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Reports until 16:00, Monday 24 August 2015
H1 General
cheryl.vorvick@LIGO.ORG - posted 16:00, Monday 24 August 2015 - last comment - 21:05, Monday 24 August 2015(20831)
Day Summary:

Calibration Measurements:

- Kiwamu, IFO down for calibrations, 9:05 - expected to be all day, continuing now

*** FYI, I move the IFO to Commissioning when this happened and should have been Calibrations - my bad.

 

Note; We are now in Calibration, so IFO has two states:

'"IFO is up'"  OR  "IFO is having calibration measurements run."

 

Today's parasitic IFO/site activities:

- JeffB to EY, dust monitor investigation, 9:07 - done

- Hugh to EX and EY, HEPI, 9:07 - done

- JeffK, ETMY, measuring coil drivers, 9:15

- Sudarshan, PEM channel check in LVEA, 9:20 - done

- TJ EX BRS reset - 9:54 - done

- Kyle, near EY (Y28) to gather stuff - done

- Dave, EX, drawing updates - 12:10 - done

- Kyle, near EY (Y28) to gather stuff, 12:54 - done

- more visits to end stations while there was the opportunity, but no changes, just monitoring or restoring equipment.

 

Currently no outstanding IFO issues.

Calibration measurements continue.

Comments related to this report
cheryl.vorvick@LIGO.ORG - 21:05, Monday 24 August 2015 (20843)

Calibration Measurements:

- Kiwamu, IFO down for calibrations, 16:05UTC - expected to be all day, continuing now

*** FYI, I move the IFO to Commissioning when this happened and should have been Calibrations - my bad.

 

Note; We are now in Calibration, so IFO has two states:

'"IFO is up'"  OR  "IFO is having calibration measurements run."

 

Today's parasitic IFO/site activities:

- JeffB to EY, dust monitor investigation, 16:07UTC - done

- Hugh to EX and EY, HEPI, 16:07UTC- done

- JeffK, ETMY, measuring coil drivers, 16:15UTC

- Sudarshan, PEM channel check in LVEA, 16:20UTC- done

- TJ EX BRS reset - 16:54UTC- done

- Kyle, near EY (Y28) to gather stuff - done

- Dave, EX, drawing updates - 19:10UTC- done

- Kyle, near EY (Y28) to gather stuff, 19:54UTC- done

- more visits to end stations while there was the opportunity, but no changes, just monitoring or restoring equipment.

 

Currently no outstanding IFO issues.

Calibration measurements continue.

H1 ISC
eleanor.king@LIGO.ORG - posted 14:43, Monday 24 August 2015 - last comment - 20:53, Monday 24 August 2015(20827)
AS36 signal with BS and SRM dither lines

Stefan, Elli

On Saturday Stefan measured the AS36 signals with dither lines from the BS and SRM (alog 20777):

Lines:
H1:SUS-SRM_M3_ISCINF_P_EXC 7.0Hz, 300cts
H1:SUS-SRM_M3_ISCINF_Y_EXC 7.5Hz, 900cts
H1:SUS-BS_M3_ISCINF_P_EXC  8.0Hz, 100cts
H1:SUS-BS_M3_ISCINF_Y_EXC  8.5Hz,  30cts

Here are some plots of the AS36 signals demodulated against these line frequencies.  These signals  show how the sensitivy of the AS_36 WFS to the BS and SRM, which changes during the heat-up stage of the whole interferometer, and during 45MHz modulation depth reduction.  Attached are plots of the original and demodulated signals vs time.  Two vertical red lines are plotted; the first corresponds with when the IFO reaches full power, the second is when the 45MHz modulation depth reduction begins.  At the end of the time series the traces go crazy-  this is where Stefan reports lock was lost due to SRC1 yaw run away.

