Displaying reports 55941-55960 of 83317.Go to page Start 2794 2795 2796 2797 2798 2799 2800 2801 2802 End
Reports until 07:09, Tuesday 05 July 2016
H1 PSL (PSL)
peter.king@LIGO.ORG - posted 07:09, Tuesday 05 July 2016 - last comment - 09:11, Tuesday 05 July 2016(28142)
Laser down
Came in to find the laser was off due to the power watchdog being tripped.
Both chillers were still running.

I have turned the laser back on but it hasn't returned to where it normally
returns to.  Looking into what happened.
Comments related to this report
peter.king@LIGO.ORG - 07:12, Tuesday 05 July 2016 (28143)
The laser tripped around 4:15 this morning.
peter.king@LIGO.ORG - 09:11, Tuesday 05 July 2016 (28144)
Looks like the NPRO tripped out.  Maybe due to a minor power surge due to the start of the
week?

    Pre-modecleaner had some problems locking irrespective of the reference level.  Found
that a small tweak to the horizontal alignment brought things back right away.

    Note in passing: with no light the output of the locking photodiode was ~ +29 mV.
Unlocked (ie with light incident on the pre-modecleaner) the output was ~ -230 mV.
Which is sort of low, which might be consistent with a small mis-alignment.  The
locking photodiode is a 1 mm InGaAs photodiode after all.
H1 ISC
marie.kasprzack@LIGO.ORG - posted 15:06, Monday 04 July 2016 (28139)
Beam position on the test masses

The beam position on the test masses is estimated from the a2l gains from the last minimization (method explained in alog 22426)

The gains values before and after the mimization are attached in a2l_gains_1151366417.mat.
The corresponding beam positions are reported in each suspension base in the Fig.1 attached. We can see that the beam is not more off-centered than previously.

However, we can observe that the beam hits the ITM and ETM in differents vertical places now in each cavity, suggesting an increase of the beam tilts in PIT with respect to the optical axes (HARD PIT).
That is what I tried to represent with the projection in Fig. 2, where you can imagine the cavities facing you: the figure axis orientation is the ETMs coordinates orientation.
The YAW tilts are reduced in both cavities. But their directions were opposite before the a2l minimization whereas now both cavity axes have a negative YAW tilt (in the ETM coordinates).

I don't know when the script was run for the last time before that, but it could give an indication that the beam is now more tilted in HARD PIT at 40W, and it enters the cavities from the lower area of the ITMs. 

 

Arm Before a2l After a2l
X

 D pit  = 1.3 mm

D yaw = 9.4 mm

D pit  = 7.8 mm

D yaw = 2.4 mm

Y

D pit  = 2.3 mm

D yaw = 6.5 mm

D pit = 8.0 mm

D yaw = 6.3 mm

Images attached to this report
Non-image files attached to this report
H1 ISC (ISC)
haocun.yu@LIGO.ORG - posted 14:30, Monday 04 July 2016 (28140)
HARD Yaw Loop Low Noise Measurements

Sheila, Jenne, Haocun

We took measurements on the C/DHARD yaw Loops with low bandwidth last Friday.

We firstly turned on the new filter to move compensation peaks for C/DHARD Yaw, then turn off the boost to win more phase. The gain was then lowered to ~half (CHARD_Y: -0.7 ---> -0.3, DHARD_Y: 40 ---> 19), and the new cutoff filters can be turned on.

These steps has been added in the Guardian, and we took measurements with the low noise loop, as attached below.

Both of the UGF are about 3.5Hz at 40 W now, which were ~5Hz before.

Images attached to this report
Non-image files attached to this report
H1 General
vernon.sandberg@LIGO.ORG - posted 14:06, Monday 04 July 2016 (28141)
Details on ER9

Engineering Run 9 (ER9) will begin next Wednesday. Here are some important details for operations:

Please see https://wiki.ligo.org/LSC/JRPComm/ER9 for more details.

LHO VE
john.worden@LIGO.ORG - posted 19:04, Sunday 03 July 2016 - last comment - 10:21, Monday 04 July 2016(28137)
CP3 Fill

Filled CP3 at ~ 1:50 UTC , 6:50 PM LOCAL Time Sunday.

Opened valve 1/2 turn and observed liquid after 5 minutes, 15 seconds. Windy on site.

