Page 3: Research news on Astronomical detectors

Astronomical detectors as a research area focuses on the development, characterization, and optimization of sensor technologies used to register electromagnetic or particle signals from astronomical sources with high sensitivity, dynamic range, and temporal and spatial resolution. It encompasses work on charge-coupled devices (CCDs), complementary metal–oxide–semiconductor (CMOS) imagers, infrared arrays, superconducting devices such as transition-edge sensors and kinetic inductance detectors, as well as photon-counting and polarimetric detectors. Research addresses quantum efficiency, noise sources, readout architectures, calibration strategies, radiation hardness, and cryogenic operation, enabling precise photometry, spectroscopy, astrometry, and time-domain observations across multiple wavelength regimes.

Researchers develop glass sensors for the Einstein Telescope

From 2035, the Einstein Telescope will be able to study gravitational waves with unprecedented accuracy. For the telescope, researchers from Jena have manufactured highly sensitive sensors made entirely of glass for the first ...

Small but mighty: TESSERACT joins the hunt for dark matter

For decades, people have been trying to directly detect dark matter: the missing mass in our universe. Now, there's a new, super-sensitive detector on the case—and even though it's still in the research and development phase, ...

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