Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sass...25...87s&link_type=abstract
The Society for Astronomical Sciences 25th Annual Symposium on Telescope Science. Held May 23-25, 2006, at Big Bear, CA. Publish
Astronomy and Astrophysics
Astrophysics
Scientific paper
Photometric observations of short-period variable stars are time constrained because each basic observational sequence must be completed before the variable significantly changes its magnitude or color. A choice must be made. Should the scarce time within a sequence be devoted to making several observations in the same color band that, when combined, will significantly improve photometric precision over that of a single observation? Or, should the single observations be spread sequentially across color bands to provide both magnitude and color, thus enhancing astrophysical interpretations? A third alternative has occasionally been employed for many years, which is one of making a sequence of simultaneous observations in two or more color bands by using a dichroic beam splitter to partition the light into separate color bands with a separate detector being devoted to each band. The two-channel CCD photometer we describe can be operated in the Johnson-Cousins V and Ic bands simultaneously (or alternatively in B and Rc). The compact photometer, which can be assembled from off-the-shelf, low-cost components, uses a dichroic beam splitter (for V and Ic), a Meade flip mirror system, and two SBIG CCD cameras. Our preliminary results suggest that this doubling of observations has been made without any sacrifice in photometric precision.
Genet Russell M.
Heather C. L.
Smith Thomas C.
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