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Figure 1
CFHT/WIRCam Ksband
photometry of
the secondary eclipse
of TrES-2b. The top
panel shows the unbinned
lightcurve,
while the panel that is
the second from the
top shows the lightcurve
with the data
binned every 7.0 minutes.
The panel that
is the second from the
bottom shows the
binned data after the
subtraction of the
best-fit background,
while the bottom panel
shows the binned
residuals from the
best-fit model. In
each one of the panels
the best-fit best-fit
secondary eclipse and
background, Bf , is
shown with the red
line. The expected
mid-secondary eclipse
is if TrES-2b has zero
eccentricity. Figure
and caption from Croll
et al (2010b).
Figure 2
Transit observations of
GJ 1214b. Black diamonds
are the weighted
mean of WIRCam
J- & Ks-band and CH4
On filter data. Red
diamonds are the
MEarth (Charbonneau
et al. 2009), and the
Kitt-peak Sada et al.
(2010) transit depth,
blue diamonds are
VLT/FORS2 points
(Bean et al. 2010)
Grey dotted curve line
is GJ 1214b atmospheric
model, orange
a solar-metallicity
model, cyan a solarmetallicity
no methane
model (Miller-Ricci
2010) for > 1 m.
For