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    Article

    ORIGIN: metal creation and evolution from the cosmic dawn

    ORIGIN is a proposal for the M3 mission call of ESA aimed at the study of metal creation from the epoch of cosmic dawn. Using high-spectral resolution in the soft X-ray band, ORIGIN will be able to identify th...

    Jan-Willem den Herder, Luigi Piro, Takaya Ohashi in Experimental Astronomy (2012)

  2. Article

    Open Access

    The SPICA-SAFARI TES Bolometer Readout: Developments Towards a Flight System

    SAFARI is an imaging Fourier Transform Spectrometer for 35–200 μm under development for flight on the Japanese IR-satellite SPICA (2018). The 3.25 m diameter actively cooled telescope (<6K) will provide a sky ...

    J. van der Kuur, J. Beyer, M. Bruijn, J. R. Gao in Journal of Low Temperature Physics (2012)

  3. Article

    Open Access

    Low-Noise Readout of TES Detectors with Baseband Feedback Frequency Domain Multiplexing

    SRON is develo** an electronic read-out system for an array of transition edge sensors (TES) based on the techniques of frequency domain multiplexing (FDM) and base-band feedback (BBFB). The astronomical app...

    R. den Hartog, M. D. Audley, J. Beyer, D. Boersma in Journal of Low Temperature Physics (2012)

  4. Article

    Open Access

    AC Bias Characterization of Low Noise Bolometers for SAFARI Using an Open-Loop Frequency Domain SQUID-based Multiplexer Operating Between 1 and 5 MHz

    SRON is develo** the Frequency Domain Multiplexing (FDM) read-out and the ultra low NEP TES bolometers array for the infra-red spectrometer SAFARI on board of the Japanese space mission SPICA. The FDM protot...

    L. Gottardi, M. Bruijn, J.-R. Gao, R. den Hartog in Journal of Low Temperature Physics (2012)

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    Article

    Effect of Magnetic Fields on TiAu TES Bolometers for the SAFARI Instrument on the SPICA FIR Telescope

    At the Netherlands Institute for Space Research (SRON) we are develo** Transition Edge Sensors (TES) bolometers for the SAFARI Imaging Spectrometer on the SPICA telescope. With the current design of the SPIC...

    R. A. Hijmering, P. Khosropanah, M. Ridder in Journal of Low Temperature Physics (2012)

  6. Article

    Open Access

    Study of the Dependency on Magnetic Field and Bias Voltage of an AC-Biased TES Microcalorimeter

    At SRON we are studying the performance of a Goddard Space Flight Center single pixel TES microcalorimeter operated in an AC bias configuration. For x-ray photons at 6 keV the pixel shows an x-ray energy resol...

    L. Gottardi, J. Adams, C. Bailey, S. Bandler in Journal of Low Temperature Physics (2012)

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    Article

    EURECA: European-Japanese Microcalorimeter Array

    The EURECA project aims to demonstrate technological readiness of a micro-calorimeter array for application in future X-ray astronomy missions, like Constellation-X, EDGE, and XEUS. The prototype instrument co...

    P. de Korte, J. Anquita, F. Bakker, X. Barcons in Journal of Low Temperature Physics (2008)

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    Article

    The soft X-ray spectrum of NGC 4151

    EXOSAT observations of the Seyfert galaxy NGC 4151 over the period July 1983 to April 1984 have revealed a decreasing flux in the 2 –10 keV band. In accord with previous measurements a power law spectrum atten...

    K A Pounds, R S Warwick, J L Culhane, P de Korte in Space Science Reviews (1985)

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    Chapter and Conference Paper

    The Soft X-Ray Spectrum of NGC 4151

    EXOSAT observations of the Seyfert galaxy NGC 4151 over the period July 1983 to April 1984 have revealed a decreasing flux in the 2 – 10 keV band. In accord with previous measurements a power law spectrum atte...

    K. A. Pounds, R. S. Warwick, J. L. Culhane in X-Ray Astronomy in the Exosat Era (1985)

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    Article

    The use of diamond turned & replicated wolter 1 telescopes for high sensitivity X-ray astronomy

    Following the success of Einstein, it is clear that telescopes of very large area (∼10 cm) with angular resolution (⪝20″) are needed for deep X-ray surveys and other observations. After a discussion of these o...

    J. L. Culhane, R. C. Catura, K. A. Pounds, P. de Korte, A. Franks in Space Science Reviews (1981)

  11. No Access

    Chapter and Conference Paper

    The Use of Diamond Turned & Replicated Wolter 1 Telescopes for High Sensitivity X-Ray Astronomy

    Following the siicces of Einstein, it is clear that telescopes of very large area ( ~ 104 cm2) with angular resolution (⪝20″) are needed for deep X-ray surveys and other observations. After a discussion of these ...

    J. L. Culhane, R. C. Catura, K. A. Pounds, P. de Korte, A. Franks in X-Ray Astronomy (1981)