The following WFS channels are fed back to the optics at this point:
AS_B_RF36_I_PIT      >>   SRC1 PIT      (seen in demodulation of 7.0Hz line. Right two plots, red trace)
AS_B_RF36_I_YAW   >>   SRC1 YAW    (7.5 Hz line.  Right two plots, blue trace)
AS_A_RF36_I_PIT      >>   MICH PIT       (8 Hz line. Left two plots, red trace)
AS_B_RF36_Q_YAW  >>  MICH YAW    (8.5Hz line.  Right two plots, brown trace)

The SRC1 PIT signal doesn't change much, which is good.  SRC1 YAW has a 180deg ohase change during the heat-up stage.  Lines 1813 and 1815 of the guardian indicate a sign change in the ASC input matrix, maybe this corresponds to this phase change (?).  MICH PIT signal looks pretty good, getting close to 180deg phase at the end of the modulation depth reduction.  MICH YAW drifts downwards in phase, it looks like it hit -180deg just at the point we lost lock.

Images attached to this report
Comments related to this report
stefan.ballmer@LIGO.ORG - 20:53, Monday 24 August 2015 (20841)
Small correction: SRC1Y uses the following input matrix (alog 20699):
   AS_A_RF36_I_YAW to SRC1_Y : -3
   AS_B_RF36_I_YAW to SRC1_Y :  1
H1 CAL (CAL)
sudarshan.karki@LIGO.ORG - posted 12:21, Monday 24 August 2015 (20803)
DELTAL CTRL Whitening Filter

Following up to the problem (insufficient whitening) reported in  alog 20700,  new dewhitening filters  are implemented in the following DEALTAL_CTRL channels:

 

H1:CAL-CS_DARM_DELTAL_CTRL_M0/L1/L2/L3_WHITEN:  Original -- (zpk([1, 1, 1], [500,500,500],1,"n")

Changed to  (zpk([0.1,0.1,0.1,0.1], [100,100,100,100],1,"n")

H1:CAL-CS_DARM_DELTAL_CTRL_SUM_WHITEN: Original --(zpk([1, 1, 1,1,1], [100,100,500,500,500],1,"n")

Changed to  (zpk([0.1,0.1,0.1,0.1], [100,100,100,100],1,"n")

The first attached plot shows DARM CTRL signal with original filter in dotted  lines and the new filter  in solid lines.

The second plot shows the effect of different filter combinations on DARM_CTRL signal. This measurement gave us an intuition on what filter to use eventually.

Images attached to this report
H1 AOS (DetChar)
paul.schale@LIGO.ORG - posted 11:34, Monday 24 August 2015 - last comment - 12:30, Monday 24 August 2015(20823)
DQ Shift 20 August 00:00 UTC - 23 August 23:59 UTC

- Duty Cycle: 54%

- range: 75 - 85 Mpc

- PRM M3 LL coil driver caused noise in 10-60 Hz range on Friday, may have been responsible for some loud glitches

- Also on Friday there were some strange lines in the strain spectrogram at around 10Hz

- loud glitches that cause brief, large drop in range that we saw in ER7 continue; the rate is improved

- link to full DQ shift

Comments related to this report
sheila.dwyer@LIGO.ORG - 12:30, Monday 24 August 2015 (20824)CAL

Please note that the range on the summary pages is not correct.  The range displayed in the control room has been hovering around 60-65 Mpc, and this is much more realistic, although not yet blessed by the calibration group. 

H1 CAL (CAL)
darkhan.tuyenbayev@LIGO.ORG - posted 10:54, Monday 24 August 2015 (20819)
DARM OLGTF model for ER8

JeffreyK, Kiwamu, Darkhan

Overview

A DARM OLG TF model and its parts, sensing and actuation functions, are used for calculating the interferometer strain, h(t), and estimation of uncertainty in reported h(t).

On last Thursday we put together a DARM OLGTF Matlab model for ER8/O1 and compared it to a DARM OLGTF measurement taken on Aug 17, 2015. This model is mainly based on a similar model for ER7 (LHO alog 18769). Currently the model agrees with the measurement to only about +/-10% in magnitude and +/- 5 deg up to 200 Hz. So there's still work need to be done, probably changing parameter file needs some fine tuning of possibly following parameters: optical gain, CC pole frequency, ESD zeros and poles, ESD gain.

