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328 results on '"den Herder, J."'

6. ATHENA X-IFU Demonstration Model: First Joint Operation of the Main TES Array and its Cryogenic AntiCoincidence Detector (CryoAC)

Author

D’Andrea, M., Ravensberg, K., Argan, A., Brienza, D., Lotti, S., Macculi, C., Minervini, G., Piro, L., Torrioli, G., Chiarello, F., Ferrari Barusso, L., Biasotti, M., Gallucci, G., Gatti, F., Rigano, M., Akamatsu, H., Dercksen, J., Gottardi, L., de Groote, F., den Hartog, R., den Herder, J.-W., Hoogeveen, R., Jackson, B., McCalden, A., Rosman, S., Taralli, E., Vaccaro, D., de Wit, M., Chervenak, J., Smith, S., and Wakeham, N.

Published
2022
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10. The Athena X-ray Integral Field Unit (X-IFU)

Author

Pajot, F., Barret, D., Lam-Trong, T., den Herder, J.-W., Piro, L., Cappi, M., Huovelin, J., Kelley, R., Mas-Hesse, J. M., Mitsuda, K., Paltani, S., Rauw, G., Rozanska, A., Wilms, J., Barbera, M., Douchin, F., Geoffray, H., den Hartog, R., Kilbourne, C., Le Du, M., Macculi, C., Mesnager, J.-M., and Peille, P.

Published
2018
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11. Oxygen and iron in interstellar dust: An X-ray investigation

Author

Psaradaki, I., Costantini, E., Rogantini, D., Mehdipour, M., Corrales, L., Zeegers, S. T., De Groot, F., Den Herder, J. W.A., Mutschke, H., Trasobares, S., De Vries, C. P., Waters, L. B.F.M., Psaradaki, I., Costantini, E., Rogantini, D., Mehdipour, M., Corrales, L., Zeegers, S. T., De Groot, F., Den Herder, J. W.A., Mutschke, H., Trasobares, S., De Vries, C. P., and Waters, L. B.F.M.

Abstract

Understanding the chemistry of the interstellar medium (ISM) is fundamental for the comprehension of Galactic and stellar evolution. X-rays provide an excellent way to study the dust chemical composition and crystallinity along different sight lines in the Galaxy. In this work, we study the dust grain chemistry in the diffuse regions of the ISM in the soft X-ray band (<1 keV). We use newly calculated X-ray dust extinction cross sections obtained from laboratory data in order to investigate the oxygen K and iron L shell absorption. We explore the XMM-Newton and Chandra spectra of five low-mass X-ray binaries (LMXBs) located in the Galactic plane and model the gas and dust features of oxygen and iron simultaneously. The dust samples used for this study include silicates with different Mg:Fe ratios, sulfides, iron oxides, and metallic iron. Most dust samples are in both amorphous and crystalline lattice configuration. We computed the extinction cross sections using Mie scattering approximation and assuming a power-law dust size distribution. We find that the Mg-rich amorphous pyroxene (Mg0.75Fe0.25SiO3) represents the largest fraction of dust towards most of the X-ray sources, namely about 70% on average. Additionally, we find that ~15% of the dust column density in our lines of sight is in metallic Fe. We do not find strong evidence for ferromagnetic compounds, such as Fe3O4 or iron sulfides (FeS, FeS2). Our study confirms that iron is heavily depleted from the gas phase into solids; more than 90% of iron is in dust. The depletion of neutral oxygen is mild, namely of between 10% and 20% depending on the line of sight.

Published
2023

12. Oxygen and iron in interstellar dust: An X-ray investigation

Author

Sub Materials Chemistry and Catalysis, Materials Chemistry and Catalysis, Psaradaki, I., Costantini, E., Rogantini, D., Mehdipour, M., Corrales, L., Zeegers, S. T., De Groot, F., Den Herder, J. W.A., Mutschke, H., Trasobares, S., De Vries, C. P., Waters, L. B.F.M., Sub Materials Chemistry and Catalysis, Materials Chemistry and Catalysis, Psaradaki, I., Costantini, E., Rogantini, D., Mehdipour, M., Corrales, L., Zeegers, S. T., De Groot, F., Den Herder, J. W.A., Mutschke, H., Trasobares, S., De Vries, C. P., and Waters, L. B.F.M.

Published
2023

13. Background rates of x-ray transition-edge sensor micro-calorimeters under a frequency domain multiplexing readout for solar axion-like particles’ detection

Author

Vaccaro, D. (author), Gottardi, L. (author), Akamatsu, H. (author), van der Kuur, J. (author), Nagayoshi, K. (author), Taralli, E. (author), de Wit, M. (author), Ravensberg, K. (author), Gao, J.R. (author), den Herder, J. W.A. (author), Vaccaro, D. (author), Gottardi, L. (author), Akamatsu, H. (author), van der Kuur, J. (author), Nagayoshi, K. (author), Taralli, E. (author), de Wit, M. (author), Ravensberg, K. (author), Gao, J.R. (author), and den Herder, J. W.A. (author)

Abstract

We report on the x-ray background rate measured with transition-edge sensors (TES) micro-calorimeters under frequency-domain multiplexing (FDM) readout as a possible technology for future experiments aiming at a direct detection of axion-like particles. Future axion helioscopes will make use of large magnets to convert axions into photons in the keV range and x-ray detectors to observe them. To achieve this, a detector array with high spectral performance and extremely low background is necessary. TES are single-photon, non-dispersive, high-resolution micro-calorimeters and represent a possible candidate for this application. We have been developing x-ray TES micro-calorimeters and an FDM readout technology in the framework of the space-borne x-ray astronomical observatories. We show that the current generation of our detectors is already a promising technology for a possible axion search experiment, having measured an x-ray background rate of 2.2(2) × 10−4 cm−2 s−1 keV−1 with a cryogenic demonstrator not optimized for this specific application. We then make a prospect to further improve the background rate down to the required value ( < 1 0 − 7 cm−2 s−1 keV−1) for an axion-search experiment, identifying no fundamental limits to reach such a level., Green Open Access added to TU Delft Institutional Repository ‘You share, we take care!’ – Taverne project https://www.openaccess.nl/en/you-share-we-take-care Otherwise as indicated in the copyright section: the publisher is the copyright holder of this work and the author uses the Dutch legislation to make this work public., ImPhys/Adam group

Published
2023
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15. Oxygen and iron in interstellar dust: An X-ray investigation

Author

Psaradaki, I., primary, Costantini, E., additional, Rogantini, D., additional, Mehdipour, M., additional, Corrales, L., additional, Zeegers, S. T., additional, de Groot, F., additional, den Herder, J. W. A., additional, Mutschke, H., additional, Trasobares, S., additional, de Vries, C. P., additional, and Waters, L. B. F. M., additional

Published
2023
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16. High aspect ratio transition edge sensors for x-ray spectrometry.

