TrES-4

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    Comments
    Basic data
    Table summary of transit measurements
    Transit LCs
    Professional light curves
    OOT LC

    Finder Image
    References

Comments on LCs on this web page

    Period is close to correct but could use a slight shortening.

Basic data - Updated 20090813
    RA = 17:53:13.0, Decl = +37:12:43
    Season = June 21
    B = 12.11, V = 11.59, R = 11.28, I = 10.99;
B-V = 0.52
    HJDo = 4230.9053 (?) & P = 3.553945 (75) day (Schneider's Extrasolar Planets Encyclopedia)
    HJDo = 4230.9053 (2) & P = 3.553924 (2) days
    Depth =
12.4 ± 1.5 (CVR bands), 10.8 mmag (z-band)
    Length = 3.54 ± 0.08 hr (CVR bands), 3.5 hr (z-band)
    Fp = 0.32 ± 0.06, F2 = 0.84 ± 0.11
    b = 0.75, Rs = 1.78 Rs, Rp = 1.67 * Rj

Table Summary of Measurements - Updated 20090813

     

       

     

       

Transit light curves not yet included in updates of previous sections


9909WPK


All LCs below here have been included in updates of previous sections



9811SG22


9717NR22


9630NWP2


9427DKS


9412GJ21


8521ROE2 



8503FC21 




7925HVP1



Great LC considering the high air mass, lightning that terminated observations and use of a portable 10-inch telescope at a remote site.

Professional Light Curves


Discovery paper LCs (Mandushev, et al, 2007).

Out-of-Transit Light Curves



9630SG2


9618SG2  Looks like a brief dip at -1.7 hrs. A 5 mmag depth would correspond to Rp = 0.6 Rj, or Mp = 5% the mass of TrES-4b. This, by itself, does not rule-out the possibility that
the dip is produced by another exoplanet orbiting the TrES-4 star. Now consider the length of the dip. Length ~ 0.5 hr, so orbital velocity would be 7 times that of TrES-4b.
For this orbital velocity the orbital radius would have to be 2% of TrES-4b's orbital radius, which would place it within the star (12% of star's radius).
Therefore this dip is not due to another exoplanet orbiting the TrES-4 star!


There's an intriguing "dip" at 1.2 hr past 08.39 UT that may be noteworthy at some future date when more OOT observations are available.

Finder Image


FOV ~ 22 x 13 'arc. Note that a nearby star is variable (Patrick Wiggins, private communication) so don't use it for reference.


References

The discovery paper by Mandushev et al, 2007 includes LCs showing depth = 10.8 mmag (z' and B-bands) with a length of ~3.5 to 3.6 hr (depending on definition used).

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WebMaster: Bruce L. GaryNothing on this web page is copyrighted. This site opened:  August 25, 2007 Last Update:  2010.07.26