Details

Please, see a summary of things to be aware of when using this model (mostly listed differences from ER7 model):

[ol, par] = H1DARMmodel_ER8('par_file');

freq = 10 : 1 : 100;

G = par.G.getFreqResp_total(freq);

A = par.A.getFreqResp_total(freq); % total actuation function

% frequency responses of actuation stages can be obtained similarly

A_tst = par.A.getFreqResp_TST(freq);

% frequency responses of C with and without CC pole

C = par.C.getFreqResp_total(freq);

C_res = par.C.getFreqResp_noCavPole(freq);

We still need to take more DARM OLGTF and PCAL to DARM TF measurements and compare them to better estimate DARM model parameters.

The model was uploaded into calibration SVN (r1095):

CalSVN/aligocalibration/trunk/Runs/ER8/H1/Scripts/H1DARMOLGTFmodel_ER8.m

The parameter file associated with measurement taken on Aug 17 is in the same directory:

CalSVN/aligocalibration/trunk/Runs/ER8/H1/Scripts/DARMOLGTFs/H1DARMparams_1123894143.m

I believe that these scripts are in a reasonable shape to try it with LLO DARM parameters.

Images attached to this report
H1 SEI
hugh.radkins@LIGO.ORG - posted 10:42, Monday 24 August 2015 (20822)
HEPI Fluid Levels Checked--all good--no leaks--Accumulators would appear charged

The fluid levels are essentially unchanged since the end of July.  The EndX is down <1/16" but I'll wait for more data to claim a trend from a leaky Accumulator.  No further HEPI Maintenance needed tomorrow.

H1 SEI
thomas.shaffer@LIGO.ORG - posted 10:21, Monday 24 August 2015 (20821)
EX BRS Restarted

BRS software crashed at the end of last week. I got a chance to head to EX and restart the code from the desktop in the rack room.

I kept the damper OFF for now to see whether or not it is rung up.

H1 CAL (ISC)
jeffrey.kissel@LIGO.ORG - posted 09:49, Monday 24 August 2015 (20818)
Sketch of the Plan for LHO's Calibration Week
J. Kissel, K. Izumi, S. Karki, D. Tuyenbayev, R. Savage

I attach a picture of the whiteboard where we've sketched out our plan for the week. We've gone through T1500443, taken off items that we've already managed to capture before this week, and prioritized the remaining tasks accordingly.

Stay tuned for daily updates on progress.
Images attached to this report
Non-image files attached to this report
H1 CAL (ISC)
jeffrey.kissel@LIGO.ORG - posted 09:05, Monday 24 August 2015 (20817)
IFO Down for Calibration Measurements
J. Kissel, K. Izumi

At 16:02 UTC, we've taken the IFO down to begin calibration measurements.

On today's docket:
- Actuation function frequency dependence checks
    - UIM, PUM Coil Driver TFs
    - ESD LVLN Driver TFs
- Sensing function frequency dependence checks
    - OMC DCPD AA Chassis
    - OMC DCPD PreAmp (with single bounce IFO)
H1 General
edmond.merilh@LIGO.ORG - posted 08:02, Monday 24 August 2015 (20816)
End of Shift Summary and Lock Log

ALL TIMES IN UTC

Science Mode Checklist: (beginning of shift)

Activity Log:

LOCK LOG:

Shift Summary:

H1 General
edmond.merilh@LIGO.ORG - posted 06:30, Monday 24 August 2015 (20815)
IFO set to Observing Mode

13:28UTC OIB and OOM set to Undisturbed/Observing

H1 General
edmond.merilh@LIGO.ORG - posted 05:11, Monday 24 August 2015 - last comment - 05:13, Monday 24 August 2015(20813)
Switching IFO to Observation Mode

ALL TIMES IN UTC

 

Science Mode Checklist:

Activity Log:


Comments related to this report
edmond.merilh@LIGO.ORG - 05:13, Monday 24 August 2015 (20814)

12:07 LockLoss. 

