Displaying reports 7461-7480 of 88158.Go to page Start 370 371 372 373 374 375 376 377 378 End
Reports until 14:45, Thursday 27 February 2025
H1 ISC
thomas.shaffer@LIGO.ORG - posted 14:45, Thursday 27 February 2025 - last comment - 15:24, Thursday 27 February 2025(83089)
Ran A2L script again

We ran the a2l_min_multi_pretty.py script again today since we made changes to the OMC offsets (alog83087). There were minimal gain changes, the only one I updated in lscparams.py was ETMY P from 5.49 -> 5.52.

The range coherence template we normally use was giving odd results during the quiet commissioning times after the OMC reverting, no coherence above 20Hz is seen. Sheila mentions that this is something she has seen before and isn't physical. We ran the script expecting changes but didn't see much change in gains or to the range.

RESULTS

|      |   | Initial | Final |  Diff |
| ETMX | P |   3.23  |  3.24 |  0.01 |
| ETMX | Y |    4.9  |   4.9 |   0.0 |
| ETMY | P |   5.49  |  5.52 |  0.03 |
| ETMY | Y |   1.35  |  1.34 | -0.01 |
| ITMX | P |  -0.53  | -0.54 | -0.01 |
| ITMX | Y |   3.21  |  3.22 |  0.01 |
| ITMY | P |   0.06  |  0.05 | -0.01 |
| ITMY | Y |  -2.74  | -2.75 | -0.01 |
 

Images attached to this report
Comments related to this report
thomas.shaffer@LIGO.ORG - 15:24, Thursday 27 February 2025 (83096)

Matt reminded me that I need to run diaggui_test with the range coherence template, so when I range it the correct way, we can see that the a2l script didn't change much or maybe even made it slightly worse. In the attached screenshot the left is before a2l was run, the right is after.

Images attached to this comment
H1 ISC (OpsInfo)
thomas.shaffer@LIGO.ORG - posted 14:41, Thursday 27 February 2025 (83092)
SRC2 P gain brought down to 40

We've been having some issues with SRC2 P starting to go unstable after engaging for DRMI (alog83080, alog82997). Ryan C tested out lower the gain from 60 -> 40 on Sheila's suggestion yesterday and it seemed to work (alog83078), and I also bashed it in during a relock today that started to go unstable. Since this seems to work and the gain is brought back to 60 later in ENGAGE_ASC_FOR_FULL_IFO, we've made the change in ISC_DRMI and loaded the guardian.

H1 SUS (SEI, SUS)
joshua.freed@LIGO.ORG - posted 14:09, Thursday 27 February 2025 (83090)
ETMY BOSEM Noise Injections

J. Freed

ETMY shows strong coupling of BOSEM noise between 9-14Hz by about a factor of 20 below DARM from most sensors.

Today I did damping loop injections on all 6 BOSEMs on the ETMY M0. This is a continuation of the work done previously for ITMX, ITMY, PR2, PR3, PRM, SR2, SR3, SRM, and ETMX. As with PRM, gains of 300 and 600 were collected for SR3 (300 is labled as ln or L).  Calibration lines were off. Data was colected in two parts, as such, f1,f2,f3 had a different background than lf,rt,sd bosems.

The plots, code, and flagged frequencies are located at /ligo/home/joshua.freed/bosem/ETMY/scripts. While the diaggui files are at /ligo/home/joshua.freed/bosem/ETMY/data and data2. I used Sheila code located under /ligo/home/joshua.freed/bosem/ETMY/scripts/osem_budgeting.py to produce the sum of all contributions as well as the individual plots.
 
main.png Shows the current noise plot for most of the suspensions done excluding ITMX, ITMY, and PR2.
 
ETMY1.png Shows the estimated contributions to DARM from the F1, F2, F3 bosems only using the 600 gain data
 
ETMY1.png Shows the estimated contributions to DARM from the LF, RT, SD bosems only using the 600 gain data. They show super strong coupling around the bounce mode but need to check the correlation between the incresed bounce mode and my measurments. This is why I collect the 300 gain data.
 
