Presentation 1 : None
SN photometric data analysis and reduction details
Julien Raux, Kyan Schamaneche
In this talk, I will describe the photometric analysis of supernovae.
In a first part, I will describe the detection pipeline within two
different strategy (standard and "rolling" search). Then, I will
talk about the construction of photmetric lightcurves using differential
analysis.
Finally, I will explain how using those lightcurves we can estimate
cosmological distances. In particular, I'll compare different methods
of absolute calibration.