Comments related to this report
chandra.romel@LIGO.ORG - 10:21, Monday 04 July 2016 (28138)
Thanks, John!
H1 ISC
stefan.ballmer@LIGO.ORG - posted 01:36, Saturday 02 July 2016 (28135)
PRC1 offsets do similar things as soft offsets

Tried to use PRC1 input offsets in pitch and yaw ro recover recycling gain, instead of SOFT imput offsets. While the carrier recycling gain responds to PRC1 input offsets similarl to soft offsets, the POP_18 couldnt care less. Thus I suspect none of these offsets is able to tackle the core issue.

 

The next thing to do is to verify that the POP18 signal is actually trustable, and not saturating,  If trustable, it will be the best indication of recycling cavity losses.

 

LHO General
thomas.shaffer@LIGO.ORG - posted 00:00, Saturday 02 July 2016 (28134)
Ops Eve Shift Summary

TITLE: 07/02 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: None
SHIFT SUMMARY: Commissioning continues. We have been sitting at NOMINAL_LOW_NOISE now for  1.5+ hours.
LOG:
fw1 has had at least a couple of restarts

Lost about 9.5hours on all DMT monitors.

23:40 - Gerardo to CP3

00:04 - Gerardo back.

H1 ISC
stefan.ballmer@LIGO.ORG - posted 23:28, Friday 01 July 2016 (28133)
8 Watt Missing Power - looks like it was lost in the power recycling cavity

Spent some time pulling together calibration numbers for AS, REFL and POP diodes, and makeing a total power budget.

Bottom line:

- The missing 20% power (8Watts!) is not coming out of any port, and thus must be absorbed in the interferometer.
- The way to distinguish loss in the recycling cavity and (280 times smaller) loss in the arms is to look at the sideband recycling gains.

Attached is a plot of power at each port, plus the power in the recycling cavity cast into cumulative arm loss (by multiplying with 279 power buildup and 95ppm round trip losses). Note that there is virtually no increase in AS power, and even a decrease in REFL power. the 8 missing Watts are absorbed in the interferometer.

Note that it is very difficult to distinguish arm losses from PRC losses using the carrier. However the two cenarios are very different for the sidebands - for arm losses both sideband hardly see anything. However, for PRC losses, the 9MHz sideband responds quickest, since it starts off with a hight recycling gain. The 2nd attached plot illustrats this. My money is on PRC losses.

The signals I picked for calibration are:

'H1:LSC-REFL_A_LF_OUTPUT':
0.1*0.5^3*(1-800e-6)^3*1000 = 12.47  mWatt REFL (=cts) / Watt from IFO
10% beam spplitter
two 50% beam splitter
three 800ppm loss mirrors
50% beam splitter
1000mW/W

'H1:LSC-POP_A_LF_OUTPUT':
229e-6*0.1*1e6 = 22.9 uWatt POP (=cts) / Watt in PRC
229 ppm of PR2
10% beam splitter
1e6uW/W

'H1:ASC-AS_C_SUM_OUTPUT':
0.965*800e-6*0.48*0.8*997*10^(36/20)*1638.4 = 3.0554e+04 cts / Watt from SRM
0.965 Faraday transmission
800ppm transmission mirror
48% beam splitter
0.8 Quantum Efficiency
997 Ohm transimpedance
36dB whitening gain
1638.4 cts/V ADC
Note: This calibration has the most estimate factors in it. I don't rust it better than ~25%.

'H1:OMC-DCPD_A_OUTPUT' & 'H1:OMC-DCPD_B_OUTPUT':
0.965*(1-800e-6)^2*0.99*0.93*0.5*0.85817*0.9*1000 = 343 mA / Watt carrier 00 mode from SRM
0.965 Faraday transmission
two 800ppm loss mirrors
1% loss mirrir
93% OMC transmission
50% splitter
0.85817 A/Watt ideal
90% Quantum Efficiency (is this right?)
1000mA/A

Images attached to this report
H1 AOS
carl.blair@LIGO.ORG - posted 21:16, Friday 01 July 2016 (28132)
SUS_PI ETMX damping now in LOWNOISE_ESD_ETMY gaurdian state

I broke lock turning the ETMX ESD low pass filters on.  I put them on as I had a feeling that this help PI damping yesterday and the ETMX 15541Hz mode was out of control and would broken lock.
We have now put this change into the LOWNOISE_ESD_ETMY gaurdian state along with the request for the ETMX_PI_DAMPING state from the SUS_PI gaurdian. 

LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 17:01, Friday 01 July 2016 (28129)
Manually over-filled CP3 at 23:50 utc

LLCV bypass valve 1/2 turn open, and the exhaust bypass valve fully open.

