THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. III. CORRELATED PROPERTIES OF TYPE Ia SUPERNOVAE AND THEIR HOSTS AT 0.9 < z < 1.46*

@inproceedings{Meyers2012THEHS,
  title={THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. III. CORRELATED PROPERTIES OF TYPE Ia SUPERNOVAE AND THEIR HOSTS AT 0.9 < z < 1.46*},
  author={Joel Meyers and Greg S. Aldering and Kyle Barbary and L. Felipe Barrientos and Mark Brodwin and Kyle S. Dawson and Susana Deustua and Masao Doi and P. Eisenhardt and Lorenzo Faccioli and H. K. Fakhouri and Andrew S. Fruchter and David G. Gilbank and Michael D. Gladders and Gerson Goldhaber and Anthony H. Gonzalez and Toshihiko Hattori and E. Hsiao and Yoshihiko Ihara and Nobunari Kashikawa and Beke Koester and K. Konishi and Chris Lidman and L. Lubin and Tomoki Morokuma and T. Oda and Saul Perlmutter and M. Postman and Paul Ripoche and Piero Rosati and David Rubin and Eli S. Rykoff and Anthony Louis Spadafora and Spencer A. Stanford and Naomichi Suzuki and Naohiro Takanashi and Kei Tokita and Naoki Yasuda and for the Supernova Cosmology Project},
  year={2012}
}
Using the sample of Type Ia supernovae (SNe Ia) discovered by the Hubble Space Telescope (HST) Cluster Supernova Survey and augmented with HST-observed SNe Ia in the Great Observatories Origins Deep Survey (GOODS) fields, we search for correlations between the properties of SNe and their host galaxies at high redshift. We use galaxy color and quantitative morphology to determine the red sequence in 25 clusters and develop a model to distinguish passively evolving early-type galaxies from star… CONTINUE READING

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