We use light-curve fitting models (MLCS2k2, SALT2, and SNooPy) as implemented in SNANA to make the YOnsei Nearby Supernova Evolution Investigation (YONSEI) Supernova Catalogue. The catalogue consists of several hundred Type Ia supernovae (SNe Ia) in the redshift range from 0.01 to 1.35, and provides distance moduli, light-curve shape parameters, and color or extinction values for each supernova. This data set will be used to study the dependence of SNe Ia luminosities on the host galaxy morphologies. In this paper, we present the YONSEI Supernova Catalogue and preliminary systematic tests for the catalogue.

ABSTRACT
1. YONSEI SUPERNOVA CATALOGUE
2. SYSTEMATIC TESTS
3. FUTURE WORK
REFERENCES

• Young-Lo Kim(Center for Galaxy Evolution Research and Department of Astronomy, Yonsei University)
• Yijung Kang(Center for Galaxy Evolution Research and Department of Astronomy, Yonsei University)
• Young-Wook Lee(Center for Galaxy Evolution Research and Department of Astronomy, Yonsei University)