  1. 5.0113km E of Ust'-Kamchatsk Staryy, Russia2015-08-24 11:51:01 UTC31.7 km
H1 ISC (GRD)
evan.hall@LIGO.ORG - posted 04:49, Monday 24 August 2015 - last comment - 12:33, Monday 24 August 2015(20811)
Some cHard/PRC WFS investigation

Sheila, Evan

We looked again at the situation with the 45 MHz REFL WFSs, which are used as sensors for the PR3 ASC loop. In the end, we didn't implement any changes to the sensors or the associated loops.

We were motivated by the following:

  1. The current demod phases for these WFSs simply do not make sense; we expect that they should be similar (since the analog delays should be fairly well matched), but instead they are scattered by 100+ degrees.
  2. The cHard and PR3 loops are strongly cross-coupled. We would like to be able to turn up the gain of cHard without impressing extra motion from other optics into DARM. [20523, 20497]
  3. Any perturbation in the PR3 seems to couple into the SRC loops. We already know that the SRM loop is quite delicate, and we would like to get rid of this coupling if possible.

We tried the following:

After that, we couldn't get to full power because of an oscillation that showed up in dHard pitch when going to 20+ W. (We've seen this before, and it seems to be distinct from the angular instability mentioned above.) To get around this, we had to slightly beef up the resonant gain that gets turned on in dHard pitch when the power is increased.

Also, there were some small maintenance tasks that we did:

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 12:33, Monday 24 August 2015 (20825)

Two of the chaanges that we made last night we kept. 

With the new phasing for refl 45, it was no longer a good sensor to use in DRMI, so we changed PRC2 in this configuration to using the sum of refl A and B 9I.  This is in the DRMI guardian and works fine, so we've left it there. 

We left the DC coupled OpLev off, we think the cage servo will have less drift. 

H1 General
edmond.merilh@LIGO.ORG - posted 03:54, Monday 24 August 2015 (20812)
Mid-Shift Update: OWL

ALL TIMES IN UTC

On my arrival, Evan, Sheila and Dan on site (of course Jim also). Not really any wind to speak of (~10mph). Minor earthquake activity in the last couple of hours after about 5 hours of quiet. Everyone gone except for Evan.

 

Science Mode Checklist: (since beginning of shift)

Activity Log:

H1 ISC
peter.fritschel@LIGO.ORG - posted 15:48, Wednesday 05 August 2015 - last comment - 10:08, Monday 24 August 2015(20270)
SRCL, MICH, and PRCL: open loop and residual noise spectra

Using the calibrated DRMI channels created and described by Kiwamu in entry 18742, I grabbed data from the lock of August 3, 2015, starting at 04:20:00 UTC. The attached 4 page PDF shows spectra of the open loop and residual displacement noise for SRCL, MICH and PRCL. The 4th page shows the coherence of SRCL with the other 2 degrees of freedom.

Degree of freedom Residual rms Shot noise level
SRCL 8 pm 1.3 x 10-15 m/rtHz
MICH 3 pm 1.5 x 10-16 m/rtHz
PRCL 0.8 pm 4 x 10-17 m/rtHz

The SRCL spectra has a curious shape: it comes down quickly with frequency to 10 Hz, then is fairly flat from 10 Hz to 50 Hz, then falls by a factor of 5 or so to the (presumed) shot noise level that is reached above 100 Hz. What is this noise shelf between 10 Hz and 80 Hz? That is exactly the region where the SRCL noise coupling to DARM is troublesome. Our usual approach is to send a SRCL correction path to DARM to reduce the coupling, but this spectrum shows that there should also be some gain to be had by reducing this noise shelf.

The last page of the PDF shows the coherence between SRCL and MICH & PRCL, and it indicates that the SRCL noise shelf could be coupling from PRCL noise -- the coherence is fairly high in this band, though not unity. This suggests that the DRMI signals could use some of the demodulator phase and input matrix tuning that Rana has recently done on L1, reported in LLO log entry 19540.

To complete this log entry, it would be useful if someone at LHO could add the open loop transfer functions for each loop (models), and other pertinent info such as DC photocurrents for these detectors and the input matrix coefficients.

