The Type Ia supernova SN 2011fe is one of the closest supernovae of the past decades. Due to its proximity and low dust extinction, this object provides a very rare opportunity to study the extremely late time evolution (>900 days) of thermonuclear su
Hubble Space Telescope spectroscopic observations of the nearby Type Ia supernova (SN Ia) SN 2011fe,...
Seitenzahl et al. have predicted that roughly three years after its explosion, the light we receive ...
Photometric and spectroscopic observations of a slowly declining, luminous type Ia supernova (SN Ia)...
The Type Ia supernova SN 2011fe is one of the closest supernovae of the past decades. Due to its pro...
We present late-time optical R-band imaging data from the Palomar Transient Factory (PTF) for the ne...
Due to the small amount of hydrogen (≤0.1 M ⊙) remaining on the surface of their progenitors, SNe II...
We present late-epoch optical photometry (BVRI) of seven normal/super-luminous Type Ia supernovae: S...
The very nearby Type Ia supernova 2014J in M82 offers a rare opportunity to study the physics of the...
Hubble Space Telescope spectroscopic observations of the nearby Type Ia supernova (SN Ia) SN 2011fe,...
We present an in-depth study of the late-time near-infrared plateau in Type Ia supernovae (SNe Ia), ...
Includes bibliographical references (pages 43-45).Type Ia supernovae (SNe Ia) are excellent cosmolog...
Hubble Space Telescope spectroscopic observations of the nearby Type Ia supernova (SN Ia) SN 2011fe,...
We use observed UV through near-IR spectra to examine whether SN 2011fe can be understood in the fra...
The UBVRI photometric follow-up of SN 2011fu has been initiated a few days after the explosion, show...
The use of Type Ia supernovae as cosmological tools has reinforced the need to better understand the...
Hubble Space Telescope spectroscopic observations of the nearby Type Ia supernova (SN Ia) SN 2011fe,...
Seitenzahl et al. have predicted that roughly three years after its explosion, the light we receive ...
Photometric and spectroscopic observations of a slowly declining, luminous type Ia supernova (SN Ia)...
The Type Ia supernova SN 2011fe is one of the closest supernovae of the past decades. Due to its pro...
We present late-time optical R-band imaging data from the Palomar Transient Factory (PTF) for the ne...
Due to the small amount of hydrogen (≤0.1 M ⊙) remaining on the surface of their progenitors, SNe II...
We present late-epoch optical photometry (BVRI) of seven normal/super-luminous Type Ia supernovae: S...
The very nearby Type Ia supernova 2014J in M82 offers a rare opportunity to study the physics of the...
Hubble Space Telescope spectroscopic observations of the nearby Type Ia supernova (SN Ia) SN 2011fe,...
We present an in-depth study of the late-time near-infrared plateau in Type Ia supernovae (SNe Ia), ...
Includes bibliographical references (pages 43-45).Type Ia supernovae (SNe Ia) are excellent cosmolog...
Hubble Space Telescope spectroscopic observations of the nearby Type Ia supernova (SN Ia) SN 2011fe,...
We use observed UV through near-IR spectra to examine whether SN 2011fe can be understood in the fra...
The UBVRI photometric follow-up of SN 2011fu has been initiated a few days after the explosion, show...
The use of Type Ia supernovae as cosmological tools has reinforced the need to better understand the...
Hubble Space Telescope spectroscopic observations of the nearby Type Ia supernova (SN Ia) SN 2011fe,...
Seitenzahl et al. have predicted that roughly three years after its explosion, the light we receive ...
Photometric and spectroscopic observations of a slowly declining, luminous type Ia supernova (SN Ia)...
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