Transient Astronomy

How stars explode?

Understanding stellar explosions through observations and radiative transfer modelling.

Synthetic nebular-phase spectrum, day +250

FIG. — Understanding stellar explosions through observations

ABOUT

Currently

I am a postdoctoral researcher working on spectral modeling of thermonuclear supernovae, using radiative transfer codes such as TARDIS. I am currently interested in non-thermal processes and late time energy deposition in supernovae. I am also interested in exotic stellar explosions which defy known explosion models.

Astrophysical Observations Radiative Transfer LSST TARDIS SEDONA

RESEARCH

Research Interests

Nebular-phase spectral modeling

One-zone and multi-zone NLTE codes for the late-time spectra of Type Ia supernovae, built to replace legacy nebular codes.

Peculiar thermonuclear explosions

Observing not so normal thermonuclear explosions and understanding how they can explode.

Faint but visible

Looking into LSST data to find faint emission from explosions.

Elusive Helium

Presence of He in stripped envelope stars.

Host or No Host?

Host galaxies of superluminous supernovae.

Gamma Rays from supernovae

COSI gamma-ray spectra of supernovae.

PUBLICATIONS

Selected papers

View full publication list →

OBSERVATIONS

Observations and Data Reduction

Photometry Spectroscopy
Visit site ↗

SOFTWARE

Tools I maintain or contributed

NEWS

Recent updates