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.

Q&A: Tracing the origins of supermassive black holes

Sarah Pappert is a Ph.D. candidate in astrophysics at the TUM School of Natural Sciences and conducts research at the Max Planck Institute for Extraterrestrial Physics. She is supervised by Prof. Dr. Reinhard Genzel and Prof. ...

NASA's tiny spacecraft sends first exoplanet images

With the first images from the spacecraft now in hand, the team behind NASA's Star-Planet Activity Research CubeSat, or SPARCS, is ready to begin charting the energetic lives of the galaxy's most common stars to help answer ...

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