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  <title><![CDATA[CRA Seminar | Dr. Arthur Daniel Adams | University of Virginia| Host: Dr. Gongjie Li]]></title>
  <body><![CDATA[<p><strong>Speaker: </strong>Dr. Arthur Daniel Adams</p><p><strong>Host: </strong>Dr. Gongjie Li</p><p><strong>Title: </strong>Mapping Sub-stellar Companions in Time and Space</p><p><strong>Abstract:</strong> Companion brown dwarfs and exoplanets are complex objects whose time and spatial variability are now being mapped with high-fidelity infrared observations from JWST. I will begin by presenting our analysis of JWST NIRSpec/IFU PRISM observations of the 2M1207 system that represent the first spectroscopic time monitoring of a planetary-mass companion simultaneously with its host. By monitoring the variability of the system as a whole, we are sensitive both to the time evolution of atmospheric structure --- including through hot spots and clouds --- as well as external variability such as the accretion of disk material. 2M1207 A's spectra show multiple time-dependent structures across the near-infrared. While we do not see a full rotation within our observations, we do capture non-linear trends in time across much of the spectra, with localized regions showing light curves that hint at the possibility of variability imparted by the circum-stellar disk. The planetary-mass 2M1207 b's spectra generally corroborate the interpretation of recent atmospheric characterizations, where a simple cloud evolution model can capture most of the short-term variability. Turning to spatial variability, I will also provide a first look at the eclipse mapping of brown dwarfs in orbit around white dwarfs. These systems provide a unique opportunity to study the spatially-resolved structures of highly-irradiated atmospheres. Finally, I will highlight ongoing student research in brown dwarfs and exoplanets at UVA, which includes the spectral and orbital characterization of the aforementioned brown-dwarf/white-dwarf binaries as a complement to atmospheric studies, as well as classifying the seasonal evolution of Earth's vegetation as spectral signatures of the response of the majority of Earth's life by mass&nbsp;to the solar energy budget.</p>]]></body>
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      <value><![CDATA[<p><strong>Abstract:</strong>&nbsp;</p><p>Companion brown dwarfs and exoplanets are complex objects whose time and spatial variability are now being mapped with high-fidelity infrared observations from JWST. I will begin by presenting our analysis of JWST NIRSpec/IFU PRISM observations of the 2M1207 system that represent the first spectroscopic time monitoring of a planetary-mass companion simultaneously with its host. By monitoring the variability of the system as a whole, we are sensitive both to the time evolution of atmospheric structure --- including through hot spots and clouds --- as well as external variability such as the accretion of disk material. 2M1207 A's spectra show multiple time-dependent structures across the near-infrared. While we do not see a full rotation within our observations, we do capture non-linear trends in time across much of the spectra, with localized regions showing light curves that hint at the possibility of variability imparted by the circum-stellar disk. The planetary-mass 2M1207 b's spectra generally corroborate the interpretation of recent atmospheric characterizations, where a simple cloud evolution model can capture most of the short-term variability. Turning to spatial variability, I will also provide a first look at the eclipse mapping of brown dwarfs in orbit around white dwarfs. These systems provide a unique opportunity to study the spatially-resolved structures of highly-irradiated atmospheres. Finally, I will highlight ongoing student research in brown dwarfs and exoplanets at UVA, which includes the spectral and orbital characterization of the aforementioned brown-dwarf/white-dwarf binaries as a complement to atmospheric studies, as well as classifying the seasonal evolution of Earth's vegetation as spectral signatures of the response of the majority of Earth's life by mass&nbsp;to the solar energy budget.</p>]]></value>
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