An overview of the second round of the mock LISA data challenges

被引:56
作者
Arnaud, K. A.
Babak, S.
Baker, J. G.
Benacquista, M. J.
Cornish, N. J.
Cutler, C.
Finn, L. S.
Larson, S. L.
Littenberg, T.
Porter, E. K.
Vallisneri, M.
Vecchio, A.
Vinet, J-Y
机构
[1] NASA, Goddard Space Flight Ctr, Gravitat Astrophys Lab, Greenbelt, MD 20771 USA
[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany
[3] Univ Texas, Ctr Gravitat Wave Astron, Brownsville, TX 78520 USA
[4] Montana State Univ, Dept Phys, Bozeman, MT 59717 USA
[5] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[6] Penn State Univ, Ctr Gravitat Wave Phys, University Pk, PA 16802 USA
[7] Weber State Univ, Dept Phys, Ogden, UT 84408 USA
[8] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[9] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA
[10] Observ Cote Azur, Dept Artemis, F-06304 Nice, France
关键词
D O I
10.1088/0264-9381/24/19/S18
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Mock Data Challenges (MLDCs) have the dual purpose of fostering the development of LISA data-analysis tools and capabilities and of demonstrating the technical readiness already achieved by the gravitational-wave community in distilling a rich science payoff from the LISA data. The first round of MLDCs has just been completed and the second-round data sets are being released shortly after this workshop. The second-round data sets contain radiation from an entire Galactic population of stellar-mass binary systems, from massive-black-hole binaries, and from extreme-mass-ratio inspirals. These data sets are designed to capture much of the complexity that is expected in the actual LISA data, and should provide a fairly realistic setting to test advanced data-analysis techniques, and in particular the global aspect of the analysis. Here we describe the second round of MLDCs and provide details about its implementation.
引用
收藏
页码:S551 / S564
页数:14
相关论文
共 30 条
  • [1] Time-delay interferometry for space-based gravitational wave searches
    Armstrong, JW
    Estabrook, FB
    Tinto, M
    [J]. ASTROPHYSICAL JOURNAL, 1999, 527 (02) : 814 - 826
  • [2] ARNAUD KA, 2007, PREPRINT GRQC0701139
  • [3] ARNAUD KA, 2006, LASER INTERFEROMETER, P625
  • [4] Arnaud KA, 2006, AIP CONF PROC, V873, P619
  • [5] LISA capture sources: Approximate waveforms, signal-to-noise ratios, and parameter estimation accuracy
    Barack, L
    Cutler, C
    [J]. PHYSICAL REVIEW D, 2004, 69 (08): : 24
  • [6] Gravitational-wave inspiral of compact binary systems to 7/2 post-Newtonian order (vol 6506, pg Nil_0002, 2002)
    Blanchet, L
    Faye, G
    Iyer, BR
    Joguet, B
    [J]. PHYSICAL REVIEW D, 2005, 71 (12)
  • [7] Gravitational-wave inspiral of compact binary systems to 7/2 post-Newtonian order
    Blanchet, L
    Faye, G
    Iyer, BR
    Joguet, B
    [J]. PHYSICAL REVIEW D, 2002, 65 (06)
  • [8] *CALT CTR ADV COMP, 2000, XSIL EXT SCI INT LAN
  • [9] COMISH NJ, 2007, PREPRINT 07041808
  • [10] COMISH NJ, 2003, PHYS REV D, V67