Dr Deepak Chahal

Postdoctoral Research Associate in Stars and Planets
Email: d.chahal@qmul.ac.ukRoom Number: G.O. Jones Building, Room 504Website: https://dchahal-stardust.lovable.app/
Profile
I am a postdoctoral researcher in the Stars and Planets group led by Dr Ed Gillen. My work focuses on constraining the stellar evolution in low-mass star regime, from working on characterising their magnetic fields – stellar activity & activity cycles, Lithium depletion, stellar rotation etc., to building a precise data-driven stellar age dating model for the main-sequence stars.
I completed my PhD, “Investigating Magnetic Activity and Activity Cycles in Cool, young main-sequence stars”, at Macquarie University, Australia, under the supervision of Prof. Richard de Grijs and Dr. Devika Kamath. Originally from India, I transitioned from a background of Mechanical Engineering to Astrophysics, obtaining my master’s degree from the Indian Institute of Space Science & Technology.
Research
Research Interests:
I am currently developing a comprehensive, data-driven stellar age-determination model for low-mass stars, capable of characterising ages from ~1 Myr to 10 Gyr. I have also developed a methodology to combine multi-survey time-series photometry to detect magnetic activity cycles in low-mass stars, which I am now applying to identify cycles in Sun-like stars.
I have extensive experience working with both space- and ground-based photometric and spectroscopic facilities, including Kepler/K2, ZTF, LAMOST, GALAH, ASAS-SN, Gaia, and TESS.
My wider research interests include:
- Stellar and exoplanet Evolution
- Stellar activity and magnetic activity cycles
- Stellar Rotation and Gyrochronology
- Impact of host-star’s activity on exoplanetary atmosphere
Publications
Chahal, D., Kamath, D., de Grijs, R., T. Montet, B. & Chen, X. (2025): Photometric Activity Cycles in fast-rotating Stars: Revisiting the Stellar Activity Cycle branches, MNRAS, 540, 1, 668-687.
Chahal, D., Kamath, D., de Grijs, R., Ventura, P. & Chen, X. (2023): Unravelling the period gap using LAMOST chromospheric activity indices, MNRAS, 525, 3, 4026-4041.
Chahal, D., de Grijs, R., Kamath, D., & Chen, X. (2022): Statistics of BY Draconis Chromospheric Variables MNRAS, 514, 4, 4932-4943.
My full publication list can be viewed on ADS.