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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.

ALMA WITNESSES STAR BIRTH BEYOND THE EDGES OF THE MILKY WAY

Apr 22, 2026

ALMA WITNESSES STAR BIRTH BEYOND THE EDGES OF THE MILKY WAY A new study, led by INAF, has mapped, for the first time, the mass distribution of newly formed cores in the Large Magellanic Cloud. Thanks to high-resolution images from ALMA, it has emerged that these cores form according to the same patterns observed in the Milky Way. The result suggests that the initial fragmentation mechanisms of gas and dust clumps, from which stars are born, are universal and independent of the galactic environment.

CALVERA EXPLODED WHERE IT SHOULDN’T HAVE: A “RUNAWAY” PULSAR DEFIES THE RULES OF THE MILKY WAY

Aug 29, 2025

CALVERA EXPLODED WHERE IT SHOULDN’T HAVE: A “RUNAWAY” PULSAR DEFIES THE RULES OF THE MILKY WAY A stellar explosion, a pulsar, and a supernova remnant - that’s the story of Calvera. Positioned more than 6,500 light-years above the Galactic plane, this system is rewriting what we know about stellar evolution in our galaxy. The research originates from a team at the Italian National Institute for Astrophysics (INAF), in collaboration with the University of Palermo, and is detailed in a study published in Astronomy & Astrophysics