reference number in diaggui files for ETMY in data 1
Background time: (ref0 DARM, ref1 F1_out, ref2 F2_out, ref3 F3_out, ref4 LF_out, ref5 RT_out, ref6 SD_out)
F1L time:                (ref7 DARM, ref8 F1_out)
F1 time:                  (ref9 DARM, ref10 F1_out)
F2L time:               (ref11 DARM, ref12 F2_out)
F2 time:                 (ref13 DARM, ref14 F2_out)
F3L time:              (ref15 DARM, ref16 F3_out)
F3 time:                (ref17 DARM, ref18 F3_out)
 
reference number in diaggui files for ETMY in data 2
Background time: (ref0 DARM, ref1 F1_out, ref2 F2_out, ref3 F3_out, ref4 LF_out, ref5 RT_out, ref6 SD_out)
LFL time:                (ref7 DARM, ref8 F1_out)
LF time:                  (ref9 DARM, ref10 F1_out)
RTL time:               (ref11 DARM, ref12 F2_out)
RT time:                 (ref13 DARM, ref14 F2_out)
SDL time:              (ref15 DARM, ref16 F3_out)
SD time:                (ref17 DARM, ref18 F3_out)
 
Images attached to this report
H1 ISC
jennifer.wright@LIGO.ORG - posted 11:00, Thursday 27 February 2025 (83087)
Reverted OMC ASC QPD offsets

Jennie W, Sheila

Since our range has been decreasing over the last week and the OMC QPD offsets did not definitely give us a clear gain long term in kappa C, we have reverted the change we did on Monday.

We might want to improve these offsets again once we sort out any other problems that are making larger impacts on our range currently.

See the below ndscope for how this affected the range and optical gain in the short term - this picture is slightly confusing as the calibration was being updated so kappa C will have been reset at the some point before or during our measurements.

The other two attached images show the QPD offsets being accepted in OBSERVE and SAFE snap files.

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:15, Thursday 27 February 2025 - last comment - 10:39, Thursday 27 February 2025(83084)
Thu CP1 Fill

Thu Feb 27 10:05:41 2025 INFO: Fill completed in 5min 38secs

For this fill I tested that the rate-of-change trip value can be changed in the configuration yaml file and then loaded into the code. For this test it was reduced from 60.0 to 50.0 DEGC.

The code which generates the plot now dynamically reads the trip PV to set the horizontal bar.

It looks like we tripped on a TC-A sputter just before the LN2 got flowing, but looks like a good fill.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 10:21, Thursday 27 February 2025 (83085)

The code currently stops updating the ROC channels at the time the fill is terminated. These channels are then zeroed at the start of the next fill. This is the reason the lower panel in the plot has bars behind the legend from yesterday's fill, and that these channels flat line from the end time onwards.

I'll work on a code change to continue calculating the ROC for a period of time after the fill ends.

david.barker@LIGO.ORG - 10:39, Thursday 27 February 2025 (83086)

New code has been loaded which continues with ROC calcs for 10 minutes post fill. I will test this during tomorrow's fill.

H1 General (Lockloss)
oli.patane@LIGO.ORG - posted 08:42, Thursday 27 February 2025 (83082)
Lockloss

Lockloss @ 2025-02-27 16:36 UTC during commissioning after 22 minutes locked. People had just entered the LVEA.

H1 CDS
david.barker@LIGO.ORG - posted 08:28, Thursday 27 February 2025 (83081)
Running local NDS version of DARM FOM diaggui

Oli, Jonathan, Dave:

The DARM FOM in the control room (running on nuc30) stopped updating and could not be restarted. Jonathan tracked it down to an ongoing NDS2 issue which will hopefully be resolved soon. In the meantime I started the "local" version of this fom which only uses the local NDS and does not try to connect to NDS2.

I'm running the diaggui by hand from a terminal as controls on nuc30, it was started with:

cd /opt/rtcds/userapps/release/cds/h1/scripts/fom_startup/nuc30

diaggui --fom ./H1_DARM_FOM_cds.xml

H1 General
oli.patane@LIGO.ORG - posted 07:33, Thursday 27 February 2025 - last comment - 08:05, Thursday 27 February 2025(83079)
Ops Day Shift Start

TITLE: 02/27 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: USEISM
    Wind: 3mph Gusts, 2mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.72 μm/s
QUICK SUMMARY:

Currently relocking and at CARM_TO_TR

Comments related to this report
oli.patane@LIGO.ORG - 08:05, Thursday 27 February 2025 (83080)ISC

So last night Ryan adjusted the SRC2 P gain down from 60 to 40 during DARM_LOCKED_CHECK_ASC in order to try and stop the oscillations, and it worked (83074),. That value though of course was just a test and wasn't changed in the code, so I would have expected the next times passing through those states for it to have the oscillations again, but it hasn't. In the three times we've passed through DARM ASC-ville since then, with the SRC2 P gain at its original value of 60, that hasn't happened.

