The Cryogenic AntiCoincidence Detector for ATHENA X-IFU: a program overview - Dr. Claudio Macculi The Cryogenic AntiCoincidence Detector for ATHENA X-IFU: preliminary test and data analysis of the new “bridges-suspended” single pixel - Dr. Matteo D’Andrea Microcalorimeter pulse analysis by means of principle component decomposition - Dr. Cor P de Vries TES pixel parameter design of the microcalorimeter array for the x-ray integral field unit on Athena - Dr. Stephen J Smith Implementation and fabrication considerations of an optimal hybrid array for the Athena X-ray Integral Field Unit instrument - Dr. Simon R Bandler The impact of crosstalk in the Athena/X-IFU instrument on the GRB/WHIM science case - Dr. Roland H den Hartog Performance assessment of different pulse reconstruction algorithms for the Athena X-ray Integral Field Unit - Mr. Philippe Peille X-Ray absorption spectroscopy on test thermal filters for the ATHENA X-IFU detector - Prof. Marco Barbera The Athena/XIFU filter wheel - Dr. Enrico Bozzo Gain stability with no-feedback-loop developed for the X-IFU/Athena readout chain - Dr. Damien Prêle Updates on the background estimates for the X-IFU instrument onboard of the ATHENA mission - Dr. Simone Lotti The Athena x-ray integral field unit - Dr. Didier Barret The mechanical and EM simulations of the CryoAC DM for the ATHENA X-IFU - Mr. Dario Corsini The focal plane assembly for the Athena X-ray Integral Field Unit instrument - Dr. Brian Jackson Preliminary thermal architecture of the X-IFU instrument - Dr. Ivan Charles X-IFU Instrument: technical challenges and preliminary design - Mr. Thien Lam Trong Conceptual design of the X-IFU instrument control unit on board the ESA Athena mission - Dr. Leonardo Corcione TESSIM: A simulator for the ATHENA X-IFU - Prof. Jörn Wilms Observing the WHIM with ATHENA - Prof. Jörn Wilms Optimising the multiplex factor of the frequency domain multiplexed...
The official X-IFU logos are available from the X-IFU web site, under RESOURCES.
The latest X-IFU response matrices produced by Didier Barret/Edoardo Cucchetti (IRAP) and verified by the Bamberg group led by Joern Wilms, with the support of the system team, including Philippe Peille. These files have been produced for the so-called Athena cost-constrained configuration, with a diameter corresponding to a peak effective area at 1 keV of ~1.4 square meters. The response files cover 50 eV to 12.5 keV but the usual range for the fits should be 0.2-12 keV. Please check the FITs headers to see the assumptions used. Check also the README file, and look at the PDF files. Further information can be found in the SPIE papers: Barret et al. (SPIE, 2018). The arf and rmf files car be downloaded from this URL. Please contact directly Didier Barret for any enquiries.
The X-IFU background files are produced by the IAPS/INAF group led by Simone Lotti. The files reflect on the new X-IFU response matrices for the so-called cost-constrained mission configuration. The files are available for point and extended sources: an extraction surface of 78,5 arcsec^2 (for point sources corresponding to an extraction radius of 5arcsec) an extraction surface of 1 arcmin^2 (for extended sources) Please contact directly Simone Lotti for any further information.
[caption id="attachment_941" align="aligncenter" width="780"] X IFU Functional block diagram[/caption]
[caption id="attachment_951" align="aligncenter" width="780"] X-IFU organization with experts with engineering teams and cnes project team[/caption]