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John J. Eldridge

Researcher at University of Auckland

Publications -  180
Citations -  11766

John J. Eldridge is an academic researcher from University of Auckland. The author has contributed to research in topics: Supernova & Stars. The author has an hindex of 52, co-authored 171 publications receiving 10527 citations. Previous affiliations of John J. Eldridge include Queen's University Belfast & University of Cambridge.

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The death of massive stars – I. Observational constraints on the progenitors of Type II-P supernovae

TL;DR: In this paper, the authors present the results of a 10.5-yr, volume-limited search for supernova (SN) progenitor stars in the Local Group of galaxies and show that low-luminosity SNe with low 56Ni production are most likely to arise from explosions of low-mass progenitors near the mass threshold.
Journal Article

The Gaia-ESO Public Spectroscopic Survey

Gerry Gilmore, +274 more
- 01 Mar 2012 - 
TL;DR: The Gaia-ESO Public Spectroscopic Survey has begun and will obtain high quality spectroscopy of some 100000 Milky Way stars, in the field and in open clusters, down to magnitude 19, systematically.
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Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results

TL;DR: The Binary Population and Spectral Synthesis suite of binary stellar evolution models and synthetic stellar populations provides a framework for the physically motivated analysis of both the integrated light from distant stellar populations and the detailed properties of those nearby as discussed by the authors.
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The effect of massive binaries on stellar populations and supernova progenitors

TL;DR: In this article, the authors compare single and binary stellar model results from the Cambridge stars code to several sets of observations and compare their models to the relative rate of Type Ib/c to Type II supernovae to measure the amount of mass lost over the entire lives of all stars.
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Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results

TL;DR: The Binary Population and Spectral Synthesis (BPASS) suite of binary stellar evolution models and synthetic stellar populations provides a framework for the physically motivated analysis of both the integrated light from distant stellar populations and the detailed properties of those nearby as mentioned in this paper.