H1 General
ryan.crouch@LIGO.ORG - posted 22:00, Wednesday 26 February 2025 (83074)
OPS Wednesday EVE shift summary

TITLE: 02/27 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: TJ
SHIFT SUMMARY: 1 lockloss and we're on our way back past the troublesome CHECK_ASC now. I had to reduce the gain of SRC2_p from 60 to 40. We're about to start powering up now.
LOG: No log.

H1 ISC (IOO, PSL)
mayank.chaturvedi@LIGO.ORG - posted 19:09, Wednesday 26 February 2025 - last comment - 14:40, Monday 03 March 2025(83077)
Opened a new ISS PD array

Jennie Siva Keita Mayank

Following our previous attempt  here .  We opened a new ISS PD array (S.N. 1202965).
This unit is in great condition. i.e. 

1) No sign of contamination.
2) All the optics are intact (No chipping)

We tried interfacing the QPD-cable S1203257 with the QPD but it turned out that they are not compatible.
We will look for the updated version of the QPD cable.   

Images attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 14:49, Thursday 27 February 2025 (83091)EPO

More photos I took of the unboxed unit,

Keita holding part of QPD connector that connects to cable,

zoom in of part of prisms close to PD array to show they don't look damaged like the previous one we unboxed,

dcc and serial number of baseplate (this is different part for each observatory due to differing beam heights).

Keita explaining the QPD cable clamp to Shiva (right) and Mayank (left).

View of optics with periscope upper mirror on the left.

View of part of prisms close to periscope.

View of back of array and strain relief.

plus a picture of an packaged coptic that was sitting on top of this capsule while it was in the storage cupboard.

 

Images attached to this comment
jennifer.wright@LIGO.ORG - 16:02, Thursday 27 February 2025 (83099)

For future reference all the ISS arrays and there serial numbers are listed in the dcc entry for the assembly drawing LIGO-D1101059-v5.

matthewrichard.todd@LIGO.ORG - 14:40, Monday 03 March 2025 (83143)

[Matthew Mayank Siva Keita]

On Friday (2025-02-28) we moved the optics onto taller posts so that we did not have to pitch the beam up to much (in hind-sight, we probably would've been okay doing this) when we align the beam into the input port of the ISS array. We have not aligned the beam yet and most likely should re-profile it(may not need to) to ensure that the planned lens position is correct.

We also spent some time checking the electronics box for proper connections and polarity; then we tested the upper row of PDs (4 top ones) by plugging in each cathode/anode to the respective port. The output DSUB we used a breakout board and threw each channel onto an oscilloscope -- it seems that all four of the top row of PDs are functioning as anticipated.


Important Note:

Keita and I looked at the "blue glass" plates that serve as beam dumps, but just looking at the ISS array we do not know how to mount them properly. We think there may be some component missing that clamps them to the array. So we repackaged the blue-glass in its excessive lens paper.

Images attached to this comment
H1 General (Lockloss)
ryan.crouch@LIGO.ORG - posted 18:46, Wednesday 26 February 2025 - last comment - 19:47, Wednesday 26 February 2025(83076)
02:44 UTC lockloss

02:44 UTC lockloss

Comments related to this report
ryan.crouch@LIGO.ORG - 19:47, Wednesday 26 February 2025 (83078)ISC

I stopped at CHECK_ASC and reduced the gain of SRC2P from 60 to 40 and we were able to stay locked as the oscillation came and went, I ran the olg measurement. After the measurement I tried to reduce the gain down to 30 but I fat fingered it and made it bigger and we lost lock.

Images attached to this comment
X1 SUS
ibrahim.abouelfettouh@LIGO.ORG - posted 18:16, Wednesday 26 February 2025 (83075)
BBSS Transfer Functions Measurement and Model Comparisons

Ibrahim, Oli

Attached are the most recent BBSS Model Comparisons with most recent BBSS parameter settings (+/- from FDR):

d0=+3.0mm

l1 = -3.0mm

m2 = +0.3kg

FDR, d1 = +3.5mm (which is equivalent to BP = -4mm)

Non-image files attached to this report
H1 General
oli.patane@LIGO.ORG - posted 16:38, Wednesday 26 February 2025 (83072)
Ops Day Shift End

TITLE: 02/27 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 145Mpc
INCOMING OPERATOR: Ryan C
SHIFT SUMMARY:
LOG:

15:30UTC Relocking
    - ISC_LOCK in PREP_FOR_LOCKING; H1_MANAGER had gone into error less than a minute before (15:29 UTC)
    - I ran an initial alignment
    - We got those saturations again during OFFLOAD_DRMI_ASC (ndscope)
    - Lockloss during LOWNOISE_ESD_ETMX due to earthquake coming in
    - Holding in DOWN until earth settles
    - Started another initial alignment
    - Another set of saturations during OFFLOAD_DRMI_ASC - this time we lost lock from them (ndscope2)
    - Saturations again but got through them this time
18:15 NOMINAL_LOW_NOISE
18:20 Observing

