Ran new power spectra over the week end, to confirm why the low frequency amplitude was high on Thursday's PRM power spectra (2013-02-14). Now the suspension is covered again, the power spectra looks better. See one of the two first attached documents (allhstss_2013-02-15) comparing L1 PRM power spectra (Jan 2013) H1 PRM uncovered (Feb 14th 2013) and H1 PRM covered (Feb 15th 2013), the difference can be clearly seen.
**the data have been commited on the svn and can be found here : /ligo/svncommon/SusSVN/sus/trunk/HSTS/Common/Data/allhstss_2013-02-15_Phase2b_H1PRM_ALL_Spectra_Doff.pdf /ligo/svncommon/SusSVN/sus/trunk/HSTS/Common/Data/allhstss_2013-02-15_Phase2b_H1PRM_ALL_Spectra_Don.pdf
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PRM/SAGM1/Results/SAGM{1,2 or 3}/2013-02-15_1700_H1SUSPRM_M{1,2 or 3}_ALL_Spectra.pdf
**Only the "good" data (=Feb 15th 2013) will be added to the plotallhsts_spectra.m script. Will commit the script with new data right after this log.
Ran new power spectra over the week end, to confirm why the low frequency amplitude was high on Thursday's PRM power spectra (2013-02-14). Now the suspension is covered again, the power spectra looks better. See one of the two first attached documents (allhstss_2013-02-15) comparing L1 PRM power spectra (Jan 2013) H1 PRM uncovered (Feb 14th 2013) and H1 PRM covered (Feb 15th 2013), the difference can be clearly seen.
**the data have been commited on the svn and can be found here :
/ligo/svncommon/SusSVN/sus/trunk/HSTS/Common/Data/allhstss_2013-02-15_Phase2b_H1PRM_ALL_Spectra_Doff.pdf
/ligo/svncommon/SusSVN/sus/trunk/HSTS/Common/Data/allhstss_2013-02-15_Phase2b_H1PRM_ALL_Spectra_Don.pdf
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PRM/SAGM1/Results/SAGM{1,2 or 3}/2013-02-15_1700_H1SUSPRM_M{1,2 or 3}_ALL_Spectra.pdf
**Only the "good" data (=Feb 15th 2013) will be added to the plotallhsts_spectra.m script. Will commit the script with new data right after this log.