Displaying reports 2261-2280 of 77273.Go to page Start 110 111 112 113 114 115 116 117 118 End
Reports until 13:39, Thursday 18 April 2024
H1 SQZ
naoki.aritomi@LIGO.ORG - posted 13:39, Thursday 18 April 2024 (77268)
PSAMS revert

Naoki, Camilla

We reverted PSAMS from 7.5/0.55 to 8.8/-0.67, which was done last Friday in 77133. Before and after PSAMS change, we ran SCAN_ALIGNMENT and took 5+5 min asqz/sqz data. The attached figure shows that 8.8/-0.67 is better than 7.5/0.55. In parallel, A2L tuning was ongoing so the noise below 100 Hz in SQZ should be due to A2L.

asqz 120/137 (strain voltage 7.5/0.55) (5 min)

PDT: 2024-04-18 10:59:48 PDT
UTC: 2024-04-18 17:59:48 UTC
GPS: 1397498406

sqz 120/137 (strain voltage 7.5/0.55) (5 min)

PDT: 2024-04-18 11:06:29 PDT
UTC: 2024-04-18 18:06:29 UTC
GPS: 1397498807

asqz 170/95 (strain voltage 8.8/-0.67) (5 min)

PDT: 2024-04-18 12:01:57 PDT
UTC: 2024-04-18 19:01:57 UTC
GPS: 1397502135

sqz 170/95 (strain voltage 8.8/-0.67) (5 min)

PDT: 2024-04-18 13:35:01 PDT
UTC: 2024-04-18 20:35:01 UTC
GPS: 1397507719

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:16, Thursday 18 April 2024 (77267)
Thu CP1 Fill

Thu Apr 18 10:06:27 2024 INFO: Fill completed in 6min 23secs

Jordan confirmed a good fill curbside.

Images attached to this report
H1 General
corey.gray@LIGO.ORG - posted 08:12, Thursday 18 April 2024 (77264)
Thurs DAY Ops Transition

TITLE: 04/18 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 117Mpc
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 7mph Gusts, 6mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.10 μm/s
QUICK SUMMARY:

H1's had range hovering between 150-155Mpc 24hrs ago.  After the EQs last night, H1 made it back UP. but seems a bit off with a range down near 110Mpc.  Sheila has just walked in and mentioned Commissioning time is planned from 8-11am this morning and she is jumping in on that---so we are out of OBSERVING.  Heard Sheila mentioned angular coupling and tried No Squeezing and is now looking at A2L (but we are at the very beginning of investigations and commissioning). 

The togglingof No Squeezing to Freq Dep Squeezing helped with the range already.  And Sheila is currently running an A2L.  And it looks like L1 is also joining us with commissioning.

H1 SUS
anthony.sanchez@LIGO.ORG - posted 02:54, Thursday 18 April 2024 (77263)
SUS SDF Diffs Accepted

I accepted these P2L spot gain SDF Diffs to get into Observing.

Images attached to this report
H1 DetChar (DetChar)
manasadevi.thirugnanasambandam@LIGO.ORG - posted 02:41, Thursday 18 April 2024 (77262)
DQ shift report for week from 2024-04-08 to 2024-04-14

Summary highlights of DQ shift the week from 2024-04-08 to 2024-04-14

Full DQ shift report with daily observations can be found in the wiki page here: https://wiki.ligo.org/DetChar/DataQuality/DQShiftLHO20240408

 

H1 SEI
anthony.sanchez@LIGO.ORG - posted 01:04, Thursday 18 April 2024 (77261)
Owl Shift update.

TITLE: 04/18 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Aligning
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
    SEI_ENV state: USEISM_EARTHQUAKE
    Wind: 3mph Gusts, 1mph 5min avg
    Primary useism: 0.97 μm/s
    Secondary useism: 1.28 μm/s
QUICK SUMMARY:

Starting the Shift Oli and I noticed that the IFO was still relocking and needed an initial_alignment.
Since then Initial_alignment had stalled and been restarted. Possibly because the IMC was unlocked. I'm usure if Oli had done that or not.

Once that completed Another earthquake hit but was not announced over verbals.
M 5.3 - 60 km WSW of Pozo Dulce, Mexico 2024-04-18 07:39:45 (UTC)26.546°N 110.267°W10.0 km depth
So I'm just waiting on the earthquake to pass.

