Displaying reports 1441-1460 of 85514.Go to page Start 69 70 71 72 73 74 75 76 77 End
Reports until 08:50, Monday 25 August 2025
H1 SUS
oli.patane@LIGO.ORG - posted 08:50, Monday 25 August 2025 (86544)
SR3 P estimator blend filters updated

I have updated the blend filters used for the SR3 P estimator to add in the osem damping for the P peaks at 0.6 and 0.7. The filters I installed were the ones Brian made last Thursday, pit_v2. The filters were installed into the filter banks SUS-SR3_M1_EST_P_FUSION_MEAS_BP and SUS-SR3_M1_EST_P_FUSION_MODL_BP with the OSEM and model blend filters, respectively. They were placed in FM2, and I swapped over from FM1 to FM2 for both of them. These changes were updated in Observe and Safe sdf.

We turned the estimator on with these new filters at 2025-08-25 15:42UTC.

Images attached to this report
H1 General
oli.patane@LIGO.ORG - posted 07:30, Monday 25 August 2025 (86542)
Ops Day Shift Start

TITLE: 08/25 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 152Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 2mph Gusts, 1mph 3min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.09 μm/s
QUICK SUMMARY:

Observing at 151Mpc and have been Locked for over 4.5 hours. Commissioning today starting at 15:30UTC

X1 SEI (SEI)
richard.savage@LIGO.ORG - posted 06:36, Monday 25 August 2025 - last comment - 14:23, Wednesday 27 August 2025(86541)
Measurement of reflectivity of SPI beamsplitters

DriptaB, TonyS, RickS

Responding to a request from Jeff Kissel, we modified the Pcal measurement setup and used the standard Pcal analysis scripts to measure the reflectivity of two types of beamsplitters that have been procured for the SPI upgrade: 50/50 and 85/15 beamsplitters (two of each).  Usually we are interested in the ratios of the responsivities of the two power sensors, but the same measurement results can be combined differently to yield the beamsplitter ratio.
 
NOTE: The Pcal system wavelength is 1047 nm, not 1064 nm.
 
The boxes containing the optics were labeled:
SPI PWR BS, 1064nm
50R:50T 45 DEG-Ppos
Batch 16075HA1
and
SPI PWR BS, 1064nm
85R:15T 45 DEG-Ppos
Batch 16075HA1
 
We measured two of each of the two beamsplitter types (50/50 and 85/15).
 
The measurement results are shown in the plots attached below.  Note that HOP stands for "hundredth of a percent."
 
The measured reflectivities are:
 
50R/50T #1, two measuremetns: R = 0.4830 ± 0.002 %; R = 0.4830 ± 0.002 %
50R/50T #2R = 0.4827. ± 0.002% 
 
85R/15T #1 two measurements: R = 0.8624 ± 0.0005%; R = 0.8625 ± 0.0005 %
85R/15T #2R = 0. ± 0.8599 ± 0.0004 %
 
Given the small specified wedges in the beamsplitter substrates, the ghost beams from the AR surface would likely pass through the entrance apertures on the power sensors (one inch diameter) and add to the received power in both reflection and transmission.  However, the AR surface reflectivty appeared to be below the specified 0.1 %.  We were not able to identify and measure the power in the beams reflecting from the AR surface.  We will have another look when we break down the measurement setup.
 
Measurement setup and details:
 
We increased the Pcal Optical Follower Servo offset  to give about 600 mW in each of the two output beams.  We blocked one of the output beams and used the other beam for the beamsplitter measurements. 
 
We aligned the laser steering mirror inside the transmitter module such that this beam propagates parallel to the table surface and along a row of holes in the optical table.
 
We found that the Pcal module output beam had some stray light of unknown origin outside the main beam (mostly three spots - see photo below) so we installed an aperture upstream at the Tx module output to block this stray light.
 
We installed a Karl Lambrect TFPC-12-1047nm thin film polarizing beamsplitter cube and aligned it such that the plane of the cube is parallel to the optical table surface.  The Pcal Tx module output beams are nominally polarized paralllel to the surface of the optical table, but we installed this BS cube and carefully aligned it's plane of incidence to ensure that the polarization would be parallel to the plane of incidence of the beamsplitter to be tested.
 
