CONSTRAINING THE DARK ENERGY EQUATION OF STATE USINGLISAOBSERVATIONS OF SPINNING MASSIVE BLACK HOLE BINARIES

SEVEN-YEARWILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION

(2011) E. Komatsu et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

The Mock LISA Data Challenges: from challenge 3 to challenge 4

(2010) Stanislav Babak et al.   CLASSICAL AND QUANTUM GRAVITY

Delensing gravitational wave standard sirens with shear and flexion maps

(2010) C. Shapiro et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Quasi-stars and the cosmic evolution of massive black holes

(2010) Marta Volonteri et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Impact of mergers on LISA parameter estimation for nonspinning black hole binaries

(2010) Sean T. McWilliams et al.   PHYSICAL REVIEW D

Search for spinning black hole binaries in mock LISA data using a genetic algorithm

(2010) Antoine Petiteau et al.   PHYSICAL REVIEW D

THEM-σ ANDM-LRELATIONS IN GALACTIC BULGES, AND DETERMINATIONS OF THEIR INTRINSIC SCATTER

(2009) Kayhan Gültekin et al.   ASTROPHYSICAL JOURNAL

THE zCOSMOS 10k-BRIGHT SPECTROSCOPIC SAMPLE

(2009) Simon J. Lilly et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

Advanced localization of massive black hole coalescences with LISA

(2009) Ryan N Lang et al.   CLASSICAL AND QUANTUM GRAVITY

Massive black-hole binary inspirals: results from the LISA parameter estimation taskforce

(2009) K G Arun et al.   CLASSICAL AND QUANTUM GRAVITY

LISA as a dark energy probe

(2009) K G Arun et al.   CLASSICAL AND QUANTUM GRAVITY

Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information

(2008) Chelsea L. MacLeod et al.   PHYSICAL REVIEW D

LISA observations of supermassive black holes: Parameter estimation using full post-Newtonian inspiral waveforms

(2008) Miquel Trias et al.   PHYSICAL REVIEW D

Use and abuse of the Fisher information matrix in the assessment of gravitational-wave parameter-estimation prospects

(2008) Michele Vallisneri   PHYSICAL REVIEW D