The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interferometer. The aim of the experiment is to operate a powerrecycled Broadband RSE interferometer with suspended optics and to achieve diagonalization of length signals of the central part of the interferometer directly through the optical setup. Details of the 4m RSE interferometer control method as well as the design of the experimental setup will be presented
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Advanced LIGO (aLIGO) requires multiple frequency sidebands to disentangle all of the main interfero...
Kilometer scale interferometers for the detection of gravitational waves are currently under constru...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
Some next-generation gravitational-wave detectors, such as the American Advanced LIGO project and th...
LCGT plans to use tuned RSE as the optical configuration for its interferometer. A tuned RSE interfe...
As a future plan, an advanced gravitational-wave detector will employ an optical configuration of re...
For a broadband-operated RSE interferometer, a simple and smart length sensing and control scheme wa...
In anticipation of an upgrade of the LIGO detector to an advanced configuration in 2004, a tabletop ...
Next generation gravitational wave antennas employ resonant sideband extraction (RSE) interferometer...
Resonant sideband extraction is a new optical configuration for laser-interferometric gravitational ...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Large Cryogenic Gravitational wave Telescope (LCGT) is the future Japanese gravitational-wave detect...
We present an experimental demonstration of a locking and control scheme for an interferometer using...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Advanced LIGO (aLIGO) requires multiple frequency sidebands to disentangle all of the main interfero...
Kilometer scale interferometers for the detection of gravitational waves are currently under constru...
The 4m Resonant Sideband Extraction (RSE) interferometer is a planned prototype of the LCGT interfer...
Some next-generation gravitational-wave detectors, such as the American Advanced LIGO project and th...
LCGT plans to use tuned RSE as the optical configuration for its interferometer. A tuned RSE interfe...
As a future plan, an advanced gravitational-wave detector will employ an optical configuration of re...
For a broadband-operated RSE interferometer, a simple and smart length sensing and control scheme wa...
In anticipation of an upgrade of the LIGO detector to an advanced configuration in 2004, a tabletop ...
Next generation gravitational wave antennas employ resonant sideband extraction (RSE) interferometer...
Resonant sideband extraction is a new optical configuration for laser-interferometric gravitational ...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Large Cryogenic Gravitational wave Telescope (LCGT) is the future Japanese gravitational-wave detect...
We present an experimental demonstration of a locking and control scheme for an interferometer using...
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) int...
Advanced LIGO (aLIGO) requires multiple frequency sidebands to disentangle all of the main interfero...
Kilometer scale interferometers for the detection of gravitational waves are currently under constru...