21:16 Commissioning to adjust A2L and PRCL FF

21:51 Back to Observing
22:48 Superevent S250226dl
00:13 Superevent S250227e                                                                                                                                                                                                                                                                                                                                               

Start Time System Name Location Lazer_Haz Task Time End
16:13 FAC Nellie OpticsLab n Tech clean 16:28
16:19 FAC Tyler MX, MY n 3IFO 18:19
17:20 FAC Kim MY, MX n Tech clean 20:47
17:29 VAC Janos EY N Parts Inventory 17:44
20:40 FIT Matt XARM n Runnin 21:31
22:49 OPT Jennie, Keita, Siva, Mayank OpticsLab n Unwrapping class A parts (Jennie out 00:10) 00:36
Images attached to this report
H1 General
ryan.crouch@LIGO.ORG - posted 16:38, Wednesday 26 February 2025 (83073)
OPS Wednesday EVE shift start

TITLE: 02/27 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 143Mpc
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 11mph Gusts, 6mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.43 μm/s
QUICK SUMMARY:

H1 SQZ
camilla.compton@LIGO.ORG - posted 15:55, Tuesday 25 February 2025 - last comment - 16:14, Wednesday 26 February 2025(83039)
Seconds take at SQZ Homodyne Measurements

Sheila, Matt, Camilla

We aligned and took some SQZ HD data this morning but realized that the ZM optics were noisy with HAM7 tripped and the increased (60mph!! wind). After un-tripping HAM7, Matt and Sheila rechecked balancing and visibility, started at 98.3% but noisy, improved to 99.0%. Since then HAM7 tripped and was un-tripped again but assumed nothing would have changed.

NLG Measurements:

opo_grTrans_ setpoint_uW Amplified Max Amplified Min UnAmp Dark NLG (usual)
120 0.108354 0.000573291 0.0018491 6.6e-5 60
110 0.0656167 0.000599855     36.8
100 0.0413918 0.00062871     23.2
80 0.0209032 0.000681607     11.7
60 0.0121804 0.000745147 0.0018428 6.2e-5 6.8
40 0.00710217 0.000852173     3.98

Data saved to camilla.compton/Documents/sqz/templates/dtt/20250225_GOOD_HD.xml

FC2 is misaligned during this dataset.

Type NLG SQZ dB  @ 1kHz Angle DTT Ref Notes
Dark Noise N/A   N/A ref 0 This and shot noise was noisy <300Hz at times when the OPO was locking or scanning, unsure why.
Shot Noise N/A   N/A ref 10
Blocked SEED, LO only.
SQZ 60 -7.4 167 ref1 opo_grTrans_setpoint_uW = 120uW, OPO gain -14
ASQZ 60 22.6 225 ref2  
MSQZ 60 19.6 N/A ref3  
SQZ 37 -7.3 164 ref4 opo_grTrans_setpoint_uW = 110uW
ASQZ 37 20.2 229 ref5  
MSQZ 37 17.2 N/A ref6  
SQZ 23 -7.4 161 ref7 opo_grTrans_setpoint_uW = 100uW
ASQZ 23 18.0 233 ref8  
MSQZ 23 15.0 N/A ref9  
SQZ 12 -7.3 151 ref11 opo_grTrans_setpoint_uW = 80uW, OPO gain -8
ASQZ 12 14.5 246 ref12  
MSQZ 12 11.7 N/A ref13  
SQZ 7 -7.0 143 ref14 opo_grTrans_setpoint_uW = 60uW
ASQZ 7 11.7 253 ref15  
MSQZ 7 8.7 N/A ref16  
SQZ 4 -5.9 132 ref17 opo_grTrans_setpoint_uW = 40uW
ASQZ 4 8.9 (-)85 ref18  
MSQZ 4 6.0 N/A ref19  
Comments related to this report
matthewrichard.todd@LIGO.ORG - 18:00, Tuesday 25 February 2025 (83054)

I'm also attaching pictures of SR785 measurements of various loop gains.

Measurement Time Notes
LO OLG 11:28 2.5kHz UGF
OPO OLG 12:06 PST -8dB gain OPO loop gain
OPO OLG 12:09 PST -14 dB on OPO loop gain
CLF OLG 12:10 PST 13.kHz UGF

 

Images attached to this comment
sheila.dwyer@LIGO.ORG - 16:14, Wednesday 26 February 2025 (83070)

This data set is nicely fit by standard squeezing equations, and suggests we have 6% unexplained losses and very little phase noise.

