Displaying reports 51221-51240 of 85402.Go to page Start 2558 2559 2560 2561 2562 2563 2564 2565 2566 End
Reports until 04:13, Wednesday 29 March 2017
LHO General
patrick.thomas@LIGO.ORG - posted 04:13, Wednesday 29 March 2017 - last comment - 06:45, Wednesday 29 March 2017(35173)
Ops Owl Mid Shift Summary
08:47 UTC Made it to NLN after earthquake rang down. Found unexpected SDF differences (attached as sdf_1.png) and accepted them to go to observing. Lost lock 3 minutes later.
09:39 UTC Made it back to NLN. SDF differences returned but with reversed values and setpoints (attached as sdf_2.png). Accepted them and went to observing. Lost lock 8 minutes later.
10:41 UTC Made it back to NLN. No SDF differences this time. Went to observing. Noticed large peak around 8 Hz to about 10^-14 in DARM.

11:10 UTC Range is dropping. Peak around pcal line at ~35 Hz seems to be broadening and contracting over time (see darm.png attached). Something is not right.
Images attached to this report
Comments related to this report
patrick.thomas@LIGO.ORG - 06:45, Wednesday 29 March 2017 (35175)
Range drop appears to occur before traffic noise (plot of range on top of SEI BLRMS usually associated with traffic attached).
Non-image files attached to this comment
LHO General
patrick.thomas@LIGO.ORG - posted 00:25, Wednesday 29 March 2017 (35172)
Ops Owl Shift Transition
TITLE: 03/29 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Earthquake
OUTGOING OPERATOR: Nutsinee
CURRENT ENVIRONMENT:
    Wind: 17mph Gusts, 12mph 5min avg
    Primary useism: 0.11 μm/s
    Secondary useism: 0.38 μm/s 
QUICK SUMMARY:

Riding out the tail end of an earthquake with the possibility of more on the way.
H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 00:00, Wednesday 29 March 2017 (35171)
Ops EVE shift summary

TITLE: 03/29 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC

STATE of H1: Earthquake

INCOMING OPERATOR: Patrick

SHIFT SUMMARY: Most of the second half of shift was down due to earthquakes. Attempting to lock but not much luck so far. Maybe seismic is still a bit high. 

LOG:

22:33 Balers done for the day.

04:18 Lockloss, there were couple of 5+ magnitudes eathquakes happened around the same time, but the seismic raised sharply to the roof implied something close by. The 6.6M earthquake in Russia was probably it.

00:00 Handling off to Patrick.

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 21:28, Tuesday 28 March 2017 - last comment - 21:32, Tuesday 28 March 2017(35168)
Down due to 6.9M earthquake in Russia

Terramon predicts R-wave to be 29.3 micron. If this is correct, we are going to be down for a whole while.

I have set the ISI config to LARGE_EQ_NOBRSXY since BRSY was still damping (and now rung up).

Images attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 21:29, Tuesday 28 March 2017 (35169)

Correction: USGS reported 6.6M, not 6.9M. I've attached another prediction from Terramon.

Images attached to this comment
nutsinee.kijbunchoo@LIGO.ORG - 21:32, Tuesday 28 March 2017 (35170)

In addition, there're couple of 5+ magnitude earthquake in Indonesia and Panama prior to the Russia earthquake. Not helping.

Images attached to this comment
H1 AOS (DetChar, PEM)
robert.schofield@LIGO.ORG - posted 19:59, Tuesday 28 March 2017 - last comment - 09:39, Wednesday 29 March 2017(35166)
Strong coupling of 8-18 Hz input beam tube vibration to the 70-200 Hz band of DARM can explain truck, fire pump, and HVAC coupling

Summary: Injections suggest that vibration of the input beam tube in the 8-18 Hz band strongly couples to DARM and is the dominant source of noise in the 70-200 Hz band of DARM for transient truck and fire pump signals, and likely also for the continuous signal from the HVAC. Identification of the coupling site is based on the observation that local shaking of the input beam tube produces noise levels in DARM similar to those produced by global corner station vibrations from the fire pump and other sources, for similar RMS at an accelerometer under the Swiss cheese baffle by HAM2. The local shaker injections were insignificant on nearby accelerometers or HEPI L4Cs, and HEPI excitations cannot account for the noise, supporting a local, off-table coupling site in the IMC beam tube.  In addition, local vibration injections occasionally produce a 12 Hz broad-band comb, which is also produced by trucks and the fire pump, possibly indicating a 12 Hz baffle resonance.  While the Swiss cheese baffle seems the most likely coupling site, we have not yet eliminated the eye baffle by HAM3.

