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The STELLA robotic observatory on tenerife
2010, Strassmeier, K.G., Granzer, T., Weber, M., Woche, M., Popow, E., Jrvinen, A., Bartus, J., Bauer, S.-M., Dionies, F., Fechner, T., Bittner, W., Paschke, J.
The Astrophysical Institute Potsdam (AIP) and the Instituto de Astrofísica de Canarias (IAC) inaugurated the robotic telescopes STELLA-I and STELLA-II (STELLar Activity) on Tenerife on May 18, 2006. The observatory is located on the Izaa ridge at an elevation of 2400m near the German Vacuum Tower Telescope. STELLA consists of two 1.2m alt-az telescopes. One telescope fiber feeds a bench-mounted high-resolution echelle spectrograph while the other telescope feeds a wide-field imaging photometer. Both scopes work autonomously by means of artificial intelligence. Not only that the telescopes are automated, but the entire observatory operates like a robot, and does not require any human presence on site. Copyright © 2010 Klaus G. Strassmeier et al.
Test beam measurement of the first prototype of the fast silicon pixel monolithic detector for the TT-PET project
2018, Paolozzi, L., Bandi, Y., Benoit, M., Cardarelli, R., Débieux, S., Forshaw, D., Hayakawa, D., Iacobucci, G., Kaynak, M., Miucci, A., Nessi, M., Ratib, O., Ripiccini, E., Rücker, H., Valerio, P., Weber, M.
The TT-PET collaboration is developing a PET scanner for small animals with 30 ps time-of-flight resolution and sub-millimetre 3D detection granularity. The sensitive element of the scanner is a monolithic silicon pixel detector based on state-of-the-art SiGe BiCMOS technology. The first ASIC prototype for the TT-PET was produced and tested in the laboratory and with minimum ionizing particles. The electronics exhibit an equivalent noise charge below 600 e− RMS and a pulse rise time of less than 2 ns , in accordance with the simulations. The pixels with a capacitance of 0.8 pF were measured to have a detection efficiency greater than 99% and, although in the absence of the post-processing, a time resolution of approximately 200 ps .
Three years of experience with the STELLA robotic observatory
2010, Granzer, T., Weber, M., Strassmeier, K.G.
Since May 2006, the two STELLA robotic telescopes at the Izaa observatory in Tenerife, Spain, delivered an almost uninterrupted stream of scientific data. To achieve such a high level of autonomous operation, the replacement of all troubleshooting skills of a regular observer in software was required. Care must be taken on error handling issues and on robustness of the algorithms used. In the current paper, we summarize the approaches we followed in the STELLA observatory. Copyright © 2010 Thomas Granzer et al.
Characterization of the demonstrator of the fast silicon monolithic ASIC for the TT-PET project
2019, Paolozzi, L., Bandi, Y., Cardarelli, R., Débieux, S., Favre, Y., Ferrère, D., Forshaw, D., Hayakawa, D., Iacobucci, G., Kaynak, M., Miucci, A., Nessi, M., Ripiccini, E., Rücker, H., Valerio, P., Weber, M.
The TT-PET collaboration is developing a small animal TOF-PET scanner based on monolithic silicon pixel sensors in SiGe BiCMOS technology. The demonstrator chip, a small-scale version of the final detector ASIC, consists of a 03 × 1 pixel matrix integrated with the front-end, a 50 ps binning TDC and read out logic. The chip, thinned down to 100 µm and backside metallized, was operated at a voltage of 180 V. The tests on a beam line of minimum ionizing particles show a detection efficiency greater than 99.9% and a time resolution down to 110 ps. © 2019 CERN.