Jul 22 – 26, 2019
Europe/Rome timezone

The Demonstration Model of the ATHENA X-IFU Cryogenic AntiCoincidence Detector

Jul 25, 2019, 5:45 PM
1h 15m
Piazza Città di Lombardia (Milano)

Piazza Città di Lombardia


Piazza Città di Lombardia, 1, 20124 Milano MI
Poster Low Temperature Detector Development and Physics Poster session


Matteo D'Andrea (INAF/IAPS)


ATHENA is a large ESA mission selected for launch in 2031. One instrument of the payload is the X-IFU, a cryogenic spectrometer providing spatially resolved high-resolution X-ray spectroscopy. The core of the instrument is a 3kilo-pixels TES array operated at 50 mK thermal bath. Since the expected particle background would degrade the instrument performance, advanced reduction techniques have been adopted to reduce it by a factor ~50. Most of the background reduction is achieved thanks to the Cryogenic AntiCoincidence detector (CryoAC), a 4 pixels TES microcalorimeter placed <1 mm below the TES array. The CryoAC is a sort of instrument-inside-the-instrument, with independent electronics and dedicated data processing chain. It shall have a wide energy band (from 6 keV to 1 MeV TBC) and a low deadtime (1%), while respecting several constraints to ensure mechanical, thermal and electromagnetic compatibility with the TES array.

The X-IFU development plan foresees to build an instrument Demonstration Model (DM) before the mission adoption. In this respect, we have developed the CryoAC DM, a single pixel detector based on a large area (1 cm2) Silicon absorber. To obtain a well-defined conductance towards the thermal bath, the absorber is connected to a silicon rim through 4 narrow silicon bridges (100x1000 μm2), achieving a suspended structure. This is sensed by a network of 96 Ir:Au TES in parallel configuration. The network is designed to achieve an efficient athermal phonons collection, and it features anti-inductive Nb wirings. Platinum heaters are also embedded on the absorber. If necessary, they could be used to increase the local temperature and reduce the current needed to operate the TES network, limiting crosstalk effects on the TES array.

Here we present the main results of the test performed on the CryoAC DM and an update about the status of the detector, which in April 2019 has been delivered to SRON for the integration in the X-IFU Focal Plane Assembly DM.

Student (Ph.D., M.Sc. or B.Sc.) N
Less than 5 years of experience since completion of Ph.D Y

Primary author

Matteo D'Andrea (INAF/IAPS)


Claudio Macculi (INAF/IAPS) Guido Torrioli (CNR/IFN Roma) Dr Andrea Argan (INAF/IAPS) Dr Daniele Brienza (INAF/IAPS) Simone Lotti (INAF/IAPS) Dr Gabriele Minervini (INAF/IAPS) Luigi Piro (INAF/IAPS) Michele Biasotti (Department of Physics, University of Genova) Dr Lorenzo Ferrari Barusso (Department of Physics, University of Genova) Flavio Gatti (Department of Physics, University of Genova) Manuela Rigano (Department of Physics, University of Genova) Angela Volpe (ASI (Italian Space Agency)) Elia Stefano Battistelli (Sapienza Universiy of Rome, INAF/IAPS, INFN-Sezione di Roma1)

Presentation materials