Several recent observations have suggested that we are limited by noise in the 100 Hz region that is produced by vibrations in the 10-30 Hz region.  There was the observation that our range increased by a couple of Mpc when the HVAC was shut down, ( https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=32886 ), and, additionally, the observations of noise from the fire pump and from trucks.

I noticed that the strongest signals in DARM produced by the fire pump and trucks had peaks that were harmonics of about 12 Hz. I injected manually all around the LVEA and found that the input beam tube was the one place where I could produce a 12 Hz comb in the 100 Hz region (injections were sub-50 Hz). Figure 1 shows that a truck, the fire pump, and my manual injections at the input beam tube produced similar upconverted noise in DARM.

I also used an electromagnetic shaker on the input beam tube.  Figure 2 is a spectrogram showing a slow shaker sweep and the strong coupling in the 8-18 Hz band. I wasn’t able to reproduce the  broad 12 Hz comb with the shaker, possibly because, as mounted, it didn’t couple well to the 12 Hz mode. But the broad-band noise produced in DARM by the shaker is more typical of trucks and the fire pump: only occasionally does the 12 Hz comb appear.  One possibility is that the bounce mode of the baffle is about 12 Hz.

Figure 3 shows that, for equivalent noise in DARM, the RMS displacement from the shaker and the fire pump were about the same at an accelerometer mounted under the Swiss cheese baffle by HAM2. Figure 4 shows that the shaker vibration is local to the beam tube. While the shaker signal is large on the beam tube accelerometer, it is almost lost in the background at the HAM2 and 3 accelerometers and the HAM2, 3 L4Cs.  Finally, the failure to reproduce the noise with HEPI injections, both during PEM injections at the beginning of the run and a recent round by Sheila, further support the off-table source of the noise.

While everything is consistent with coupling at the Swiss cheese baffle near HAM2, we haven’t eliminated the eye baffle near HAM3. This might be done by comparing a second accelerometer under the eye baffle to the one under the Swiss cheese baffle, but I didn’t have another spare PEM channel.

If it is the Swiss cheese baffle, it might be worth laying it down during a vent. Two concerns are the blocking of any beams that are dumped on the baffle, and the shiny reducing flange at the end of the input beamt ube that would be exposed.

An immediate mitigation option is to try and move beams relative to the Swiss cheese baffle while monitoring the noise from an injection. Sheila and I started this but ran out of commissioning time and LLO was up for most of the weekend so I didn’t get back to it.  If someone else wants to try this, either turn on the fire pump or, for even more noise in DARM, the shaker by HAM3 (the cable goes across the floor to the driver by the wall, enter 17 Hz on the signal generator and turn on the amp, it should still be set).

Shaker injections have shown the input beamtube to be sensitive for some time ( https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=31016). During pre-run PEM injections, an 8 to 100 Hz broad-band shaker injection on the input beamtube showed strong coupling. However the broad-band injection was smaller in the sensitive 10-18 Hz band then in other sub-bands and so the magnitude of the up-converted coupling from this narrow sub-band was not evident. When we have detected upconversion during PEM injections in the past, we have narrowed down the sensitive frequency band with a shaker sweep, but, for the input beam tube, we didn’t get to this until last week.

Figure 5 shows fire pump, trucks and the HVAC on input beam tube accelerometers and DARM.