H1 General
oli.patane@LIGO.ORG - posted 00:10, Thursday 18 April 2024 (77260)
Ops EVE Shift End

TITLE: 04/18 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Tony
SHIFT SUMMARY: Quiet night most of the night, but had a local earthquake knock us out close to the end of my shift. Currently running an initial alignment with the help of H1 MANAGER running an initial alignment and Tony watching H1 MANAGER run the initial alignment to make sure H1 MANAGER gets us locking once that's done.
LOG:

23:00 Detector Observing and Locked for over 15 hours

06:08 Earthquake mode activated
06:11 Lockloss due to local earthquake
    - ALS flashed were really low and took a while to get up
07:03 Started an Initial Alignment

 

H1 General (Lockloss)
oli.patane@LIGO.ORG - posted 23:12, Wednesday 17 April 2024 (77259)
Lockloss

Lockloss 04/18 06:11UTC due to local earthquake :( We were locked for 22.5 hours

H1 General
oli.patane@LIGO.ORG - posted 20:45, Wednesday 17 April 2024 (77258)
Ops Eve Midshift Status

Observing at 155Mpc and locked for 20 hours exactly. Calm evening with low wind

H1 SQZ (ISC, SQZ)
jennifer.wright@LIGO.ORG - posted 17:12, Wednesday 17 April 2024 - last comment - 20:43, Monday 06 May 2024(77213)
OMC Scan with SQZ beam yesterday

Naoki, Vicky, Jennie W

 

Naoki followed the directions in to set up the SQZ beam OMC scan.

We had a problem with the DC centering loops. After we switched them on they saturated the OM1 and OM2 suspensions.

We got around this by switching each of the 4 degrees of freedom on first - ie. DC3 Y, DC3 P, DC4 Y, DC4 P.

Then we engaged OMC ASC and this seemed to work ok.

When we tried to manually lock the OMC length loop we had problems as when we switched the gain of 1 on it would lose lock, even when on a TM00 mode of the expected height (0.6mA on DCPD_SUM).

Vicky got around this this using a lower gain and not engaging the BOOST filter in the servo filter bank.

Then she had to touch up the alignment in lock with OM3.

locked quiet time 1397329970 GPS 1 min:

OMC-REFL_A_LF_OUT16 = 0.0930255 mW

OMC-DCPD_SUM_OUTPUT = 0.652156 mA

 

unlocked quiet time 1397330106 GPS 1 minute:

OMC-REFL_A_LF_OUT16  = 1.04825 mW

OMC-DCPD_SUM_OUTPUT = -0.00133668 mA

 

dark measurement 1397330625 GPS 1 minute:

OMC-REFL_A_LF_OUT16  = -0.0133655 mW

OMC-DCPD_SUM_OUTPUT = -0.00133668 mA

 

I noticed after I took the dark measurement that OM1 and 2 were staurating again and need to clear history twice on OM1 to remove this.

Reverted OM1 and 2, 3 OMC sliders at 8:33 am (local time) on the 16th April.

Data is saved as REf 3, 4 and 5 in /ligo/home/jennifer.wright/Documents/OMC_scan/2024_04_16_OMC_scan.xml. Where 3 is the scan channel OMC-DCPD_SUM_OUT_DQ on the bottom right plot, 4 is the PZT excitation channel OMC-PZT2_EXC on the bottom left plot, and 5 is the monitor of the actual PZT output voltage OMC-PZT2_MON_DC_OUT_DQ on the top right plot.

Images attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 20:43, Monday 06 May 2024 (77672)

Using Sheila's code from this entry and updating the code with the current OMC values for transmission of the mirrors:

Tio = 7670e-6 #according to T1500060 page 116 input and output mirror transmission

R_inBS = 1-7400e-6

The outout of the code gives us the following values for the cavity incident power, efficiency and finesse:

Power on refl diode when cavity is off resonance: 1.062 mW

Incident power on OMC breadboard (before QPD pickoff): 1.078 mW

Power on refl diode on resonance: 0.106 mW

Measured effiency (DCPD current/responsivity if QE=1)/ incident power on OMC breadboard: 70.5 %

assumed QE: 100 %

power in transmission (for this QE) 0.760 mW

HOM content infered: 8.748 %

Cavity transmission infered: 77.827 %

predicted efficiency () (R_inputBS * mode_matching * cavity_transmission * QE): 70.493 %

omc efficency for 00 mode (including pick off BS, cavity transmission, and QE): 77.251 %

round trip loss: 2063 (ppm)

Finesse: 362.923

 

I need to compare the HOM content measurement with that derived from the mode scan.

