Related references
Note: Only part of the references are listed.An improved method for estimating the masses of stars with transiting planets
B. Enoch et al.
ASTRONOMY & ASTROPHYSICS (2010)
A CORRELATION BETWEEN STELLAR ACTIVITY AND HOT JUPITER EMISSION SPECTRA
Heather A. Knutson et al.
ASTROPHYSICAL JOURNAL (2010)
CORRELATION BETWEEN STELLAR ACTIVITY AND THE SURFACE GRAVITY OF HOT JUPITERS
J. D. Hartman
ASTROPHYSICAL JOURNAL LETTERS (2010)
Improved parameters for the transiting hot Jupiters WASP-4b and WASP-5b
M. Gillon et al.
ASTRONOMY & ASTROPHYSICS (2009)
The generalised Lomb-Scargle periodogram A new formalism for the floating-mean and Keplerian periodograms
M. Zechmeister et al.
ASTRONOMY & ASTROPHYSICS (2009)
The main-sequence rotation-colour relation in the Coma Berenices open cluster
A. Collier Cameron et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
MOST1 space-based photometry of the transiting exoplanet system HD 189733:: Precise timing measurements for transits across an active star
Eliza Miller-Ricci et al.
ASTROPHYSICAL JOURNAL (2008)
WASP-4b: A 12th magnitude transiting hot Jupiter in the southern hemisphere
D. M. Wilson et al.
ASTROPHYSICAL JOURNAL LETTERS (2008)
WASP-3b:: a strongly irradiated transiting gas-giant planet
D. Pollacco et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)
Ages for illustrative field stars using gyrochronology: Viability, limitations, and errors
Sydney A. Barnes
ASTROPHYSICAL JOURNAL (2007)
Efficient identification of exoplanetary transit candidates from SuperWASP light curves
A. Collier Cameron et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)
The WASP project and the SuperWASP cameras
D. L. Pollacco et al.
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC (2006)
Time scales of Li evolution: a homogeneous analysis of open clusters from ZAMS to late-MS
P Sestito et al.
ASTRONOMY & ASTROPHYSICS (2005)
No planet for HD 166435
D Queloz et al.
ASTRONOMY & ASTROPHYSICS (2001)
Evolutionary tracks and isochrones for low- and intermediate-mass stars:: From 0.1.5 to 7 M⊙ and from Z=0.0004 to 0.03
L Girardi et al.
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES (2000)