Swift UV light curves of recent M 31 novae (original) (raw)

Abstract

In the latest monitoring observations of the central region of the Andromeda Galaxy with the Ultra-violet/Optical Telescope (UVOT) on board the Swift satellite from 2012-05-24.62 UT to 2012-07-19.09 UT, we observe five recently discovered novae and one apparent UV variable. For all observations the UVOT uvw1 filter (181-321nm) is used. The following table shows UVOT uvw1 magnitudes (Vega system) and 1σ errors for each observed M 31 nova (see identification at the top of each column).

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