Optical and Near-IR Follow-up of SN 2010da: Evidence for Warm Dust

Details Optical and Near-IR Follow-up of SN 2010da: Evidence for Warm Dust Optical and Near-IR Follow-up of SN 2010da: Evidence for Warm Dust

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2660....1p&link_type=abstract

The Astronomer's Telegram, #2660

Astronomy and Astrophysics

Astronomy

3

Infra-Red, Optical, Novae, Supernovae, Transients

Scientific paper

New optical and near-IR (BVRI + JHK) images of the transient SN 2010da in NGC 300 (CBET #2289, ATEL #2632, #2633, #2636, #2637, #2638, #2639, #2640, #2648, #2658) were obtained on 2010 June 3.4 (UT) by A. Miranda with the SMARTS 1.3m telescope at Cerro Tololo and the ANDICAM camera, as part of our follow-up campaign. The magnitudes of the transient in the optical are: B=17.40, V=16.97, R=16.40, I=16.24 (+/- 0.05 mag).

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