Author

de Wit, M., Gottardi, L., Taralli, E., Nagayoshi, K., Ridder, M. L., Akamatsu, H., Bruijn, M. P., D'Andrea, M., van der Kuur, J., Ravensberg, K., Vaccaro, D., Visser, S., Gao, J. R., and den Herder, J.-W. A.

Subjects
SUPERCONDUCTING transitions, X-rays, SPECTROMETRY, CRITICAL temperature, DETECTORS
Abstract

We are developing large Transition Edge Sensor (TES) arrays in combination with a frequency domain multiplexing readout for the next generation of X-ray space observatories. For operation under an AC-bias, the TESs have to be carefully designed and optimized. In particular, the use of high aspect ratio devices will help us to mitigate non-ideal behavior due to the weak-link effect. In this paper, we present a full characterization of a TES array containing five different device geometries, with aspect ratios (width:length) ranging from 1:2 up to 1:6. The complex impedance of all geometries is measured in different bias configurations to study the evolution of the small-signal limit superconducting transition parameters α and β , as well as the excess noise. We show that high aspect ratio devices with properly tuned critical temperatures (around 90 mK) can achieve excellent energy resolution, with an array average of 2.03 ± 0.17 eV at 5.9 keV and a best achieved resolution of 1.63 ± 0.17 eV. This demonstrates that AC-biased TESs can achieve a very competitive performance compared to DC-biased TESs. The results have motivated a push to even more extreme device geometries currently in development. [ABSTRACT FROM AUTHOR]

Published
2020
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17. An AOCS concept for the X-ray Interferometer mission

Author

den Hartog, R., Uttley, P., Hoevers, H., den Herder, J.-W., Wise, M., den Herder, J.-W.A., Nikzad, S., Nakazawa, K., High Energy Astrophys. & Astropart. Phys (API, FNWI), and Low Energy Astrophysics (API, FNWI)

Abstract

An X-ray Interferometer (XRI) has recently been proposed as a theme for ESA's Voyage 2050 planning cycle, with the prospect to observe the X-ray sky with unprecedented angular resolution. A scientifically very interesting mission is possible on the basis of a single spacecraft with a resolving power of 100 micro arcsec (~0.5 nrad), owing to the compact 'telephoto' design proposed in 2004 by Willingale. One of the key challenges for such a mission is to acquire and maintain pointing to an absolute accuracy below that resolution. This challenge was already identified by Gendreau et al. in 2003. In this paper we re-address this issue in the light of recent technological developments.

Published
2022

18. TES-Based X-ray Microcalorimeter Performances Under AC Bias and FDM for Athena

Author

Akamatsu, H., Gottardi, L., de Vries, C. P., Adams, J. S., Bandler, S. R., Bruijn, M. P., Chervenak, J. A., Eckart, M. E., Finkbeiner, F. M., Gao, J. R., den Herder, J.-W., den Hartog, R., Hoevers, H., Kelley, R. E., Khosropanah, P., Kilbourne, C. A., van der Kuur, J., Lee, S.-J., van den Linden, A. J., Porter, F. S., Ravensberg, K., Sadleir, J. E., Smith, S. J., Suzuki, T., Wassell, E. J., and Kiviranta, M.

Published
2016
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21. Mitigation of the Magnetic Field Susceptibility of Transition-Edge Sensors Using a Superconducting Groundplane

Author

de Wit, M. (author), Gottardi, L (author), Ridder, Marcel L. (author), Nagayoshi, K. (author), Taralli, E. (author), Akamatsu, H. (author), Vaccaro, D. (author), den Herder, J. W.A. (author), de Bruijn, M.P. (author), Gao, J.R. (author), de Wit, M. (author), Gottardi, L (author), Ridder, Marcel L. (author), Nagayoshi, K. (author), Taralli, E. (author), Akamatsu, H. (author), Vaccaro, D. (author), den Herder, J. W.A. (author), de Bruijn, M.P. (author), and Gao, J.R. (author)

Abstract

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 normal-to-superconducting transition, and are thus intrinsically sensitive to magnetic fields. Conventionally the detectors are shielded from stray magnetic fields using external magnetic shields. However, in particular for applications with strict limits on the available space and mass of an instrument, external magnetic shields might not be enough to obtain the required shielding factors or field homogeneity. Additionally, these shields are only effective for magnetic fields generated external to the TES array, and are ineffective to mitigate the impact of internally generated magnetic fields. Here we present an alternative shielding method based on a super-conducting groundplane deposited directly on the backside of the silicon nitride membrane on which the TESs are located. We demonstrate that this local shielding for external magnetic fields has a shielding factor of at the least approximately 80, and is also effective at reducing internal self-induced magnetic fields, as demonstrated by measurements and simulation of the eddy current losses in our ac-biased detectors. Measurements of 5.9-keV x-ray photons show that our shielded detectors have a high resilience to external magnetic fields, showing no degradation of the energy resolution or shifts of the energy-scale calibration for fields of several microtesla, values higher than expected in typical real-world applications., ImPhys/Optics

Published
2022
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22. Background rates of x-ray transition-edge sensor micro-calorimeters under a frequency domain multiplexing readout for solar axion-like particles' detection.

Author

Vaccaro, D., Gottardi, L., Akamatsu, H., van der Kuur, J., Nagayoshi, K., Taralli, E., de Wit, M., Ravensberg, K., Gao, J. R., and den Herder, J. W. A.

Subjects
AXIONS, X-rays, ASTRONOMICAL observatories, DETECTORS
Abstract

We report on the x-ray background rate measured with transition-edge sensors (TES) micro-calorimeters under frequency-domain multiplexing (FDM) readout as a possible technology for future experiments aiming at a direct detection of axion-like particles. Future axion helioscopes will make use of large magnets to convert axions into photons in the keV range and x-ray detectors to observe them. To achieve this, a detector array with high spectral performance and extremely low background is necessary. TES are single-photon, non-dispersive, high-resolution micro-calorimeters and represent a possible candidate for this application. We have been developing x-ray TES micro-calorimeters and an FDM readout technology in the framework of the space-borne x-ray astronomical observatories. We show that the current generation of our detectors is already a promising technology for a possible axion search experiment, having measured an x-ray background rate of 2.2(2) × 10−4 cm−2 s−1 keV−1 with a cryogenic demonstrator not optimized for this specific application. We then make a prospect to further improve the background rate down to the required value (< 1 0 − 7 cm−2 s−1 keV−1) for an axion-search experiment, identifying no fundamental limits to reach such a level. [ABSTRACT FROM AUTHOR]