Sheila, Anamaria, Robert

Non-image files attached to this report
Comments related to this report
peter.fritschel@LIGO.ORG - 06:18, Wednesday 29 March 2017 (35174)

The current plan of the stray light upgrade team is to completely remove the aluminum panels of the Swiss cheese baffle, but leave the oxidized stainless outer ring to shield the flat shiny reducing flange. This is planned for post-O2.

keita.kawabe@LIGO.ORG - 09:39, Wednesday 29 March 2017 (35182)

Seems like 12.1Hz harmonics observed yesterday was also due to this?

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=35136

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 19:58, Tuesday 28 March 2017 (35167)
Ops EVE mid-shift summary

Been locked and Observing for 3 hrs 44 mins. Wind is coming down. BRSY is still not in use. Not much else going on.

H1 ISC (DetChar)
keith.riles@LIGO.ORG - posted 18:32, Tuesday 28 March 2017 - last comment - 16:38, Wednesday 29 March 2017(35146)
Narrow lines in H1 - Increased amplitudes and new combs in recent data
It appears that some maintenance work on Tuesday March 14 led to degradation
with respect to narrow lines in H1 DARM. The attached inverse-noise-weight spectra 
compare 1210 hours of data from the start of O2 until early morning of March 14 with 
242 hours since that time.

Summary of substantial comb changes:

The comb with 0.9999-Hz spacing nearly aligned with N + 0.25 Hz (N = 15-55) is stronger.

There is a new comb with 0.999984-Hz spacing visible nearly aligned with N + 0.75 Hz (N = 41-71)

There is a new comb with 1.0000-Hz spacing visible at N - 0.0006 Hz (N = 104-125)

Much activity was reported in the alog for March 14, but what jumps out at me
are two references to HWS work: here and here. 

Are there HWS cameras running during observing mode? 

I had thought those things were verboten in observing mode, given their
propensity to make combs.

Fig 1: 20-50 Hz comparison (before and after March 14 maintenance)
Fig 2: 50-100 Hz (before and after March 14 maintenance)
Fig 3: 100-150 Hz  (before and after March 14 maintenance)

Attachment has full set of comparison sub-bands up to 2000 Hz with both A-B and B-A orderings to make clear which lines are truly new or louder.
Images attached to this report
Non-image files attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 11:23, Wednesday 29 March 2017 (35185)TCS

We didn't change any configuration of the HWS camera that day. All HWS cameras have been turned on since the beginning of O2 and have been hooked up to the external power supplies (alog30799) since O1. Since then I haven't heard any complains about HWS cameras making noises. HWS cameras ON has been a nominal configuration since the beginning of O2.

keith.riles@LIGO.ORG - 11:50, Wednesday 29 March 2017 (35187)DetChar
I was asked via e-mail if this problem might have started later in March
with the replacement of the Harmonic Frequency Generator. but explicit
comparisons of daily spectra below show conclusively that the N + 0.25 Hz and
N + 0.75 Hz combs are not present before Tuesday maintenance ("March 14" ends
at 6:00 a.m. CDT on March 14 in the FSCan dating convention), but are present 
individually on March 15, 16 and 17. The new  N Hz comb reported above is too weak
to show up well in a single day's measurement with 1800-second SFTs.

I was also told via e-mail (and just saw Nutsinee's note above) that HWS systems
are run routinely during observing mode and that no configuration changes 
were made on March 14 (although there are some new cables in place). So perhaps 
there is a different culprit among the March 14 activities.

Fig 1: Zoom in of line at 28.25 Hz
Fig 2: Zoom in of line at 38.25 Hz
Fig 3: Zoom in of line at 88.75 Hz
Fig 4: Zoom in of line at 98.75 Hz
Images attached to this comment
evan.goetz@LIGO.ORG - 13:25, Wednesday 29 March 2017 (35190)DetChar
Looking back at the aLOGs from the March 14th period, some possibilities of activities that may be related stick out:

1) PSL bullseye detector for jitter studies installed
2) ITMY OpLev power supply moved
3) New cables for GigE and camera installed
4) ETM OpLevs laser power increased
5) CPS electronics power cycled and board reseated on WBSC1 ITMY
6) DBB powered up and supposedly powered off; is it still on?? Kiwamu says he is 99% sure the DBB is off
ansel.neunzert@LIGO.ORG - 16:38, Wednesday 29 March 2017 (35201)

It looks like all three combs jump in magnetometers at EX and EY between 3/14 and 3/15, but don't have any notable presence in the CS magnetometers.

