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Status of NINJA: the Numerical INJection Analysis project

Cadonati, Laura and Aylott, Benjamin and Baker, John G. and Boggs, William D. and Boyle, Michael and Brady, Patrick R. and Brown, Duncan A. and Brügmann, Bernd and Buchman, Luisa T. and Buonanno, Alessandra and Camp, Jordan and Campanelli, Manuela and Centrella, Joan and Chatterji, Shourov and Christensen, Nelson and Chu, Tony and Diener, Peter and Dorband, Nils and Etienne, Zachariah B. and Faber, Joshua and Fairhurst, Stephen and Farr, Benjamin and Fischetti, Sebastian and Guidi, Gianluca and Goggin, Lisa M. and Hannam, Mark and Herrmann, Frank and Hinder, Ian and Husa, Sascha and Kalogera, Vicky and Keppel, Drew and Kidder, Lawrence E. and Kelly, Bernard J. and Krishnan, Badri and Laguna, Pablo and Lousto, Carlos O. and Mandel, Ilya and Marronetti, Pedro and Matzner, Richard and McWilliams, Sean T. and Matthews, Keith D. and Mercer, R. Adam and Mohapatra, Satyanarayan R. P. and Mroué, Abdul H. and Nakano, Hiroyuki and Ochsner, Evan and Pan, Yi and Pekowsky, Larne and Pfeiffer, Harald P. and Pollney, Denis and Pretorius, Frans and Raymond, Vivien and Reisswig, Christian and Rezzolla, Luciano and Rinne, Oliver and Robinson, Craig and Röver, Christian and Santamaría, Lucía and Sathyaprakash, Bangalore S. and Scheel, Mark A. and Schnetter, Erik and Seiler, Jenninfer and Shapiro, Stuart L. and Shoemaker, Dierdre and Sperhake, Ulrich and Stroeer, Alexander and Sturani, Riccardo and Tichy, Wolfgang and Liu, Yuk Tung and van der Sluys, Marc and van Meter, James R. and Vaulin, Ruslan and Vecchio, Alberto and Veitch, John and Viceré, Andrea and Whelan, John T. and Zlochower, Yosef (2009) Status of NINJA: the Numerical INJection Analysis project. Classical and Quantum Gravity, 26 (11). Art. No. 114008. ISSN 0264-9381. doi:10.1088/0264-9381/26/11/114008. https://resolver.caltech.edu/CaltechAUTHORS:20090812-091217588

