Swift/UVOT Observations of SN 2010da in NGC 300

Details Swift/UVOT Observations of SN 2010da in NGC 300 Swift/UVOT Observations of SN 2010da in NGC 300

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2633....1b&link_type=abstract

The Astronomer's Telegram, #2633

Astronomy and Astrophysics

Astronomy

1

Ultra-Violet, Novae, Supernovae

Scientific paper

The Ultraviolet/Optical Telescope (UVOT) on board the Swift satellite started observing the possible Supernova 2010da in NGC 300 (CBET #2289) at 2010-05-24.7 UT. The following UVOT magnitudes were measured: v = 16.3±0.1 (157 s exposure time), b = 16.6±0.1 (157 s), u = 15.7±0.1 (157 s), uvw1 [181-321nm] = 16.0±0.1 (314 s), uvm2 [166-268nm] = 16.2±0.1 (2462 s), uvw2 [112-264 nm] = 16.4±0.1 (629 s). These magnitudes are on the UVOT photometric system (Poole et al.

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