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20062009
most citedA neutron-star-driven X-ray flash associated with supernova SN 2006aj

313 citations · 1.9k across the 16 of their papers we have counts for

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astro-ph200842 cited

Optical photometry and spectroscopy of the type Ibn supernova SN 2006jc until the onset of dust formation

G. C. Anupama, D. K. Sahu, U. K. Gurugubelli +4

We present optical UBVRI photometric and spectroscopic data of the type Ibn supernova SN 2006jc, until the onset of the dust forming phase. The optical spectrum shows a blue contin…

astro-ph2008213 cited

Tycho Brahe's 1572 supernova as a standard type Ia explosion revealed from its light echo spectrum

Oliver Krause, Masaomi Tanaka, Tomonori Usuda +4

Type Ia supernovae (SNe Ia) are thermonuclear explosions of white dwarf stars in close binary systems. They play an important role as cosmological distance indicators and have led…

astro-ph2008258 cited

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

Paolo A. Mazzali, Stefano Valenti, Massimo Della Valle +38

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 n…

astro-ph200831 cited

Optical Spectropolarimetry and Asphericity of Type Ic SN 2007gr

Masaomi Tanaka, Koji S. Kawabata, Keiichi Maeda +2

We present optical spectropolarimetric observations of Type Ic supernova (SN) 2007gr with Subaru telescope at 21 days after the maximum brightness (~37 days after the explosion). N…

astro-ph200883 cited

Early Formation of Dust in the Ejecta of Type Ib SN 2006jc and Temperature and Mass of the Dust

T. Nozawa, T. Kozasa, N. Tominaga +8

SN 2006jc is a peculiar supernova (SN), in which the formation of dust has been confirmed at an early epoch of ~50 days after the explosion. We investigate the possibility of such…

astro-ph2008248 cited

Asphericity in Supernova Explosions from Late-Time Spectroscopy

Keiichi Maeda, Koji Kawabata, Paolo A. Mazzali +15

Core-collapse supernovae (CC-SNe) are the explosions that announce the death of massive stars. Some CC-SNe are linked to long-duration gamma-ray bursts (GRBs) and are highly aspher…