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DIVISION IX / COMMISSION 9 / WORKING GROUP DETECTORS

  • Timothy M. C. Abbott, Dennis Crabtree, Craig D. Mackay and Christopher G. Tinney

Extract

The same general claims hold true as in the last report and the field is as busy as ever. Community focus is on the deployment of large mosaics (up to 108 pixels) to telescopes, the pursuit of programs to build next generation mosaics (of order 109 pixels), and the investigation of novel variations in CCD design.

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References

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Simons, D. A., Amico, P., Baade, D., Barden, S., Campbell, R., Finger, G., Gilmore, K., Gredel, R., Hickson, P., Howell, S., Hubin, N., Kaufer, A., Kohley, R., MacQueen, P., Markelov, S., Merrill, M., Miyazaki, S., Nakaya, H., O'Donoghue, D., Oliva, T., Richichi, A., Salmon, D., Schmidt, R., Su, H., Tulloch, S., Vargas, M. M. Wagner, R. M., Wiecha, Ol, Ye, B. 2005, in: Beleteic, J. E., Beletic, J. W., Amico, P. (eds.), Scientific Detectors for Astronomy, 2005, Proc. Workshop, Taormina, Sicily, 19-25 June 2005, (Springer) p. 13
Burke, B., Jorden, P., Vu, P. 2005, in: Beleteic, J. E., Beletic, J. W., Amico, P. (eds.), Scientific Detectors for Astronomy, 2005, Proc. Workshop, Taormina, Sicily, 19-25 June 2005, (Springer) p. 225
Hoffman, A., Loose, M., Suntharalingam, V. 2005, in: Beleteic, J. E., Beletic, J. W., Amico, P. (eds.), Scientific Detectors for Astronomy, 2005, Proc. Workshop, Taormina, Sicily, 19-25 June 2005, (Springer) p. 225
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