Non-image files attached to this report
Comments related to this report
evan.hall@LIGO.ORG - 17:54, Saturday 22 August 2015 (20789)

The shelf appears to be gain peaking in SRCL. We have an 80 LPF to get rid of SRCL control noise in the bucket, but it makes the control noise from 30 to 60 Hz a bit worse.

I had the filter off between 2015-08-23 00:36:00 Z and 00:39:00 Z. The attachment shows the error and control signals with filter off (dashed) versus filter on (solid).

Images attached to this comment
keita.kawabe@LIGO.ORG - 10:08, Monday 24 August 2015 (20820)

Evan, is the shelf in Peter's open loop spectrum there because of OLTF model without LPF? Otherwise, we still need to investigate.

H1 ISC (ISC)
stefan.ballmer@LIGO.ORG - posted 02:41, Thursday 23 July 2015 - last comment - 14:53, Monday 24 August 2015(19856)
Coherent broadband noise in OMC_DC_SUM
We observed broadband coherence of OMC_DC_SUM with ASC_AS_C_LF_SUM and ASC_A_RF36_PIT. We made some numbers and plots, using the 64kHz version of the channels.

First the measurements we made on OCXO oscillator:
- ASC_AS_C sees a RIN of about 5e-7/rtHz above 100Hz (either from H1:ASC-AS_C_SUM_OUT_DQ or from H1:IOP-ASC0_MADC6_TP_CH11). The same is true for its segment 1.
- The calculated shot noise RIN at 20mA (quantum efficiency 0.87) detected is 4.0e-9/rtHz.
- The 4.0e-9/rtHz agrees with DCPD_NULL_OUT_DQ's prediction (8.0e-8 mA/rtHz/20mA).
- DCPD_SUM_OUT_DQ sees a slightly elevated RIN of 4.6e-9/rtHz (9.2e-8 mA/rtHz/20mA).

- The RIN in DCPDA (H1:IOP-LSC0_MADC0_TP_CH12, corrected for the whitening) is about 5.9e-8 mA/rtHz, or RIN = 5.9e-9/rtHz at 20mA/2diodes (~15pm DARM offset)...
- ...or about 3.3e-8 mA/rtHz or 1.2e-8/rtHz at 5.7mA/2diodes (~8pm DARM offset).

- ASC-AS_C_SEG1 (H1:IOP-ASC0_MADC6_TP_CH11) and OMC-DCPD_A (H1:IOP-LSC0_MADC0_TP_CH12) shows a coherence of 0.053 at 20mA, suggesting a white noise floor a factor of 0.23 below shot noise.
- At 5.7mA the same coherence is about 0.13, i.e. the white noise floor is a factor of 0.39 below shot noise.
- These two measurements are in plot 1.

- Taking the last two statements together, we predict a coherent noise of
  - 5.9e-8 mA/rtHz *0.23 = 1.4e-8 mA/rtHz at 20mA/2diodes (~15pm DARM offset)  (RIN of coherent noise = 1.4e-9/rtHz) - The pure shot noise part is thus 5.7e-8 mA/rtHz
  - 3.3e-8 mA/rtHz *0.39 = 1.3e-8 mA/rtHz at 5.7mA/2diodes (~8pm DARM offset)  (RIN of coherent noise = 4.5e-9/rtHz) - The pure shot noise part is thus 3.0e-8 mA/rtHz.

- AS_C calibration:
 - 200V/W (see alog 15431)
 - quantum efficiency 0.8 (see alog 15431)
 - 0.25% of the HAM 6 light (see alog 15431)
 - We have 39200cts in the AS_C_SUM. Thus we have
   - 39200cts / (1638.4cts/V) * 10^(-36/40) (whitening) / (200V/W) = 1.89mW and AS_C. (shot noi
   - 1.89mW/0.025 = 76mW entering HAM6. I.e. we have slightly more sideband power than carrier power (Carrier: 27mW in OMC transmission).
   - Shot noise level on AS_C_SUM is at 2.0e-8 mA/rtHz, corresponding to a RIN of 1.6e-8/rtHz. I.e. the coherent noise seen at 5e-7/rtHz is high above the shot noise. Dark noise TBD.
   - The light entering HAM 6 has a white noise of 5e-7/rtHz*76mW = 3.8e-5 mW/rtHz 
    

