Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Astronomy, Ejecta, Supernova, and Radiative transfer.
A JWST Survey of the Supernova Remnant Cassiopeia A
Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
Serendipitous detection of the dusty Type IIL SN 1980K with <i>JWST</i>/MIRI
Deep <i>JWST</i>/NIRCam imaging of Supernova 1987A
Shockingly Bright Warm Carbon Monoxide Molecular Features in the Supernova Remnant Cassiopeia A Revealed by JWST
Disentangling Dust Components in SN 2010jl: The First 1400 Days
The dust content of the Crab Nebula
A decade of ejecta dust formation in the Type IIn SN 2005ip
η Carinae's Dusty Homunculus Nebula from Near-infrared to Submillimeter Wavelengths: Mass, Composition, and Evidence for Fading Opacity
<i>Herschel</i>detects oxygen in the<i>β</i>Pictoris debris disk
Early dust formation and a massive progenitor for SN 2011ja?
A STUBBORNLY LARGE MASS OF COLD DUST IN THE EJECTA OF SUPERNOVA 1987A
The second data release of the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS DR2)
DUST PRODUCTION AND PARTICLE ACCELERATION IN SUPERNOVA 1987A REVEALED WITH ALMA
Civil War Book Review 2014cited by 119position: middle
DISCOVERY OF TIME VARIATION OF THE INTENSITY OF MOLECULAR LINES IN IRC+10216 IN THE SUBMILLIMETER AND FAR-INFRARED DOMAINS
SPECTRAL AND MORPHOLOGICAL ANALYSIS OF THE REMNANT OF SUPERNOVA 1987A WITH ALMA AND ATCA
EXTREME CONDITIONS IN A CLOSE ANALOG TO THE YOUNG SOLAR SYSTEM: <i>HERSCHEL</i> OBSERVATIONS OF ϵ ERIDANI
The wind of W Hydrae as seen by<i>Herschel</i>
Alignment in star–debris disc systems seen by <i>Herschel</i>
CARBON MONOXIDE IN THE COLD DEBRIS OF SUPERNOVA 1987A
<i>Herschel</i>images of Fomalhaut
The enigmatic nature of the circumstellar envelope and bow shock surrounding Betelgeuse as revealed by<i>Herschel</i>
On the physical structure of IRC +10216
Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt
An independent distance estimate to CW Leonis
On the physical structure of IRC +10216 - Ground-based and Herschel observations of CO and C2H