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The Exoplanet Mass-Ratio Function from the MOA-II Survey: Discovery of a Break and Likely Peak at a...

The Exoplanet Mass-Ratio Function from the MOA-II Survey: Discovery of a Break and Likely Peak at a...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2080382327

The Exoplanet Mass-Ratio Function from the MOA-II Survey: Discovery of a Break and Likely Peak at a Neptune Mass

About this item

Full title

The Exoplanet Mass-Ratio Function from the MOA-II Survey: Discovery of a Break and Likely Peak at a Neptune Mass

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2016-12

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

We report the results of the statistical analysis of planetary signals discovered in MOA-II microlensing survey alert system events from 2007 to 2012. We determine the survey sensitivity as a function of planet-star mass ratio, \(q\), and projected planet-star separation, \(s\), in Einstein radius units. We find that the mass ratio function is not...

Alternative Titles

Full title

The Exoplanet Mass-Ratio Function from the MOA-II Survey: Discovery of a Break and Likely Peak at a Neptune Mass

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2080382327

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2080382327

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1612.03939

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