Published
2023
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23. Maximum Likelihood Method Applied to COMPTEL Source Recognition and Analysis

Author

den Herder, J. W., Lichti, G., de Boer, H., McConnell, M., Ryan, J., Bennett, K., Bloemen, H., Hermsen, W., Klumper, A., Schönfelder, V., Strong, A. W., de Vries, C., Zichichi, Antonino, editor, Di Gesù, V., editor, Scarsi, L., editor, Buccheri, R., editor, Crane, P., editor, Maccarone, M. C., editor, and Zimmermann, H. U., editor

Published
1992
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24. Neural Net Approaches for Event Location in the Detector Modules

Author

Connors, A., Aarts, H., Bennett, K., Deerenberg, A., Diehl, R., den Herder, J. W., Hermsen, W., Lichti, G., Lockwood, J., Loomis, M., Macri, J., McConnell, M., Morris, D., Reinhard, K., Ryan, J., Schönfelder, V., Simpson, G., Swanenberg, B. N., Steinle, H., Strong, A., Varendorff, M., de Vries, C., Webber, W. E., Winkler, C., Zeitlmeyer, V., Zichichi, Antonino, editor, Di Gesù, V., editor, Scarsi, L., editor, Buccheri, R., editor, Crane, P., editor, Maccarone, M. C., editor, and Zimmermann, H. U., editor

Published
1992
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25. COMPTEL as a Solar Gamma Ray and Neutron Detector

Author

Ryan, J. M., Aarts, H., Bennett, K., Byrd, R., de Vries, C., den Herder, J. W., Deerenberg, A., Diehl, R., Eymann, G., Forrest, D. J., Foster, C., Hermsen, W., Lockwood, J., Lichti, G., Macri, J., McConnell, M., Morris, D., Schönfelder, V., Simpson, G., Snelling, M., Steinle, H., Strong, A., Swanenburg, B. N., Taddeucci, T., Webber, W. R., Winkler, C., Zichichi, Antonino, editor, Di Gesù, V., editor, Scarsi, L., editor, Buccheri, R., editor, Crane, P., editor, Maccarone, M. C., editor, and Zimmermann, H. U., editor

Published
1992
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26. Maximum Entropy Imaging and Spectral Deconvolution for COMPTEL

Author

Strong, A. W., Cabeza-Orcel, P., Bennett, K., Collmar, W., Diehl, R., den Herder, J. W., Hermsen, W., Lichti, G., McConnell, M., Ryan, J., Steinle, H., Schönfelder, V., Winkler, C., Zichichi, Antonino, editor, Di Gesù, V., editor, Scarsi, L., editor, Buccheri, R., editor, Crane, P., editor, Maccarone, M. C., editor, and Zimmermann, H. U., editor

Published
1992
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27. Pulsar Analysis within COMPASS

Author

Busetta, M., Bennett, K., Buccheri, R., Clear, J., Diehl, R., den Herder, J. W., Hermsen, W., Kuiper, L., Lockwood, J., McConnell, M., Ryan, J., Schönfelder, V., Strong, A., Taylor, B. G., Winkler, C., Zichichi, Antonino, editor, Di Gesù, V., editor, Scarsi, L., editor, Buccheri, R., editor, Crane, P., editor, Maccarone, M. C., editor, and Zimmermann, H. U., editor

Published
1992
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28. Response Determinations of COMPTEL from Calibration Measurements, Models, and Simulations

Author

Diehl, R., Aarts, H., Bennett, K., Collmar, W., deBoer, H., Deerenberg, A. J. M., den Herder, J. W., deVries, C., Hermsen, W., Kippen, M., Knödlseder, J., Kuiper, L., Lichti, G. G., Lockwood, J. A., Macri, J., McConnell, M., Much, R., Morris, D., Ryan, J., Schönfelder, V., Simpson, G., Steinle, H., Strong, A. W., Swanenburg, B. N., van Sant, T., Webber, W. R., Winkler, C., Zichichi, Antonino, editor, Di Gesù, V., editor, Scarsi, L., editor, Buccheri, R., editor, Crane, P., editor, Maccarone, M. C., editor, and Zimmermann, H. U., editor

Published
1992
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29. COMPTEL Processing and Analysis Software System: COMPASS (Requirements and Overview)

Author

den Herder, J. W., Aarts, H., Bennett, K., Diehl, R., Hermsen, W., Johnson, M., Lockwood, J., McConnell, M., Ryan, J., Schönfelder, V., Simpson, G., Steinle, H., Strong, A. W., Swanenburg, B. N., de Vries, C., Winkler, C., Wood, I., Zichichi, Antonino, editor, Di Gesù, V., editor, Scarsi, L., editor, Buccheri, R., editor, Crane, P., editor, Maccarone, M. C., editor, and Zimmermann, H. U., editor

Published
1992
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30. The GRO - COMPTEL Mission: Instrument Description and Scientific Objectives

Author

Schönfelder, V., Bennett, K., Collmar, W., Connors, A., Deerenberg, A., Diehl, R., den Herder, J. W., Hermsen, W., Lichti, G. G., Lockwood, J. A., Macri, J., McConnell, M., Morris, D., Ryan, J., Simpson, G., Steinle, H., Strong, A., Swanenburg, B. N., Taylor, B. G., Varendorff, M., de Vries, C., Winkler, C., Zichichi, Antonino, editor, Di Gesù, V., editor, Scarsi, L., editor, Buccheri, R., editor, Crane, P., editor, Maccarone, M. C., editor, and Zimmermann, H. U., editor

Published
1992
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31. Calibration of the Microcalorimeter Spectrometer On-Board the Hitomi (Astro-H) Observatory (invited)

Author

Eckart, M. E, Boyce, K. R, Brown, G. V, Chiao, M. P, Fujimoto, R, Haas, D, Den Herder, J.-W, Ishisaki, Y, Kelley, R. L, Kilbourne, C. A, Leutenegger, M. A, McCammon, D, Mitsuda, K, Porter, F. S, Sawada, M, Sneiderman, G. A, Szymkowiak, A. E, Takei, Y, Tashiro, M, Tsujimoto, M, de Vries, C. P, Watanabe, T, Yamada, S, and Yamasaki, N. Y

Subjects
Astrophysics
Abstract

The Hitomi Soft X-ray Spectrometer (SXS) was a pioneering non-dispersive imaging x-ray spectrometer with 5 eV FWHM energy resolution, consisting of an array of 36 silicon-thermistor microcalorimeters at the focus of a high-throughput soft x-ray telescope. The instrument enabled astrophysical plasma diagnostics in the 0.3-12 keV band. We introduce the SXS calibration strategy and corresponding ground calibration measurements that took place from 2012-2015, including both the characterization of the microcalorimeter array and measurements of the x-ray transmission of optical blocking filters.