H1 TCS
camilla.compton@LIGO.ORG - posted 16:29, Wednesday 17 April 2024 (77255)
CO2Y and CO2X Beam Scan

TJ, Camilla. WP 11811

Yesterday, we repeated the  76715 CO2 beam scan using a razor blade on a 25mm transition stage while measuring the power transmitted to our PD (channel H1:TCS-ITMX/Y_CO2_LSRPWR_MTR_OUTPUT).

We realized that some of the blocked beam was transmitted through a hole in the razor blade in our first set of measurements (changed radius measurement ~1mm) so the CO2X 76715  are not as trusted. 

All data taken for CO2X and CO2Y attached and summarized below:

Position Downstream of CO2Y Annular Mask [mm]
Downstream = (+), Upstream = (-)
Beam Raduis [mm] Prev. measured with hole in razor 
- 238 11.39 12.34
0 N/A 11.27 (think hole was covered)
+143 10.77 11.17
+194 10.61 11.39
Position Downstream of CO2X Annular Mask [mm]
Downstream = (+), Upstream = (-)
Beam Raduis [mm]
+ 32 9.85
+ 133 10.01
+184 10.49
Non-image files attached to this report
LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 16:00, Wednesday 17 April 2024 (77256)
OPS Day Shift Summary

TITLE: 04/17 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 126Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY:

IFO is in NLN and OBSERVING

Comissioning today went well. We survived a few high magntitude earthquakes.
 

LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:14 FAC Karen Optics, Vac Prep Labs N Technical Cleaning 15:43
15:43 FAC Ken FC Enclosure N Electrical maintenance 16:43
15:44 FAC Karen MY N Technical Cleaning 16:44
17:17 FAC Fil CS Recieving Door N Roll up recieving door 18:17
21:16 SQZ Andrei, Sheila Optics Lab N Tour 22:16
H1 General
oli.patane@LIGO.ORG - posted 16:00, Wednesday 17 April 2024 (77257)
Ops EVE Shift Start

TITLE: 04/17 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 146Mpc
OUTGOING OPERATOR: Ibrahim
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 16mph Gusts, 12mph 5min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.10 μm/s
QUICK SUMMARY:

We're Observing and have been Locked for over 15 hours.

H1 ISC (SEI)
jim.warner@LIGO.ORG - posted 14:34, Wednesday 17 April 2024 - last comment - 12:27, Thursday 18 April 2024(77254)
New HAM1 FF

Jennie, Jim

We tried Gabriele's newest version of the HAM1 ASC feedforward. New filters were installed last week, but we ran out of time during the commissioning window. It seems like we can still only get good subtraction from the pitch degrees of freedom, we got a lot of 10-ish hz injection when we engaged the yaw degrees of freedom.

To start we turned off the HAM1 ff, by setting H1:HPI-HAM1_TTL4C_FF_INF_{RX,RY,Z,X)}_GAIN to zero, then shutting off the H1:HPI-HAM1_TTL4C_FF_OUTSW. While collecting that data we switched to the new filters, and zerod the gains for all of the individual H1:HPI-HAM1_TTL4C_FF_CART2ASC{P,Y}_{DOF}_{DOF}_GAIN filter banks.  We then tried turning on all of the pitch feedforward first, by ramping the gains in a couple of steps from 0 to 1. It seemed like it worked well, but I don't think we actually got to full gain of 1. We then tried turning on the yaw FF, but that pretty quickly started injecting noise around 10hz, first attached spectra, red traces are with the new ff, blue are with ff off.

Second image are trends where Jennie tries to reconstruct the timeline, which is how we found the first pitch test wasn't complete. Sheila ran an A2L measurement, then we tried the pitch ff again, spectra in the third plot. All of the red traces are new P ff (1397415884), blue is the old (1397407980), green is with the ff off (1397405754).  This worked well, we got some slight improvements around 15hz, new chard p gets rid of some noise injection around 2hz. We didn't see the pitch ff affect the yaw dofs.

We left the new pitch filters running, and accepted in the Observe SDF. The yaw filters were left off.

