The wavelength dependence of the extinction of Type Ia SN 2014J in the nearby galaxy M82 has been measured using UV to near-IR photometry obtained with the Hubble Space Telescope, the Nordic Optical Telescope, and the Mount Abu Infrared Telescope. This is the first time that the reddening of an SN Ia is characterized over the full wavelength range of 0.2-2 μm. A total-to-selective extinction, RV ≥ 3.1, is ruled out with high significance. The best fit at maximum using a Galactic type extinction law yields RV = 1.4 ± 0.1. The observed reddening of SN 2014J is also compatible with a power-law extinction, A λ/AV = (λ/λ V )p as expected from multiple scattering of light, with p = -2.1 ± 0.1. After correcting for differences in reddening, SN 201...
We present the intensive spectroscopic follow up of the Type Ia supernova (SN Ia) 2014J in the starb...
We present optical (UBVRI) and near-IR (YJHK) photometry of the normal Type Ia supernova (SN) 2004S....
We employ 76 type Ia supernovae (SNe Ia) with optical spectrophotometry within 2.5 days of B-band ma...
The wavelength dependence of the extinction of Type Ia SN 2014J in the nearby galaxy M82 has been me...
The wavelength-dependence of the extinction of Type Ia SN 2014J in the nearby galaxy M82 has been me...
We present optical and ultraviolet (UV) photometry and spectra of the very nearby and highly reddene...
We present ultraviolet (UV) observations of six nearby Type Ia supernovae (SNe Ia) obtained with the...
We present ultraviolet (UV) observations of six nearby Type Ia supernovae (SNe Ia) obtained with the...
We present ultraviolet (UV) observations of six nearby Type Ia supernovae (SNe Ia) obtained with the...
We report on the discovery of SN 2014J in the nearby galaxy M82. Given its proximity, it offers the ...
International audienceWe report on the discovery of SN 2014J in the nearby galaxy M82. Given its pro...
We report on the discovery of SN 2014J in the nearby galaxy M82. Given its proximity, it offers the ...
A precise extinction law is a critical input when interpreting observations of highly reddened sourc...
Artículo de publicación ISIWe present the intensive spectroscopic follow up of the Type Ia supernova...
Arítulo de publicación ISI.We present infrared photometry of supernova (SN) 1999em, plus optical pho...
We present the intensive spectroscopic follow up of the Type Ia supernova (SN Ia) 2014J in the starb...
We present optical (UBVRI) and near-IR (YJHK) photometry of the normal Type Ia supernova (SN) 2004S....
We employ 76 type Ia supernovae (SNe Ia) with optical spectrophotometry within 2.5 days of B-band ma...
The wavelength dependence of the extinction of Type Ia SN 2014J in the nearby galaxy M82 has been me...
The wavelength-dependence of the extinction of Type Ia SN 2014J in the nearby galaxy M82 has been me...
We present optical and ultraviolet (UV) photometry and spectra of the very nearby and highly reddene...
We present ultraviolet (UV) observations of six nearby Type Ia supernovae (SNe Ia) obtained with the...
We present ultraviolet (UV) observations of six nearby Type Ia supernovae (SNe Ia) obtained with the...
We present ultraviolet (UV) observations of six nearby Type Ia supernovae (SNe Ia) obtained with the...
We report on the discovery of SN 2014J in the nearby galaxy M82. Given its proximity, it offers the ...
International audienceWe report on the discovery of SN 2014J in the nearby galaxy M82. Given its pro...
We report on the discovery of SN 2014J in the nearby galaxy M82. Given its proximity, it offers the ...
A precise extinction law is a critical input when interpreting observations of highly reddened sourc...
Artículo de publicación ISIWe present the intensive spectroscopic follow up of the Type Ia supernova...
Arítulo de publicación ISI.We present infrared photometry of supernova (SN) 1999em, plus optical pho...
We present the intensive spectroscopic follow up of the Type Ia supernova (SN Ia) 2014J in the starb...
We present optical (UBVRI) and near-IR (YJHK) photometry of the normal Type Ia supernova (SN) 2004S....
We employ 76 type Ia supernovae (SNe Ia) with optical spectrophotometry within 2.5 days of B-band ma...