I've continued to analyze stochmon's results (found here) for coherence between the h(t) channels of L1 and H1. One interesting line is at 74 Hz, at which I get coherences at both H1 and L1 from corner station accelerometers. You can find the full results for the coherence here and here, but I've attached some relevant summary slides. Any idea where this is coming from?
Tagging the SEI, SUS, AOS, ISC, and SYS group, since the majority of these channels are projected versions of the ITMY ST2 GS13s and I suspect solving the problem will require action from a broad number of groups. ~74 [Hz] is roughly the right frequency for the fundamental of QUAD cage resonances. For H1 and L1 ITMY specifically, See LHO aLOG 5322; The X (beamline) direction attachment shows a broad resonance at ~75 [Hz]. Similarly for LLO LLO aLOG 7214, though the Q of the resonance is significantly lower. Suggested mechanism for coupling to DARM: the QUAD's cage is attached (mechanically) to the the ISI-ITMY's ST2. Thus the GS13s (the most sensitive local sensor in the chamber at those frequencies) are likely to see these resonance, where the resonance is excited by residual ground motion. However, the QUADs are great isolators at least frequencies, so we can rule out "traditional" coupling via direct transmission of this residual motion through the suspension chain to the test mass. What's more likely is that the cage itself is picking up scattered light from some source, and coupling it directly into the cavity's beam line. Note that a similar frequency, low Q feature was found on H1 ETMX while our end-station beam diverter was inadvertently left open for the beginning of the run, see LHO aLOG 22350. I suspect the same mechanism is at play here -- scattered light glinting off the QUAD cage into the IFO beamline.
TITLE: 12/18 OWL Shift: 08:00-16:00UTC (00:00-08:00PST), all times posted in UTC
STATE of H1: Observing at ~75 Mpc.
Incoming Operator: Jim
Support: Jim, Jenne
Quick Summary:
The range has been ratty since 8 hours ago. Omicron shows band of glitches around 20 Hz and between 100-200 Hz. I don't see any significance changes in environment from 8 hours ago. I dig through the summary page breifly and found SR3 oplev spectogram looking very nasty started 8 hours ago, but the spectrum doesn't show any misbehave osems. So the cause of these glitches is still unknown.
Shift Activities:
Nutsinee asked me to have a look-see at SR3. As you can see in the attached plot (1 day trend), the oplev sum is doing something very weird starting a few hours ago, but the optic motion (as seen by both the oplev and the osems) seems totally fine. So, something is likely funny with the SR3 optical lever laser, but since we don't ever use it in-loop, it's not a high priority for fixing right now.
DMT Omega looks glitchy between 100-200Hz. Useism have reached 90th percentile. Low wind (<5mph). A 5.6M earthquake at North of Ascension Island is coming through. LLO is already down. Hope we ride this one......
TITLE: 12/17 OWL Shift: 08:00-16:00UTC (00:00-08:00PDT), all times posted in UTC
STATE of H1: Observing
Incoming Operator: Jim
Support:
Quick Summary:
Very quiet night. Nothing to complain.
Shift Activities:
TITLE: 12/17 EVE Shift: 00:00-08:00UTC (16:00-00:00PDT), all times posted in UTC
STATE of H1: Observing for last 8+hrs with range of ~75Mpc
Incoming Operator: Nutsinee
Support: None needed
Quick Summary:
A nice quiet shift. useism holding steady at 0.4um/s for the last 24hrs. The winds seem to be calming down. And the snow is still on the ground. Range has been a little ratty-looking 70-80Mpc.
Shift Activities:
Evan G, Jeff K
Summary:
We finally processed the data Jeff collected (aLOG 21325) to investigate the mysterious zero near 100 Hz. Unfortunately, while we began to further understand the calibration measurements, we also uncovered new issues needing investigation.
