On the night of UT Apr 13, 2008, the SDSS Photometric Telescope ("PT" for short) took a series of exposures of TrES-3. We detected an entire transit. The transit is (as usual with this system) briefer than the ephemeris predicts.
Notes from the night
This is a chart of the field. TrES-3 orbits the is the bright star indicated by the crosshairs. The star labelled "C" will appear in later graphs.
The host star of TrES-3 has a magnitude V=12.40 according to TrES-3: A Nearby, Massive, Transiting Hot Jupiter in a 31-Hour Orbit .
Following the procedures outlined by Kent Honeycutt's article on inhomogeneous ensemble photometry, I used all stars available in each image to define a reference frame, and measured each star against this frame. You can find the software package used to do the ensemble photometry online; it's free!
The night was good. The graph below shows the amount by which instrumental magnitudes from each image needed to be shifted to match the ensemble reference. On a clear night, this graph would show a straight horizontal line.
Below is a graph of the scatter in differential magnitude versus magnitude in the ensemble solution.
TrES-3 is the star at differential mag 0.74; it shows a very small excess of scatter than neighboring stars of the same brightness. The "noise floor" in these measurements is about 0.002 mag -- as low as I've ever seen for the PT. Many of the outliers in the plot above are real variable stars (which were removed from the ensemble solution).
Below are the light curves for the target (green symbols) and four comparison stars in the field.
In this closeup, I have shifted the data for two comparison stars to move them closer in magnitude to the target.
There is no "preliminary dip" this time. My eyeball estimate for the start of the transit is 569.906, and my estimate for the end is 569.960.
An ephemeris grabbed from transitsearch.org predicts for this night
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Begin Transit Window PREDICTED CENTRAL TRANSIT End Transit Window
All Times UT
HJD Year M D H M
2454569.89 2008 4 13 9 21 2454569.93 2008 4 13 10 19 2454569.97 2008 4 13 11 16
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The ephemeris ingress of UT 2008 Apr 13 09:21:00 corresponds to JD 2,454,569.890, which is about 23 minutes EARLIER than the observed ingress. The ephemeris egress of UT 2008 Apr 13 11:16:00 corresponds to JD 2,454,569.969, which is about 13 minutes LATER than the observed egress.
This pattern confirms the indications from earlier nights,
You can grab the measurements for your own analysis. Below is a table with three flavors of time, plus the differential magnitude of the target and an estimate of the uncertainty in each measurement. I show the first few lines of the file to give you an idea of its format.
# Measurements of TrES-3 made with APO PT, Apr 13, 2008 UT. # Each exposure 30 seconds long in SDSS i-band; # Tabulated times are midexposure (FITS header time - half exposure length) # and accurate only to +/- 1 second (??). # 'mag' is a differential magnitude based on ensemble photometry # using a circular aperture of radius 5.25 arcseconds. # # UT day JD-2,450,000 HJD-2,450,000 mag uncert Apr13.86379 4569.86379 4569.86506 0.726 0.003 Apr13.86511 4569.86511 4569.86638 0.731 0.003 Apr13.86644 4569.86644 4569.86771 0.730 0.003
Last modified 05/03/2008 by MWR.