activity
20072011
most citedThe Type Ic SN 2007gr: a census of the ejecta from late-time optical-infrared spectra

83 citations · 333 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2011★ 19 cited

NERO - A Post Maximum Supernova Radiation Transport Code

I. Maurer, A. Jerkstrand, P. A. Mazzali +5

The interpretation of supernova (SN) spectra is essential for deriving SN ejecta properties such as density and composition, which in turn can tell us about their progenitors and t…

astro-ph.SR2011★ 43 cited

The nebular spectrum of the type Ia supernova 2003hv: evidence for a non-standard event

Paolo A. Mazzali, I. Maurer, M. Stritzinger +3

The optical and near-infrared late-time spectrum of the under-luminous Type Ia supernova 2003hv is analysed with a code that computes nebular emission from a supernova nebula. Synt…

astro-ph.SR2010★ 44 cited

Abundance stratification in Type Ia supernovae - III. The normal SN 2003du

Masaomi Tanaka, Paolo A. Mazzali, Vallery Stanishev +3

The element abundance distributions in the ejecta of Type Ia supernova (SN) is studied by modelling a time series of optical spectra of SN 2003du until ~1 year after the explosion.…

astro-ph.HE2010★ 43 cited

Hydrogen and helium in the late phase of SNe IIb

I. Maurer, P. Mazzali, S. Taubenberger +1

Supernovae of Type IIb contain large fractions of helium and traces of hydrogen, which can be observed in the early and late spectra. Estimates of the hydrogen and helium mass and…

astro-ph.HE2010★ 83 cited

The Type Ic SN 2007gr: a census of the ejecta from late-time optical-infrared spectra

P. A. Mazzali, I. Maurer, S. Valenti +2

Nebular spectra of Supernovae (SNe) offer an unimpeded view of the inner region of the ejecta, where most nucleosynthesis takes place. Optical spectra cover most, but not all of th…

astro-ph.HE2010★ 17 cited

Oxygen Recombination in the nebular phase of supernovae 1998bw and 2002ap

Immanuel Maurer, Paolo Mazzali

Late-time spectra of stripped-envelope CC-SNe are dominated by strong [O {\sc i}] 6300,6363 emission, caused by thermal electron excitation of forbidden [O {\sc i}] transitions…

astro-ph.HE2009★ 42 cited

Characteristic velocities of stripped-envelope core-collapse supernova cores

I. Maurer, P. A. Mazzali, J. Deng +9

The velocity of the inner ejecta of stripped-envelope core-collapse supernovae (CC-SNe) is studied by means of an analysis of their nebular spectra. Stripped-envelope CC-SNe are th…

astro-ph2007★ 42 cited

Ignition latitude and the shape of Type I X-ray bursts

Immanuel Maurer, Anna L. Watts

The shape of the lightcurve during the rising phase of Type I X-ray bursts is determined by many factors including the ignition latitude, the accretion rate, and the rotation rate…