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20012025
most citedDust and the type II-plateau supernova 2004et

209 citations · 523 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2025★ 1 cited

Evidence for inefficient dust production in a massive, metal-rich galaxy at uncovered by JWST and ALMA

Kasper E. Heintz, Darach Watson, Francesco Valentino +17

Recent observations have revealed a remarkably rapid buildup of cosmic dust in the interstellar medium (ISM) of high redshift galaxies, with complex dust compositions and large abu…

astro-ph.GA2023★ 27 cited

Dust depletion of of metals from local to distant galaxies II: Cosmic dust-to-metal ratio and dust composition

Christina Konstantopoulou, Annalisa De Cia, Cédric Ledoux +10

The evolution of the cosmic dust content and the cycle between metals and dust in the interstellar medium (ISM) play a fundamental role in galaxy evolution. The chemical enrichment…

astro-ph.GA2014★ 62 cited

The Herschel exploitation of local galaxy Andromeda (HELGA) V: Strengthening the case for substantial interstellar grain growth

L. Mattsson, H. L. Gomez, A. C. Andersen +7

In this paper we consider the implications of the distributions of dust and metals in the disc of M31. We derive mean radial dust distributions using a dust map created from Hersch…

astro-ph.SR2011★ 88 cited

Dust and the type II-Plateau supernova 2004dj

Peter Meikle, Rubina Kotak, Duncan Farrah +13

We present mid-infrared (MIR) spectroscopy of a Type II-plateau supernova, SN 2004dj, obtained with the Spitzer Space Telescope, spanning 106--1393 d after explosion. MIR photometr…

astro-ph.SR2009★ 209 cited

Dust and the type II-plateau supernova 2004et

Rubina Kotak, Peter Meikle, Duncan Farrah +14

We present mid-infrared (MIR) observations of the Type II-plateau supernova (SN) 2004et, obtained with the {\it Spitzer Space Telescope} between days 64 and 1406 past explosion. La…

astro-ph2007★ 1 cited

The Nature of the Far-UV Break in the Energy Distribution of Quasars

L. Binette, S. Haro-Corzo, Y. Krongold +1

A prominent continuum steepening is observed in quasar energy distributions near 1100A. We review possible interpretations for the physical origin of this so-called far-UV break.