More clues: at EX, there was a recent change point in the combs (strength drop) between 2/28 and 3/1. At EY, there was one (also a strength drop) between 3/7 and 3/8. These are Fscan dates, covering 24 hours back from the morning when they were run-- in any case, it looks like two prior Tuesdays may be involved. 

As a side note, the 1 Hz comb with 0.5 Hz offset mirrors the stated behavior in several channels, at least one magnetometer at EX and one at EY.

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 16:44, Tuesday 28 March 2017 (35162)
CDS Maintenance summary, Tuesday 28th March 2017

WP6540 Reduce cronjobs on HEPI Pump Controllers

Dave:

Completed EY config, applied config to EX and L0.

WP6539 Relocate HWS frame grabber card from EX to MSR1

Carlos, Nutsinee, Dave:

Card was relocated, but we appear to have driver issues on the spare HWS machine. Carlos is working with TCS to install this machine from scratch and put the configuration into puppet.

WP6543 Upgrade cdslogin to Debian8

Carlos, Jonathan, Jim, Dave

cdslogin was upgraded from U12 to Deb8.

WP6544 New code h1calcs and h1omc

Daniel, Kiwamu, Jim, Dave:

New code was installed on h1omc and h1calcs. A new dolphin sender was installed on omc, with corresponding receiver on calcs. Two 4k DQ channels were added to the DAQ, along with a few dozen slow channels.

WP6546 New PCAL guardian node

TJ, Rick, Sudarshan

A new temporary guardian node named HIGH_FREQ_LINES was added

WP6519 Put seismon channels into DAQ.

Not done, defer to later time

H1 CDS
david.barker@LIGO.ORG - posted 16:34, Tuesday 28 March 2017 (35161)
cdslogin machine upgraded from U12.04 to Debian 8

Carlos, Jonathan, Jim, Dave:

the sshd and alarms machine cdslogin was upgraded from Ubuntu 12.04LTS to Debian 8 (Jessie) today. This is a 2FA sshd server machine, which also runs EPICS CA client code to send vacuum and fmcs alerts to lho staff cell phones as text messages. Due to Carlos and Jonathan's hard work in putting this configuration into puppet, the entire upgrade only took a couple of hours.

H1 SEI
hugh.radkins@LIGO.ORG - posted 16:17, Tuesday 28 March 2017 - last comment - 12:05, Friday 31 March 2017(35160)
Exiting BRSY Remote Desktop trips ISI! But not always, eh!

Was logged on checking health from the earlier invasive work.  Everything was working fine so I closed (pushed X) on the remote desktop shell.  The BRS output went to never never land and the ISI tripped.  This of course did nothing useful for the the IFO or Observation mode.

When I logged back onto the BRSY, it was still running but giving some errors and the output was still very rung up.  I am not sure which was causing which though.  Following the BRS2 Manual (T1600103), restarted the TwinCat code, killed the old occurance and restarted the C#, and finally the EPICS.  Exited the session the same way and this time it survived.  Yikes!

The amplitude is still a bit large with the camera image swinging into the reference image on the edge.  When that stays off the edge during its cycle, the BRS will be useful again.

 

Comments related to this report
hugh.radkins@LIGO.ORG - 17:34, Tuesday 28 March 2017 (35164)

The BRSY is now damping itself down and is no longer swinging out of range.  But it is still getting itself under control.  It is coming down quickly but may be some time.  Operators should feel free to contact me if they aren't sure if it can be returned to service.

krishna.venkateswara@LIGO.ORG - 12:05, Friday 31 March 2017 (35247)

It is strongly advised to not login to the BRS machines when they are being used. This is because the spike in CPU-use disrupts the autocollimator fitting routine. This causes ~seconds long delays in the tilt output which affects the tilt-subtraction and so on.