We then installed the beamsplitter to be tested in the transmitted (polarized parallel to the surface of the table) beam and aligned it such that  the plane of incidence is parallel to the optical table surface and the reflected beam is parallel to a row of holes on the optical table (45 deg. AOI, p-pol) and centered on the entrance aperture of one of the Pcal integrating spheres.  The power incident on the beamsplitter was measured to be 570 mW.
 
The beams transmitted by the beamsplitter to be tested was reflected by a Pcal HR mirror (Precision Photonics / ATFilms Y1S-1025-45, Lot# WO22401, ITM100509, Run# 213472) and aligned to propagate along a row of holes and be centered on the entrance aperture of the second Pcal integrating sphere.  The fractional power transmission of this HR mirror was measured twice to be: 3.2e-4 and 3.9 e-4.  Average = 3.6e-4. We correct for this loss of power in the transmitted beam in the BS reflectivity calculations.
 


 

Images attached to this report
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 14:23, Wednesday 27 August 2025 (86599)CAL
J. Kissel, quoting R. Savage:

A few extra explanatory words for the uninitiated on how this measurement works / how the results were derived:

The uncertainties reported are the statistical variations for the measurements we made, highlighted in the attached plots.  The authors have not attempted an assessment of potential systematic errors.  

I suspect that the largest sources of systematic error would likely result from 
   - deviations of the incident polarization (as defined by the plane of incidence of the beamsplitter) from pure p-pol and 
   - deviations of the Angle of Incdence from 45 deg.  
I also suspect that the errors we might have in this regard are much smaller than what you will have in the SPI installation given the much longer path lengths measured here vs. the SPI in-chamber setup.  The next largest source of systematic errors might be 
   - the temperature dependence of the reflectivity of the beamsplitters.  
We did not attempt to quantify this.  We do measure, and correct for, the temperature dependence of the power sensor responsivities and their dark levels during the measurements. I suspect these will have a negligible impact on the measurement results reported for this effort.

Regarding the measurement setup and math to derive the answers:
The description of the responsivity ratio measurements given in  D. Bhattacharjee et al., CQG 38.1 (2020): 015009 (P2000113) -- specifically the caption and text surrounding Figure 3 -- is the gist of the measurement method - simply replace  "... the square root of the product of the ratios... replaced with "... the square root of the quotient of the ratios ..." from that caption. This yields the beamsplitter ratio, T/R, rather than the responsivity ratio of the two integrating sphere PDs that the PCAL team is after. (called \alpha_{W1W2} in the caption, but could also be any two responsivities, \alpha_{WG}, \alpha_{RW}, etc).   
Only 
 - laser power variations that occur over the difference between times of recording the two power sensor outputs (less than 0.1 sec)
 - variations of the reflectivity of the BS or the responsivities of the two power sensors that occur over the time difference between measuring in the A-B and B-A configurations (less than 40 seconds) 
should impact the measurements.

We record four time series: the output of both power sensors (in volts) and the temperatures (in volts) recorded by sensors on the circuit boards of both power sensors. The any temperature variation in the power sensor time series is normalized out, leaving two conditioned voltage time series for a given physical arrangement of PDs -- and thus are the (power) transmission, T, and (power) reflection, R, of the beam splitter (the A path's HR steering mirror -- that reflects light 90 [deg] to be parallel with the B path -- reflectivity is measured and taken into account as well -- see details below). The responsivity of these PCAL integration sphere + photodiode assemblies -- here we'll call them \rho_1 and \rho_2 -- is known to extremely high accuracy.

Each data point you see in the plot is the ratio of [[ the BS ratio (T/R) resulting from one set of (two conditioned) time series when the sensors are in one configuration ]] and [[ a second BS Ratio (T/R) when PD positions have been swapped ]], i.e. accounting for
    - what was the T time series (from \rho_1 PD in the B position; the "A-B" configuration) becomes the R time series (from \rho_1 PD in the A Position; the "B-A"  configuration).
    - what was the R time series (from \rho_2 PD in the A position; the "A-B" configuration) becomes the T time series (from \rho_2 PD in the B Position; the "B-A" configuration), and conversely


