activity
20062008
most citedOptical and IR observations of SN 2002dj: some possible common properties of fast expanding SNe Ia

96 citations · 239 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph200836 cited

Early-type galaxies in the near-infrared: 1.5-2.4\mum spectroscopy

M. Cesetti, V. D. Ivanov, L. Morelli +6

Near-infrared (hereafter NIR) data may provide complementary information to the traditional optical population synthesis analysis of unresolved stellar populations because the spec…

astro-ph200896 cited

Optical and IR observations of SN 2002dj: some possible common properties of fast expanding SNe Ia

G. Pignata, S. Benetti, P. A. Mazzali +17

As part of the European Supernova Collaboration we obtained extensive photometry and spectroscopy of the type Ia SN 2002dj covering epochs from 11 days before to nearly two years a…

astro-ph2008

The GALEX UV emission in shell galaxies

A. Marino, R. Rampazzo, R. Tantalo +4

Shell galaxies are widely considered the debris of recent accretion/merging episodes. Their high frequency in low density environment suggests that such episodes could be among the…

astro-ph200764 cited

The GALEX UV emission in shell galaxies: tracing galaxy "rejuvenation" episodes

R. Rampazzo, A. Marino, R. Tantalo +6

We present the GALEX far FUV and near NUV ultraviolet imaging of three nearby shell galaxies, namely NGC 2865, NGC 5018 and NGC 7135. The system of shells and fine structures visib…

astro-ph20071 cited

Early Type Galaxies in the Mid Infrared: a new flavor to their stellar populations

A. Bressan, P. Panuzzo, O. Vega +6

The mid infrared emission of early type galaxies traces the presence of intermediate age stellar populations as well as even tiny amounts of ongoing star formation. Here we discuss…

astro-ph200642 cited

NGC5719/13: interacting spirals forming a counter-rotating stellar disc

D. Vergani, A. Pizzella, E. M. Corsini +4

(Context) When a galaxy acquires material from the outside, it is likely that the resulting angular momentum of the accreted material is decoupled from that of the pre-existing gal…