Bottom line:
 -We have ~1.4e-8mA/rtHz, or 1.9e-8mW/rtHz of coherent white noise on each DCPD.
 -It corresponds to 3.8e-5mW/rtHz before the OMC, i.e. the the OMC seems to attenuate this component by 2000.
 -This noise stays at the same level (in mW/rtHz) for different DCPD offsets.


Next, we switched back to the IFR for testing. plot 2 shows the same coherences (all at 5.7mA / 8pm DARM offset), but on the IFR. Interestingly now AS_C and AS_A_RF36 start seeing different noise below 2kHz. We convinced our selfs that the higher excess noise seen in AS_A_RF36 is indeed oscillator phase noise from the IFR - so that is clearly out of the picture once of the OCXO. (Evan will shortly log the oscillator phase noise predictions.)


64k Channel list:
H1:IOP-LSC0_MADC0_TP_CH12:     OMC-DCPD_A  (used in plot)
H1:IOP-LSC0_MADC0_TP_CH13:     OMC-DCPD_B
H1:IOP-LSC0_MADC1_TP_CH20:     REFLAIR_A_RF9_Q
H1:IOP-LSC0_MADC1_TP_CH21:     REFLAIR_A_RF9_I
H1:IOP-LSC0_MADC1_TP_CH22:     REFLAIR_A_RF45_Q
H1:IOP-LSC0_MADC1_TP_CH23:     REFLAIR_A_RF45_I
H1:IOP-LSC0_MADC1_TP_CH28:     REFL_A_RF9_Q
H1:IOP-LSC0_MADC1_TP_CH29:     REFL_A_RF9_I
H1:IOP-LSC0_MADC1_TP_CH30:     REFL_A_RF45_Q
H1:IOP-LSC0_MADC1_TP_CH31:     REFL_A_RF45_I


H1:IOP-ASC0_MADC4_TP_CH8:      ASC-AS_A_RF36_I1
H1:IOP-ASC0_MADC4_TP_CH9:      ASC-AS_A_RF36_Q1
H1:IOP-ASC0_MADC4_TP_CH10:     ASC-AS_A_RF36_I2
H1:IOP-ASC0_MADC4_TP_CH11:     ASC-AS_A_RF36_Q2
H1:IOP-ASC0_MADC4_TP_CH12:     ASC-AS_A_RF36_I3
H1:IOP-ASC0_MADC4_TP_CH13:     ASC-AS_A_RF36_Q3   (used in plot)
H1:IOP-ASC0_MADC4_TP_CH14:     ASC-AS_A_RF36_I4
H1:IOP-ASC0_MADC4_TP_CH15:     ASC-AS_A_RF36_Q4

H1:IOP-ASC0_MADC6_TP_CH11:     ASC-AS_C_SEG1  (used in plot)
H1:IOP-ASC0_MADC6_TP_CH10:     ASC-AS_C_SEG2
H1:IOP-ASC0_MADC6_TP_CH9:      ASC-AS_C_SEG3
H1:IOP-ASC0_MADC6_TP_CH8:      ASC-AS_C_SEG4





Images attached to this report
Comments related to this report
stefan.ballmer@LIGO.ORG - 17:01, Thursday 23 July 2015 (19882)
Some more estimation - this time for frequency noise:

- Shot noise on the refl diodes is given by Pshot=sqrt(2*h*nu*Pr_lock)
- The cavity sensing function is P_9_pk = 4*Gam9*P0 * dNu(f)/(f_p + i*f), where P0 would be the carrier power incident on the PD without the IFO.
- from this we can estimate a frequency (phase) noise of about 8e-11 rad/rtHz.