So the math is 
    T/R = sqrt {  [(P x T x rho_1) / (P x R x rho_2)]_{A-B} / [(P x R x rho_1) / (P x T x rho_2)]_{B-A} } = sqrt{ (T/R)^2 }
where again 
    - P is the input power (in [W]),
    - R and T are the beam splitter reflectivity and transmission (in power; [W]), 
    - \rho_1 and \rho_2 are the two different working standards, and
    - the subscript _{A-B} and _{B-A} are the answers in the two different physical configurations of the integrating spheres.
Assuming no other loss or absorption, then the (power) reflectivity, R, displayed on the plots is 
    R + T = 1
    1 + T/R = 1/R
    R = 1 / (1 + T/R)

As noted earlier, the powers (sensor outputs) for the transmitted path are multiplied by about 1.00035 to account for the transmissivity of the the HR mirror that reflects the transmitted beam to the power sensor.  
H1 General
anthony.sanchez@LIGO.ORG - posted 22:05, Sunday 24 August 2025 (86540)
Sunday Ops Eve Shift End

TITLE: 08/25 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 155Mpc
INCOMING OPERATOR: TJ
SHIFT SUMMARY:
H1 has been locked for 41+ hours
All systems still running well.
No events to report.

LOG:
No Log

 

H1 SEI
anthony.sanchez@LIGO.ORG - posted 20:04, Sunday 24 August 2025 (86539)
BSC & HAM CPS Spectra

H1 ISI CPS Sensor Noise Spectra Famis 26545

No obvious  or alarming changes from the last CPS Sensor Noise Spectra.

Non-image files attached to this report
H1 General
anthony.sanchez@LIGO.ORG - posted 16:36, Sunday 24 August 2025 (86538)
Sunday Ops Eve Shift Start

TITLE: 08/24 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 10mph Gusts, 4mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.09 μm/s
QUICK SUMMARY:
H1 has been locked for 35 hours and 45 min.
All systems appear to be running smoothly.
 

 

H1 General
oli.patane@LIGO.ORG - posted 16:32, Sunday 24 August 2025 (86537)
Ops Day Shift End

TITLE: 08/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY: Observing at 152 Mpc and have been Locked for almost 37 hours. Once again nothing at all happened during my shift
LOG:

no log

LHO VE
david.barker@LIGO.ORG - posted 10:12, Sunday 24 August 2025 (86536)
Sun CP1 Fill

Sun Aug 24 10:09:25 2025 INFO: Fill completed in 9min 21secs

 

Images attached to this report
H1 General
oli.patane@LIGO.ORG - posted 07:38, Sunday 24 August 2025 - last comment - 07:46, Sunday 24 August 2025(86534)
Ops Day Shift Start

TITLE: 08/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 2mph Gusts, 0mph 3min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.10 μm/s
QUICK SUMMARY:

Currently Observing at 150Mpc and have been Locked for almost 27 hours

Comments related to this report
oli.patane@LIGO.ORG - 07:46, Sunday 24 August 2025 (86535)

Looks like there were a couple of GRB-Short alerts that came in early this morning (but no superevent candidates :( ):

2025-08-24 11:25 UTC GRB-Short E592892

2025-08-24 13:38 UTC GRB-Short E593158

H1 General
anthony.sanchez@LIGO.ORG - posted 22:00, Saturday 23 August 2025 (86533)
Saturday Night Ops shift End.

TITLE: 08/24 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 152Mpc
INCOMING OPERATOR: TJ
SHIFT SUMMARY:
H1 has been locked for 17+ hours.
All systems are still running smoothly.
No events to report.

LOG:
No Log

 

H1 General
anthony.sanchez@LIGO.ORG - posted 17:00, Saturday 23 August 2025 (86532)
Satuday Night Ops Shift

STATE of H1: Observing at 153Mpc
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 14mph Gusts, 9mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.15 μm/s
QUICK SUMMARY:
H1 has been locked for 12 + Hours.
All systems seem to be running smoothly.
Secondardy useism looks to be falling & Wind forcasting is single digit wind speeds for the night, so it looks like a good night for Observing.
 