Solved:
New mysteries:

Details:
Taking Jeff's measurements of the driver electronics (plotted magnitude only called rawXX.pdf attached) and dividing by the fitted values for the low-pass filters from aLOG 21283, we can see the remaining effect of the BOSEM in the circuit (see XX.pdf attached). We plot the magnitude and phase of each state. Left hand plots are over the full range of 1 Hz to 10 kHz, while right hand plots are zooms from 1 Hz to 200 Hz.
Fortunately, from these measurements, we can confirm that the DC transconductance is: UL = 578 uA/V, LL = 589 uA/V, UR = 582 uA/V, LR = 600 uA/V. Earlier measurements (see 21127 and 21142) had found that this was off by a factor of 2, but we do find the expected value. However, when trying to understand the "zero-like device" we found that the frequency dependence at higher frequency goes like f^{3/4}! Now we are confused.
Looking closely at the low frequency region, and in the zoom (right hand plots) we see that the fitted zero-pole pair doesn't quite take out the low-pass filters for state 3 and state 4 (last two low-pass stages). This could be because of the buffers in the driver electronics, but we are not sure if this is really the cause.
We also started looking at the parameters file for the CAL model and found that the UIM parameters have the wrong zero-pole pair and, in addition, are not using the fitted low-pass filter values. This needs to be rectified.
The script that plots these results is in:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER8/H1/Scripts/Electronics/analyze_uimdriver_wBOSEM_20150908.m
Integration Issue 1179 filed regarding the lack of using the measured UIM z:p parameters in the DARM model.
J. Kissel As a part / start of the review process for the calibration pipeline, it has been requested that -- along with a long-term view of the PCAL to GDS-CALIB_STRAIN ratios (as shown in LHO aLOG 24285) -- we take snap-shots of the entire C01 GDS-CALIB_STRAIN spectrum at a smattering of times, and take the ASD ratios as has been done for the official strain sensitivity plots (see e.g. G1501223). I've done so over the early part of the run, between Sep 11 and Oct 22 2015, every 5 days or so, Sep 11 2015 20:30:43 UTC Sep 18 2015 04:50:43 UTC Sep 25 2015 07:23:43 UTC Oct 01 2015 01:30:43 UTC Oct 05 2015 05:31:43 UTC Oct 11 2015 18:57:43 UTC Oct 17 2015 07:41:43 UTC Oct 22 2015 03:12:43 UTC (recall that we get 420 [sec] of data for each ASD -- see T1500365). Attached are the zooms of the ASDs of both GDS-CALIB_STRAIN and PCAL displacement around the three PCAL frequencies ( C01_H1_O1_Sensitivity_displacement_asd_pcalzoom.pdf) and the ratio of these ASDs (C01_H1_O1_Sensitivity_displacement_asd_pcalzoomratio.pdf) for these 8 data sets. I figured this was plot overload, so I leave all nine plots that come with each official strain simply committed to the CalSVN here: /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O1/H1/Results/DARMASDs/ where the collection of plots are dated accordingly (e.g. 2015-10-22_C01_H1_O1_Sensitivity.pdf). The message: for these spot-checks, the ratio between GDS C01 calibrated displacement and PCAL calibrated displacement is within the expected 10%, and all but the earliest data point data point is better than 5%. Very good -- great job CAL team! ------- These plots were made with a generalization of the official strain producing script that now lives in /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O1/Common/Scripts/produceofficialstrainasds_O1_C01.m
Per the Shift Check Sheet (for Thursday's task), I went and checked on the Crystal & Diode Chillers for the PSL. The Crystal Chiller was not at maximum, so I added 125mL (basically to get the water's meniscus close to the "MAX" level). NOTE: according to the notepad, this was filled on 12/16 with 125mL also.
Diode Chiller was fine (no red error light).
H1 has been locked for 5.5+ hrs with a range between 70-80Mpc (only one ETMy saturation).
All running well here. I was not able to log into the ops workstation (operator0) at the beginning of the shift, but Jim B was able to remedy that.