Flow was noted after 56 seconds, closed LLCV valve, and 3 minutes later the exhaust bypass valve was closed.

H1 CAL (CAL)
darkhan.tuyenbayev@LIGO.ORG - posted 16:01, Friday 01 July 2016 - last comment - 13:18, Tuesday 05 July 2016(28126)
DQ channels need to be added to the SUS ETMY model to track new calibration lines

Jeff K, Darkhan

Summary

Three DQ channels need to be added to the H1SUSETMY front-end model:

H1:SUS-ETMY_L1_CAL_LINE_OUT_DQ
H1:SUS-ETMY_L2_CAL_LINE_OUT_DQ
H1:SUS-ETMY_LKIN_P_LO_DQ

Details

SUSETMY model (both at H1 and L1) was updated to use synchronized oscillators to inject calibration lines into L1, L2 and L3 actuation stages to track temporal variations in the strengths of the drivers (LHO alog 27733). An additional calibration line is injected through Lock In oscillator (see attached screenshot 1).

In order to analyze time-dependent calibration of the drivers we need the excitation signals to be stored in the frames.

Hopefully, we will update the H1SUSETMY model on next Tuesday, Jul 5, 2016.

Images attached to this report
Comments related to this report
gregory.mendell@LIGO.ORG - 17:50, Friday 01 July 2016 (28131)

Darkhan suggests these are the channels to use:


TST / L3                 35.3              0.11       H1:SUS-ETMY_LKIN_P_LO_DQ
PUM / L2                 34.7              1.1        H1:SUS-ETMY_L2_CAL_LINE_OUT_DQ
UIM / L1                 33.7              11.0       H1:SUS-ETMY_L1_CAL_LINE_OUT_DQ

With his help, for the pcalmon SLM pipeline  looking at these "new" frequencies here,

https://ldas-jobs.ligo-wa.caltech.edu/~gmendell/pcalmon_new_freqs/daily-pcalmonNavigation.html

the configuration is now set to:


set channelFrequencyList {H1_R,H1:SUS-ETMY_LKIN_P_LO_DQ,35.3aup;H1_R,H1:SUS-ETMY_L2_CAL_LINE_OUT_DQ,34.7aup;H1_R,H1:SUS-ETMY_L1_CAL_LINE_OUT_DQ,33.7aup;H1_R,H1:CAL-PCALY_EXC_SUM_DQ,35.3aup,34.7aup,33.7aup,331.9aup;H1_R,H1:CAL-DARM_ERR_WHITEN_OUT_DBL_DQ,35.3aup,34.7aup,33.7aup,331.9aup;H1_R,H1:CAL-DARM_CTRL_WHITEN_OUT_DBL_DQ,35.3aup,34.7aup,33.7aup,331.9aup;H1_R,H1:CAL-PCALY_TX_PD_OUT_DQ,35.3aup,34.7aup,33.7aup,331.9aup;H1_R,H1:CAL-PCALY_RX_PD_OUT_DQ,35.3aup,34.7aup,33.7aup,331.9aup;H1_R,H1:CAL-DELTAL_EXTERNAL_DQ,35.3aup,34.7aup,33.7aup,331.9aup;H1_HOFT_C00,H1:GDS-CALIB_STRAIN,35.3aup,34.7aup,33.7aup,331.9aup}

I've regenerated the SLM data for July 1.  The suggested channels above do not yet exist, and SLM will put 0's in for these until they do.

 

jeffrey.kissel@LIGO.ORG - 13:18, Tuesday 05 July 2016 (28158)
These new channels has now been added to the frames. See LHO aLOG 28156
H1 General
travis.sadecki@LIGO.ORG - posted 16:00, Friday 01 July 2016 (28124)
Ops Day Shift Summary

TITLE: 07/01 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: TJ
SHIFT SUMMARY:  Tough day for locking.  Several issues involving the DOWN state of ISC_LOCK as TJ has noted yesterday.  Also new issue where the DOWN state caused the FSS to oscillate when attempting to do initial alignment.  Still babysitting SRM during ENGAGE_SOFT_LOOPS and INCREASE_POWER.
LOG:

Chandra to LVEA looking for serial numbers.  I forgot to record the time, but it didn't effect locking.
 

