Ever since the early 1980s, microcalorimeters were thought to have the potential to determine the energy of an x-ray photon with an accuracy of 1eV, a goal that promises to greatly enhance our understanding of astrophysics.1 Amicrocalorimeter detector at the focus of a high-angular-resolution x-ray telescope is a unique instrument because of its ability to simultaneously determine the energy of each x-ray photon extremely precisely while also producing x-ray images of various astronomical sources with very high detection efficiency. By studying the precisely measured distribution of x-ray photon energies emitted by various astronomical objects, we learn important information about them such as their composition, temperature, density, and dynamics. We can study a broad spectrum of astrophysical sources, such as the matter-accretion process near black holes, supernovae remnants, and the growth and evolution of galaxies and galaxy clusters. Since the invention of microcalorimeters, scientists around the world have developed ever more sensitive and innovative techniques to detect photons.2 At present, microcalorimeters with superconducting transition-edge sensors (TESs) hold the record for the best energy resolution (1.8eV) for detecting a 6keV x-ray.3 Metallic magnetic microcalorimeters (MMCs) are now on the verge of demonstrating the first ever ‘sub-eV’ energy-resolution x-ray detector. MMCs use magnetism to produce a high-precision temperature sensor. The MMCs that have been developed use the paramagnetic susceptibility of gold doped with a low concentration of erbium ions (Au:Er) when placed in a dc magnetic field.4 In a paramagnet, the magnetization is inversely proportional to temperature, making it very sensitive to small changes at low temperatures. The paramagnet is attached to an x-ray absorber as depicted in Figure 1. When an incoming x-ray hits the microcalorimeter’s absorber, its energy is converted into heat, which a thermometer then measures. The temperature rise is Figure 1. Schematic representation of a magnetic calorimeter. SQUID: Superconducting quantum interference device.
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