activity
20002025
most citedFirst Light Measurements with the XMM-Newton Reflection Grating Spectrometers: Evidence for an Inverse First Ionisation Potential Effect and Anomalous Ne A bundance in the Coronae of HR 1099

190 citations · 1.8k across the 52 of their papers we have counts for

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26 papers · 1 filter

astro-ph.IM2025★ 4 cited

Ground calibration plan for the Athena/X-IFU microcalorimeter spectrometer

Alexeï Molin, François Pajot, Marc Audard +24

The X-ray Integral Field Unit is the X-ray imaging spectrometer on-board one of ESA's next large missions, Athena. Athena is set to investigate the theme of the Hot and Energetic U…

astro-ph.IM2024★ 7 cited

Developments on frequency domain multiplexing readout for large arrays of transition-edge sensor X-ray micro-calorimeters

D. Vaccaro, H. Akamatsu, L. Gottardi +8

At SRON we have been developing X-ray TES micro-calorimeters as backup technology for the X-ray Integral Field Unit (X-IFU) of the Athena mission, demonstrating excellent resolving…

astro-ph.IM2024

System performance of a TDM test-bed with long flex harness towards the new X-IFU FPA-DM

D. Vaccaro, M. de Wit, J. van der Kuur +17

SRON (Netherlands Institute for Space Research) is developing the Focal Plane Assembly (FPA) for Athena X-IFU, whose Demonstration Model (DM) will use for the first time a time dom…

astro-ph.IM2022★ 3 cited

Frequency domain multiplexing readout for large arrays of transition-edge sensors

Davide Vaccaro, Hiroki Akamatsu, Luciano Gottardi +13

We report our most recent progress and demonstration of a frequency domain multiplexing (FDM) readout technology for transition-edge sensor (TES) arrays, both of which we have been…

astro-ph.IM2022★ 14 cited

Performance of the SRON Ti/Au Transition Edge Sensor X-ray Calorimeters

Martin de Wit, Luciano Gottardi, Kenichiro Nagayoshi +7

In the early 2030s, ESAs new X-ray observatory, Athena, is scheduled to be launched. It will carry two main instruments, one of which is the X-ray Integral Field Unit (X-IFU), an X…

astro-ph.IM2022★ 9 cited

Susceptibility study of TES micro-calorimeters for X-ray spectroscopy under FDM readout

Davide Vaccaro, Hiroki Akamatsu, Luciano Gottardi +15

We present a characterization of the sensitivity of TES X-ray micro-calorimeters to environmental conditions under frequency-domain multiplexing (FDM) readout. In the FDM scheme, e…

astro-ph.IM2022★ 10 cited

Mitigation of the Magnetic Field Susceptibility of Transition Edge Sensors using a Superconducting Groundplane

Martin de Wit, Luciano Gottardi, Marcel L. Ridder +7

Transition edge sensor (TES) microcalorimeters and bolometers are used for a variety of applications. The sensors are based on the steep temperature-dependent resistance of the nor…

astro-ph.IM2022★ 20 cited

ATHENA X-IFU Demonstration Model: First joint operation of the main TES Array and its Cryogenic AntiCoincidence Detector (CryoAC)

M. D'Andrea, K. Ravensberg, A. Argan +28

The X-IFU is the cryogenic spectrometer onboard the future ATHENA X-ray observatory. It is based on a large array of TES microcalorimeters, which works in combination with a Cryoge…

astro-ph.IM2021★ 6 cited

Thermal crosstalk of X-ray transition-edge sensor micro-calorimeters under frequency domain multiplexing readout

Davide Vaccaro, Hiroki Akamatsu, Marcel P. Bruijn +12

We have measured and characterized the thermal crosstalk in two different arrays of transition-edge sensor (TES) X-ray micro-calorimeters with frequency-domain multiplexing (FDM) r…

astro-ph.IM2021★ 29 cited

High Aspect Ratio Transition Edge Sensors for X-ray Spectrometry

M. de Wit, L. Gottardi, E. Taralli +11

We are developing large TES arrays in combination with FDM readout for the next generation of X-ray space observatories. For operation under AC-bias, the TESs have to be carefully…

astro-ph.IM2018★ 8 cited

The Athena X-ray Integral Field Unit

Didier Barret, Thien Lam Trong, Jan-Willem den Herder +100

The X-ray Integral Field Unit (X-IFU) is the high resolution X-ray spectrometer of the ESA Athena X-ray observatory. Over a field of view of 5' equivalent diameter, it will deliver…

astro-ph.IM2018★ 2 cited

Simulating Modulated X-ray calibration Sources for future X-ray missions, using GEANT4

