activity
20022015
most citedThe LISA Optimal Sensitivity

297 citations · 696 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2015★ 60 cited

Systematic and Stochastic Variations in Pulsar Dispersion Measures

Michael T. Lam, James M. Cordes, Shami Chatterjee +3

We analyze deterministic and random temporal variations in dispersion measure (DM) from the full three-dimensional velocities of pulsars with respect to the solar system, combined…

gr-qc2012

Single-detector searches for a stochastic background of gravitational radiation

Massimo Tinto, J. W. Armstrong

We propose a data processing technique that allows searches for a stochastic background of gravitational radiation with data from a single detector. Our technique exploits the diff…

gr-qc2008★ 10 cited

Improved spacecraft radio science using an on-board atomic clock: application to gravitational wave searches

Massimo Tinto, George J. Dick, John D. Prestage +1

Recent advances in space-qualified atomic clocks (low-mass, low power-consumption, frequency stability comparable to that of ground-based clocks) can enable interplanetary spacecra…

gr-qc2007★ 8 cited

Modulator noise suppression in the LISA Time-Delay Interferometric combinations

Massimo Tinto, John W. Armstrong, Frank B. Estabrook

We previously showed how the measurements of some eighteen time series of relative frequency or phase shifts could be combined (1) to cancel the phase noise of the lasers, (2) to c…

gr-qc2004★ 54 cited

TDIR: Time-Delay Interferometric Ranging for Space-Borne Gravitational-Wave Detectors

Massimo Tinto, Michele Vallisneri, J. W. Armstrong

Space-borne interferometric gravitational-wave detectors, sensitive in the low-frequency (mHz) band, will fly in the next decade. In these detectors, the spacecraft-to-spacecraft l…

gr-qc2003★ 4 cited

SyZyGy: A Straight Interferometric Spacecraft System for Gravity Wave Observations

F. B. Estabrook, J. W. Armstrong, Massimo Tinto +1

We apply TDI, unfolding the general triangular configuration, to the special case of a linear array of three spacecraft. We show that such an array ("SyZyGy") has, compared with an…