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Past, present and future of Gravitational Wave detection Science

Past, present and future of Gravitational Wave detection Science

Past, present and future of Gravitational Wave detection Science. J. Alberto Lobo, Bellaterra, 13-O ct o be r -2004. Presentation summary. Current GW detection research status: Acoustic detectors Interferometers LISA LPF and the LTP The Diagnostics and DMU subsystems

By clarke-burch
(227 views)


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LIGO SCIENCE

LIGO SCIENCE

LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology LIGO PAC Meeting Pasadena, 5 June 2003 LIGO-G030293-00-R. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate. Most Pessimistic

By adah (141 views)

LIGO SCIENCE

LIGO SCIENCE

LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology NSF LIGO Operations Panel Hanford - 26 February 2001. LIGO-G010183-00-M. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate.

By wilda (106 views)

Running at design sensitivity: The fifth LIGO Science Run

Running at design sensitivity: The fifth LIGO Science Run

Running at design sensitivity: The fifth LIGO Science Run. Brian O’Reilly LIGO Livingston Observatory. The LIGO Observatories Interferometers are aligned along the great circle connecting the sites. LIGO Hanford Observatory (LHO) H1 : 4 km arms H2 : 2 km arms.

By lorene (156 views)

ADVANCED LIGO SCIENCE

ADVANCED LIGO SCIENCE

ADVANCED LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology NSF Advanced R&D Panel - 29 January 2001. 300 in h ~10 7 in rate. h rms = h(f) f 10 h(f). Open up wider band. 15 in h ~3000 in rate. From Initial Interferometers to Advanced. Most Optimistic Source

By rodney (115 views)

LIGO Science Education Center:

LIGO Science Education Center:

LIGO Science Education Center:. Research Labs Universities Education Agencies Informal Learning Centers. Partnering. John Thacker. May 19, 2005. SUBR. Our Partnership. LIGO. LIGO SEC. LaSIP/La GEAR UP. Exploratorium. Teaching & Learning. Exploratorium.

By cheveyo-gimenez (96 views)

Multidimensional classification of burst triggers from the fifth science run of LIGO

Multidimensional classification of burst triggers from the fifth science run of LIGO

Multidimensional classification of burst triggers from the fifth science run of LIGO. Soma Mukherjee CGWA, UTB GWDAW11, Potsdam, 12/18/06 LIGO-G060648-00-0. Why and What. kleine Welle (Blackburn, L. et. al. 2005 LIGO-050158-00-Z) is an algorithm that picks up

By kayla (73 views)

Multidimensional classification of burst triggers from the fifth science run of LIGO

Multidimensional classification of burst triggers from the fifth science run of LIGO

Multidimensional classification of burst triggers from the fifth science run of LIGO. Soma Mukherjee CGWA, UTB GWDAW11, Potsdam, 12/18/06 LIGO Tech doc # LIGO-G060648-00-0. Why and What. kleine Welle (Blackburn, Katsavounidis et. al.) is an algorithm that picks up burst

By hartfordc (0 views)

Data analysis with the E7 run data and plan for LIGO I Science Run(s) Albert Lazzarini

Data analysis with the E7 run data and plan for LIGO I Science Run(s) Albert Lazzarini

Data analysis with the E7 run data and plan for LIGO I Science Run(s) Albert Lazzarini 15 March 2002 CaJAGWR Seminar at Caltech. Outline of Talk . Organization of the LIGO I Collaboration Data Access, Use Models Data Analysis Model E7 Run Summary Upper Limit Groups Burst search

By rasha (142 views)

Status of the untriggered burst search in S3 LIGO data

Status of the untriggered burst search in S3 LIGO data

Status of the untriggered burst search in S3 LIGO data. Igor Yakushin (LIGO Livingston Observatory) For the LIGO Scientific Collaboration GWDAW-9, December 15-18, 2004, Annecy, France. Overview. Differences in comparison with S2 run Data quality

By lei (108 views)