This is a talk given at lunch time, usually in the conference room at noon.
Less than 1 billion year after the Big Bang (< 8% of today’s age of the Universe), the cosmic star formation rate and stellar mass density of gala
During the last decade observations of galaxies across cosmic times coupled
The field of type Ia Supernovae (SNe) is in crisis.
Planet occurrence rates increase toward later spectral types; therefore, M dwarf systems are our most promising targets in the search for exoplanets.