Published
2016
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32. Ground Calibration of the Astro-H (Hitomi) Soft X-Ray Spectrometer

Author

Eckart, M. E, Adams, J. S, Boyce, K. R, Brown, G. V, Chiao, Meng P, Fujimoto, R. J, Haas, D, Den Herder, J. W, Ishisaki, Y, Kelley, R. L, Kilbourne, C. A, Leutenegger, M. A, McCammon, D, Mitsuda, K, Porter, F. S, Sato, K, Sawada, M, Seta, H, Sneiderman, G. A, Szymkowiak, A. E, Takei, Y, Tashiro, M, Tsujimoto, M, De Vries, C. P, Watanabe, T, Yamada, S, and Yamasaki, N. Y

Subjects
Astrophysics
Abstract

The Astro-H (Hitomi) Soft X-ray Spectrometer (SXS) was a pioneering imaging x-ray spectrometer with 5 eV energy resolution at 6 keV. The instrument used a microcalorimeter array at the focus of a high-throughput soft x-ray telescope to enable high-resolution non-dispersive spectroscopy in the soft x-ray waveband (0.3-12 keV). We present the suite of ground calibration measurements acquired from 2012-2015, including characterization of the detector system, anti-coincidence detector, optical blocking filters, and filter-wheel filters. The calibration of the 36-pixel silicon thermistor microcalorimeter array includes parameterizations of the energy gain scale and line spread function for each event grade over a range of instrument operating conditions, as well as quantum efficiency measurements. The x-ray transmission of the set of five Al/polyimide thin-film optical blocking filters mounted inside the SXS dewar has been modeled based on measurements at synchrotron beamlines, including with high spectral resolution at the C, N, O, and Al K-edges. In addition, we present the x-ray transmission of the dewar gate valve and of the filters mounted on the SXS filter wheel (external to the dewar), including beryllium, polyimide, and neutral density filters.

Published
2016
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33. The Focal Plane Assembly for the Athena X-Ray Integral Field Unit Instrument

Author

Jackson, B. D, Van Weers, H, van der Kuur, J, den Hartog, R, Akamatsu, H, Argan, A, Bandler, S. R, Barbera, M, Barret, D, Bruijn, M. P, Chervenak, J. A, Dercksen, J, Gatti, F, Gottardi, L, Haas, D, den Herder, J.-W, Kilbourne, C. A, Kiviranta, M, Lam-Trong, T, van Leeuwen, B.-J, Macculi, C, Piro, L, and Smith, S. J

Subjects
Astrophysics
Abstract

This paper summarizes a preliminary design concept for the focal plane assembly of the X-ray Integral Field Unit on the Athena spacecraft, an imaging microcalorimeter that will enable high spectral resolution imaging and point-source spectroscopy. The instrument's sensor array will be a 3840-pixel transition edge sensor (TES) microcalorimeter array, with a frequency domain multiplexed SQUID readout system allowing this large-format sensor array to be operated within the thermal constraints of the instrument's cryogenic system. A second TES detector will be operated in close proximity to the sensor array to detect cosmic rays and secondary particles passing through the sensor array for off-line coincidence detection to identify and reject events caused by the in-orbit high-energy particle background. The detectors, operating at 55 mK, or less, will be thermally isolated from the instrument cryostat's 2 K stage, while shielding and filtering within the FPA will allow the instrument's sensitive sensor array to be operated in the expected environment during both on-ground testing and in-flight operation, including stray light from the cryostat environment, low-energy photons entering through the X-ray aperture, low-frequency magnetic fields, and high-frequency electric fields.

Published
2016
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34. The LOFT Mission Concept - A Status Update

