Stefano Benetti

Extensive optical and near-infrared observations of the nearby, narrow-lined type Ic SN 2007gr: days 5 to 415 (2009)

Hunter, Deborah J., Valenti, Stefano, Kotak, Rubina, Meikle, Peter, Taubenberger, Stefan, Pastorello, Andrea, ...

We present photometric and spectroscopic observations at optical and near-infrared wavelengths of the nearby type Ic SN 2007gr. These represent the most extensive data-set to date of any supernova of...

A low energy core-collapse supernova without a hydrogen envelope (2009)

Valenti, Stefano, Pastorello, Andrea, Cappellaro, Enrico, Benetti, Stefano, Mazzali, Paolo, Manteca, Jose, ...

The final fate of massive stars depends on many factors, including mass, rotation rate, magnetic fields and metallicity. Theory suggests that some massive stars (initially greater than 25-30 solar...

Reflections on reflexions – II. Effects of light echoes on the luminosity and spectra of Type Ia supernovae (2008)

O Patat, Stefano Benetti, Massimo Turatto

Due to the crucial role played by Type Ia supernovae (SNe) in modern cosmology (see e.g. the review by Leibundgut 2001), it is essential to understand the systematics which might affect the recent...

The metamorphosis of Supernova SN2008D/XRF080109: a link between Supernovae and GRBs/Hypernovae (2008)

Mazzali, Paolo A., Valenti, Stefano, Della Valle, Massimo, Chincarini, Guido, Sauer, Daniel N., Benetti, Stefano, ...

The only supernovae (SNe) to have shown early gamma-ray or X-ray emission thus far are overenergetic, broad-lined Type Ic SNe (Hypernovae - HNe). Recently, SN 2008D shows several novel features: (i)...

Spectral luminosity indicators in SNe Ia - Understanding the R(SiII) line strength ratio and beyond (2008)

Hachinger, Stephan, Mazzali, Paolo A., Tanaka, Masaomi, Hillebrandt, Wolfgang, Benetti, Stefano

SNe Ia are good distance indicators because the shape of their light curves, which can be measured independently of distance, varies smoothly with luminosity. This suggests that SNe Ia are a single...

The Outermost Ejecta of Type Ia Supernovae (2007)

Tanaka, Masaomi, Mazzali, Paolo A., Benetti, Stefano, Nomoto, Ken'ichi, Elias-Rosa, Nancy, Kotak, Rubina, ...

The properties of the highest velocity ejecta of normal Type Ia supernovae (SNe Ia) are studied via models of very early optical spectra of 6 SNe. At epochs earlier than 1 week before maximum, SNe...

Hypernova Signatures in the Late Rebrightening of GRB 050525A (2007)

Della Valle, Massimo, Malesani, Daniele, Bloom, Joshua S., Benetti, Stefano, Chincarini, Guido, D'Avanzo, Paolo, ...

We report observations of GRB 050525A, for which a Gemini North spectrum shows its redshift to be z = 0.606. This is the third closest long GRB discovered by Swift. We observed its afterglow using...

Consistent estimates of (56)Ni yields for type Ia supernovae (2006)

Stritzinger, Maximilian, Mazzali, Paolo, Sollerman, Jesper, Benetti, Stefano

We present (56)Ni mass estimates for seventeen well-observed type Ia supernovae determined by two independent methods. Estimates of the (56)Ni mass for each type Ia supernova are determined from (1)...

Spectroscopy of the type Ia supernova SN 2002er: days -11 to +215 (2005)

Kotak, Rubina, Meikle, Peter, Pignata, Giuliano, Stehle, Matthias, Smartt, Steve, Benetti, Stefano, ...

We present an extensive set of optical spectroscopy of the nearby type Ia supernova, SN 2002er, with 24 epochs spanning -11 to +34 days. Its spectral evolution is fairly typical of a type Ia...

The tetra-lobed planetary nebula NGC 1501 (2000)

Sabbadin, Franco, Benetti, Stefano, Cappellaro, Enrico, Turatto, Massimo

Direct imagery and long-slit, spatially resolved echellograms of the high excitation planetary nebula NGC 1501 allowed us to study in detail the expansion velocity field, the physical conditions...

SN 1995ah-the first supernova observed in a Blue Compact Dwarf galaxy (1997)

Popescu, Cristina C., Rafanelli, Piero, Benetti, Stefano, Hopp, Ulrich, Birkle, Kurt, Elsaesser, Hans

We present the properties of the supernova SN 1995ah discovered in a Blue Compact Dwarf galaxy (BCD) around 10 days after the maximum. This is the first supernova event observed in a BCD. The...