LHO General
vernon.sandberg@LIGO.ORG - posted 16:13, Tuesday 28 March 2017 (35158)
Work Permit Summary for 2017 March 28
Work Permit Date Description alog/status
6546.html 03/27/17 04:05 PM Create and test a Guardian node that will turn on and adjust a set of Cal lines for later analysis. 35153
6545.html 03/27/17 01:43 PM Inject blip-like glitches to test performance of NOISEMON channels 35116
6544.html 03/27/17 01:20 PM We will add a new signal path in h1omc and h1calcs models in order to implement the DCPD cross correlation scheme (whose ECR, E1700107, has been approved). Because this implementation is independent of the main interferometer control signals, we don't expect any impact on locking or sensitivity. DAQ restart is required. 35156, 35139, 35115
6543.html 03/27/17 09:56 AM Upgrade LHO CDS login servers cdsssh, cdslogin and opslogin to Debian8. Needed because current OS is near end-of-support. 35119
6542.html 03/27/17 09:03 AM Repair underground water leak on feed line to VPW. This will require digging up asphalt and digging down to the PVC line.  
6541.html 03/27/17 08:40 AM Perform scheduled maintenance to scroll compressors at Y-MID vent/purge-air supply skid. Maintenance activity will require for the compressors to run for brief periods of time to check compression. Lock-out/tag-out power to skid as required. 35149
6540.html 03/23/17 12:57 PM Reduce crontab tasks on h1hpipumptrcl[l0,EX] to be that used on EY unit. Check local clocks are correct. 35141
6539.html 03/23/17 11:36 AM We would like to "borrow" a HWS PCIe card from one of the end stations (whichever one we can get to on Tuesday) and put it on the spared HWS machine at the corner station so we can get HWSY running. Transfer of PCIe card completed.
6538.html 03/23/17 11:03 AM Remove the INSTAIR alarms for the MX compressor from the cell phone text alarm system.  
6537.html 03/23/17 07:04 AM Swap out the harmonic frequency generator with a spare to see if this is the cause of glitches in the RF 45. Swap complete, now monitor for glitches.
       
Updates to previous Work Permits      
6527.html 03/19/17 09:36 PM Access to pcal system and camera to take pictures and possibly move the pcal beams 34980, 35137
H1 CAL (TCS)
david.barker@LIGO.ORG - posted 16:13, Tuesday 28 March 2017 (35159)
ITMX HWS had duplicate channels for a while today

Aidan, Nutsinee, Dave:

during the HWS image grabber card swap this morning, a duplicate of the ITMX EPICS  IOC was running on the h1hwsmsr1 machine. The DAQ EDCU incorrectly connected to the duplicate and had bad data between the times 19:45 and 22:56 UTC. I powered h1hwsmsr1 down and the EDCU reconnected to the correct channels sometime later. 

H1 ISC
kiwamu.izumi@LIGO.ORG - posted 16:05, Tuesday 28 March 2017 (35156)
Infrastructure for DCPD cross correlation installed

WP 6544, ECR E1700107,

Related alogs: 35115, 35139

We have installed the infrastructure in the frontend models to relatively easily produce the DCPD cross correlation spectrum.

It seems to do what it is supposed to do. See the first attachment for demonstration of data acquisition and calibration using DTT.


[Additional model changes]

In addition to what we have reported yesterday (35115), we implemented two additional minor changes today.

[Front end settings and other settings]

Also, I have made a DTT template in which the frequency-domain calibration (33161) is applied to all the relevant spectra. The template is saved at

/opt/rtcds/userapps/release/isc/h1/scripts/CrossCorrTemplate.xml

Two MEDM screens are newly made for this infrastructure:

A screenshot of each MEDM screen is attached as well. They are saved in common medm directories at

/opt/rtcds/userapps/release/omc/common/medm/OMC_NULL_READOUT.adl

/opt/rtcds/userapps/release/cal/common/medm/CAL_CS_CUST_CROSSCORR.adl

[A quick verification: it seems OK]

To check whether the new infrastructure is doing the right thing or not, I exported the spectra from the DTT (the ones shown in the first attachment). I then computed the difference between the ordinary DARM spectrum and the cross correlated spectrum by subtracting one from the other. If things are correct, this leaves only sensing noise which should be dominated by shot noise at most of frequencies. The result is shown in the last attachment-- the difference seems reasonably smooth in its spectral shape as expected at most of frequencies.

