We propose to monitor 1ES 2344+514 over seven months with the goal of better understanding its intermittent extreme behaviour. 1ES 2344+514 is a nearby (z=0.044) high energy peaked BL Lac. So far clea
We examine the absolute magnitudes and light-curve shapes of 14 nearby (redshift z=0.004-0.027) Type Ia supernovae (SNe Ia) observed in the ultraviolet (UV) with the Swift...
