36 citations · 143 across the 6 of their papers we have counts for
6 papers
Quantifying the dust in SN 2012aw and iPTF14hls with ORBYTS
Maria Niculescu-Duvaz, M. J. Barlow, W. Dunn +32
Core-collapse supernovae (CCSNe) are potentially capable of producing large quantities of dust, with strong evidence that ejecta dust masses can grow significantly over extended pe…
Dust masses for a large sample of core-collapse supernovae from optical emission line asymmetries: dust formation on 30-year timescales
Maria Niculescu-Duvaz, Michael J Barlow, Antonia Bevan +7
Modelling the red-blue asymmetries seen in the broad emission lines of core-collapse supernovae (CCSNe) is a powerful technique to quantify total dust mass formed in the ejecta at…
Spitzer's Last Look at Extragalactic Explosions: Long-Term Evolution of Interacting Supernovae
Tamás Szalai, Ori D. Fox, Richard G. Arendt +10
Here we present new - and, nevertheless, last - mid-infrared (mid-IR) data for supernovae (SNe) based on measurements with the Spitzer Space Telescope. Comparing our recent 3.6 and…
Disentangling Dust Components in SN 2010jl: The First 1400 Days
A. M. Bevan, K. Krafton, R. Wesson +6
The luminous Type IIn SN 2010jl shows strong signs of interaction between the SN ejecta and dense circumstellar material. Dust may be present in the unshocked ejecta, the cool, den…
Supernova 2017eaw: molecule and dust formation from infrared observations
Samaporn Tinyanont, Mansi M Kasliwal, Kelsie Krafton +15
We present infrared (IR) photometry and spectroscopy of the Type II-P SN 2017eaw and its progenitor in the nearby galaxy NGC 6946. Progenitor observations in the Ks band in 4 epoch…
Early Dust Formation and a Massive Progenitor for SN 2011ja?
J. E. Andrews, Kelsie M. Krafton, Geoffrey C. Clayton +6
SN 2011ja was a bright (I = -18.3) Type II supernova occurring in the nearby edge on spiral galaxy NGC 4945. Flat-topped and multi-peaked H-alpha and H-beta spectral emission lines…