Gam9=0.219; %alog15874
PSL_low=2; %W
Pr_nolock_low=13.7e-3; %W
PSL_lock=24;
Pr_lock=3.5e-3; %W
IMCt=0.88; 
att=Pr_nolock_low/(PSL_low*IMCt);
P0=PSL_lock*IMCt*att;
inlockdrop=Pr_lock/(P0);

Pshot=sqrt(2*h*nu*Pr_lock);
dphi=Pshot/P0/4/pi/Gam9;
stefan.ballmer@LIGO.ORG - 12:28, Monday 27 July 2015 (19963)
For reference, I ran the numbers on where we would expect the sidebands to show a resonance feature.

I used the following values:
RITM=1939.3m
RETM=2241.54m
L=3994.485m

Checking accidental sideband resonances in the arm cavities:
Resonance condition: fres = FSR * (q  + (l+m+1)*fTM/FSR)
Free Spectral Range (FSR)    : 37.5258 kHz
Transverse Mode Spacing (fTM): 32.4297 kHz
Checking f1 sideband:
q=242	l+m=0	 Freq. diff. = 18.2284 kHz
q=242	l+m=0				 Freq. from antiresonant = 0.534516 kHz
q=242	l+m=1	 Freq. diff. = 14.2013 kHz
q=241	l+m=1				 Freq. from antiresonant = 4.56162 kHz
q=241	l+m=2	 Freq. diff. = 9.10514 kHz
q=-242	l+m=0	 Freq. diff. = 18.2284 kHz
q=-243	l+m=0				 Freq. from antiresonant = 0.534516 kHz
q=-243	l+m=1	 Freq. diff. = 13.1322 kHz
q=-244	l+m=1				 Freq. from antiresonant = 5.63065 kHz
q=-244	l+m=2	 Freq. diff. = 8.0361 kHz
Checking f2 sideband:
q=1212	l+m=0	 Freq. diff. = 16.0903 kHz
q=1212	l+m=0				 Freq. from antiresonant = 2.67258 kHz
q=1212	l+m=1	 Freq. diff. = 16.3393 kHz
q=1211	l+m=1				 Freq. from antiresonant = 2.42356 kHz
q=1211	l+m=2	 Freq. diff. = 11.2432 kHz
q=-1212	l+m=0	 Freq. diff. = 16.0903 kHz
q=-1213	l+m=0				 Freq. from antiresonant = 2.67258 kHz
q=-1213	l+m=1	 Freq. diff. = 10.9942 kHz
q=-1214	l+m=1				 Freq. from antiresonant = 7.76872 kHz
q=-1214	l+m=2	 Freq. diff. = 5.89804 kHz

stefan.ballmer@LIGO.ORG - 00:19, Wednesday 29 July 2015 (20014)ISC
Evan, Matt, Lisa

We did one more test for the broadband coherence noise: Common mode gain +3dB vs -3dB

We see no chnge in the broadband level of the noise below 10000Hz.
However, we do see an FSS gain oscillation at 7320Hz showing up in the OMC_DCPD_SUM - but not in AS_C_LF or AS_A_RF36 - in fact that coherence has adip where we get the frequency noise oscillation.
This strongly suggests that our broadband noise is NOT frequency noise.

Evan also took the frequency noise transfer function - a preliminary analysis here also confirms: the frequency noise should be significantly below the O(1e-8mA/rtHz) noise level we see.
Images attached to this comment
stefan.ballmer@LIGO.ORG - 18:53, Sunday 02 August 2015 (20150)
Note that the higher order mode estimates above were made using a slightly wrong modulation frequency. Updated estimates for the correct modulation frequency are attached to alog 20147
stefan.ballmer@LIGO.ORG - 14:20, Monday 24 August 2015 (20826)
 - ASC-AS_C GETS 2.5% of the HAM 6 light (see alog 15431) (NOT 0.25%)
daniel.hoak@LIGO.ORG - 14:53, Monday 24 August 2015 (20828)

Actually AS_C gets 400ppm of the light entering HAM6 -- the OM1 mirror was swapped from 5% transmission to 800ppm transmission in early April.  See alog:17738.

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