Gold antenna increases sensitivity detectors for proto-planetary systems

Researchers at SRON and TU Delft have made bolometer detectors thirty percent more sensitive. Bolometers form the heart of terahertz spectrometers that can distinguish colors up to one-millionth of their wavelength. This is needed to observe astrophysical processes such as the birth of stars and planets from gas and dust clouds. The enhancement should cut the time in half that it takes a space telescope to take a spectrum.

PRIMA selected as candidate for NASA’s Probe mission

Out of the eight projects that competed to become NASA’s Probe mission, only two remain. The Probe far-Infrared Mission for Astrophysics (PRIMA) and the Advanced X-ray Imaging Satellite (AXiS) have been selected for the second round. SRON delivers the detectors for PRIMA, developed together with TU Delft.

Astrophysics in the lab: TES detectors measure X-rays from hot plasma

SRON has joined forces with the Max Planck Institute for Nuclear Physics (MPIK) and the Institut de Recherche en Astrophysique et Planetologie (IRAP) to generate reference data for astronomical observations and scrutinize the laws of hot plasma physics. The electron beam ion trap (EBIT) at MPIK in Heidelberg simulates a hot plasma, while superconducting transition-edge sensors (TES) developed by SRON measure the emitted  X-ray spectra with unprecedented energy resolution.