• DOI:10.1093/mnras/sty245
• Corpus ID: 55776991

The first sub-70 minute non-interacting WD-BD system: EPIC212235321

@article{Casewell2018TheFS,
  title={The first sub-70 minute non-interacting WD-BD system: EPIC212235321},
  author={S. L. Casewell and Ian P. Braker and Steven G. Parsons and J. J. Hermes and Matthew R. Burleigh and Claudia Belardi and Alexander Chaushev and Nicolle L. Finch and Manami Roy and Stuart P. Littlefair and M. R. Goad and Erik Dennihy},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2018},
  volume={476},
  pages={1405-1411}
}

• S. Casewell, I. Braker, +9 authors E. Dennihy
• Published 23 January 2018
• Physics
• Monthly Notices of the Royal Astronomical Society

S.L. Casewell acknowledges support from the University of
Leicester Institute for Space and Earth Observation and I.P
Braker acknowledges support from the University of Leicester
College of Science and Engineering. S.G. Parsons acknowledges
the support of the Leverhulme Trust. Support
for this work was provided by NASA through Hubble Fellowship
grant HST-HF2-51357.001-A, awarded by the Space
Telescope Science Institute, which is operated by the Association
of Universities for Research in Astronomy, Incorporated,
under NASA contract NAS5- 26555. This work is
based on observations obtained at the Southern Astrophysical Research (SOAR) telescope, which is a joint project
of the Minist´erio da Ciˆencia, Tecnologia, Inova¸c˜aos e Comunica¸c˜aoes
(MCTIC) do Brasil, the U.S. National Optical
Astronomy Observatory (NOAO), the University of North
Carolina at Chapel Hill (UNC), and Michigan State University
(MSU). This paper also uses observations made at
the South African Astronomical Observatory (SAAO). The
WHT is operated on the island of La Palma by the Isaac
Newton Group of Telescopes in the Spanish Observatorio
del Roque de los Muchachos of the Instituto de Astrof´isica
de Canarias. Also based on data products from observations
made with ESO Telescopes at the La Silla Paranal Observatory
under program ID 177.A-3011(A,B,C,D,E,F,G,H,I,J),
and 099.D-0252.