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Abstract

The 2008 NRDA conference introduced the Numerical INJection Analysis project (NINJA), a new collaborative effort between the numerical relativity community and the data analysis community. NINJA focuses on modeling and searching for gravitational wave signatures from the coalescence of binary system of compact objects. We review the scope of this collaboration and the components of the first NINJA project, where numerical relativity groups, shared waveforms and data analysis teams applied various techniques to detect them when embedded in colored Gaussian noise.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0264-9381/26/11/114008DOIArticle
http://www.iop.org/EJ/abstract/0264-9381/26/11/114008/PublisherArticle
ORCID:
AuthorORCID
Brady, Patrick R.0000-0002-4611-9387
Brown, Duncan A.0000-0002-9180-5765
Faber, Joshua0000-0003-1724-3474
Fischetti, Sebastian0000-0002-2783-211X
Kalogera, Vicky0000-0001-9236-5469
Kidder, Lawrence E.0000-0001-5392-7342
Mandel, Ilya0000-0002-6134-8946
Pfeiffer, Harald P.0000-0001-9288-519X
Schnetter, Erik0000-0002-4518-9017
Sperhake, Ulrich0000-0002-3134-7088
Vecchio, Alberto0000-0002-6254-1617
Additional Information:© 2009 IOP Publishing Ltd. Received 10 March 2009, in final form 8 April 2009. Published 19 May 2009. We thank the Kavli Institute for Theoretical Physics (KITP) Santa Barbara for hospitality during the workshop ‘Interplay between Numerical Relativity and Data Analysis,’ where the NINJA project was initiated. The Kavli Institute is supported by National Science Foundation grant PHY-0551164. This project was supported in part by DFG grant SFB/Transregio 7 ‘Gravitational Wave Astronomy’ (BB, MH, SH, DP, LR, US); by the National Science Foundation grants PHY-0114375 (CGWP), PHY-0205155 (UIUC), PHY-0354842 (RM), DMS-0553302 (MB, LB, TC, KM, HP, MS), DMS-0553677 (LK, AM), PHY-0553422 (NC), PHY-0555436 (PL), PHY-0600953 (PB, LG, RAM, RV), PHY-0601459 (MB, LB, TC, KM, HP, MS), PHY-0603762 (AB, EO, YP), PHY-0649224 (BF), PHY-0650377 (UIUC), PHY- 0652874 (FAU), PHY-0652929 (LK, AM), PHY-0652952 (LK, AM), PHY-0652995 (MB, LB, TC, KM, HP, MS), PHY-0653303 (PL, DS, MC, CL), PHY-0653321 (VK, IM, VR, MvdS), PHY-0653443 (DS), PHY-0653550 (LC), PHY-0701566 (ES), PHY-0701817 (PB, LG, RAM, RV), PHY-0714388 (MC, CL, YZ), OCI-0721915 (ES), PHY-0722315 (MC, CL), PHY-0745779 (FP), PHY-0801213 (FH), PHY-0838740 (BF, LS, VR) and NSF-0847611 (DB, LP); by NASA grants HST-AR-11763 (CL, MC, JF, YZ), NNG-04GK54G (UIUC), NNG-04GL37G (RM), NNG-05GG51G (LK, AM), NNG-05GG52G (MB, LB, TC, KM, HP, MS), 05-BEFS-05-0044 (GSFC), 06-BEFS06-19 (GSFC), 07-ATFP07-0158 (MC, CL, YZ), and NNX-07AG96G (UIUC) and by NSF cooperative agreement PHY-0107417 (DK, SC). BA was supported by a Vacation Bursary of the UK Engineering and Physical Sciences Research Council. AV, JV and BS acknowledge support by the UK Science and Technology Facilities Council. SF acknowledges the support of the Royal Society. MH was supported by SFI grant 07/RFP/PHYF148. FP acknowledges support from the Alfred P. Sloan Foundation. SH acknowledges support from DAAD grant D/07/13385, grant FPA-2007-60220 from the Spanish Ministry of Science and Education and VESF. MB, LB, TC, KM, HP and MS acknowledge support from the Sherman Fairchild Foundation and the Brinson Foundation. LK and AM acknowledge support from the Fairchild Foundation. BK was supported by the NASA Postdoctoral Program at the Oak Ridge Associated Universities. SM was supported in part by the Leon A. Herreid Graduate Fellowship. RS was supported by an EGO sponsored fellowship, EGO-DIR-105-2007. Computations were carried out under LRAC allocations MCA08X009 (PL, DS), TG-MCA08X010 (FAU), TG-MCA02N014 (LSU), TG-MCA99S008 (UIUC), TG-PHY990002 (MB, LB, TC, LK,KM, AM,HP, MS), on LONI systems (LSU), and on the clusters at the AEI, Cardiff University, Northwestern University (NSF MRI grant PHY- 0619274 to VK), the LIGO Laboratory, NASA Advanced Supercomputing Division (Ames Research Center), Syracuse University, LRZ Munich (BB, MH, SH, US), the University of Birmingham and the RIT NewHorizons cluster. PACS numbers: 04.30.−w, 04.80.Nn, 04.25.D−, 04.25.dg
Group:TAPIR, LIGO
Funders:
Funding AgencyGrant Number
NSFPHY-0551164
Deutsche Forschungsgemeinschaft (DFG)UNSPECIFIED
NSFPHY-0114375
NSFPHY-0205155
NSFPHY-0354842
NSFDMS-0553302
NSFDMS-0553677
NSFPHY-0553422
NSFPHY-0555436
NSFPHY-0600953
NSFPHY-0601459
NSFPHY-0603762
NSFPHY-0649224
NSFPHY-0650377
NSFPHY-0652874
NSFPHY-0652929
NSFPHY-0652952
NSFPHY-0652995
NSFPHY-0653303
NSFPHY-0653321
NSFPHY-0653443
NSFPHY-0653550
NSFPHY-0701566
NSFPHY-0701817
NSFPHY-0714388
NSFOCI-0721915
NSFPHY-0722315
NSFPHY-0745779
NSFPHY-0801213
NSFPHY-0838740
NSFNSF-0847611
NASAHST-AR-11763
NASANNG-04GK54G
NASANNG-04GL37G
NASANNG-05GG51G
NASANNG-05GG52G
NASA05-BEFS-05-0044
NASA06-BEFS06-19
NASA07-ATFP07-0158
NASANNX-07AG96G
NSFPHY-0107417
Engineering and Physical Sciences Research Council (EPSRC)UNSPECIFIED
Science and Technology Facilities Council (STFC)UNSPECIFIED
Royal SocietyUNSPECIFIED
Science Foundation Ireland07/RFP/PHYF148
Alfred P. Sloan FoundationUNSPECIFIED
Deutscher Akademischer AustauschdienstDAAD/07/13385
Spanish Ministry of Science and EducationFPA-2007-60220
Sherman Fairchild FoundationUNSPECIFIED
Brinson FoundationUNSPECIFIED
Virgo–EGO Scientific ForumUNSPECIFIED
NASA Postdoctoral ProgramUNSPECIFIED
Leon A. Herreid Graduate FellowshipUNSPECIFIED
Eccentric Geophysical ObservatoryEGO-DIR-105-2007
NSFMCA08X009
NSFTG-MCA08X010
NSFTG-MCA02N014
NSFTG-MCA99S008
NSFTG-PHY990002
NSFPHY-0619274
Issue or Number:11
DOI:10.1088/0264-9381/26/11/114008
Record Number:CaltechAUTHORS:20090812-091217588
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20090812-091217588
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:14979
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:12 Aug 2009 18:32
Last Modified:12 Jul 2022 19:51

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