In the attached PDF I took the median of the ASD from 500-700 Hz, subtracted dark noise in quadrature from each ASD, then calculated the dB relative to shot noise for squeezing, anti-squeezing and mean squeeze.  I used the squeezing and anti-squeezing and opo transmission numbers to fit for the OPO threshold (in units of transmitted power), total efficiency of squeezing, and phase noise.  The attached plot shows the resulting model plotted against the data, including mean squeezing and NLG measurements that were not used for fitting.  The NLG plot does suggest that we are slightly underestimating our NLG with our measurements. 

This suggests that the OPO threshold is at 156uW transmitted power, and that the totall efficiency is 83%.  This can be compared to 73365 and to the expected losses from the loss tracking sheet and sqz wiki.  Expected losses:

opo escape efficiency 0.985  
3 SFI passes (0.99)^3 = 0.97  
B:BS1 0.9897 HAM7 total = 0.946
SQZT7 0.98  
visibilty 0.99^2  
homodyne QE 0.977  
total expected in homodyne   0.887

With the measured efficiency of 0.833, this means we have 6% unexplained losses in HAM7 or SQZT7. 

Non-image files attached to this comment
H1 CAL (CAL)
joseph.betzwieser@LIGO.ORG - posted 12:31, Thursday 20 February 2025 - last comment - 10:15, Thursday 27 February 2025(82935)
Calibration debugging
[Vlad, Louis, Jeff, Joe B]
So while exercising the latest pydarm code with an eye towards correcting the issues noted in LHO alog 82804, we ran into a few issues which we are still trying to resolve.

First, Vlad was able to recover all but the last data point from the simulines run on Feb 15th, which lost lock at the very end of the sweeps.  See his LHO alog 82904 on that process.

I updated the pydarm_H1.ini file to account for the current drive align gains and point at the current L1SUSETMX foton file (saved in the calibration svn as /ligo/svncommon/CalSVN/aligocalibration/trunk/Common/H1CalFilterArchive/h1susetmx/H1SUSETMX_1421694933.txt ).  However, I had to also merge some changes for it submitted from offsite.  Specifically https://git.ligo.org/Calibration/ifo/H1/-/commit/05c153b1f8dc7234ec4d710bd23eed425cfe4d95, which is associated with MR 10 which was intended to add some improvements to the FIR filter generation.

Next, Louis updated the pydarm install at LHO from tag 20240821.0 to tag 202502220.0.

We then generated the report and associated GDS FIR filters.  This is /ligo/groups/cal/H1/reports/20250215T193653Z.  The report and fits to the sweeps looked reasonable, however, the FIR generation did not look good.  The combination of the newly updated pydarm and ini changes was producing some nonsensical filter fits.  This is the first attachment.

We reverted the .ini file changes, and this helped to recover more expected GDS filters, however, there's still a bit of a small ~1% change visible around 10 Hz (instead of being a flat 1.0 ratio) in the filter response using the new pydarm tag versus the old pydarm tag which we don't understand quite yet, and would like to before updating the calibration.  I'm hoping we can do this in the next day or two after going through the code changes between the versions.

Given the measured ~6 Hz SRC detuning spring frequency (as seen in the reports), we will need to include that effect in the calcs front end to eliminate a non-trivial error when we do get around to updating the calibration.  I created a quick plot based off the 20250215T193653Z measured parameters, comparing the full model over a model without the SRC detuning included.  This is the attached New_over_nosrc.png image.
Images attached to this report
Non-image files attached to this report
Comments related to this report
joseph.betzwieser@LIGO.ORG - 10:15, Thursday 27 February 2025 (83083)
The slight difference we were seeing in old report GDS filters vs new report GDS filters was actually due to a mcmc fitting change.  We had changed the pydarm_cmd_H1.yaml to fit down to 10 or 15 Hz instead 40 Hz, which means it is in fact properly fitting the SRC detuning, which in turn means the model the FIR filter generation is correcting has changed significantly at low frequencies.

We have decided to use the FIR filter fitting configuration settings we've been using for the entire run for the planned export today.

Louis has pushed to LHO a pydarm code which we expect will properly install the SRC detuning into the h1calcs model.

I attach a text file of the diff of the FIR filter fitting configuration settings for the pydarm_H1.ini file between Aaron's new proposal (which seems to work better for DCS offline filters based only looking at ~6 reports) and the one's we've been using this run so far to fit the GDS online filters.

The report we are proposing to push today is: 20250222T193656Z





Non-image files attached to this comment
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