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update Design content
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skterry committed Feb 20, 2025
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Expand Up @@ -8,12 +8,13 @@ gravitational microlensing survey from space. In order to maximize the number of
Roman will detect, the survey fields will be placed in the highly-crowded stellar region towards
the galactic bulge.

There have been several proposed designs for the GBTDS observing strategy,
There have been several provisional designs for the GBTDS observing strategy,
a recap of these designs can be found in the following works:

1. [Spergel et al. 2015](https://arxiv.org/abs/1503.03757){:target="_blank"}
2. [Penny et al. 2019](https://iopscience.iop.org/article/10.3847/1538-4365/aafb69/meta){:target="_blank"}
3. [GBTDS Definition Committee Report](https://asd.gsfc.nasa.gov/roman/comm_forum/forum_17/Core_Community_Survey_Reports-rev03-compressed.pdf){:target="_blank"}
2. [Akeson et al. 2019](https://arxiv.org/abs/1902.05569){:target="_blank"}
3. [Penny et al. 2019](https://iopscience.iop.org/article/10.3847/1538-4365/aafb69/meta){:target="_blank"}
4. [GBTDS Definition Committee Report (2025)](https://asd.gsfc.nasa.gov/roman/comm_forum/forum_17/Core_Community_Survey_Reports-rev03-compressed.pdf){:target="_blank"}

## Pre-launch Observing Strategy (as of 2025)
The nominal GBTDS observing strategy will use the wide-field instrument (WFI) to image a total of seven fields
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