Detection of a giant white-light flare on an L2.5 dwarf with the Next Generation Transit Survey
arXiv:1902.00900 · doi:10.1093/mnrasl/slz039
Abstract
We present the detection of a -10 flare from the ultracool L2.5 dwarf ULAS J224940.13-011236.9 with the Next Generation Transit Survey (NGTS). The flare was detected in a targeted search of late-type stars in NGTS full-frame images and represents one of the largest flares ever observed from an ultracool dwarf. This flare also extends the detection of white-light flares to stars with temperatures below 2000 K. We calculate the energy of the flare to be erg, making it an order of magnitude more energetic than the Carrington event on the Sun. Our data show how the high-cadence NGTS full-frame images can be used to probe white-light flaring behaviour in the latest spectral types.
arXiv comment5 pages, 2 figures, Accepted for Publication in the Monthly Notices of the Royal Astronomical Society
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