H1 IOO (IOO)
cheryl.vorvick@LIGO.ORG - posted 12:38, Friday 01 July 2016 - last comment - 16:21, Friday 01 July 2016(28120)
IO IM1-4 alignment changes as IMC oscillates from 25W to 57W

I looked at 1 hour of the input power / IMC power oscillations that occurred last weekend and how that power change effected the alignment of the IO IMs, IM1, IM2, IM3, and IM4.

4 attachments: 

One explanation for the difference of IM2 compared to IM1, IM3, and IM4, is that the beam on IM2 is no longer centered, so the change in IMC power causes the optic to change alignment.

If this is true, the change of the beam centering on IM2 could be big enough to have significantly changed the alignment of the beam through the Input FI.

Images attached to this report
Comments related to this report
cheryl.vorvick@LIGO.ORG - 15:57, Friday 01 July 2016 (28125)

UPDATE: IM1 glitching

IM1 UR OSEM signal is glitching and the glitches can be seen in DAMP_P and DAMP_Y at about 0.1urad in both signals. 

These glitches do not show up in IM4 Trans.

Images attached to this comment
cheryl.vorvick@LIGO.ORG - 16:21, Friday 01 July 2016 (28127)

UPDATE: IM2 oscillations clearly seen on IM4 Trans:

  amplitude (p-p)
IM4 trans pitch 0.035
IM2 pitch 0.25urad
IM4 trans yaw 0.015
IM2 yaw 0.25urad

Plot attached shows IM4 trans pitch and IM2 damp_p in blue, IM4 trans yaw and IM2 damp_y in green.

Images attached to this comment
H1 CAL
jeffrey.kissel@LIGO.ORG - posted 22:11, Thursday 30 June 2016 - last comment - 13:18, Tuesday 05 July 2016(28107)
Baseline Calibration Measurements for ER9 Complete!
J. Kissel, J. Driggers, T. Shaffer, D. Tuyenbayev, E. Goetz, K. Izumi

Over two ~1-2 hour lock stretches, I've managed to get the measurements needed for a baseline calibration update for ER9. Complete success! We'll work on the data analysis tomorrow, but I list the locations where all measurements have been committed to the CAL repo below. 

Of particular notes for the configuration of the IFO while doing these measurements:
- The OMC DCPDs have *no* stages of whitening employed. We've decreed that given the unknown success rate of PI damping over the next few days, it's more robust to leave the whitening off. We're not gaining too much in the high frequency end of the sensitivity anyways.
- All suspensions, including ETMY, have had their PUM stage switched to "Acq ON, LP OFF," i.e. state 2, or the highest range (i.e. not low noise). After some digging, Jenne found this was changed for some reason about a month ago, and maybe a setting that got lost in the power outage or something. 
I don't think either of these seemingly detrimental configurations are all that bad for ER9, given the bigger sensitivity issues elsewere.

Also note, in order to break the correlations we've found in O1 data between measurements of Actuation Stage Strength (see e.g. LHO aLOG 28096), I've taken an independent PCAL2DARM sweep for every isolation stage.

Measurements needed for Sensing Function:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PreER9/H1/Measurements/PCAL/
2016-07-01_H1_PCAL2DARMTF_4to1200Hz_SRCTuned.xml
    Exported as:
    2016-07-01_PCALY2DARMTF_4to1200Hz_A_PCALRX_B_DARMIN1_coh.txt
    2016-07-01_PCALY2DARMTF_4to1200Hz_A_PCALRX_B_DARMIN1_tf.txt

/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PreER9/H1/Measurements/DARMOLGTFs/
2016-07-01_H1_DARM_OLGTF_4to1200Hz_SRCTuned.xml
    2016-07-01_H1_DARM_OLGTF_4to1200Hz_A_ETMYL3LOCKIN2_B_ETMYL3LOCKIN1_tf.txt
    2016-07-01_H1_DARM_OLGTF_4to1200Hz_A_ETMYL3LOCKIN2_B_ETMYL3LOCKIN1_coh.txt
    2016-07-01_H1_DARM_OLGTF_4to1200Hz_A_ETMYL3LOCKIN2_B_ETMYL3LOCKEXC_tf.txt
    2016-07-01_H1_DARM_OLGTF_4to1200Hz_A_ETMYL3LOCKIN2_B_ETMYL3LOCKEXC_coh.txt


Measurements needed for Actuation Function:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PreER9/H1/Measurements/FullIFOActuatorTFs/
2016-07-01_PCALYtoDARM_FullLock_L1.xml
    2016-07-01_H1SUSETMY_PCALYtoDARM_ForL1Drive_FullLock_tf.txt
    2016-07-01_H1SUSETMY_PCALYtoDARM_ForL1Drive_FullLock_coh.txt

