About
								
								 My name is Nishil Mehta, and I am a PhD student at Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, 
								Laboratoire Lagrange, France. I am working with Vivien Parmentier and Tristan Guillot on the topic of "Study of atmosphere 
								of exoplanets". I use the ADAM (SPARC/MITgcm) to 3D model the atmosphere of exoplanets. Using the GCMs, 
									I model the planet and it's spectra and compare it with the observations. For more details check my research.
								 
								
								I did my BS-MS Dual Degree (Combined Bachelor's and Master's) at Indian 
								Institute of Science Education and Research, Thiruvananthapuram with Major in Physics and minor in Data Science. My Minor thesis 
								project was based on using Machine Learning to characterize Gamma-ray Bursts (GRBs), it was published in 
								The Astophysical Journal. 
								For my Masters' Thesis, I worked on the topic "The study of the Exoplanetary Atmosphere and investigation of biosignatures" 
								(Mehta et. al. in prep.) where I develop an astrobiology model for Archean Earth-like planet to study biosignatures.
								For the entire duration of my BS-MS Dual Degree, I was awarded the 
								INSPIRE 
								(Innovation in Scientific Pursuit for Inspired Research) Scholarship - Scholarship for Higher Education by the Department 
								of Science and Technology (DST), Government of India.
								I also started an Astronomy club at IISER-TVM called Parsec (check out the 
								website).
								 
								I love skating and was a part of the Indian team. I represented India at 
								World Slalom Skating Association at China and Thailand Slalom Association where I secured 3rd rank. 
								
							
						
							
								Research
								
								 
								Planets are 3D!
Video credit: T. Mikal-Evans (MPIA) / T. Müller (MPIA/HdA)
								Planets are 3D, and modelling the atmosphere using General Circulation 
								Models can help us understand the atmosphere and the observations in detail. 
								
								 
								I use ADAM (SPARC/MITgcm) to model the atmosphere of exoplanets. 
								This model has been successfully applied to a wide range of exoplanets, including hot Jupiters (e.g. Showman et al. 2009, 2015; 
								Liu and Showman 2013; Parmentier et al. 2013, 2016, 2018, 2021; Kataria et al. 2015, 2016; Lewis et al. 2017; Steinrueck et al. 2019; 
								Tan et al. 2024), highly eccentric hot Jupiters (e.g. Kataria et al. 2013; Lewis et al. 2014), warm Jupiters (Showman, Lewis & Fortney 2015), 
								mini-Neptunes (Kataria et al. 2014; Zhang and Showman 2017), and terrestrial exoplanets (Carone, Keppens & Decin 2014). This model couples the 
								dynamical code from the MITgcm (Adcroft et al. 2004) with the plane-parallel radiative transfer code of 
								Marley & McKay (1999) and solves the primitive equations on a cube-sphere grid.
								
								 
								Temperature Map at different pressures
								
								
								 
								Credit: D. Spiegel.  Related paper: Burrows et al. (2010)
								
								
								 I am a member of MANATEE: MIRI And NIRCam Assay for the Transmission 
								and Emission of Exoplanets, a JWST guaranteed time observations program. 
								 
								
							
						
							
								About
								 
							
						
							
								Publications
								
								
									
										- Heat Reveals What Clouds Conceal: Global Carbon & Longitudinally Asymmetric Chemistry on LTT 9779 b
											
 Ashtari, R., et al., including Mehta N. | Submitted to The Astrophysical Journal
- How clear are the skies of WASP-80b?: 3D Cloud feedback on the atmosphere and spectra of the warm Jupiter
											
 Mehta N. et al. | Submitted to Astronomy & Astrophysics
- A Precise Metallicity and Carbon-to-Oxygen Ratio for a Warm Giant Exoplanet from its Panchromatic JWST Emission Spectrum
											
 Wiser, L., et al., including Mehta N. | Journal: Proceedings of the National Academy of Sciences | U.S.A. 122 (39) e2416193122
- A Panchromatic Characterization of the Evening and Morning Atmosphere of WASP-107 b: Composition and Cloud Variations, and Insight into the Effect of Stellar Contamination
											
 Murphy, M., et al., including Mehta N. | Journal: The Astronomical Journal | AJ 170 61
- A Possible Metal-Dominated Atmosphere Below the Thick Aerosols of GJ 1214 b Suggested by its JWST Panchromatic Transmission Spectrum
											
 Ohno, K., et al., including Mehta N. | Journal: The Astrophysical Journal Letters | ApJL 979, L7 (2025)
- Possible Carbon Dioxide above the Thick Aerosols of GJ 1214 b
											
 Schlawin, E., et al., including Mehta N. | Journal: The Astrophysical Journal Letters | ApJL 974, L33 (2024)
- Multiple Clues for Dayside Aerosols and Temperature Gradients in WASP-69 b from a Panchromatic JWST Emission Spectrum
											
 Schlawin, E., et al., including Mehta N. | Journal: The Astrophysical Journal | ApJ 168, 104 (2024)
- Exploring Gamma-Ray Burst Diversity: Clustering Analysis of the Emission Characteristics of Fermi- 
										and BATSE-detected Gamma-Ray Bursts
											
 Nishil Mehta and Shabnam Iyyani | Journal: The Astrophysical Journal | ApJ 969, 88 (2024)
Contact
								
								
							
						
							
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									i = 0;
while (!deck.isInOrder()) {
    print 'Iteration ' + i;
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}
print 'It took ' + i + ' iterations to sort the deck.';
								
								
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