The are a few points/regions where the difference deviated from shot noise. The peaks/valleys at 35 Hz, 60 Hz, 350 Hz and 500 Hz and low frequency wall below 30 Hz are reasonably suppressed by at least roughly 20 dB from the ordinary DARM which may be limited by lack of number of averages. On the other hand, the peak at 180 Hz was reduced only by 6 dB or so. I am not sure why. Otherwise, it looks reasonably good.

Images attached to this report
H1 General
edmond.merilh@LIGO.ORG - posted 16:01, Tuesday 28 March 2017 (35129)
Shift Summary - Day

TITLE: 03/28 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Nutsinee
SHIFT SUMMARY:

LOG:

15:06 Intention bit set to "Preventative Maintenance"

15:07 Peter and Jeff B to PSL enclosure

15:08 Fire Dept. on site smoke/heat testing

15:15 Hugh to EX

15:35 Travis to EX for PCAL work

15:50 Fil to EX for Interlock cabling.

15:53 Christina and Karen to out buildings

15:55 Gerardo to mid-stations

16:00 NORCO LN2 Y-ARM

16:13 Jeff B going to End Stations for FAMIS dust monitor checks

16:13 Hugh back from EX?

16:31 TJ doing Charge measurements on ETMY

16:34 More FD personell on site 

16:40 Taking FD to CER

16:43 NORCO LN2 X-ARM

16:45 More fire personnell on site

16:45 Betsy to LVEA for parts. HWS work is postponed.

17:04 Travis back from EX

17:05 Karen leaviong EY

17:09 Jeff B back

17:14 Carlos out to EX to retrieve HWS card

17:31 Bubba bringing FD into LVEA

17:44 Dick into LVEA - non invasive

17:44 Carlos reported back from EX

17:53 Fire testing in OSB is done

17:54 Hugh into CER

18:00 Bubba out of LVEA with FD

18:28 DAQ restart

18:38 Paradise Water on site for delivery

19:06 FIll back 

19:07 Bailing still going on

21:31 Betsy, Travis and TJ to MX

22:34 Lockloss - yet undetermined but possibly linked to some BRS issue that Hugh was doing. He and Jeff K are hashing it out.

22:41 Switched ISI_CONFIG back to NOBRSY and recovered ETMY ISI to resume.

22:49 TJ, Betsy, and Travis back

23:00 Handing of to Nutsinee

H1 TCS (TCS)
aidan.brooks@LIGO.ORG - posted 15:38, Tuesday 28 March 2017 (35157)
HWS-ITMX EPICS channels are not updating because of H1HWSMSR1

In prepping for the high-power PRMI test tomorrow, I noticed that the HWS-ITMX EPICS channels are not being updated in the MEDM screens. The gradient field data is still being written to file.

Looking at the frames, we can see normal data until 19:47 UTC (around 12:47PM PDT).

I ran a CAGET on the H1HWSMSR and can see the data just fine in the channels. The same CAGET on OPSWS4 returns zero.

Dave Barker and Nutsinee are looking into this.

 

Images attached to this report
H1 CDS (CAL, GRD)
thomas.shaffer@LIGO.ORG - posted 14:30, Tuesday 28 March 2017 - last comment - 18:12, Tuesday 28 March 2017(35153)
Added new HIG_FREQ_LINES PCal node

Sudarshan, Shaffer

Today I created, started, and tested a node that Sudarshan made to change some EX PCal lines every 24hrs while we are not locked. The code will wait for the gps time to get greater than a day since its last change, then it will wait till the IFO is not locked, and finally it will adjust the frequency by 500hz and jump to waiting for a day to go by. Once the frequency has reached 5100hz it will then hang our in the FINISHED state. Here, Sudarshan can let us know what he wants to do with it.

