International audienceWe present VLT–FORS spectropolarimetric observations of the type II supernova (SN) 2012aw taken at seven epochs during the photospheric phase, from 16 to 120 d after explosion. We corrected for interstellar polarization by postulating that the SN polarization is naught near the rest wavelength of the strongest lines – this is later confirmed by our modeling. SN 2012aw exhibits intrinsic polarization, with strong variations across lines, and with a magnitude that grows in the 7000 Å line-free region from 0.1% at 16 d up to 1.2% at 120 d. This behavior is qualitatively similar to observations gathered for other type II SNe. A suitable rotation of Stokes vectors places the bulk of the polarization in q, suggesting the eje...
Aims. The main goal of this study is to probe the ejecta geometry and to get otherwise unobtainable ...
We present multiple spectropolarimetric observations of the nearby Type. Ia supernova (SN) 2011fe in...
Aims. We study possible signs of asymmetry in the luminous type IIn SN 2010jl, to obtain i...
We present VLT–FORS spectropolarimetric observations of the type II supernova (SN) 2012aw taken at s...
The origin of the diverse light-curve shapes of Type II supernovae (SNe), and whether they come from...
We present six epochs of optical spectropolarimetry of the Type II supernova (SN) 2023ixf ranging fr...
We present deep, nebular-phase spectropolarimetry of the Type II-P/L SN 2013ej, obtained 167 days af...
We present the first spectropolarimetric observations of a hydrogen-free superluminous supernova (SL...
We present a compilation of the geometry measures acquired using optical and IR spectroscopy and opt...
Unvealing the explosion geometry of core-collapse supernovae (CC SNe) helps to understand the explos...
Aims. We study possible signs of asymmetry in the luminous Type IIn SN 2010jl, to obtain independent...
Detailed spectropolarimetric studies may hold the key to probing the explosion mechanisms and the pr...
Spectropolarimetry provides the means to probe the 3D geometries of Supernovae at early times. We re...
The explosion processes of supernovae (SNe) are imprinted in their explosion geometries. Here, we st...
International audienceWe present synthetic single-line and continuum linear-polarization signatures ...
Aims. The main goal of this study is to probe the ejecta geometry and to get otherwise unobtainable ...
We present multiple spectropolarimetric observations of the nearby Type. Ia supernova (SN) 2011fe in...
Aims. We study possible signs of asymmetry in the luminous type IIn SN 2010jl, to obtain i...
We present VLT–FORS spectropolarimetric observations of the type II supernova (SN) 2012aw taken at s...
The origin of the diverse light-curve shapes of Type II supernovae (SNe), and whether they come from...
We present six epochs of optical spectropolarimetry of the Type II supernova (SN) 2023ixf ranging fr...
We present deep, nebular-phase spectropolarimetry of the Type II-P/L SN 2013ej, obtained 167 days af...
We present the first spectropolarimetric observations of a hydrogen-free superluminous supernova (SL...
We present a compilation of the geometry measures acquired using optical and IR spectroscopy and opt...
Unvealing the explosion geometry of core-collapse supernovae (CC SNe) helps to understand the explos...
Aims. We study possible signs of asymmetry in the luminous Type IIn SN 2010jl, to obtain independent...
Detailed spectropolarimetric studies may hold the key to probing the explosion mechanisms and the pr...
Spectropolarimetry provides the means to probe the 3D geometries of Supernovae at early times. We re...
The explosion processes of supernovae (SNe) are imprinted in their explosion geometries. Here, we st...
International audienceWe present synthetic single-line and continuum linear-polarization signatures ...
Aims. The main goal of this study is to probe the ejecta geometry and to get otherwise unobtainable ...
We present multiple spectropolarimetric observations of the nearby Type. Ia supernova (SN) 2011fe in...
Aims. We study possible signs of asymmetry in the luminous type IIn SN 2010jl, to obtain i...