Author

Feroci, M, Bozzo, E, Brandt, S, Hernanz, M, van Der Klis, M, Liu , L. -P, Orleanski, P, Pohl, M, Santangelo, A, Schanne, S, Stella, L, Takahashi, T, Tamura, H, Watts, A, Wilms, J, Zane, S, Zhang, S. -N, Bhattacharyya, S, Agudo, I, Ahangarianabhari, M, Albertus, C, Alford, M, Alpar, A, Altamirano, D, Alvarez, L, Amati, L, Amoros, C, Andersson, N, Antonelli, A, Argan, A, Artigue, R, Artigues, B, Atteia, J. -L, Azzarello, P, Bakala, P, Ballantyne, D. R, Baldazzi, G, Baldo, M, Balman, S, Barbera, M, van Baren, C, Barret, D, Baykal, A, Begelman, M, Behar, E, Behar, O, Belloni, T, Belluti, P, Bernardini, F, Bertuccio, G, Bianchini, A, Binko, P, Blay, P, Bocchino, P, Bode, M, Bodin, P, Bombaci, I, Bonnet Bidaud, J. -M, Schnittman, Jeremy David, Borghi, G, Boutloukos, N, Bouyjou, F, Bradley, L, Braga, J, Briggs, M. S, Brown, E, Buballa, M, Bucciantini, N, Burderi, L, Burgay, M, Bursa, M, Budtz-Jorgensen, C, Cackett, E, Cadoux, F. R, Cais, P, Caliandro, G. A, Campana, R, Campana, S, Cao, X, Capitanio, F, Casares, J, Casella, P, Castro-Tirado, A. J, Cavazzuti, E, Cavechi, Y, Celestin, S, Cerda-Duran, P, Chakrabarty, D, Chamel, N, Chateau, F, Chen, C, Chen, Y, Chenevez, J, Chernyakova, M, Coker, J, Cole, R, Collura, A, Coriat, M, Cornelisse, R, Costamante, L, Cros, A, Cui, W, Cumming, A, Cusumano, G, Czerny, B, D'Ai, A, D'Ammando, J. P. C, D'Elia, V, Dai, Z, Del Monte, E, De Luca, A, De Martino, D, Dercksen, J. P. C, De Pasquale, M, De Rosa, A, Del Santo, M, Di Cosimo, S, Degenaar, N, den Herder, J. W, Diebold, S, Di Salvo, T, Dong, Y, Donnarumma, I, Doroshenko, V, Doyle, G, Drake, S. A, Durant, M, Emmanoulopoulos, D, Enoto, T, Erkut, M. H, Esposito, P, Evangelista, Y, Fabian, A, Falanga, M, Favre, Y, Feldman, C, Fender, R, Feng, H, Ferrari, V, Ferrigno, C, Ficorella, F, Finger, M, Finger, M. H, Fraser, G. W, Frericks, N, Fullekrug, M, Fuschino, F, Gabler, M, Galloway, D. K, Galvez Sanchez, J. L, Gandhi, P, Gao, Z, Garcia-Berro, E, Gendre, B, Gevin, O, Gezari, S, Giles, A. B, Gilfanov, M, Giommi, P, Giovannini, G, Giroletti, M, Gogus, E, Goldwurm, A, Goluchova, K, Gotz, D, Gou, L, Gouiffes, C, Grandi, P, Grassi, M, Greiner, J, Grinberg, V, Groot, P, Gschwender, M, Gualtieri, L, Guedel, M, Guidorzi, C, Guy, L, Haas, D, Haensel, P, Hailey, M, Hamuguchi, K, Hansen, F, Hartmann, D. H, Haswell, C. A, Hebeler, K, Heger, A, Hempel, M, Hermsen, W, Homan, J, Hornstrup, A, Hudec, R, Huovelin, J, Huppenkothen, A, Inam, S. C, Ingram, A, in't Zand, J. J. M, Israel, G, Iwasawa, K, Izzo, L, Jacobs, H. M, Jetter, F, Johannsen, T, Jenke, P. A, Jonker, P, Jose, J, Kaaret, P, Kalamkar, M, Kalemci, E, Kanbach, G, Karas, V, Karelin, D, Kataria, D, Keek, L, Kennedy, T, Klochkov, D, Kluzniak, W, Koerding, E, Kokkotas, K, Komossa, S, Korpela, S, Kouveliotou, C, Kowalski, A. F, Kreykenbohm, I, Kuiper, L. M, Kunneriath, D, Kurkela, A, Kuvvetli, I, La Franca, F, Labanti, C, Lai, D, Lamb, F. K, Lachaud, C, Laubert, P. P, Lebrun, F, Li, X, Liang, E, Limousin, O, Lin, D, Linares, M, Linder, D, Lodato, G, Longo, F, Lu, F, Lund, N, Maccarone, T. J, Macera, D, Maestre, S, Mahmoodifar, S, Maier, D, Malcovati, P, Malzac, J, Malone, C, Mandel, D, Mangano, V, Manousakis, A, Marelli, M, Margueron, J, Marisaldi, M, Markoff, S. B, Markowitz, A, Marinucci, A, Martindale, A, Martinez, G, McHardy, I. M, Medina-Tanco, G, Mehdipour, M, Melatos, A, Mendez, M, Mereghetti, S, Migliari, S, Mignani, R, Michalska, M, Mihara, T, Miller, M. C, Miller, J. M, Mineo, T, Miniutti, G, Morsink, S, Motch, C, Motta, S, Mouchet, M, Mouret, G, Mulacova, J, Muleri, F, Munoz-Darias, T, Negueruela, I, Neilsen, J, Neubert, T, Norton, A. J, Nowak, M, Nucita, A, O'Brien, P, Oertel, M, Olsen, P. E. H, Orienti, M, Orio, M, Orlandini, M, Osborne, J. P, Osten, R, Ozel, F, Pacciani, L, Paerels, F, Paltini, S, Paolillo, M, Papadakis, I, Papitto, A, Paragi, Z, Paredes, J. M, Patruno, A, Paul, B, Pederiva, F, Perinati, E, Pellizzoni, A, Penacchioni, A. V, Peretz, U, Perez, M. A, Perez-Torres, M, Petersen, B. M, Petracek, V, Picciotto, A, Piemonte, C, Pittori, C, Pons, J, Portell, J, Possenti, A, Postnov, K, Poutanen, J, Prakash, M, Prandoni, I, Provost, H. Le, Psaltis, D, Pye, J, Qu, J, Rambaud, D, Ramon, P, Ramsay, G, Rapisarda, M, Rachevski, A, Rashevskaya, I, Ray, P. S, Rea, N, Reddy, S, Reig, P, Reina, M. Aranda, Remillard, R, Reynolds, C, Rezzolla, L, Ribo, M, Rie, R. de la, Riggio, A, Rios, A, Rischke, D. H, Rodríguez-Gil, P, Rodriguez, J, Rohlfs, R, Romano, P, Rossi, E. M .R, Rozanska, A, Rousseau, A, Rudak, B, Russell, D. M, Ryde, F, Sabau-Graziati, L, Sakamoto, T, Sala, G, Salvaterra, R, Salvetti, D, Sanna, A, Sandberg, J, Savolainen, T, Scaringi, S, Schaffner-Bielich, J, Schatz, H, Schee, J, Schmid, C, Serino, M, Shakura, N, Shore, S, Schnittman, J. D, Schneider, R, Schwenk, A, Schwope, A. D, Sedrakian, A, Seyler, J.-Y, Shearer, A, Slowikowska, A, Sims, M, Smith, A, Smith, D. M, Smith, P. J, Sobolewska, M, Sochora, V, Soffitta, P, Soleri, P, Song, L, Spencer, A, Stamerra, A, Stappers, B, Staubert, R, Steiner, A. W, Stergioulas, N, Stevens, A. L, Stratta, G, Strohmayer, T. E, Stuchlik, Z, Suchy, S, Suleimanov, V, Tamburini, F, Tauris, T, Tavecchio, F, Tenzer, C, Thielemann, F. K, Tiengo, A, Tolos, L, Tombesi, F, Tomsick, J, Torok, G, Torrejon, J. M, Torres, D. F, Torresi, E, Tramacere, A, Traulsen, I, Trois, A, Turolla, R, Turriziani, S, Typel, S, Uter, P, Uttley, P, Vacchi, A, Varniere, P, Vaughan, S, Vercellone, S, Vietri, M, Vincent, F. H, Vrba, V, Walton, D, Wang, J, Wang, Z, Watanabe, S, Wawrzaszek, R, Webb, N, Weinberg, N, Wende, H, Wheatley, P, Wijers, R, Wijnands, R, Wille, M, Wilson-Hodge, C. A, Winter, B, Walk, S. J, Wood, K, Woosley, S. E, Wu, X, Xiao, L, Xu, R, Yu, W, Yuan, F, Yuan, W, Yuan, Y, Zampa, G, Zampa, N, Zampieri, L, Zdunik, L, Zdziarski, A, Zech, A, Zhang, B, Zhang, C, Zhang, S, Zingale, M, Zorzi, N, and Zwart, F

Subjects
Astrophysics
Abstract

The Large Observatory For x-ray Timing (LOFT) is a mission concept which was proposed to ESA as M3 and M4 candidate in the framework of the Cosmic Vision 2015-2025 program. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument and the uniquely large field of view of its wide field monitor, LOFT will be able to study the behaviour of matter in extreme conditions such as the strong gravitational field in the innermost regions close to black holes and neutron stars and the supra-nuclear densities in the interiors of neutron stars. The science payload is based on a Large Area Detector (LAD, is greater than 8m2 effective area, 2-30 keV, 240 eV spectral resolution, 1 degree collimated field of view) and a Wide Field Monitor (WFM, 2-50 keV, 4 steradian field of view, 1 arcmin source location accuracy, 300 eV spectral resolution). The WFM is equipped with an on-board system for bright events (e.g., GRB) localization. The trigger time and position of these events are broadcast to the ground within 30 s from discovery. In this paper we present the current technical and programmatic status of the mission.

