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# Program information file
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PROGRAM_ID 2024A991
PROGRAM_TITLE iSHELL Determination of Mass and Age of Stars with Protoplanetary Disks
PROGRAM_INV1 Ellen Lee
PROGRAM_INV2
PROGRAM_INV3
PROGRAM_INV4
PROGRAM_INV5
PROGRAM_SCICAT stellar
PROGRAM_ABSTRACT_BEG
We plan to use the K2 mode of iSHELL to observe metal (esp. Al, Ca, Na, and Fe) and the CO
absorption lines at high resolution to model the physical properties of young stars. These stars have disks that will be mapped at very high spatial resolution with Subaru/SCExAO.
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