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55 Cancri e Atmospheric Analysis

I aided to the analysis of the atmosphere of the lava planet, 55 cancri e, by tophatting the spectra, which is essential because it reverses the effects of signal smearing over the pixels caused by long exposure times.

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Gaia releases uncalibrated spectra of variable light sources. In order to unlock spectra for thousands of variable stellar objects, I built a data-driven response model using the Gaia Photometric Science epochal BP/RP spectra from Type Ia supernoave that accurately calibrates these spectra.

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Gaia Photometric Science Alerts Response Model

Do you have any questions?

Please feel free to contact me! I would love to help answer any questions you may have about my undergraduate research.

CONTACT ME

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Post-Bac Researcher

Personal Email:

hagee.celeste.2020 @ gmail.com

NASA email:

celeste.hagee @ nasa.gov

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