2016-07-01_H1SUSETMY_L1toDARM_FullLock.xml
    2016-07-01_H1SUSETMY_L1toDARM_State1_FullLock_tf.txt
    2016-07-01_H1SUSETMY_L1toDARM_State1_FullLock_coh.txt


2016-07-01_PCALYtoDARM_FullLock_L2.xml
    2016-07-01_H1SUSETMY_PCALYtoDARM_ForL2Drive_FullLock_tf.txt
    2016-07-01_H1SUSETMY_PCALYtoDARM_ForL2Drive_FullLock_coh.txt

2016-07-01_H1SUSETMY_L2toDARM_FullLock.xml
    2016-07-01_H1SUSETMY_L2toDARM_State2_FullLock_tf.txt
    2016-07-01_H1SUSETMY_L2toDARM_State2_FullLock_coh.txt


2016-07-01_PCALYtoDARM_FullLock_L3.xml
    2016-07-01_H1SUSETMY_PCALYtoDARM_ForL3Drive_FullLock_tf.txt
    2016-07-01_H1SUSETMY_PCALYtoDARM_ForL3Drive_FullLock_coh.txt

2016-07-01_H1SUSETMY_L3toDARM_LVLN_LPON_FullLock.xml
    2016-07-01_H1SUSETMY_L3toDARM_LVLN_LPON_FullLock_tf.txt
    2016-07-01_H1SUSETMY_L3toDARM_LVLN_LPON_FullLock_coh.txt
Comments related to this report
jeffrey.kissel@LIGO.ORG - 15:53, Friday 01 July 2016 (28123)
J. Kissel, E. Goetz

Just to post a status report before I disappear for the 4th, Evan and I have used Evan's new infrastructure to produce a model of the DARM open loop gain and sensing function from the above measurement. As one can see, there's still some work to do cleaning up the systematics in the model, but we're close. 

There're several things that are immediately evident:
- We have not changed the model's optical gain value from O1, so it's not terribly surprising that the optical gain model is high by 20%. 
- There is total and obvious detuning. So much so, that I think this is what's causing the severe drop in open loop gain.
- The drop in open loop gain is pretty nasty -- it causes sharp gain peaking at 10 Hz (as shown by the screenshot of the DTT template).

Kiwamu's working on a fitting routine that is similar to Evan's MCMC results from O1 (see T1500553), but advancing those results to include the effects of detuning so that we can add this to the model.

Stay tuned! Lots of work to do before Wednesday!
Images attached to this comment
Non-image files attached to this comment
evan.goetz@LIGO.ORG - 17:19, Friday 01 July 2016 (28130)

Evan G., Jeff K.

I processed the suspension actuation coefficients for the L1, L2, and L3 stages using the preliminary DARM model based on the one used during O1. We know that there need to be some modifications made, but the take home message here is that the actuation coefficients are about as to be expected. All are within ~5% of their O1 values. See attached figures.

The first attachment shows the UIM stage actuation coefficient. We have not yet included the BOSEM inductance and we have not yet included any actuator dynamics, so there is remaining discrepancy above ~20 Hz. There also appears to be some sort of phase wrapping issue that we still need to sort out.

The second attachment shows the PUM stage actuation coefficient. Things look pretty good here, although there may be some fluctuating optical gain which we have not yet accounted for in the measurement.

The third attachment shows the TST stage actuation coefficient. Again, there may be some fluctuating optical gain not accounted for in the measurement, and there is a phase wrapping issue to be sorted out.


Next on the agenda is to sort out the above issues and establish the actuation coefficients for the ER9 run.
 

Non-image files attached to this comment
evan.goetz@LIGO.ORG - 13:18, Tuesday 05 July 2016 (28157)

The sensing function attached above includes uncompensated high frequency poles from the whitening chassis and the transimpedence amplifier, so there will be some delay assocated with these values.

To see only the optical response, we have removed these high frequency poles, as well as the analog AA and digital AA transfer functions, in the attached data file.

