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-permalink: /about/
-title: "About RGES PIT"
----
-
-RGES PIT stands for the **R**oman **G**alactic **E**xoplanet **S**urvey 
-**P**roject **I**nfrastructure **T**eam. Formed in 2023, our NASA-funded team is
-building the software and human infrastructure required to successfully execute the exoplanet component of the
-GBTDS. The 2020 Decadal Survey states that Roman is *“the only platform in the coming decades 
-that can produce a statistical census of planetary occurrence as a function of orbital 
-separation and mass, from terrestrials to gas giants, beyond 1 AU”*.
-
-
-The exoplanet survey will make use of Roman's wide-field instrument (WFI): The RGES PIT
-has four major scientific and programmatic objectives:
-
-* Confirm and/or reconfirm the five level-1 RGES science requirements
-* Improve the microlensing event rate and yield calculations by improving the input Galactic models, 
-incorporating new measurements of the near-infrared event rate obtained by the PRIME survey
-* Develop and test the prototype photometry and astrometry pipeline, event detection pipeline, 
-lightcurve modeling pipeline, and detection efficiency (or completeness) pipeline, with the goal of 
-making these publicly-available and user-friendly
-* Develop the occurrence rate formalism and methodology.
-
-Click through for more details on the [Team]({{ site.url }}{{
-site.baseurl }}/about/team/), [RGES Design]({{ site.url }}{{
-site.baseurl }}/design/), or [RGES Science]({{ site.url }}{{
-site.baseurl }}/science/).
-
-
-