HAT-P-3
Light Curves & Finder Chart
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Comments
Basic data
Summary of transit measurements
Transit
LCs
OOT LC
Finder image
Comments
The period should be increased. Length is constant.
Depth might decrease with wavelength.
Basic Data
RA = 13:44:22.6, DE = +48:01:43
Season = April 15
V = 11.86, B-V
= 0.80 (?)
HJDo = 4218.7594, AXA fit
= 4218.7566 (21)
P = 2.899703 day , AXA fit = 2.90088 (52)
HJDo = 4218.7594 (6)
and P = 2.899703 (54) days (as listed in Schneider's Extrasolar Planets Encyclopaedia)
HJDo = 4218.75855 (66) and P
= 2.8997405 (16) days (as derived from AXA submitted
data); or even better: JDo = 4566.72741 (38), P = 2.8997405 (16)
Depth = 16.0
± 0.8 mmag (R & C-band), 14
mmag (i-band)
Length = 2.01
± 0.04 hr
Fp = 0.33 ± 0.04, F2 =
0.83 ± 0.08
Summary of Transit Light
Curves
Transit Light Curves
9616WPK
9526NR2
9427MQZ
9427WMK
9427JA2
9424PS2
9329GJ21
9326NR21
8512roe2 Note: It's very difficult
to observe exoplanet transits with a Dobsonian because of large image
rotation.
8512RMU1
8509fcn1
8317hnx1 This data has been shifted
-1 hour to acommodate what must have been a 1 hour clock error; without
this correction mid-transit would have been 66 minutes late.
8217dsx1
8215sgx1
8117nra1 Good!
7c21HVP1
7830HVP1
7804vmt1 Partial transits are useful
for investigating the presence of anomalous brightenings after egress
(or before ingress) that could be caused by the hot Jupiter having a
ring system or dust cloud (i.e., forward scattering).
7801gjl1 Valiant effort 3.5 months
after the object's "season." Large air mass seems OK. Length &
mid-transit are uncertain due to lack of pre-ingress OOT. Depth differs
from discovery paper's 14 mmag but the filter bands are at opposite
ends of the visible spectrum (IR-blocking versus Sloan i-band). [Based
on revised submission, 7903]
7801nra1
Out-of-Trransit
(OOT) Light Curves
9301LC21
Finder Image
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WebMaster: Bruce
L. Gary. Nothing on this web page is copyrighted. This site opened: August 06, 2007. Last Update: 2009.06.19