618). We wrapped up a few SDFs that were left over from maintenance day activities, and then to observing at 2109 UTC.

H1 ISC
elenna.capote@LIGO.ORG - posted 13:35, Tuesday 02 September 2025 (86694)
Updated PRC1 error signal in PRMI

After problems with PRC1 ASC, reported here, I checked the PRC1 P error signal and saw that the REFL signal seems to have a small offset. However, it appears that the POP X I signal has no offset, so I updated the error signal and tested the sign. The ISC DRMI code is updated with this new matrix.

H1 SQZ
sheila.dwyer@LIGO.ORG - posted 12:09, Tuesday 02 September 2025 (86683)
filter cavity injection during maintence day

Sheila, Matt, Camilla

As the interferometer stayed locked during the early part of maintence day, we did some injections into the filter cavity length to try to measure the noise caused by backscatter.  (Previous measurements 78579 and 78262, recent range drops that we think are filter cavity related: 86596)

The attached screenshot from Camilla shows the excitations and their appearance in DARM. (Compare to Naoki's measurement here, and to the time with no injection but elevated noise here).   I made a simple script to make the projection based on this injection, which is available here.  It does show about a factor of 3 a higher level of noise in DARM than Naoki's projection 78579, this is large enough that we should add it to our noise budget but far too small to explain our low range times last week.

 

Images attached to this report
Non-image files attached to this report
H1 General
matthewrichard.todd@LIGO.ORG - posted 12:01, Tuesday 02 September 2025 (86693)
H1 Sweep 2025-09-01 before transistion back to observing

M. Todd


I did a sweep of the LVEA, everything looked fine.

I unplugged an extension cord from outside the PSL racks, and noted that a forklift by the 3IFO racks was left plugged it. I left it plugged in as it was.

Robert was still in there while I was doing my sweep, and he was notified that he was the last one.

 

LHO General
thomas.shaffer@LIGO.ORG - posted 10:39, Tuesday 02 September 2025 (86690)
Ops Day Shift Start

TITLE: 09/02 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
    SEI_ENV state: MAINTENANCE
    Wind: 5mph Gusts, 2mph 3min avg
    Primary useism: 0.30 μm/s
    Secondary useism: 0.13 μm/s
QUICK SUMMARY: A bit delayed of a entry, but we are in maintenance mode. We stayed locked until 1627 UTC (927PT) before we were knocked out by some maintenance activities.

H1 PSL
jason.oberling@LIGO.ORG - posted 10:26, Tuesday 02 September 2025 (86689)
PSL PMC and RefCav Remote Beam Alignment Tweaks

The FSS TPD has been slowly trending down again, so I did a quick remote adjustment of beam alignment into both the PMC and FSS RefCav today.

Starting with the PMC, I turned the ISS OFF, then adjusted the beam alignment from the Control Room using our picomotor mirrors.  Unfortunately, I did not get any improvement in either PMC Trans or PMC Refl.  PMC Refl has been very slowly increasing over the last couple of months, it may be time to take a look at adjusting the amplifier pump currents; we'll monitor this over the next week or two and move forward from there as necessary.  To end the PMC adjustments, I turned the ISS back ON.  It was diffracting ~4.2% (jumping between 4% and 4.5%), so I decreased the ISS RefSignal -1.99 V (from -1.98 V) to lower this a small bit.  The ISS diffracted power is now hanging around 3.8% (jumping between 3.6% and 4%); at this new diffracted power, PMC Trans is ~105.7 W.

Moving on to the FSS RefCav, with the IMC unlocked the TPD began at ~0.78 V.  I was able to get the TPD up to ~0.809 V, an OK improvement but not back where it was at the end of the last on-table alignment.  With the IMC locked the TPD is ~0.813 V.

LHO VE
david.barker@LIGO.ORG - posted 10:11, Tuesday 02 September 2025 (86688)
Tue CP1 Fill

Tue Sep 02 10:08:32 2025 INFO: Fill completed in 8min 29secs

Gerardo confirmed a good fill curbside.

Images attached to this report
H1 SEI
jim.warner@LIGO.ORG - posted 10:06, Tuesday 02 September 2025 (86687)
Sept 2025 wind fence inspections

No new issues found.

Images attached to this report
H1 ISC
daniel.sigg@LIGO.ORG - posted 10:01, Tuesday 02 September 2025 (86686)
Whitening chassis for ASC-AS_C and OMC-REFL_A changed

Rinse and repeat.

H1 SEI
jim.warner@LIGO.ORG - posted 16:42, Wednesday 18 June 2025 - last comment - 14:10, Tuesday 02 September 2025(85162)
St0 to St1 feedforward on HAM1 ISI today

During the commissioning window this morning, I worked on the St0 to St1 feedforward for the HAM1 ISI. This time I borrowed some code from Huyen to try the RIFF frequency domain fitting package from Nikhil. This required using matlab 2023b which seems to have a lot of computationally heavy stuff like code suggestions added so it was kind of clunky to use and I'm not sure what all of the different fitting options do, so each dof took multiple rounds of fitting to get working. I also had to add an ac-coupling high pass after the fact to the filters because they all went to 1 at 0hz. Still the results I got for HAM1 seem to work pretty well. Attached spectra are the on-off data I collected for the X,Y and Z dofs. Refs are the ff off, live traces ff on spectra. Top of each image are the asds for the ff on & off, bottom is the magnitude of the st0 l4c to st1 gs13 tf. The improvement is broad ~10x less motion from 5 hz up to ~50hz. I'm looking at the rotational dofs still, but there is less coherence there, so not as much to win.

Elenna has said this seemed to have improved chard asc, maybe she has some plots to add.

Images attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 18:19, Wednesday 18 June 2025 (85168)

There is about an order of magnitude improvement in the CHARD P error signal between 10-20 Hz as a result of these improvements, comparing the NLN spectra from three days ago versus today. Fewer noisy peaks are also present in INP1 P. I included the CHARD P coherence with GS13s, focusing on the three DoFs with the most coherence: RX, RZ, and Z. The improvements Jim made greatly reduced that coherence. To achieve the CHARD P shot noise floor at 10 Hz and above, there is still some coherence of CHARD P with GS13 Z that is likely contributing noise. However, for the IFO, this is sufficient noise reduction to ensure that CHARD P is not directly limiting DARM above 10 Hz. I also compare the CHARD P coherence with OMC DCPD sum from a few days ago to today, see plot.

In terms of how this compares with our passive stack + L4C feedforward performance, I found some old templates where I compared upgrades to our HAM1 feedforward. I compare our ISI performance now with the passive stack, no L4C feedforward to ASC, and passive stack with the best-performance feedforward we achieved: the results. It's actually a pretty impressive difference! (Not related to the ISI seems to be a change in the shot noise floor- looks like the power on the REFL WFS may have changed from the vent.)

The coupling of CHARD P to DARM appears to be largely unchanged, so this generally means we are injecting about 10x less noise from CHARD into DARM. from 10-30 Hz.

Images attached to this comment
elenna.capote@LIGO.ORG - 14:10, Tuesday 02 September 2025 (86695)

Using the calibration factors I report in this alog, here is the CHARD plot roughly calibrated into radians.

Images attached to this comment
Displaying reports 1-20 of 84233.Go to page 1 2 3 4 5 6 7 8 9 10 End