Area of research
Astronomy and Astrophysics · Nuclear and High Energy Physics
Research interest
Research interests include Physics, Astrophysics, Supernova, Ejecta, Astronomy, and White dwarf.
SN 2018is: A low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases
A radio-detected type Ia supernova with helium-rich circumstellar material
Evidence for Multiple Shocks from the γ-Ray Emission of RS Ophiuchi
Another shipment of six short-period giant planets from <i>TESS</i>
The multiwavelength view of shocks in the fastest nova V1674 Her
The Early Light Curve of SN 2023bee: Constraining Type Ia Supernova Progenitors the Apian Way
Strong Carbon Features and a Red Early Color in the Underluminous Type Ia SN 2022xkq
The first nova eruption in a novalike variable: YZ Ret as seen in X-rays and <i>γ</i>-rays
A Bright Ultraviolet Excess in the Transitional 02es-like Type Ia Supernova 2019yvq
Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
Circumstellar Medium Constraints on the Environment of Two Nearby Type Ia Supernovae: SN 2017cbv and SN 2020nlb
Constraints on the sub-pc environment of the nearby Type Iax SN 2014dt from deep X-ray and radio observations
A Bright Ultraviolet Excess in the Transitional 02es-like Type Ia Supernova 2019yvq
Circumstellar Medium Constraints on the Environment of Two Nearby Type Ia Supernovae: SN 2017cbv and SN 2020nlb
Improved Dynamical Constraints on the Masses of the Central Black Holes in Nearby Low-mass Early-type Galactic Nuclei and the First Black Hole Determination for NGC 205
SN 2017gmr: An Energetic Type II-P Supernova with Asymmetries
ThunderKAT: The MeerKAT Large Survey Project for Image-Plane Radio Transients
A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray-luminous Classical Nova to Date
Ejection of the Massive Hydrogen-rich Envelope Timed with the Collapse of the Stripped SN 2014C
Deep radio imaging of 47 Tuc identifies the peculiar X-ray source X9 as a new black hole candidate
RELATIVISTIC SUPERNOVAE HAVE SHORTER-LIVED CENTRAL ENGINES OR MORE EXTENDED PROGENITORS: THE CASE OF SN 2012ap
ON THE SOURCE OF THE DUST EXTINCTION IN TYPE Ia SUPERNOVAE AND THE DISCOVERY OF ANOMALOUSLY STRONG Na I ABSORPTION
A PANCHROMATIC VIEW OF THE RESTLESS SN 2009ip REVEALS THE EXPLOSIVE EJECTION OF A MASSIVE STAR ENVELOPE
THE ULTRAVIOLET-BRIGHT, SLOWLY DECLINING TRANSIENT PS1-11af AS A PARTIAL TIDAL DISRUPTION EVENT
MULTI-WAVELENGTH OBSERVATIONS OF SUPERNOVA 2011ei: TIME-DEPENDENT CLASSIFICATION OF TYPE IIb AND Ib SUPERNOVAE AND IMPLICATIONS FOR THEIR PROGENITORS
PS1-10afx AT<i>z</i>= 1.388: PAN-STARRS1 DISCOVERY OF A NEW TYPE OF SUPERLUMINOUS SUPERNOVA
PS1-12sk IS A PECULIAR SUPERNOVA FROM A He-RICH PROGENITOR SYSTEM IN A BRIGHTEST CLUSTER GALAXY ENVIRONMENT
An ultraviolet–optical flare from the tidal disruption of a helium-rich stellar core
Two stellar-mass black holes in the globular cluster M22
PANCHROMATIC OBSERVATIONS OF SN 2011dh POINT TO A COMPACT PROGENITOR STAR