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SUMMARY:High Resolution Atmospheric Retrieval on an Ultra Hot Jupiter
DTSTART;VALUE=DATE-TIME:20220907T081500Z
DTEND;VALUE=DATE-TIME:20220907T083000Z
DTSTAMP;VALUE=DATE-TIME:20241101T160812Z
UID:indico-contribution-139@meetings.aip.de
DESCRIPTION:Speakers: Jorge Sanchez (Arizona State University)\nWe present
  High Resolution Cross Correlation Spectroscopy (HRCCS) observations and a
 tmospheric retrieval results of the Ultra Hot Jupiter\, MASCARA-1b. HRCCS 
 is a novel technique used to characterize exoplanets with ground-based ins
 truments by utilizing the planet's time-resolved Doppler shifted signal to
  separate it from the dominant stellar and telluric lines. The high spectr
 al resolution along with wide wavelength coverage allows for robust constr
 aints on molecular abundances and thermal structures using bayesian retrie
 val techniques. \n\n\nWe present our atmospheric retrieval results of MASC
 ARA-1b using data taken from the IGRINS instrument (R~45000) at Gemini Sou
 th. This high fidelity data provides robust constraints on molecular abund
 ances in order to calculate C/O ratios and probe the thermal structure of 
 the planet.\n\nhttps://iaus379.aip.de/event/16/contributions/139/
LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall
URL:https://iaus379.aip.de/event/16/contributions/139/
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