C. P. de Vries, V. Fioretti, J. W. den Herder +2

The XIFU X-ray spectrometer instrument on the future Athena mission needs X-ray calibration sources to calibrate the gains of the individual detector pixels. For this purpose, elec…

astro-ph.IM2016★ 2 cited

The Filter Wheel and Filters development for the X-IFU instrument on-board Athena

E. Bozzo, M. Barbera, L. Genolet +7

Athena is the large mission selected by ESA in 2013 to investigate the science theme "Hot and Energetic Universe" and presently scheduled for launch in 2028. One of the two instrum…

astro-ph.IM2016★ 123 cited

The Athena X-ray Integral Field Unit (X-IFU)

Didier Barret, Thien Lam Trong, Jan-Willem den Herder +88

The X-ray Integral Field Unit (X-IFU) on board the Advanced Telescope for High-ENergy Astrophysics (Athena) will provide spatially resolved high-resolution X-ray spectroscopy from…

astro-ph.IM2016★ 23 cited

Development of the superconducting detectors and read-out for the X-IFU instrument on board of the X-ray observatory Athena

Luciano Gottardi, Hiroki Akamatsu, Marcel P. Bruijn +6

The Advanced Telescope for High-Energy Astrophysics (Athena) has been selected by ESA as its second large-class mission. The future European X-ray observatory will study the hot an…

astro-ph.IM2014★ 38 cited

Calibration and in orbit performance of the reflection grating spectrometer onboard XMM-Newton

C. P. de Vries, J. W. den Herder, C. Gabriel +6

Context: XMM-Newton was launched on 10 December 1999 and has been operational since early 2000. One of the instruments onboard XMM-Newton is the reflection grating spectrometer (RG…

astro-ph.IM2014★ 1 cited

The LOFT Ground Segment

E. Bozzo, A. Antonelli, A. Argan +27

LOFT, the Large Observatory For X-ray Timing, was one of the ESA M3 mission candidates that completed their assessment phase at the end of 2013. LOFT is equipped with two instrumen…

astro-ph.IM2014★ 6 cited

The design of the wide field monitor for LOFT

S. Brandt, M. Hernanz, L. Alvarez +41

LOFT (Large Observatory For x-ray Timing) is one of the ESA M3 missions selected within the Cosmic Vision program in 2011 to carry out an assessment phase study and compete for a l…

astro-ph.IM2014

Optimisation of the design for the LOFT Large Area Detector Module

D. Walton, B. Winter, S. Zane +25

LOFT (Large Observatory for X-ray Timing) is an X-ray timing observatory that, with four other candidates, was considered by ESA as an M3 mission (with launch in 2022-2024) and has…

astro-ph.IM2014★ 2 cited

Hyper-velocity impact test and simulation of a double-wall shield concept for the Wide Field Monitor aboard LOFT

E. Perinati, M. Rott, A. Santangelo +10

The space mission LOFT (Large Observatory For X-ray Timing) was selected in 2011 by ESA as one of the candidates for the M3 launch opportunity. LOFT is equipped with two instrument…

astro-ph.IM2013★ 4 cited

The LOFT mission: new perspectives in the research field of (accreting) compact objects

E. Bozzo, L. Stella, M. van der Klis +6

LOFT, the Large Observatory For X-ray Timing, is one of five ESA M3 candidate missions. It will address the Cosmic Vision theme: "Matter under Extreme Conditions". By coupling for…

astro-ph.IM2012

Accelerator experiments with soft protons and hyper-velocity dust particles: application to ongoing projects of future X-ray missions

E. Perinati, S. Diebold, E. Kendziorra +31

We report on our activities, currently in progress, aimed at performing accelerator experiments with soft protons and hyper-velocity dust particles. They include tests of different…

astro-ph.IM2012★ 1 cited

Calibration strategies for the LAD instrument on-board LOFT

Luigi Pacciani, Paolo Soffitta, Andrea Argan +12

The Scientific objectives of the LOFT mission, e.g., the study of the Neutron Star equation of state and of the Strong Gravity, require accurate energy, time and flux calibration f…

astro-ph.IM2012★ 16 cited

The LOFT Wide Field Monitor

S. Brandt, M. Hernanz, L. Alvarez +32

LOFT (Large Observatory For x-ray Timing) is one of the four missions selected in 2011 for assessment study for the ESA M3 mission in the Cosmic Vision program, expected to be laun…