Snowed earlier in the shift, and we have about 0.75" of snow on the ground currently. Winds are at about 6mph & useism is at 0.4um/s
The omicron scans of the top ten Hanford BBH/BNS triggers on December 16th show a notable recurring wave-like glitch. The glitches are present in the following scans: https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/BBH/GW/1134302174/ https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/BBH/GW/1134294300/ https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/BBH/GW/1134291513/ https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/BNS/GW/1134295111/ Inspection of the auxiliary channels revealed that these signals seem to stem from one channel: H1:ASC-Y_TR_B_PIT_OUT_DQ.The scans for this channel are visible here: https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/BBH/1134302174/#H1:ASC-Y_TR_B_PIT_OUT_DQ https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/BBH/1134294300/#H1:ASC-Y_TR_B_PIT_OUT_DQ https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/BBH/1134291513/#H1:ASC-Y_TR_B_PIT_OUT_DQ https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/BNS/1134295111/#H1:ASC-Y_TR_B_PIT_OUT_DQ The rest of the scans from December 16th can be accessed from the chart here: https://ldas-jobs.ligo-wa.caltech.edu/~jacob.broida/Dec16/Results.html
BCV Results for the above glitches. BBH Glitches https://ldas-jobs.ligo-wa.caltech.edu/~sudarshan.ghonge/BCV/O1/H1_glitch_151216_bbh/H1_1134289817_1134329417_webpage/ BNS Glitches https://ldas-jobs.ligo-wa.caltech.edu/~sudarshan.ghonge/BCV/O1/H1_glitch_151216_bns/H1_1134282617_1134336617_webpage/
TITLE: 12/17 Day Shift: 16:00-24:00UTC
STATE of H1: Observing, only just
Support: Yes
Quick Summary: Quiet shift until an earthquake knocked us out of lock
Shift Activities:
17:45 Mitch to Optics Lab
19:00 Jodi to Mid-y and EndX, back 19:45
It was a relatively quiet shift. We were locked at about 75 Mpc until about 15 minutes ago when a 6.4 earthquake in Mexico hit us. .03-.1 hz ground motion is about 5 microns. Otherwise, wind is moderate, microseism was about .5 microns. Now we play the waiting game.
I've taken some measurements indicating the EX sensor correction in Z is causing problems for the ISI. I've ramped it off, watching the IFO for issues and will be taking some measurements. This may result in a change of configuration for the ISI, eventually.
All these analysis were done in C00 data and I am sure these discrepancy in phase will disappear on C01 data. I will analyze and confirm it once the SLM data for C01 is available.
J. Kissel, K. Izumi, J. Betzwieser Since we've last taken the full actuation characterization measurement suite (see LHO aLOG 20940, T1500383), we've revised a few bits of the measurement methodology such that we might have more successful measurements. I recall them here to help us remember what we plan to do. The major differences are as follows: (1) Order of measurements (LLO innovation). In order to try to make the suite as robust against environmental or other reasons for lock-loss, Joe has suggested that we take the full IFO portions of the suite *first* while the IFO is stable and fully operational. These "final results" are really the only measurements that *need* to be in the same lock stretch, such that we can make sure that the optical gain of the FULL IFO is the same. Only after all 6 of those sweeps are complete, *then* we intentionally break the IFO and begin the ALS DIFF and Free-swinging Michelson measurements with lesser configurations of the IFO. The full outline of the measurements is attached as a picture. (2) Merging of Free-swinging Michelson and ALS DIFF, IFO propogation measurements (LLO innovation). To-date, LHO has propagated the Free-Swinging Michelson absolute calibration from