The two goals of the research on angular fluctuations will be: 1) investigate the correlation between servo signals and mirror angular motion. This is to say, we want to know how much of the angular motion is large enough to dominate the interferometer signals. 2) investigate the cause for mirrors' angular motion: straight seismic motion, control forces through cross couplings, mechanical cross coupling, excess motion of the stacks, etc. We will work with a single arm cavity configuration, and preferably with both arms (that is, one at a time, but some time with both). Since we need interferometer signals, we will need the LSC-PD signals for the arm cavity (preferably the control signal). We would also like the error signal of the mode cleaner, to determine the frequency region which is not explained by frequency noise. We need DC signals, but a sampling rate of 256 Hz is enough. Thus, we request the relevant H2:LSC-AS#_I(Q?), at 2048 Hz and H2:IOO_MC_I at 16384 Hz (or L, at 256 Hz). We'd like WFS signals for the arm cavities: we know they are not ready to run yet, but if they are, we'd like the ASC channels for WFS at the reflection and antisymmetric ports, in pitch and yaw (H2:ASC-WFS3,4_P,Y). These are 2 channels at 2048 Hz. We will take care of the calibration of these signals, if needed. We also request the optical lever signals for the relevant ITM mirror, pitch and yaw: H2:ASC-QPDX(or Y)_P,Y: these are 2 channels sampled at 2048 Hz. It would be nice to have the similar signals for ASC (fast) signals for the ETM mirrors, but we understand they are not available yet. If not, we'll take the slow (4 or 16 Hz?) optical lever channels (I think they exist, but didn't find them in the list?) We also want the 4 local sensor channels for the ITM and ETM of the arm in use: H2:SUS-ITMX(Y)-SENSOR1,2,3,4 and H2:SUS-ETMX(Y)-SENSOR1,2,3,4 (8 channels, at 256 Hz). We also want to information on beam pointing, from QPD in transmission at the mid stations: H2:ASC-QPDX(Y)-Y1,P1 : these are 2 channels at 2048 Hz. About enviromental channels, we need: *seismometers X,Y,Z in corner station and relevant mid station *tiltmeters P,Y at LVEA and relevant mid-station *accelerometers X,Y,Z in BSC where relevant ITM is, and at midstation *magnetometers X,Y,Z in LVEA and relevant midstation. Locking durations needed: I think we can do most of the things we need to do with a few hours of each arm cavity, assuming they are "quality time". Segments longer than 15' are probably needed, for all the transients to go away and a good alignment to be achieved. We'd like to have a few hours of each cavity (X and Y). Many of the investigations involving optical levers, local sensors and environmental channels can be done without the interferometer, so they don't pose any requirement on the configuration or the time length, except that we'd like a total of a few hours with the interferometer "off" (which may happen anyway).