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.

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 ...

The HWO must be picometer perfect to observe Earth 2.0

Lately we've been reporting about a series of studies on the Habitable Worlds Observatory (HWO), NASA's flagship telescope mission for the 2040s. These studies have looked at the type of data they need to collect, and what ...

Gravitational wave detectors affected by daylight savings time

Interference from human activity has always been a sticking point in astronomical observations. Radio astronomy is notoriously sensitive to unintentional interference—hence why there are "radio silent" zones near telescopes ...

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