Present:
Caltech: Ben Cusack,
Ron Drever, Szabi Marka, Peter Shawhan, Stan Whitcomb, John Zweizig
Hobart: Steve Penn
LHO: Dick Gustafson,
Mike Landry, Rick Savage, Robert Schofield
Michigan: Keith Riles
MIT: Rana Adhikari,
Laura Cadonati,
Oregon: Ray Frey, Masahiro
Ito, Rauha Rahkola, Brian Stubbs
Penn State: Mike Ashley,
Patrick Sutton
S2 Status Update Reports
KR gave a brief update on the status of the DQ segment repository. Many new studies have been completed (or are nearly completed) and will be incorporated into version 3 segments.
One point of discussion was flagging periods when calibration drift coefficients are "out of bounds". It was decided to flag periods when alpha is not between 0.5 and 2.0 (1.0 is nominal). PatrickS agreed to generate tables of bad times. He has already produced tables of times when no coefficients could be determined.
One recent piece of bad news was that a number of H1 channels had a
byte-swapping bug at the hardware level during all of S2 (see
note from Daniel Sigg). Robert pointed out, however, that the
PEM channels affected have not proven useful in the past in understanding
H1 behavior. For historical reasons, many H1-related PEM channels are read
out via H2 ADC crates.
The iteration 2 calibration is now complete! More information can be found at the calibration team home page and at Patrick's S2 SenseMonitor page. Although a careful error accounting has not been done yet, it is believed that iteration 2 is comparable in accuracy to the final S1 calibration, i.e., at the 10% level.
The final (iteration 3) calibration is expected to be ready at about the time of the LSC meeting at Hannover. The changes between iterations 2 and 3 come from incorporating measurements of electronics delays and transfer functions and are expected to be most important at frequencies above 1 kHz. The regeneration of alpha coefficients should go much faster in the next iteration because it will not be necessary to go back to the raw data. MikeL confirmed that the team believes the timing uncertainties in transfer functions that prevented coherent, multi-IFO pulsar tracking at 1.3 kHz in S1 will be much smaller after the final calibration. (Note: it is planned to use atomic clocks in the S3 run to give backup timing info / confidence.)
MikeL is now generating "stardard" S2 power spectral estimates for use
in external LSC presentations. He is producing one representative curve
each for H1 and H2, but expects to produce three curves for L1, since its
inspiral range improved dramatically during the course of the run.
Laura provided a link to the glitches team web page and gave an overview of ongoing work. The MIT group is running glitchmon on triple-coincident H1 & H2 playground RDS data at MIT (but is having technical problems running on the LHO fortress machine to look at other data samples). The Syracuse team continues looking through L1 playground segments to understand glitch and glitchmon triggers; and is learning how to do glitchmon reruns to try varying thresholds. The Florida team continues WaveMon studies, but has also had trouble running at LHO (Note by KR: later e-mail exchanges resolved at least one of these troubles.).
MikeA reported on some calibration line tracking he has been doing,
using a straight heterodyne of ASQ. He confirms drifts in phase of the
lines and wants to use those drifts to flag data quality. KR suggested
comparing his magnitude/phase determinations with those recorded by Sergey's
LineMon monitor (available as minute trends). Rana was happy to see a heterodyne
approach being used, but warned that one should use filtering in addition.
PeterSh pointed out that MikeA was incorrectly assuming all IFO's had the
same calibration line frequency. KR volunteered to send MikeA the correct
values for each IFO.
Following discussions at the last detchar, Peter put together a web page with a detailed list of the locations of all S2 data samples (full and RDS), including channel lists and applicable DMT computers with data access. KR suggested sending out an announcement of this quite useful page to the ligo-dc mailing list.
Peter also reported that the second trends now in HPSS storage at Caltech
are being moved to the new SAM-QFS facility, which should allow much better
access to those trends via LDAS. A number of persons have requested access
to that information for the S2 run.
A.O.B.