S Mukherjee (for the LIGO Science collaboration) 2006 J. Phys.: Conf. Ser. 32 44 doi:10.1088/1742-6596/32/1/008
S Mukherjee (for the LIGO Science collaboration)
Show affiliationsPresence of slow non-stationarities has been seen in a series of studies with LIGO engineering and science data. It is important to track these slow variations or 'drifts' to diagnose their origin and correct them, as nonstationary data can affect sensitivity of astrophysical searches. A DMT (Data Monitoring Tool) monitor has been built to track slow non-stationarities in LIGO data. The monitor, tested on S4 data, will be operational during LIGO S5 data run. Offline analysis will be performed to unearth details of patterns thus obtained in the output of the monitor.
Issue 1 (2006)
S Mukherjee (for the LIGO Science collaboration) 2006 J. Phys.: Conf. Ser. 32 44
Pierre Otal et al 2008 Metrologia 45 07004
Peter T Beyersdorf et al 2002 Class. Quantum Grav. 19 1585
V Yazdanpanah et al 2006 New J. Phys. 8 233
L G Moretto and R P Schmitt 1981 Rep. Prog. Phys. 44 533
C H Sim 2007 Metrologia 44 29
T A Kaplan and S D Mahanti 1979 J. Phys. C: Solid State Phys. 12 L23
A Hasumi et al 1979 J. Phys. A: Math. Gen. 12 L217
F I Cooperstock et al 1997 Class. Quantum Grav. 14 2195
U Engberg et al 1993 J. Phys.: Condens. Matter 5 5543