Swift Observations of SN 2010bj in NGC 2357

Astronomy and Astrophysics – Astronomy

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Optical, Ultra-Violet, X-Ray

Scientific paper

The Ultraviolet/Optical Telescope (UVOT) and X-Ray Telescope (XRT) on board the Swift satellite started observing the Type IIP supernova 2010bj in NGC 2357 (CBET #2230, #2232) on 2010-04-13.4 UT. The following UVOT magnitudes were measured: v = 16.0±0.1 (373 s exposure time), b = 16.5±0.1 (373 s), u = 16.6±0.1 (373 s), uvw1 [181-321nm] = 17.9±0.1 (1123 s), uvm2 [166-268nm] = 18.6±0.1 (2863 s), uvw2 [112-264 nm] = 18.5±0.1 (1877 s).

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