Images attached to this report
Comments related to this report
gabriele.vajente@LIGO.ORG - 12:27, Thursday 18 April 2024 (77271)

I looked at the attempt of engaging the HAM1 yaw FF:
1) the filter that were loaded were correct, meaning they were what I expected
2) retraining with a time when the HAM1 pitch FF were on yields yaw filters that are similar to what was tried, so it doesn't look like it's a pitch / yaw interaction (Jennie also pointed to some evidence of this in the alog)

I suspect there might be cross coupling between the various yaw dofs. I would suggest that we upload the newly trained filters (attached) and try to engage the yaw FF one by one, starting from CHARD that is the one we care most

Images attached to this comment
Non-image files attached to this comment
H1 TCS (TCS)
ibrahim.abouelfettouh@LIGO.ORG - posted 13:09, Wednesday 17 April 2024 (77253)
TCS Chiller Water Level Top-Off (Bi-Weekly, FAMIS #27787)

 TCS Chiller Water Level Top-Off (Bi-Weekly, FAMIS #27787)

Closes FAMIS 27787

H1 ISC
sheila.dwyer@LIGO.ORG - posted 13:06, Wednesday 17 April 2024 (77252)
PRCL exctitation

We wanted to check the PRCL offset during our commissoning time this morning, we ended up not having much time for that but did re-run Elenna's template from 76814.  It looks like the PRCL to REFL RIN transfer function is much the same as at that time.  It seems as though there was a change in the PRCL to DARM transfer function, but that measurement has low coherence at most frequencies.

Images attached to this report
H1 INJ
thomas.shaffer@LIGO.ORG - posted 12:59, Wednesday 17 April 2024 (77248)
Stochastic injection ran with LLO

Joe B from LLO and I ran the short and long stochastic injections with the commands below starting at 19:08UTC. Both ran successfully, back to Observing at 1955UTC

 

 

hwinj stochastic short --time 1397416098  --run

ifo: H1
waveform root: /ligo/groups/cal/H1/hwinj
config file: /ligo/groups/cal/H1/hwinj/hwinj.yaml
GraceDB url: https://gracedb.ligo.org/api/
GraceDB group: Detchar
GraceDB pipeline: HardwareInjection
excitation channel: H1:CAL-INJ_TRANSIENT_EXC
injection group: stochastic
injection name: short
reading waveform file...
injection waveform file: /ligo/groups/cal/H1/hwinj/stochastic/SB_ER15HLShort_H1.txt
injection waveform sample rate: 16384
injection waveform length: 780.0 seconds

injection start GPS: 1397416098.0

 

 

 

 

hwinj stochastic long --time 1397417118 --run


ifo: H1
waveform root: /ligo/groups/cal/H1/hwinj
config file: /ligo/groups/cal/H1/hwinj/hwinj.yaml
GraceDB url: https://gracedb.ligo.org/api/
GraceDB group: Detchar
GraceDB pipeline: HardwareInjection
excitation channel: H1:CAL-INJ_TRANSIENT_EXC
injection group: stochastic
injection name: long
reading waveform file...
injection waveform file: /ligo/groups/cal/H1/hwinj/stochastic/SB_ER15HLLong_H1.txt
injection waveform sample rate: 16384
injection waveform length: 1800.0 seconds
injection start GPS: 1397417118.0

 

LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 12:59, Wednesday 17 April 2024 (77251)
OPS Day Midshift Update

H1 is now finished with comissioning and IFO is now OBSERVING

H1 SQZ (OpsInfo)
camilla.compton@LIGO.ORG - posted 09:20, Wednesday 17 April 2024 - last comment - 09:13, Thursday 18 April 2024(77238)
SCAN_SQZANG added to nominal SQZ path

Sheila, Naoki, Vicky, Camilla

As we continue to see the nominal SQZ angle change lock-to-lock (attached BLRMs). We edited SQZ_MANAGER to scan sqz angle (takes 120s) every time the SQZ locks, i.e. every time we go into NLN.

In  SQZ_MANAGER we have:

We tested this taking SQZ_MANAGER down and back up, it went though SCAN_SQZANG as expected and improved the SQZ by 1dB, range improved by ~10MPc.

We'll want to monitor that the change as SCAN_SQZANG may not give us the best angle at the start of the lock when SQZ is very variable. We expect this won't delay us going into observing as only added 120s and ISC_LOCK is often still waiting for ADS to converge during  this time.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 09:13, Thursday 18 April 2024 (77266)

I have removed this change of path by removing thew weighting as we can see last night SCAN_SQZANG at the start of the lock took us to a bad squeezing once thermalized.

We weren't seeing this changing angular dependence as much before 77133 with the older PSAMS settings (8.8V,-0.7V)  or (7.2V, -0.72V). Current (7.5V,0.5V). We think we should revert to the older setting.

Images attached to this comment
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