Updates on the background estimates for the X-IFU instrument onboard of the ATHENA mission
Author:
Affiliation:
1. Istituto di Astrofisica e Planetologia Spaziali (Italy)
2. INAF-IASF Milano (Italy)
3. IASF-Palermo (Italy)
4. IASF-Bologna (Italy)
5. IRAP-CDPP (France)
6. CEA/DSM/IRFU/SAp (France)
Publisher
SPIE
Reference9 articles.
1. The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission;Nandra,2013
2. The Hot and Energetic Universe: The Wide Field Imager (WFI) for Athena+;Rau,2013
3. The ATHENA X-ray Integral Field Unit;Barret,2016
4. In-orbit background of X-ray microcalorimeters and its effects on observations
5. The “effective” penetration depth of backscattered electrons associated with electron channeling patterns (ECPs)
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1. Effect of Space Radiation on Transition-Edge Sensor Detectors Performance;IEEE Transactions on Applied Superconductivity;2023-08
2. Thermal Impact of Cosmic Ray Interaction with an X-Ray Microcalorimeter Array;Journal of Low Temperature Physics;2020-02-13
3. A Deep Extragalactic Survey with the ART-XC Telescope of the Spectrum-RG Observatory: Simulations and Expected Results;Astronomy Letters;2018-02
4. Optical simulations for design, alignment, and performance prediction of silicon pore optics for the ATHENA x-ray telescope;Optics for EUV, X-Ray, and Gamma-Ray Astronomy VIII;2017-09-19
5. The particle background of the X-IFU instrument;Experimental Astronomy;2017-05-17
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