1 code implementation • 14 Nov 2023 • Kaiming Cui, D. J. Armstrong, Fabo Feng
We train our model on datasets obtained from both space-based and ground-based multi-band observations of variable stars and transients.
no code implementations • 5 Jan 2021 • A. M. S. Smith, J. S. Acton, D. R. Anderson, D. J. Armstrong, D. Bayliss, C. Belardi, F. Bouchy, R. Brahm, J. T. Briegal, E. M. Bryant, M. R. Burleigh, J. Cabrera, A. Chaushev, B. F. Cooke, J. C. Costes, Sz. Csizmadia, Ph. Eigmüller, A. Erikson, S. Gill, E. Gillen, M. R. Goad, M. N. Günther, B. A. Henderson, A. Hogan, A. Jordán, M. Lendl, J. McCormac, M. Moyano, L. D. Nielsen, H. Rauer, L. Raynard, R. H. Tilbrook, O. Turner, S. Udry, J. I. Vines, C. A. Watson, R. G. West, P. J. Wheatley
Methods: Transits of NGTS-14Ab were discovered in photometry from the Next Generation Transit Survey (NGTS).
Earth and Planetary Astrophysics
1 code implementation • 11 Dec 2015 • H. P. Osborn, D. J. Armstrong, D. J. A. Brown, J. McCormac, A. P. Doyle, T. M. Louden, J. Kirk, J. J. Spake, K. W. F. Lam, S. R. Walker, F. Faedi, D. L. Pollacco
Photometric surveys such as Kepler have the precision to identify exoplanet and eclipsing binary candidates from only a single transit.
Earth and Planetary Astrophysics