Published
2016
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35. TESSIM: A Simulator for the Athena-X-IFU

Author

Wilms, J, Smith, S. J, Peille, P, Ceballos, M. T, Cobo, B, Dauser, T, Brand, T, Den Hartog, R. H, Bandler, S. R, De Plaa, J, and Den Herder, J.- W. A

Subjects
Numerical Analysis, Astrophysics
Abstract

We present the design of tessim, a simulator for the physics of transition edge sensors developed in the framework of the Athena end to end simulation effort. Designed to represent the general behavior of transition edge sensors and to provide input for engineering and science studies for Athena, tessim implements a numerical solution of the linearized equations describing these devices. The simulation includes a model for the relevant noise sources and several implementations of possible trigger algorithms. Input and output of the software are standard FITS-les which can be visualized and processed using standard X-ray astronomical tool packages. Tessim is freely available as part of the SIXTE package (http:www.sternwarte.uni-erlangen.deresearchsixte).

Published
2016
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36. Demonstration of MHz frequency domain multiplexing readout of 37 transition edge sensors for high-resolution x-ray imaging spectrometers

Author

Akamatsu, H., primary, Vaccaro, D., additional, Gottardi, L., additional, van der Kuur, J., additional, de Vries, C. P., additional, Kiviranta, M., additional, Ravensberg, K., additional, D'Andrea, M., additional, Taralli, E., additional, de Wit, M., additional, Bruijn, M. P., additional, van der Hulst, P., additional, den Hartog, R. H., additional, van Leeuwen, B.-J., additional, van der Linden, A. J., additional, McCalden, A. J., additional, Nagayoshi, K., additional, Nieuwenhuizen, A. C. T., additional, Ridder, M. L., additional, Visser, S., additional, van Winden, P., additional, Gao, J. R., additional, Hoogeveen, R. W. M., additional, Jackson, B. D., additional, and den Herder, J.-W. A., additional

Published
2021
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38. The Large Observatory for X-ray Timing (LOFT)

Author

Feroci, M., Stella, L., van der Klis, M., Courvoisier, T. J. -L., Hernanz, M., Hudec, R., Santangelo, A., Walton, D., Zdziarski, A., Barret, D., Belloni, T., Braga, J., Brandt, S., Budtz-Jørgensen, C., Campana, S., den Herder, J. -W., Huovelin, J., Israel, G. L., Pohl, M., Ray, P., Vacchi, A., Zane, S., Argan, A., Attinà, P., Bertuccio, G., Bozzo, E., Campana, R., Chakrabarty, D., Costa, E., De Rosa, A., Del Monte, E., Di Cosimo, S., Donnarumma, I., Evangelista, Y., Haas, D., Jonker, P., Korpela, S., Labanti, C., Malcovati, P., Mignani, R., Muleri, F., Rapisarda, M., Rashevsky, A., Rea, N., Rubini, A., Tenzer, C., Wilson-Hodge, C., Winter, B., Wood, K., Zampa, G., Zampa, N., Abramowicz, M. A., Alpar, M. A., Altamirano, D., Alvarez, J. M., Amati, L., Amoros, C., Antonelli, L. A., Artigue, R., Azzarello, P., Bachetti, M., Baldazzi, G., Barbera, M., Barbieri, C., Basa, S., Baykal, A., Belmont, R., Boirin, L., Bonvicini, V., Burderi, L., Bursa, M., Cabanac, C., Cackett, E., Caliandro, G. A., Casella, P., Chaty, S., Chenevez, J., Coe, M. J., Collura, A., Corongiu, A., Covino, S., Cusumano, G., D’Amico, F., Dall’Osso, S., De Martino, D., De Paris, G., Di Persio, G., Di Salvo, T., Done, C., Dovčiak, M., Drago, A., Ertan, U., Fabiani, S., Falanga, M., Fender, R., Ferrando, P., Della Monica Ferreira, D., Fraser, G., Frontera, F., Fuschino, F., Galvez, J. L., Gandhi, P., Giommi, P., Godet, O., Göǧüş, E., Goldwurm, A., Götz, D., Grassi, M., Guttridge, P., Hakala, P., Henri, G., Hermsen, W., Horak, J., Hornstrup, A., in’t Zand, J. J. M., Isern, J., Kalemci, E., Kanbach, G., Karas, V., Kataria, D., Kennedy, T., Klochkov, D., Kluźniak, W., Kokkotas, K., Kreykenbohm, I., Krolik, J., Kuiper, L., Kuvvetli, I., Kylafis, N., Lattimer, J. M., Lazzarotto, F., Leahy, D., Lebrun, F., Lin, D., Lund, N., Maccarone, T., Malzac, J., Marisaldi, M., Martindale, A., Mastropietro, M., McClintock, J., McHardy, I., Mendez, M., Mereghetti, S., Miller, M. C., Mineo, T., Morelli, E., Morsink, S., Motch, C., Motta, S., Muñoz-Darias, T., Naletto, G., Neustroev, V., Nevalainen, J., Olive, J. F., Orio, M., Orlandini, M., Orleanski, P., Ozel, F., Pacciani, L., Paltani, S., Papadakis, I., Papitto, A., Patruno, A., Pellizzoni, A., Petráček, V., Petri, J., Petrucci, P. O., Phlips, B., Picolli, L., Possenti, A., Psaltis, D., Rambaud, D., Reig, P., Remillard, R., Rodriguez, J., Romano, P., Romanova, M., Schanz, T., Schmid, C., Segreto, A., Shearer, A., Smith, A., Smith, P. J., Soffitta, P., Stergioulas, N., Stolarski, M., Stuchlik, Z., Tiengo, A., Torres, D., Török, G., Turolla, R., Uttley, P., Vaughan, S., Vercellone, S., Waters, R., Watts, A., Wawrzaszek, R., Webb, N., Wilms, J., Zampieri, L., Zezas, A., and Ziolkowski, J.

