(1) ********
Luca will talk about his study of LSC. The pdf file of his talk is 
available in http://www.ligo.caltech.edu/~e2e/pdfs/luca-10-23-01.pdf.

(2) PEM (Robert)
I have been helping Bill B. obtain seismic data (coherence vs. distance)
along the 2k input for use in his e-to-e based modeling. More recently,
I also made seismic measurements comparing the LHO 4k input area to
the beer garden.
I have not made any impulse transfer function measurements since the
acoustic coupling measurements I made in the 2k PSL area during the summer.

(3) From: Peter King <pking@ligo.caltech.edu

The requested ASCII format data for the LLO PSL is now available under:
         ~pking/psl/e2e/llopsl-data.tar.gz
The file is a gzipped tar file that can be extracted with
         gzip -d llopsl-data.tar.gz
         tar -xvf llopsl-data.tar
There is an index file that explains what the filenames are.

Inside the datasets are:
         PSL frequency noise as measured by the suspended modecleaner both
before and after the IO main beam periscope replacement.  Both measurements
were obtained with the latest rev. of the modecleaner servo.

         Closed loop transfer functions of the frequency stabilization servo
and transfer functions out to the fast path and Pockels cell path.  These
are taken with
         IN: IN TEST 2   OUT: MIXER OUT
         IN: IN TEST 2   OUT: fast monitor
         IN: IN TEST 2   OUT: PC monitor
respectively.

         The PSL intensity noise as measured after the pre-modecleaner.  The
latest intensity noise as seen by the modecleaner could not be obtained due
to some pickup problems with the signal cables.


(4) *******
Special topic: Who & how to answer Stan's questions? (see 
http://www.ligo.caltech.edu/~coyne/e2e/G010387-00.pdf or soon in the DCC 
electronic files)

There are many issues which can be studied using e2e simulation package
without the knowledge of the details of the internal structure of e2e.
Hiro will provide a package which can be used as a blackbox, so please
contact hiro@ligo.caltech.edu.

Dennis, Luca and Hiro will look into Question 1 on Page 5
"How accurately do these matrix elements need to be determined ?"

Hiro will look into issues on page 5 (effect of as-built IFO), and 
Q5 on page 6, the difference of cold and hot LIGO.

Biplab will look into the relative size of SBs in Michelson (p8).

Virginio will look into Q2 on p10,
"Is the excitation of the violin modes "intrinsic" to the MSEM drive 
or is it enhanced as imbalance in the drive to the various OSEMs?"

David will compile a list of bilinear noise sources.

Mike Smith and Hiro will work on the clipping effect. Mike will provide
information about the field propagation from IFO to a photo diode.
e2e has a photo diode simulation with finite apperture.