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T. Mazeh

14 papers hereh-index 6923.3k citations450 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author3
  • middle author4
  • last author5

Across the 12 of 14 papers where every author was matched, so the position is known.

fields
  • astro-ph14
same name
  • T. Mazeh — 10 papers
  • T. Mazeh — 9 papers
  • T. Mazeh — 2 papers, h 24

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20002007
most citedHD147506b: A Super-Massive Planet in an Eccentric Orbit Transiting a Bright Star

205 citations · 409 across the 8 of their papers we have counts for

collaborators
Showing 2001Show all

4 papers · 1 filter

astro-ph2001

A Planet Candidate in the Stellar Triple System HD178911

S. Zucker, D. Naef, D. W. Latham +9

We report the detection of a low-mass companion orbiting the solar-type star HD178911B, the distant component of the stellar triple system HD178911. The variability of HD178911B wa…

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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.