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DEMONEX: The DEdicated MONitor of EXotransits

Published online by Cambridge University Press:  01 May 2008

J. D. Eastman
Affiliation:
The Ohio State University140 W 18th Ave.Columbus OH43210 email: jdeast@astronomy.ohio-state.edu, gaudi@astronomy.ohio-state.edu, depoy@astronomy.ohio-state.edu
B. S. Gaudi
Affiliation:
The Ohio State University140 W 18th Ave.Columbus OH43210 email: jdeast@astronomy.ohio-state.edu, gaudi@astronomy.ohio-state.edu, depoy@astronomy.ohio-state.edu
D. L. DePoy
Affiliation:
The Ohio State University140 W 18th Ave.Columbus OH43210 email: jdeast@astronomy.ohio-state.edu, gaudi@astronomy.ohio-state.edu, depoy@astronomy.ohio-state.edu
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Abstract

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DEMONEX is a low-cost, 0.5 meter, robotic telescope assembled mostly from commercially available parts dedicated to obtaining precise photometry of bright stars with transiting planets. This photometry will provide a homogeneous data set for all transits visible from its location at Winer Observatory in Sonoita, Arizona. We will also search for additional planets via transit timing variations, measure or place limits on the albedos from secondary eclipses, systematically search known radial velocity planets for those that transit, and follow up promising KELT candidates. Despite its modest size, the signal-to-noise ratio per transit is comparable to that obtained with larger, 1m-class telescopes because of its short readout time and high z-band quantum efficiency. However, its main strength is that it will be used every night for transit follow-up and gather an unprecedented data set on transiting planets. With the 24 known transiting planets and 112 radial velocity planets visible from Winer Observatory, over 90% of all nights have at least one full event to observe.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Agol, E., Steffen, J., Sari, R., & Clarkson, W. 2005, MNRAS, 359, 567CrossRefGoogle Scholar
Bundy, K. A. & Marcy, G. W. 2000, PASP, 112, 1421CrossRefGoogle Scholar
Pepper, J., Pogge, R. W., DePoy, D. L., Marshall, J. L., Stanek, K. Z., Stutz, A. M., Poindexter, S., Siverd, R., O'Brien, T. P., Trueblood, M., & Trueblood, P. 2007, PASP 119, 923CrossRefGoogle Scholar
Queloz, D., Eggenberger, A., Mayor, M., Perrier, C., Beuzit, J. L., Naef, D., Divan, J. P., & Udry S. 2000, A&A, 359, L13Google Scholar
Rowe, J. F., Matthews, J. M., Seager, S., Kuschnig, R., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M., Sasselov, D., Walker, G. A. H., & Weiss, W. W. 2006, ApJ, 646, 1241CrossRefGoogle Scholar
Winn, J. N. et al. 2005, ApJ, 631, 1215CrossRefGoogle Scholar