12/1/2023 0 Comments Color me courtney internship![]() Dust storms can significantly influence atmospheric circulation and albedo. They are the most prominent meteorological phenomena in the Martian atmosphere. Project Description: Dust storms on Mars have long been an object of interest to the astronomical community. Student: Sierra Genne (University of Colorado Boulder) ![]() This planet, along with others detected from this follow-up project from 2020 to 2022, provides evidence against a break in the mass-ratio function that was suggested to account for a lack of low-mass-ratio planetary detections.Ģ. Of them, KMT-202Lb, is a sub-Neptune/super-Earth planet with a planet-to-host mass ratio of $7 \times 10^$. This project detected one confirmed planet, KMT-202Lb, and one candidate planet, KMT-202Lb. In this project, the student predicted high-magnification microlensing events using the microlensing survey data, took 50-100 hours of LCO observations, reduced the LCO images using difference imaging analysis, and searched for microlensing planets using the LCO and survey data. The powerful Las Cumbres Observatory (LCO) global network () can provide important observations for high-magnification microlensing events. The high-magnification microlensing events are sensitive to planets but need high-cadence follow-up observations to capture planetary signals. Project Description: The gravitational microlensing technique is most sensitive to long-period exoplanets and is currently the only method that can probe low-mass long-period exoplanets. Project Title: Detecting Microlensing Planets from LCO Follow-up Observations Student: Aislyn Bell (University of Colorado Boulder)Īdvisor: Weicheng Zang (CfA Fellow SSP) Mentor: Jennifer C.
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