Attached are the graph for the node and the Guardian overview

Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 18:12, Tuesday 28 March 2017 (35165)CDS, DetChar, GRD
Just a few points of verification, clarification, and tagging DetChar, letting them (especially the CW group) know this sweeping PCAL X calibration line has been turned on.

I attach a full and zoomed CAL-DELTAL spectrum against a PCALX spectrum (among the other usual things from the front wall's sensitivity FOM). 

Note that Pulsar injections are on-going, and it doesn't look like these features will interfere. This calibration line regime is sticking to the 2000 to 5000 Hz regions, and pulsar injections only go up to 1991.2 Hz (For a reminder of the full list of pulsar injection frequencies, see LHO aLOG 27642.

The starting frequency is 2001.3 Hz, and the starting excitation amplitude is 30000 [ct], and has been hard-coded to remain this amplitude for all frequencies. The excitation frequency can be tracked using EPICs via this channel: 
    H1:CAL-PCALX_PCALOSC1_OSC_FREQ
and you can see a fast-channel version of the requested output here:
    H1:CAL-PCALX_EXC_SUM_DQ

The guardian code for this node lives here 
/opt/rtcds/userapps/release/cal/h1/guardian/HIGH_FREQ_LINES.py

and is attached for ease of reference.

After some initial debugging, it guardian's log suggests that TJ left the frequency at 2001.3 starting at 2017-03-28 17:16:31 UTC, though it looks like the frequency has only been stable at 2001.3 since 19:49:00 UTC. TJ has the CHECK_IFO_STATUS state look whether the ISC_LOCK guardian's state is lower than 11, 
which means the excitation is killed if we're in
    - INITIAL ALIGNMENT
    - DOWN
    - IDLE
    - LOCKLOSS
    - LOCKLOSS_DRMI
    - INIT
but maybe we want to rethink this, because it seems to turn off the excitation at unnecessary times (see attached dataviewer trend, where the guardian has changed the frequency twice since TJ left it).
Images attached to this comment
Non-image files attached to this comment
H1 CAL (CAL, ISC)
evan.goetz@LIGO.ORG - posted 11:23, Tuesday 21 March 2017 - last comment - 17:11, Tuesday 28 March 2017(34967)
Trends of H1 optical response parameters for ER10 and thus far in O2
Using MCMC fitting to the sensing function measurements made in ER10 and O2, we can establish an estimate on the variation of the optical response parameters. The table below gives the typical (simple mean), maximum, and minimum of the measured maximum a posteriori values from the MCMC fits.

Parameter             typical    maximum    minimum
---------------------------------------------------
Gain (ct/m)           1.143e6    1.166e6    1.085
Cavity pole (Hz)      347.1      358        341
Time delay (usec)     0.5        2.5        -1.3
Detuned spring (Hz)   7.3        8.8        4.9
Detuned spring 1/Q    0.04       0.08       1e-3
This covers measurement dates from Nov 07 2016 through Mar 06 2017. Attached are plots showing these trends for ER10 and O2. Note that I have added--where possible--the GDS calculated values for kappa_C and f_c (black crosses). Note that these values do not come with error bars because the uncertainty would need to be computed from the measurement uncertainty of what goes into the calculate of kappa_C and f_c. It would be useful to have calibration lines running during the measurements to see if there is any trend or drift during the measurements themselves.
Non-image files attached to this report
Comments related to this report
evan.goetz@LIGO.ORG - 17:11, Tuesday 28 March 2017 (35163)
Attached are trend plots for all ER10 and O2 measurements.

The plots are stored at:
${CALSVN}/aligocalibration/trunk/Runs/O2/H1/Results/SensingFunctionTFs

The script to produce plots is:
${CALSVN}/aligocalibration/trunk/Runs/O2/H1/Scripts/SensingFunctionTFs/runSensingAnalysis_H1_O2.m
Non-image files attached to this comment
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