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
- 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. | Accepted by PNAS (Proceedings of the National Academy of Sciences)
- 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. | Accepted by The Astronomical Journal
- 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
Elements
Text
This is bold and this is strong. This is italic and this is emphasized.
This is superscript text and this is subscript text.
This is underlined and this is code: for (;;) { ... }
. Finally, this is a link.
Heading Level 2
Heading Level 3
Heading Level 4
Heading Level 5
Heading Level 6
Blockquote
Preformatted
i = 0;
while (!deck.isInOrder()) {
print 'Iteration ' + i;
deck.shuffle();
i++;
}
print 'It took ' + i + ' iterations to sort the deck.';
Lists
Unordered
- Dolor pulvinar etiam.
- Sagittis adipiscing.
- Felis enim feugiat.
Alternate
- Dolor pulvinar etiam.
- Sagittis adipiscing.
- Felis enim feugiat.
Ordered
- Dolor pulvinar etiam.
- Etiam vel felis viverra.
- Felis enim feugiat.
- Dolor pulvinar etiam.
- Etiam vel felis lorem.
- Felis enim et feugiat.
Icons
Actions
Table
Default
Name |
Description |
Price |
Item One |
Ante turpis integer aliquet porttitor. |
29.99 |
Item Two |
Vis ac commodo adipiscing arcu aliquet. |
19.99 |
Item Three |
Morbi faucibus arcu accumsan lorem. |
29.99 |
Item Four |
Vitae integer tempus condimentum. |
19.99 |
Item Five |
Ante turpis integer aliquet porttitor. |
29.99 |
|
100.00 |
Alternate
Name |
Description |
Price |
Item One |
Ante turpis integer aliquet porttitor. |
29.99 |
Item Two |
Vis ac commodo adipiscing arcu aliquet. |
19.99 |
Item Three |
Morbi faucibus arcu accumsan lorem. |
29.99 |
Item Four |
Vitae integer tempus condimentum. |
19.99 |
Item Five |
Ante turpis integer aliquet porttitor. |
29.99 |
|
100.00 |