Published April 21, 2006 | Version v1
Journal article

Status of the LIGO detectors

  • 1. LIGO Hanford Observatory, PO Box 159, Richland, WA 99352 (United States)

Description

All three LIGO detectors have reached sensitivities within a factor of 2 of design over a wide range of frequencies. A sky-averaged detection range (SNR > 8) of more than 10 Mpc for inspiral binary neutron stars with masses of 1.4 Msol has been achieved with the best instrument. The fourth LIGO science run taking data for 30 days has been completed earlier this year with a triple coincidence duty cycle greater than 50%. A commissioning effort to scale up the cavity powers to design sensitivity as well as preparations for an extended science run is underway. The data from the first two science runs were fully analysed and results are summarized

Availability note (English)

Available online at http://stacks.iop.org/0264-9381/23/S51/cqg6_8_s07.pdf or at the Web site for the journal Classical and Quantum Gravity (ISSN 1361-6382) http://www.iop.org/

Additional details

Publishing Information

Journal Title
Classical and Quantum Gravity
Journal Volume
23
Journal Issue
8
Journal Page Range
p. S51-S56
ISSN
0264-9381
CODEN
CQGRDG

Conference

Title
6. Edoardo Amaldi conference on gravitational waves
Dates
20-24 Jun 2005
Place
Okinawa (Japan)

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
37063303
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COSMOLOGY; DESIGN; DETECTION; GRAVITATIONAL WAVE DETECTORS; GRAVITATIONAL WAVES; MASS; NEUTRON STARS; SENSITIVITY
Descriptors DEC
MEASURING INSTRUMENTS; RADIATION DETECTORS; STARS

Optional Information