On the night of UT Feb 22, 2008, the SDSS Photometric Telescope ("PT" for short) took a series of exposures of TrES-3. We detected ingress only, at roughly the time predicted.
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 pretty 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 small excess of scatter than neighboring stars of the same brightness. The "noise floor" in these measurements is about 0.003 mag -- pretty good. 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.
My eyeball estimate for the ingress is 518.967. The egress clearly occurred after our measurements ended.
Justin's notes indicate that ingress should have occurred at 518.961, roughly at the same time as my eyeball estimate. The egress was predicted to occur at 519.018, which is indeed after the end of our run.
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, Feb 22, 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 Feb22.92055 4518.92055 4518.91943 0.717 0.005 Feb22.92187 4518.92187 4518.92075 0.727 0.004 Feb22.92322 4518.92322 4518.92210 0.726 0.005
Last modified 07/03/2008 by MWR.