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most citedOur Peculiar Motion Away from the Local Void

382 citations · 451 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2022★ 9 cited

Galaxy flows within 8,000 km/s from Numerical Action methods

Edward Shaya, R. Brent Tully, Daniel Pomarède +1

The trajectories since z=4 of systems of galaxies (`halos') with cz < 8,000 km/s are found through Numerical Action reconstructions. A set of 9,719 halos from a 2MASS group catalog…

astro-ph2007★ 382 cited

Our Peculiar Motion Away from the Local Void

R. Brent Tully, Edward J. Shaya, Igor D. Karachentsev +4

The peculiar velocity of the Local Group of galaxies manifested in the Cosmic Microwave Background dipole is found to decompose into three dominant components. The three components…

astro-ph2003★ 22 cited

COMPASS: An Upper Limit on CMB Polarization at an Angular Scale of 20 arc minutes

Philip C. Farese, Giorgio Dall'Oglio, Joshua O. Gundersen +10

COMPASS is an on-axis 2.6 meter telescope coupled to a correlation polarimeter operating at a wavelength of 1 cm. The entire instrument was built specifically for CMB polarization…

astro-ph2003★ 5 cited

COMPASS: An Instrument for Measuring the Polarization of the CMB on Intermediate Angular Scales

Philip C. Farese, Giorgio Dall'Oglio, Josh Gundersen +9

COMPASS is an on-axis 2.6 meter telescope coupled to a correlation polarimeter. The entire instrument was built specifically for CMB polarization studies. Careful attention was giv…

astro-ph2002★ 8 cited

Gravitational Potential Reconstruction from Peculiar Velocity and Weak Lensing Measurements

Olivier Doré, Lloyd Knox, Alan Peel

We present an analytic method for rapidly forecasting the accuracy of gravitational potential reconstruction possible from measurement of radial peculiar velocities of every galaxy…

astro-ph2002★ 5 cited

Using Galaxy Cluster Peculiar Velocities to Constrain Cosmological Parameters

A. Peel, L. Knox

Galaxy cluster peculiar velocities can be inferred from high-sensitivity, high-resolution multiple-frequency observations in the 30 to 400 GHz range. While galaxy cluster counts an…