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Quantum detectors for the CMB

One field seeing a very rapid evolution, in which Italian groups were included from the very start and are obtaining prominent results, is that which uses KIDs, Kinetic Inductance Detectors.

Kinetic Inductance Detectors are the latest generation of detectors based on the presence of a gap between the energy levels of a superconductor. This is analogous to what happens in semiconductor detectors, but the gap in the case of superconductors is about one thousand times smaller, allowing for the detection of much lower frequency photons (down to about 90 GHz).

The characteristic that makes these detectors ideal candidates for future balloon or satellite missions is the possibility to read even 104-105 pixels via a single coaxial cable and a wide band HEMT (High Electron Mobility Transistor) amplifier, enormously reducing the thermal load on the cryogenic stage of the experiment.

In addition, the manufacturing process is relatively simple and flexible, feasible in Italian facilities, and the freedom in the choice of materials allows KIDs to be used for wavelengths that go from the millimetre to the X-ray band.

PLANETARY SYSTEMS, TWO DISTINCT FAMILIES: THE HOST STAR LEAVES ITS SIGNATURE

Oct 13, 2026

PLANETARY SYSTEMS, TWO DISTINCT FAMILIES: THE HOST STAR LEAVES ITS SIGNATURE An international team led by INAF analysed multi-planet systems and found that they split into two distinct families born around different types of stars. The study, published in Nature Astronomy, shows for the first time that the host star's properties determine the architecture and dynamical evolution of the entire planetary system

NGC 362D: TWO RECORD-BREAKING FINDINGS SHED LIGHT ON THE EVOLUTION OF MILLISECOND PULSARS

Sep 30, 2026

NGC 362D: TWO RECORD-BREAKING FINDINGS SHED LIGHT ON THE EVOLUTION OF MILLISECOND PULSARS An INAF- and University of Bologna-led research team has discovered a binary system caught in an exceptionally rare evolutionary stage, consisting of a millisecond pulsar and the youngest white dwarf ever observed in a system of this kind

AN "IMPROBABLE" PLANETARY SYSTEM: COMPACT, COPLANAR, AND SHAPED BY A BROWN DWARF

Jun 17, 2026

AN "IMPROBABLE" PLANETARY SYSTEM: COMPACT, COPLANAR, AND SHAPED BY A BROWN DWARF An international team involving over ten institutions, with a strong participation from ESO and INAF, has characterised TOI-201 c, the transiting brown dwarf with the longest period for which mass has been measured. The study, published today in Nature, reveals a compact, coplanar system in which the presence of a massive, eccentric object redefines the stability boundaries for the inner planets