THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE

@article{Stritzinger2010THECS,
  title={THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE},
  author={Maximilian D. Stritzinger and Mark M. Phillips and Luis Boldt and Christopher R. Burns and Abdo Campillay and Carlos Contreras and Sergio Mart{\'i}nez Gonz{\'a}lez and Gast{\'o}n Folatelli and Nidia I. Morrell and Wojtek Krzemiński and Miguel R. Roth and Francisco Salgado and Darren Lee Depoy and M. Hamuy and Wendy L. Freedman and Barry F. Madore and Jennifer L. Marshall and Sven Eric Persson and J. P. Rheault and Nicholas B. Suntzeff and Steven Villanueva and Weidong Li and Alexei V. Filippenko},
  journal={The Astronomical Journal},
  year={2010},
  volume={142}
}
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 (SNe Ia). Presented here is the second data release of nearby SN Ia 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… 
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References

SHOWING 1-10 OF 73 REFERENCES
THE CARNEGIE SUPERNOVA PROJECT: FIRST PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE
The Carnegie Supernova Project (CSP) is a five-year survey being carried out at the Las Campanas Observatory to obtain high-quality light curves of ∼100 low-redshift Type Ia supernovae (SNe Ia) in a
THE CARNEGIE SUPERNOVA PROJECT: ANALYSIS OF THE FIRST SAMPLE OF LOW-REDSHIFT TYPE-Ia SUPERNOVAE
An analysis of the first set of low-redshift (z < 0.08) Type Ia supernovae (SNe Ia) monitored by the Carnegie Supernova Project between 2004 and 2006 is presented. The data consist of well-sampled,
THE CARNEGIE SUPERNOVA PROJECT: FIRST NEAR-INFRARED HUBBLE DIAGRAM TO z ∼ 0.7
The Carnegie Supernova Project (CSP) is designed to measure the luminosity distance for Type Ia supernovae (SNe Ia) as a function of redshift, and to set observational constraints on the dark energy
THE CARNEGIE SUPERNOVA PROJECT: LIGHT-CURVE FITTING WITH SNooPy
In providing an independent measure of the expansion history of the universe, the Carnegie Supernova Project (CSP) has observed 71 high-z Type Ia supernovae (SNe Ia) in the near-infrared bands Y and
The Carnegie Supernova Project: The Low‐Redshift Survey
Supernovae are essential to understanding the chemical evolution of the universe. Type Ia supernovae also provide the most powerful observational tool currently available for studying the expansion
NEARBY SUPERNOVA FACTORY OBSERVATIONS OF SN 2007if: FIRST TOTAL MASS MEASUREMENT OF A SUPER-CHANDRASEKHAR-MASS PROGENITOR
We present photometric and spectroscopic observations of SN 2007if, an overluminous (MV = −20.4), red (B − V = 0.16 at B-band maximum), slow-rising (trise = 24 days) type Ia supernova (SN Ia) in a
UBVRI Light Curves of 44 Type Ia Supernovae
We present UBVRI photometry of 44 Type Ia supernovae (SNe Ia) observed from 1997 to 2001 as part of a continuing monitoring campaign at the Fred Lawrence Whipple Observatory of the
Hubble Diagrams of Type Ia Supernovae in the Near-Infrared
From observations of seven Type Ia supernovae obtained during the last 4 years at the Las Campanas and Cerro Tololo Inter-American Observatories, along with previous published data for nine
CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA
We present multiband photometry of 185 type-Ia supernovae (SNe Ia), with over 11,500 observations. These were acquired between 2001 and 2008 at the F. L. Whipple Observatory of the
Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el
We present well-sampled optical (UBVRI) and infrared (JHK) light curves of the nearby (≈18.0 Mpc) Type Ia supernova SN 2001el, from 11 days before to 142 days after the time of B-band maximum. The
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