activity
20002003
most citedCross-Correlation and Maximum Likelihood Analysis: A New Approach to Combine Cross-Correlation Functions

166 citations · 178 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph200312 cited

A Possible Correlation between Mass Ratio and Period Ratio in Multiple Planetary Systems

Tsevi Mazeh, Shay Zucker

We report on a possible correlation between the mass ratio and period ratio of pairs of adjacent planets in extra-solar planetary systems. Monte-Carlo simulations show that the eff…

astro-ph2003166 cited

Cross-Correlation and Maximum Likelihood Analysis: A New Approach to Combine Cross-Correlation Functions

Shay Zucker

This paper presents a new approach to combine cross-correlation functions. The combination is based on a maximum-likelihood approach and uses a non-linear combination scheme. It ca…

astro-ph2002

A Statistical Analysis of The Extrasolar Planets and The Low-Mass Secondaries

Tsevi Mazeh, Shay Zucker

We show that the astrometric Hipparcos data of the stars hosting planet candidates are not accurate enough to yield statistically significant orbits. Therefore, the recent suggesti…

astro-ph2001

Analysis of the Hipparcos Observations of the Extrasolar Planets and the Brown-Dwarf Candidates

Shay Zucker, Tsevi Mazeh

We analyzed the Hipparcos astrometric observations of 47 stars that were discovered to harbor giant planets and 14 stars with brown-dwarf secondary candidates. The Hipparcos measur…

astro-ph2001

Derivation of the Mass Distribution of Extrasolar Planets with MAXLIMA - a Maximum Likelihood Algorithm

Shay Zucker, Tsevi Mazeh

We construct a maximum-likelihood algorithm - MAXLIMA, to derive the mass distribution of the extrasolar planets when only the minimum masses are observed. The algorithm derives th…

astro-ph2001

On the Statistical Significance of the Hipparcos Astrometric Orbit of rho Coronae Borealis

Shay Zucker, Tsevi Mazeh

Recently Gatewood, Han & Black presented an analysis of the Hipparcos stellar positions and their own ground-based measurements of rho CrB, suggesting an astrometric orbit of 1.5 m…