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Sky Conditions Summary (S126) |
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As part of an ongoing project examining the variability
in RT Auriga, further image sets of the variable star RT Aur & the reference star SAO
SAO 78571 were recorded. Image sets comprised 7 sequences of
images (3 x 2s V & 3 x 5s B) alternated between RT Aur & reference
star. These and previous image sets from previous session from Feb-May
2006 were analyzed using the
methodology previously described under 2005-10-05
Notes. Results are shown in graphs below. Data is
consistent with a regular variation with a period of 3.728115 days.
Quality control was less tight than ideal due to the faintness of the available
check star (particularly in B). Data quality, particularly in B Band,
suffered from increasing Airmass through May, which hampered ability to confirm
B-V trends through the magnitude minima. Nevertheless the light curve for RT
Auriga has been reasonably well constrained by the total dataset.
RT Aur (Auriga) |
CCD Image (50% size) 60 sec exposure, 1x1 binning, C Filter 2006-02-10 22:11h UT (#114120) [ Full Size Image ] |
V Band Magnitude estimates for RT
Aug |
B Band Magnitude estimates for RT
Aug |
V Band Light Curve for RT Aug |
B Band Light Curve for RT Aug |
B Band Light Curve for RT Aug |
Light Curve for RT Aug Magnitude and colour variation in RT Auriga based on observations on 12 observing sessions between 2006-02-10 and 2006-05-12 [ Reference Star SAO 78571 ] |
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This Web Page: | CCD Image Notes - (2006-05-12) |
Last Updated : | 2015-05-16 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |