The Carnegie Supernova Project (CSP) was a five-year observational survey conducted at Las Campanas Observatory that obtained, among other things, high-quality light curves of 100 low-redshift Type Ia supernovae (SNeIa). Presented here is the second data release of nearby SNIa photometry consisting of 50 objects, with a subset of 45 having near-infrared follow-up observations. Thirty-three objects have optical pre-maximum coverage with a subset of 15 beginning at least five days before maximum light. In the near-infrared, 27 objects have coverage beginning before the epoch of B-band maximum, with a subset of 13 beginning at least five days before maximum. In addition, we present results of a photometric calibration program to measure the CS...
The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical an...
Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near infrared (NIR) is a promising ...
Artículo de publicación ISIAn analysis of the first set of low-redshift (z < 0.08) Type Ia supernova...
The Carnegie Supernova Project (CSP) was a five-year observational survey con-ducted at Las Campanas...
Artículo de publicación ISIThe Carnegie Supernova Project is a five-year survey being carried out at...
The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up progra...
The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up progra...
We present final natural-system optical (ugriBV) and near-infrared (YJH) photometry of 134 supernova...
Artículo de publicación ISISupernovae are essential to understanding the chemical evolution of the u...
© 2018. The Astronomical Society of the Pacific. All rights reserved. Printed in the U.S.A.The Carne...
ABSTRACT. Supernovae are essential to understanding the chemical evolution of the universe. Type Ia ...
The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical an...
Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near-infrared (NIR) is a promising ...
The Carnegie Supernova Project (CSP) is designed to measure the luminosity distance for Type Ia supe...
The La Silla/QUEST Variability Survey (LSQ) and the Carnegie Supernova Project (CSP II) are collabor...
The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical an...
Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near infrared (NIR) is a promising ...
Artículo de publicación ISIAn analysis of the first set of low-redshift (z < 0.08) Type Ia supernova...
The Carnegie Supernova Project (CSP) was a five-year observational survey con-ducted at Las Campanas...
Artículo de publicación ISIThe Carnegie Supernova Project is a five-year survey being carried out at...
The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up progra...
The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up progra...
We present final natural-system optical (ugriBV) and near-infrared (YJH) photometry of 134 supernova...
Artículo de publicación ISISupernovae are essential to understanding the chemical evolution of the u...
© 2018. The Astronomical Society of the Pacific. All rights reserved. Printed in the U.S.A.The Carne...
ABSTRACT. Supernovae are essential to understanding the chemical evolution of the universe. Type Ia ...
The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical an...
Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near-infrared (NIR) is a promising ...
The Carnegie Supernova Project (CSP) is designed to measure the luminosity distance for Type Ia supe...
The La Silla/QUEST Variability Survey (LSQ) and the Carnegie Supernova Project (CSP II) are collabor...
The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical an...
Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near infrared (NIR) is a promising ...
Artículo de publicación ISIAn analysis of the first set of low-redshift (z < 0.08) Type Ia supernova...