H1 General
oli.patane@LIGO.ORG - posted 16:30, Saturday 23 August 2025 (86531)
Ops Day Shift End

TITLE: 08/23 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 153Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY: We're Observing at 153 Mpc and have been Locked for almost 12 hours. Besides going out of Observing for the calibration measuremnts, I haven't had to do anything for the ifo. We had a GRB-Short alert come in at 20:11 UTC for E592892
LOG:

14:30 UTC Observing and have been Locked for almost 3 hours
18:30 Dropped Observing to run calibration
19:02 Back into Observing
20:11 GRB-Short E592892

Start Time System Name Location Lazer_Haz Task Time End
17:09 EPO Sam + tour Overpass n Passing over 17:39
H1 CAL
oli.patane@LIGO.ORG - posted 12:09, Saturday 23 August 2025 (86530)
Calibration Measurement August 23, 2025

Calibration suite run with IFO fully thermalized, having been Locked for over 6.5 hours.

calibration monitor screen

pydarm report 20250823T183838

Broadband
2025-08-23 18:31:57 - 18:37:08 UTC
/ligo/groups/cal/H1/measurements/PCALY2DARM_BB/PCALY2DARM_BB_20250823T183157Z.xml

Simulines
2025-08-23 18:38:37 - 19:01:56 UTC
/ligo/groups/cal/H1/measurements/DARMOLG_SS/DARMOLG_SS_20250823T183838Z.hdf5
/ligo/groups/cal/H1/measurements/PCALY2DARM_SS/PCALY2DARM_SS_20250823T183838Z.hdf5
/ligo/groups/cal/H1/measurements/SUSETMX_L1_SS/SUSETMX_L1_SS_20250823T183838Z.hdf5
/ligo/groups/cal/H1/measurements/SUSETMX_L2_SS/SUSETMX_L2_SS_20250823T183838Z.hdf5
/ligo/groups/cal/H1/measurements/SUSETMX_L3_SS/SUSETMX_L3_SS_20250823T183838Z.hdf5

Images attached to this report
Non-image files attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:18, Saturday 23 August 2025 (86529)
Sat CP1 Fill

Sat Aug 23 10:08:18 2025 INFO: Fill completed in 8min 14secs

 

Images attached to this report
H1 AOS
oli.patane@LIGO.ORG - posted 07:35, Saturday 23 August 2025 (86528)
Ops Day Shift Start

TITLE: 08/23 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 4mph Gusts, 2mph 3min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.19 μm/s
QUICK SUMMARY:

Observing at 150Mpc and have been Locked for almost 3 hours

H1 General
anthony.sanchez@LIGO.ORG - posted 22:22, Friday 22 August 2025 (86527)
Friday Night Ops Eve Shift

TITLE: 08/23 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
INCOMING OPERATOR: TJ
SHIFT SUMMARY:
H1 has been locked for 21+ Hours.

Dropped from observing during an earthquake but stayed locked.

Handful of small earthquakes and survived them.
Nothing else to report.

LOG:
No Log

H1 SQZ (SEI)
anthony.sanchez@LIGO.ORG - posted 18:32, Friday 22 August 2025 (86526)
Dropped from Observing due to SQZr unlock from 5.5 Mag EQ in Tonga.

At 00:42:03 UTC  Verbals announced an incoming 5.5M Earthquake from Tonga.
At 00:56:16:UTC H1 dropped from Observing due to a SQZr Unlock that was very likely caused by the increased ground motion.
We went back to Observing at 01:01:39 UTC after the SQZ Man relocked itself.
I did put the OPS mode into earthquake for that moment.
At 01:02:10 UTC Earthquake mode was activated.

Images attached to this report
H1 General
anthony.sanchez@LIGO.ORG - posted 16:46, Friday 22 August 2025 (86525)
Ops Eve shift for Friday Night

TITLE: 08/22 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 154Mpc
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 16mph Gusts, 9mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.19 μm/s
QUICK SUMMARY:

I inherited a 15+ hour lock from the day shift operator.
Everything looks like its running well.
Wind forcast looks great as well.

 

H1 General
oli.patane@LIGO.ORG - posted 16:30, Friday 22 August 2025 (86524)
Ops Day Shift End

TITLE: 08/22 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 154Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY: Observing at 155Mpc and have been Locked for over 15 hours. Nothing happened during my shift at all.
LOG:

14:30 UTC Observing and have been Locked for 6.5 hours
                                                                                                                                                                        

Start Time System Name Location Lazer_Haz Task Time End
15:37 FAC Kim OpticsLab n Tech clean 15:56
17:17 SPI Jeff OpticsLab n SPI Inventory 21:06
Displaying reports 1441-1460 of 85514.Go to page Start 69 70 71 72 73 74 75 76 77 End