Published
2012
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39. EDGE: Explorer of diffuse emission and gamma-ray burst explosions

Author

Piro, L., den Herder, J. W., Ohashi, T., Amati, L., Atteia, J. L., Barthelmy, S., Barbera, M., Barret, D., Basso, S., Boer, M., Borgani, S., Boyarskiy, O., Branchini, E., Branduardi-Raymont, G., Briggs, M., Brunetti, G., Budtz-Jorgensen, C., Burrows, D., Campana, S., Caroli, E., Chincarini, G., Christensen, F., Cocchi, M., Comastri, A., Corsi, A., Cotroneo, V., Conconi, P., Colasanti, L., Cusumano, G., de Rosa, A., Del Santo, M., Ettori, S., Ezoe, Y., Ferrari, L., Feroci, M., Finger, M., Fishman, G., Fujimoto, R., Galeazzi, M., Galli, A., Gatti, F., Gehrels, N., Gendre, B., Ghirlanda, G., Ghisellini, G., Giommi, P., Girardi, M., Guzzo, L., Haardt, F., Hepburn, I., Hermsen, W., Hoevers, H., Holland, A., in’t Zand, J., Ishisaki, Y., Kawahara, H., Kawai, N., Kaastra, J., Kippen, M., de Korte, P. A. J., Kouveliotou, C., Kusenko, A., Labanti, C., Lieu, R., Macculi, C., Makishima, K., Matt, G., Mazzotta, P., McCammon, D., Méndez, M., Mineo, T., Mitchell, S., Mitsuda, K., Molendi, S., Moscardini, L., Mushotzky, R., Natalucci, L., Nicastro, F., O’Brien, P., Osborne, J., Paerels, F., Page, M., Paltani, S., Pareschi, G., Perinati, E., Perola, C., Ponman, T., Rasmussen, A., Roncarelli, M., Rosati, P., Ruchayskiy, O., Quadrini, E., Sakurai, I., Salvaterra, R., Sasaki, S., Sato, G., Schaye, J., Schmitt, J., Sciortino, S., Shaposhnikov, M., Shinozaki, K., Spiga, D., Suto, Y., Tagliaferri, G., Takahashi, T., Takei, Y., Tawara, Y., Tozzi, P., Tsunemi, H., Tsuru, T., Ubertini, P., Ursino, E., Viel, M., Vink, J., White, N., Willingale, R., Wijers, R., Yoshikawa, K., and Yamasaki, N.

Published
2009
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40. EURECA: European-Japanese Microcalorimeter Array

Author

de Korte, P., Anquita, J., Bakker, F., Barcons, X., Bastia, P., Beyer, J., Boersma, D., Briones, F., Bruijn, M., Bussons, J., Camòn, A., Carrera, F., Ceballos, M., Colasanti, L., Drung, D., Fabrega, L., Ferrari, L., Gatti, F., Gonzalez-Arrabal, R., Gottardi, L., Hajdas, W., Helistö, P., den Herder, J. W., Hoevers, H., Ishisaki, Y., Kiviranta, M., van der Kuur, J., Macculi, C., Mchedlishvili, A., Mitsuda, K., Monna, B., Mossel, R., Ohashi, T., Pantali, S., Parra, M., Piro, L., Rohlfs, R., Sésé, J., Takei, Y., Torrioli, G., van Weers, H., and Yamasaki, N.

Published
2008
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41. Frequency shift algorithm: Application to a frequency-domain multiplexing readout of x-ray transition-edge sensor microcalorimeters

Author

Vaccaro, D., primary, Akamatsu, H., additional, van der Kuur, J., additional, van der Hulst, P., additional, Nieuwenhuizen, A. C. T., additional, van Winden, P., additional, Gottardi, L., additional, den Hartog, R., additional, Bruijn, M. P., additional, D’Andrea, M., additional, Gao, J. R., additional, den Herder, J. W. A., additional, Hoogeveen, R. W. M., additional, Jackson, B., additional, van der Linden, A. J., additional, Nagayoshi, K., additional, Ravensberg, K., additional, Ridder, M. L., additional, Taralli, E., additional, and de Wit, M., additional

Published
2021
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42. Study of TES Detector Transition Curve to Optimize the Pixel Design for Frequency-Division Multiplexing Readout

Author

Ridder, M. L. (author), Nagayoshi, K. (author), Bruijn, M. P. (author), Gottardi, L. (author), Taralli, E. (author), Khosropanah, P. (author), Akamatsu, H. (author), van der Kuur, J. (author), Ravensberg, K. (author), Visser, S. (author), Nieuwenhuizen, A. C.T. (author), Gao, J. (author), den Herder, J. W. (author), Ridder, M. L. (author), Nagayoshi, K. (author), Bruijn, M. P. (author), Gottardi, L. (author), Taralli, E. (author), Khosropanah, P. (author), Akamatsu, H. (author), van der Kuur, J. (author), Ravensberg, K. (author), Visser, S. (author), Nieuwenhuizen, A. C.T. (author), Gao, J. (author), and den Herder, J. W. (author)

Abstract

Superconducting transition-edge sensors (TESs) are highly sensitive detectors. Based on the outstanding performance on spectral resolution, the X-ray integral field unit (X-IFU) instrument on-board athena will be equipped with a large array of TES-based microcalorimeters. For optimal performance in terms of the energy resolution, it is essential to limit undesirable nonlinearity effects in the TES detector. Weak-link behavior induced on the TES by superconducting leads is such a nonlinearity effect. We designed and fabricated smart test structures to study the effect of the superconducting leads on the intrinsic transition curve of our TiAu-based TES bilayer. We measured and analyzed the resistance versus temperature transition curves of the test structures. We found relations of long-distance proximity effects with TES length and different lead materials. Based on these results, we can redesign and further optimize our TES-based X-ray detectors., Accepted Author Manuscript, ImPhys/Optics

Published
2020
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44. Low-noise microwave SQUID multiplexed readout of 38 x-ray transition-edge sensor microcalorimeters

Author

Nakashima, Y., primary, Hirayama, F., additional, Kohjiro, S., additional, Yamamori, H., additional, Nagasawa, S., additional, Sato, A., additional, Yamada, S., additional, Hayakawa, R., additional, Yamasaki, N. Y., additional, Mitsuda, K., additional, Nagayoshi, K., additional, Akamatsu, H., additional, Gottardi, L., additional, Taralli, E., additional, Bruijn, M. P., additional, Ridder, M. L., additional, Gao, J. R., additional, and den Herder, J. W. A., additional

Published
2020
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47. Design of the detection chain for Athena X-IFU

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Geoffray, H., Jackson, B. D., Bandler, S. R., Smith, S. J., Doriese, W. B., Durkin, M., van der Kuur, J., van Leeuwen, B.-J., Kiviranta, M., Prêle, D., Ravera, L., Parot, Y., van Weers, H., den Herder, J. W., Adams, J., Chervenak, J. A., Reintsema, C. D., Ullom, J. N., Brachet, F., Ledot, A., Peille, P., and Barret, D.

