Published June 7, 2008 | Version v1
Journal article

Report on the second Mock LISA data challenge

  • 1. Max-Planck-Institut fuer Gravitationsphysik (Albert-Einstein-Institut), Am Muehlenberg 1, D-14476 Golm bei Potsdam (Germany)
  • 2. Gravitational Astrophysics Laboratory, NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771 (United States)
  • 3. Center for Gravitational Wave Astronomy, University of Texas at Brownsville, Brownsville, TX 78520 (United States)
  • 4. Department of Physics, Montana State University, Bozeman, MT 59717 (United States)
  • 5. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)
  • 6. Department of Physics, Weber State University, 2508 University Circle, Ogden, UT 84408 (United States)
  • 7. School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B152TT (United Kingdom)
  • 8. APC, UMR 7164, University Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, 75025 Paris Cedex 13 (France)
  • 9. School of Mathematics, University of Southampton, Southampton SO171BJ (United Kingdom)
  • 10. Institute of Theoretical Physics, University of Wroclaw, Wroclaw (Poland)
  • 11. Department of Physics and Astronomy, University of Glasgow, Glasgow (United Kingdom)
  • 12. Theoretical Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States)
  • 13. Physics and Astronomy, Carleton College, Northfield, MN (United States)
  • 14. Institute of Astronomy, University of Cambridge, Cambridge CB30HA (United Kingdom)

Description

The Mock LISA data challenges are a program to demonstrate LISA data-analysis capabilities and to encourage their development. Each round of challenges consists of several data sets containing simulated instrument noise and gravitational waves from sources of undisclosed parameters. Participants are asked to analyze the data sets and report the maximum information about the source parameters. The challenges are being released in rounds of increasing complexity and realism: here we present the results of Challenge 2, issued in Jan 2007, which successfully demonstrated the recovery of signals from nonspinning supermassive-black-hole binaries with optimal SNRs between ∼10 and 2000, from ∼20 000 overlapping galactic white-dwarf binaries (among a realistically distributed population of 26 million), and from the extreme-mass-ratio inspirals of compact objects into central galactic black holes with optimal SNRs ∼100

Availability note (English)

Available from http://dx.doi.org/10.1088/0264-9381/25/11/114037

Additional details

Identifiers

DOI
10.1088/0264-9381/25/11/114037;
PII
S0264-9381(08)65039-X;

Publishing Information

Journal Title
Classical and Quantum Gravity
Journal Volume
25
Journal Issue
11
Journal Page Range
[8 p.]
ISSN
0264-9381
CODEN
CQGRDG

Conference

Title
18. international conference on general relativity and gravitation; Amaldi7: 7. Edoardo Amaldi conference on gravitational waves
Acronym
GRG18
Dates
8-14 Jul 2007
Place
Sydney (Australia)

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
39111463
Subject category
S99: GENERAL AND MISCELLANEOUS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
BLACK HOLES; DATA ANALYSIS; GRAVITATIONAL WAVES; INFORMATION; MASS; NOISE; SIGNALS; SIMULATION; WHITE DWARF STARS
Descriptors DEC
DWARF STARS; STARS