ITMX L2 stage to ETMX using the traditional single arm locked on red. However, during his last attempt, Joe had used ALS DIFF to propagate the the absolute calibration because (a) ALS DIFF is a more sensitive measurement and (b) we need to lock ALS DIFF anyways in our path propogate the ALS DIFF absolute calibration. (3) Using the "super actuator" ALS DIFF transfer function (LHO innovation). This was mentioned in LHO's last attempt (see 20940). The idea being to reduce the number of seeps by one, by taking advantage of a little loop math: From a simple diagram of the loop, one can show that L3 LOCK IN2 1 ----------- = ---------- L3 LOCK EXC 1 + G_DIFF which is true with any excitation at any point around the loop, just like is done "normally" done with a DARM IN2 / DARM EXC TF. Further, DIFF_PLL_CTRL 1 ------------- = ---------- x ETMX x DIFF L3 LOCK EXC 1 + G_DIFF one can immediately see that the absolute calibration of the super-actuator ETMX falls out of ratio of these two transfer functions, assuming you have the absolute calibration of DIFF such that you can divide it out (i.e. the [Hz/ct] and z:p = 40:1.6 Hz pair of the VCO, i.e. measurements (3) and (4), which we do, a priori). What's great, is that since you're using the same excitation, as long as you store both of these channels in the template, you can directly measure and export the transfer function ratio that you really want, DIFF_PLL_CTRL ------------- = ETMX x DIFF L3 LOCK IN2 and thus you've reduced two measurments into one.
BNS range is taking a small dip of ~5 Mpc. Probably due to an increasing traffic. Otherwise everything looks good. Wind speed < 10mph. Useism hanging out at 50th percentile. Ground motion in EQ band is trending downward. Couple of ETMY saturation since shift started.
Summary: There were 11 scheduled hardware injections: 1134345924 1 1.0 coherentbbh10_1128678894_ 1134348928 1 1.0 coherentbbh11_1128678894_ 1134353728 1 1.0 coherentbbh15_1128678894_ 1134354928 1 1.0 coherentbbh16_1128678894_ 1134356128 1 1.0 coherentbbh17_1128678894_ 1134357328 1 1.0 coherentbbh18_1128678894_ 1134359800 1 1.0 coherentbbh11_1128678894_ 1134361000 1 1.0 coherentbbh12_1128678894_ 1134362200 1 1.0 coherentbbh13_1128678894_ 1134363400 1 1.0 coherentbbh14_1128678894_ 1134364600 1 1.0 coherentbbh19_1128678894_ The first column is the start time of the injection. The second column is an integer that specifies that it was a CBC injection. The third column is the scale factor. And the fourth column is the beginning prefix of the parameter/waveform files. The waveform files can be found here: https://daqsvn.ligo-la.caltech.edu/svn/injection/hwinj/Details/Inspiral/H1/ and https://daqsvn.ligo-la.caltech.edu/svn/injection/hwinj/Details/Inspiral/L1/ The parameter files can be found here: https://daqsvn.ligo-la.caltech.edu/svn/injection/hwinj/Details/Inspiral/ Two of these happened in L1 only because H1 lost lock. Those two are: 1134348928 1 1.0 coherentbbh11_1128678894_ 1134357328 1 1.0 coherentbbh18_1128678894_ Segments: The segment database reports 9 injections for the H1:ODC-INJECTION_CBC:2 flag: 1134345929,1134345931 1134353734,1134353735 1134354934,1134354935 1134356134,1134356135 1134359806,1134359807 1134361005,1134361007 1134362206,1134362207 1134363405,1134363407 1134364606,1134364607 And 11 for L1:ODC-INJECTION_CBC:2 flag: 1134345929,1134345931 1134348934,1134348935 1134353734,1134353735 1134354934,1134354935 1134356134,1134356135 1134357333,1134357335 1134359806,1134359807 1134361005,1134361007 1134362206,1134362207 1134363405,1134363407 1134364606,1134364607
Parameter estimation started. Results will appear here https://www.lsc-group.phys.uwm.edu/ligovirgo/cbcnote/ParameterEstimationModelSelection/O1_PE/HardwareInjs_12162015 ping salvo or john for questions/comments