Luis Boldt
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View article: SN 2009bb: A PECULIAR BROAD-LINED TYPE Ic SUPERNOVA,
SN 2009bb: A PECULIAR BROAD-LINED TYPE Ic SUPERNOVA, Open
Ultraviolet, optical, and near-infrared photometry and optical spectroscopy of the broad-lined Type Ic supernova (SN) 2009bb are presented, following the flux evolution from -10 to +285 days past B ...
View article: Erratum: “The Carnegie Supernova Project. I. Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions” (2017, AJ, 154, 211)
Erratum: “The Carnegie Supernova Project. I. Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions” (2017, AJ, 154, 211) Open
https://doi.org/10.3847/1538-3881/aa8df0This is an erratum for the article 2017 AJ 154 211
View article: The Carnegie Supernova Project: Absolute Calibration and the Hubble Constant
The Carnegie Supernova Project: Absolute Calibration and the Hubble Constant Open
We present an analysis of the final data release of the Carnegie Supernova Project I , focusing on the absolute calibration of the luminosity–decline rate relation for Type Ia supernovae (SNe Ia) using new intrinsic color relations with re…
View article: The Carnegie Supernova Project I
The Carnegie Supernova Project I Open
The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected science data of young, low-redshift supernovae between 2004 and 2009. Presented in t…
View article: The Carnegie Supernova Project I: photometry data release of low-redshift stripped-envelope supernovae
The Carnegie Supernova Project I: photometry data release of low-redshift stripped-envelope supernovae Open
The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected science data of young, low-redshift supernovae between 2004 and 2009. Presented in t…
View article: A hydrostatic MHD code for modeling stellar interiors
A hydrostatic MHD code for modeling stellar interiors Open
\n In gravitationally stratified fluids, the length scales of fluid motion are often much\n greater in the horizontal direction than in the vertical. When modeling these fluids, it\n can be advantageous to use the hydrostatic approximation…