Non-image files attached to this comment
H1 SUS (DetChar)
betsy.weaver@LIGO.ORG - posted 15:15, Tuesday 21 June 2016 - last comment - 23:54, Saturday 02 July 2016(27893)
TUESDAY Maintenance SUS OSEM noise hunt - SAT AMP Power Cycles

Richard, Filiberto, Ed, Betsy

Following on from Andy's probing alog 27841 regarding funny looking OSEM spectra, today we looked into a few fishy signals.  Based on spectra he took from before and after the early June power outage which show signal changes, he and Jenne identified the following set of problematic OSEM signals.  I've annotated the list with status as to what we found or fixed today:

 

ITMY L2 LR - Fixed after power cycling the Satallite Amp box (see alog below)

ITMY R0 RT - Signal looks funny before power outage, old problem, TBC...

MC1 M3 UL - Signal looks funny before power outage, old problem, TBC...

PRM M2 UR - Fixed after power cycling the Satallite Amp box (see alog below)

PR2 M1 T2 - TBC...

PR2 M3 UL - Giant nominal YAW Bias which has been on this SUS for over a year - very little signal on OSEM - mechanical fix when vent

PR2 M3 LL - Giant nominal YAW Bias which has been on this SUS for over a year - very little signal on OSEM - mechanical fix when vent

SR2 M1 LF - Funny comb feature, TBC...

SR2 M1 T1 - Funny comb feature, TBC...

SR2 M1 T3 - Funny comb feature, TBC... 

ETMX L2 LL - 50Hz turn up noise, TBC... Turn up is due to LOCK ACQ PUSHING, turn up not present during nominal SUS damping, no LOCK ACQ, see below plot

ETMX L2 LR - 50Hz turn up noise, TBC... Turn up is due to LOCK ACQ PUSHING, turn up not present during nominal SUS damping, no LOCK ACQ, see below plot

ETMX L2 UR - 50Hz turn up noise, TBC... Turn up is due to LOCK ACQ PUSHING, turn up not present during nominal SUS damping, no LOCK ACQ, see below plot

 

ETMY L2 UR - 50Hz turn up noise, TBC... Turn up is due to LOCK ACQ PUSHING, turn up not present during nominal SUS damping, no LOCK ACQ, see below plot

IM3 M1 LL - TBC...

 

We plan to pursue ITMy R0 and SR2 this week at next opportunity.

Comments related to this report
betsy.weaver@LIGO.ORG - 15:43, Tuesday 21 June 2016 (27894)

Before doing the sat amp power cycle, we first tried a coil driver power cycle on a few of our funny OSEM sets.  This did not appear to clear the errant noise in any of the 4 cases.  We then embarked on the sat amp power cycle which cured the 2 shown in the above list.  Tomorrow we hope to revisit ITMY R0 RT and SR2 M1 which we have left off troubleshooting today with only coil driver OFF spectra.  (Betsy, tomorrow you should use the attached spectra as a jump off point.) 

TBC...  Note the wildly different looking symptoms both of which were seen by Lundgren in 20675 AUG 2015.

Images attached to this comment
betsy.weaver@LIGO.ORG - 15:45, Tuesday 21 June 2016 (27896)

Attached is the ITMY L2 OSEM signal spectra shown from before and after today's fix.  The PRM M2 OSEM before and after-fix spectra are very similar to this.

Images attached to this comment
betsy.weaver@LIGO.ORG - 09:58, Wednesday 22 June 2016 (27911)

ETMX High freq turn up during LOCK ACQ, not a stand alone OSEM signal feature.

Images attached to this comment
betsy.weaver@LIGO.ORG - 10:03, Wednesday 22 June 2016 (27912)

ITMy R0 RT investigation - this morning Richard and Fil performed another round of tests on the ITMy R0 RT (shared cable and electronics with R0 LF, M0 RT, M0 LF).  After power cycling the SAT box, other SAT box cable reseating, and reseating of the main cable to the chamber, the noise on this channel still exists.

SR2 M1 bouncy noise on 3 of 4 TOP investigation - Richard and Fil powert cycled the Sat AMp box for this set of 4 OSEMs, but the noise is still there.

TBC...

andrew.lundgren@LIGO.ORG - 23:54, Saturday 02 July 2016 (28136)DetChar, ISC, SUS
As requested by Betsy, I've made another set of spectra of the OSEMs. The green line is July 1 10:18 UTC. The reference time (black) is a time near the Boxing Day event (Dec 26 2015 4:30 UTC). This is because the OSEMINF channels are only stored in the commissioning frames, and those aren't stored for very long. But we did store them around events in O1.

If we need to do these checks often, then we will need to 1) Store the OSEMINF channels in raw frames. 2) Occasionally save commissioning frames for some time in known-good states 3) Write some code to dump spectra to a file occasionally.
Non-image files attached to this comment
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