Issue Date | Title | Author(s) | Citation |
29-Oct-2009 | Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors | Buonanno, Alessandra; Iyer, B.R.; Ochsner, Evan; Pan, Yi; Sathyaprakash, B.S. | Physical Review D, 2009, Vol.80, p084043 |
15-Feb-2001 | Comparison of search templates for gravitational waves from binary inspiral | Damour, Thibault; Iyer, B.R.; Sathyaprakash, B.S. | Physical Review D, 2001, Vol.63, 044023 |
31-Jul-2002 | Comparison of search templates for gravitational waves from binary inspiral: 3.5 PN update | Damour, Thibault; Iyer, B.R.; Sathyaprakash, B.S. | Physical Review D, 2002, Vol.66, 027502 |
6-Sep-2005 | Complete adiabatic waveform templates for a test mass in the Schwarzschild spacetime: VIRGO and advanced LIGO studies | Ajith, P.; Iyer, B.R.; Robinson, C.A.K.; Sathyaprakash, B.S. | Classical and Quantum Gravity, 2005, Vol.22, pS1179-1188 |
2001 | Detecting binary black holes with efficient and reliable templates | Damour, Thibault; Iyer, B.R.; Sathyaprakash, B.S. | Gravitational waves: A challenge to theoretical astrophysics, ICTP lecture notes 3, Eds. V Ferrari et al. 2001, p179-188 |
15-Oct-2000 | Frequency-domain P-approximant filters for time-truncated inspiral gravitational wave signals from compact binaries | Damour, Thibault; Iyer, B.R.; Sathyaprakash, B.S. | Physical Review D, 2000, Vol.62, 084036 |
31-Mar-2003 | Gravitational waves from black hole binary inspiral and merger: The span of third post-Newtonian effective-one-body templates | Damour, Thibault; Iyer, B.R.; Jaranowski, P.; Sathyaprakash, B.S. | Physical Review D, 2003, Vol.67, 064028 |
Jun-2007 | Higher harmonics increase LISA's mass reach for supermassive black holes | Arun, K.G.; Iyer, B.R.; Sathyaprakash, B.S.; Sinha, Siddhartha | Physical Review D, 2007, Vol.75, p124002 |
Nov-2007 | Higher signal harmonics, LISA's angular resolution, and dark energy | Arun, K.G.; Iyer, B.R.; Sathyaprakash, B.S.; Sinha, Siddhartha; Van den Broeck, Chris | Physical Review D, 2007, Vol.76, p104016-1 |
Nov-2007 | Higher signal harmonics, LISA's angular resolution, and dark energy | Arun, K.G.; Sathyaprakash, B.S.; Sinha, Siddhartha; Van den Broeck, Chris | Physical Review D, 2007,Vol.76, 104016 |
15-Jan-1998 | Improved filters for gravitational waves from inspiraling compact binaries | Damour, Thibault; Iyer, B.R.; Sathyaprakash, B.S. | Physical Review D, 1998, Vol.57, 885-–907 |
Apr-2009 | LISA as a dark energy probe | Arun, K.G.; Mishra, Chandrakanth; Broeck, C.V.D.; Iyer, B.R.; Sathyaprakash, B.S.; Sinha, Siddhartha | Classical and Quantum Gravity, 2009, Vol.26, p094021 |
25-Feb-2005 | New class of post-Newtonian approximants to the waveform templates of inspiralling compact binaries: Test mass in the Schwarzschild spacetime | Ajith, P.; Iyer, B.R.; Robinson, C.A.K.; Sathyaprakash, B.S. | Physical Review D, 2005, Vol.71, 044029 |
2001 | Padé approximants for gravitational waves from inspiralling compact binaries | Damour, Thibault; Iyer, B.R.; Sathyaprakash, B.S. | Proceedings of the 10th workshop on general relativity and gravitation in Japan. Eds. M Sasaki et al. 2001, p49-59 |
6-Apr-2005 | Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The nonspinning case | Arun, K.G.; Iyer, B.R.; Sathyaprakash, B.S.; Sundarajan, P.A. | Physical Review D, 2005, Vol.71, 084008 |
7-Sep-2010 | Parametrized tests of post-Newtonian theory using advanced LIGO and Einstein telescope | Mishra, Chandrakanth; Arun, K.G.; Iyer, B.R.; Sathyaprakash, B.S. | Physical Review D, 2010, Vol.82, 064010 |
21-Jun-2012 | Scientific objectives of Einstein telescope | Sathyaprakash, B.S.; Abernathy, M.; Acernese, F; Ajith, P.; Mishra, Chandrakanth; +150 Co-authors; Iyer, B.R. | Classical and Quantum Gravity, 2012, Vol.29, p124013 |
9-May-2006 | Testing post-Newtonian theory with gravitational wave observations | Arun, K.G.; Iyer, B.R.; Qusailah, M.S.S.; Sathyaprakash, B.S. | Classical and Quantum Gravity, 2006, Vol.23 pL37-L43 |