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Notes - Session 397 (2009-11-08)

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2009-11-08
Bullet XO-2b Exoplanet Transit
 
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Goto Images from 2009-11-08


XO-2b Exoplanet Transit

  1. Identifying the Transit Opportunity 

  2. Preparing for the Transit 

  3. Recording the Transit

  4. Analysing the Transit

 

1) Identifying the Transit Opportunity

XO-2b Transit Opportunities – Nov 2009
Excel graph showing calculated transit opportunities during November 2009
Opportunity on Nov 8th (highlighted) coincided with an evening of very good weather conditions
Image
 
XO-2b Transit Opportunity – 2009-11-08
Excel graph showing calculated airmass for the transit opportunity on Nov 8th
Airmass during the opportunity is not ideal, being greater than 1.5 throughout. 
Conditions at Ingress (airmass 2.5) were expected to be particularly challenging
Image
 

2) Preparing for the Transit

XO-2  – Earlier Image from May 2007
XO-2 (GSC 3413:0005) shown
Image
Annotated CCD Image 
3 x 60s (average combine), 2x2 binning, C Filter
2007-05-07 22:56 hUT (#196028-30)
 
XO-2 Reference Stars  – Earlier Image from May 2007
Image
Annotated CCD Image 
30s, 2x2 binning, R Filter
2007-05-07 23:07 hUT (#196040)
    
    
    
    
    
 
 
XO-2 with comparison/check stars ,  2009-11-08 
Single 15s V frame (captured in CCDsoft, displayed in AIS/Image Viewer)
Image
  
'StarGraph'
showing star data for above 15s V frame
Data confirms good signal/noise ratios, no pixel saturation
FWHM values at 21 deg altitude (3.6") are reasonable to good for my site
 Image

 

3) Recording the Transit

XO-2b Transit,  2009-11-08 - Time Series Data
Real time graphs showing instrumental magnitudes, ambient temperature, 
sky brightness and FWHM across the transit window
Conditions were good good for entire run, atmosphere pretty steady except for a slightly anomalies 
at around mid-transit and just after Egress.  Temperature falling by 2.25 degC across the run
Improving instrumental magnitudes and FWHM values through the run reflect the impact of decreasing airmass.
Scope was auto-guided between frames to keep the comparison and variable star on approximately the same pixel positions
Focusing was auto-compensated for temperature changes 
Image
 
XO-2b Transit,  2009-11-08 - Calculated Magnitudes
Time Series graphs showing calculated magnitude of XO-2 and the control star
Calculated magnitudes are determined using the differential magnitudes between respective star and the Comparison Star
Calculated data looks reasonably flat and indicate that the instrumental magnitude fluctuations have been 
appropriately correctly. Data scatter is noted to reduce through the run as the airmass decreases.
Average Magnitude of XO-2 for entire period is 11.22 (V), compared to expected XO-2 magnitude of 11.18 (V)
Image
 
XO-2b Transit,  2009-11-08 - Normalised Differential Magnitudes
Time Series graphs showing
differential magnitudes (normalised based on average pre-ingress values)
Data scatter is rather high at start of run due to airmass (2.5) but improves as airmass decrease through the run>
Control star data appears flat throughout the run, whereas the XO-2 data takes a slight, but noticeable dip 
during the predicted transit window.
Image
 
XO-2b Transit,  2009-11-08 - Detail
Time Series graphs showing normalised differential magnitudes in detail
Blue dots at datavalues  associated with individual frames whilst yellow dots are a moving average 
Whilst data scatter (+/-0.032m to +/-0.018m) is larger than the expected  transit depth (0.015 mag), 
and there the control star data is not totally flat, the overall dip in XO-2 brightness through the transit window is still
noticeable.
Image
 
 

4) Analysing the Transit

XO-2 with comparison/check stars,  2009-11-08
Image
 Annotated CCD Image (full frame)
25 x 15 sec exposure (average combine), 3x3 binning, V Filter 
2009-11-08 18:53 h UT  (#397043-67)
12" LX200R  (at f/5.7) + ST-10XME
 

 

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This Web Page: Notes - Session 397 (2009-11-08)
Last Updated : 2015-05-16
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