The mass-radius relationship for very low mass stars: Four new discoveries from the HATSouth Survey
2013
Development of the HATSouth project was funded by NSF MRI
grant NSF/AST-0723074, operations are supported by NASA grant
NNX09AB29G and follow-up observations receive partial support
from grant NSF/AST-1108686. Work at the Australian National
University is supported by ARC Laureate Fellowship Grant
FL0992131. Follow-up observations with the ESO 2.2 m/FEROS
instrument were performed under MPI guaranteed time [P087.A9014(A),
P088.A-9008(A), P089.A-9008(A)]. AJ acknowledges
support from FONDECYT project 1130857, BASAL CATA PFB06
and the Millenium Science Initiative, Chilean Ministry of Economy
(Nuclei: P10-022-F, P07-021-F). RB and NE are supported
by CONICYT-PCHA/Doctorado Nacional and MR is supported by
FONDECYT postdoctoral fellowship 3120097. We acknowledge the use
of the AAVSO Photometric All-Sky Survey (APASS), funded by
the Robert Martin Ayers Sciences Fund, and the SIMBAD data
base, operated at CDS, Strasbourg, France. Operations at the
MPG/ESO 2.2 m telescope are jointly performed by the Max Planck
Gesellschaft and the European Southern Observatory.
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