The Hot and Energetic Universe: The X-ray Integral Field Unit (X-IFU) for Athena+
arXiv:1308.6784
Abstract
The Athena+ mission concept is designed to implement the Hot and Energetic Universe science theme submitted to the European Space Agency in response to the call for White Papers for the definition of the L2 and L3 missions of its science program. The Athena+ science payload consists of a large aperture high angular resolution X-ray optics and twelve meters away, two interchangeable focal plane instruments: the X-ray Integral Field Unit (X-IFU) and the Wide Field Imager (WFI). The X-IFU is a cryogenic X-ray spectrometer, based on a large array of Transition Edge Sensors (TES), offering 2.5 eV spectral resolution, with ~5" pixels, over a field of view of 5 arc minutes in diameter. In this paper, we briefly describe the Athena+ mission concept and the X-IFU performance requirements. We then present the X-IFU detector and readout electronics principles, the current design of the focal plane assembly, the cooling chain and review the global architecture design. Finally, we describe the current performance estimates, in terms of effective area, particle background rejection, count rate capability and velocity measurements. Finally, we emphasize on the latest technology developments concerning TES array fabrication, spectral resolution and readout performance achieved to show that significant progresses are being accomplished towards the demanding X-IFU requirements.
Supporting paper for the science theme "The Hot and Energetic Universe" to be implemented by the Athena+ X-ray observatory (http://www.the-athena-x-ray-observatory.eu). 17 pages, 19 figures
References in corpus (13)
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- Reflection spectra of accretion disks illuminated by disk-like coronae
- Searching for Intermediate Mass Black Holes in galaxies with Low Luminosity AGN: A multiple-method approach
- In-orbit background of X-ray microcalorimeters and its effects on observations
- Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
- The particle background of the X-IFU instrument
- Athena+: The first Deep Universe X-ray Observatory
- Fe xxv line profiles in colliding wind binaries
- Soft X-ray absorption excess in gamma-ray burst afterglow spectra: Absorption by turbulent ISM
- Computation of the transmitted and polarized scattered fluxes by the exoplanet HD 189733b in X-rays
- Microcalorimeter pulse analysis by means of principle component decomposition
- Opening the low-background and high-spectral-resolution domain with the ATHENA large X-ray observatory: Development of the Cryogenic AntiCoincidence Detector for the X-ray Integral Field Unit