Microlensing Resources in the Exoplanet Archive

This page describes the resources available in the Exoplanet Archive for planets discovered using the microlensing technique.

Technique Overview

Gravitational microlensing refers to the transient magnification of the apparent brightness of a distant star that is caused by the gravitational potential of an intervening "lensing" system. If this lens system contains one or more planets, it is often possible to measure their properties from the structure of the resulting light curve. For more details, see this review on planet detection with microlensing or this community-maintained web resource with introductory microlensing explanations and interactive demonstrations of the effect.

Microlensing Table

This interactive table contains all microlensing-specific observational and model parameters for confirmed planets discovered with the microlensing technique. If more than one solution or model is presented, they will get listed in this table as separate rows. The columns available in this table are listed here.

To compare and review microlensing planets against other confirmed planets, use the Confirmed Planets interactive table (see next section).

Confirmed Planets

Planets discovered with the microlensing technique that meet the Archive's exoplanet criteria are included in the Confirmed Planets table. To see only the microlensing planets, enter microlensing in the filter box under Discovery Method. The count of microlensing planets is available on the Statistics page. (Note that clicking on microlensing in the Confirmed Exoplanets Statistics table takes you to the Confirmed Planet table with that filter already applied.)

A single set of default stellar and planetary parameters is listed in the Confirmed Planets table. Additional references are listed in the Overview page for each object (click for example). Microlensing-specific parameters for all solutions within a paper are listed in the Microlensing table (see previous section).

Contributed Data

Many members of the community have provided the data for their microlensing light curves. These are available either as a set from the Bulk Download page or individually by object. Instructions on how to access these for an individual object are here. Please note that we currently have data for most, but not all, microlensing objects.

The archive also hosts statistically large ensembles of light curve data from ground-based microlensing surveys. Specifically, our holdings include 78.2 million light curves (205 GB) for the UKIRT microlensing survey, collected from 2015–2018, as well as approximately 6,000 light curves (22 GB) for the MOA survey, collected from 2006–2014.

If you have data from a peer-reviewed paper that you would like to contribute, please read the guidelines on how to contribute data.

ExoFOP Support for K2 Microlensing Campaign 9 (C9)

K2 Campaign 9 took place from April 22 to July 2, 2016 and was dedicated to a study of gravitational microlensing events. The C9 microlensing experiment involves the Kepler spacecraft observing in the +VV direction at fields toward the Galactic bulge. The aim of this program is to simultaneously observe gravitational microlensing events with K2 and from Earth to see a parallax effect in the shape and time of the lensing event. This white paper describes the ground-based observing resources and scientific motivations of this experiment.

The Exoplanet Follow-up Observing Program (ExoFOP) web site is designed to optimize resources and facilitate collaboration in follow-up studies of exoplanet candidates. ExoFOP serves as a repository for community-gathered follow-up data by allowing upload and display of data and derived astrophysical parameters.

The ExoFOP-K2 C9 site includes a list of microlensing events within the K2 field and lists of telescope resources for follow-up observations. Users can upload their own data to the site.

Additional Links



Last updated 4 April 2019