Published
2022
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48. The LOFT mission: new perspectives in the research field of (accreting) compact objects

Author

Bozzo E., Stella L., van der Klis M., Watts A., Barret D., Wilms J., Uttley P., den Herder J. W., and Feroci M.

Subjects
Physics, QC1-999
Abstract

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 the first time a huge collecting area for the detection of X-ray photons with CCD-quality spectral resolution (15 times bigger in area than any previously flown X-ray instrument and >100 times bigger for spectroscopy than any similar-resolution instrument), the instruments onboard LOFT have been designed to (i) determine the properties of ultradense matter by reconstructing its Equation of State through neutron star mass and radius measurements of unprecedented accuracy; (ii) measure General Relativity effects in the strong field regime in the stationary spacetimes of neutron stars and black holes of all masses down to a few gravitational radii. Besides the above two themes, LOFT’s observations will be devoted to “observatory science”, providing new insights in a number of research fields in high energy astrophysics (e.g. Gamma-ray Bursts). The assessment study phase of LOFT, which ended in September 2013, demonstrated that the mission is low risk and the required Technology Readiness Level can be easily reached in time for a launch by the end of 2022.

Published
2014
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50. Atmospheric gas dynamics in the Perseus cluster observed with Hitomi*

Author

Aharonia, F., Aharonian, F., Akamatsu, H., Akimoto, F., Allen, S. W., Angelini, L., Audard, M., Awaki, H., Axelsson, M., Bamba, A., Bautz, M. W., Blandford, R., Brenneman, L. W., Brown, G. V., Bulbul, E., Cackett, E. M., Canning, R. E. A., Chernyakova, M., Chiao, M. P., Coppi, P. S., Costantini, E., Plaa, J., Vries, C. P., Den Herder, J. -W, Done, C., Dotani, T., Ebisawa, K., Eckart, M. E., Enoto, T., Ezoe, Y., Fabian, A. C., Ferrigno, C., Foster, A. R., Fujimoto, R., Fukazawa, Y., Furuzawa, A., Galeazzi, M., Gallo, L. C., Gandhi, P., Giustini, M., Goldwurm, A., Gu, L., Guainazzi, M., Haba, Y., Hagino, K., Hamaguchi, K., Harrus, I. M., Hatsukade, I., Hayashi, K., Hayashi, T., Hayashida, K., Hiraga, J. S., Hornschemeier, A., Hoshino, A., Hughes, J. P., Ichinohe, Y., Iizuka, R., Inoue, H., Inoue, S., Inoue, Y., Ishida, M., Ishikawa, K., Ishisaki, Y., Iwai, M., Kaastra, J., Kallman, T., Kamae, T., Kataoka, J., Katsuda, S., Kawai, N., Kelley, R. L., Kilbourne, C. A., Kitaguchi, T., Kitamoto, S., Kitayama, T., Kohmura, T., Kokubun, M., Koyama, K., Koyama, S., Kretschmar, P., Krimm, H. A., Kubota, A., Kunieda, H., Laurent, P., Lee, S. -H, Leutenegger, M. A., Limousin, O., Loewenstein, M., Long, K. S., Lumb, D., Madejski, G., Maeda, Y., Maier, D., Makishima, K., Markevitch, M., Matsumoto, H., Kyoko Matsushita, Mccammon, D., Mcnamara, B. R., Mehdipour, M., Miller, E. D., Miller, J. M., Mineshige, S., Mitsuda, K., Mitsuishi, I., Miyazawa, T., Mizuno, T., Mori, H., Mori, K., Mukai, K., Murakami, H., Mushotzky, R. F., Nakagawa, T., Nakajima, H., Nakamori, T., Nakashima, S., Nakazawa, K., Nobukawa, K. K., Nobukawa, M., Noda, H., Odaka, H., Ohashi, T., Ohno, M., Okajima, T., Ota, N., Ozaki, M., Paerels, F., Paltani, S., Petre, R., Pinto, C., Porter, F. S., Pottschmidt, K., Reynolds, C. S., Safi-Harb, S., Saito, S., Sakai, K., Sasaki, T., Sato, G., Sato, K., Sato, R., Sawada, M., Schartel, N., Serlemtsos, P. J., Seta, H., Shidatsu, M., Simionescu, A., Smith, R. K., Soong, Y., Stawarz, Ł., Sugawara, Y., Sugita, S., Szymkowiak, A., Tajima, H., Takahashi, H., Takahashi, T., Takeda, S., Takei, Y., Amagawa, T. T., Tamura, T., Tanaka, K., Tanaka, T., Tanaka, Y., Tanaka, Y. T., Tashiro, M. S., Tawara, Y., Terada, Y., Erashima, Y. T., Tombesi, F., Tomida, H., Tsuboi, Y., Tsujimoto, M., Tsunemi, H., Tsuru, T. G., Uchida, H., Uchiyama, H., Uchiyama, Y., Ueda, S., Ueda, Y., Uno, S., Urry, C. M., Ursino, E., Wang, Q. H. S., Watanabe, S., Werner, N., Wilkins, D. R., Williams, B. J., Yamada, S., Yamaguchi, H., Yamaoka, K., Yamasaki, N. Y., Yamauchi, M., Yamauchi, S., Yaqoob, T., Yatsu, Y., Yonetoku, D., Zhuravleva, I., Zoghbi, A., AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Hitomi, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), and Commissariat à l'énergie atomique et aux énergies alternatives ( CEA )

Subjects
galaxies: clusters: individual, galaxies: clusters: intracluster medium, Active galactic nucleus, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], individual (NGC 1275) [galaxies], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, galaxies: individual, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, clusters: individual (Perseus) [galaxies], 01 natural sciences, Intracluster medium, 0103 physical sciences, Emission spectrum, Brightest cluster galaxy, 010303 astronomy & astrophysics, STFC, Astrophysics::Galaxy Astrophysics, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Settore FIS/05, 010308 nuclear & particles physics, Velocity gradient, RCUK, Velocity dispersion, Astronomy and Astrophysics, Redshift, ST/J003697/2, clusters: intracluster medium [galaxies], Space and Planetary Science, X-rays: galaxies: clusters, Electron temperature, galaxies: clusters [X-rays], ST/L00075X/1, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

著者人数: Hitomi Collaboration 197名（所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 堂谷, 忠靖; 海老沢, 研; 林, 克洋; 林, 佑; 飯塚, 亮; 井上, 芳幸; 石田, 学; 石川, 久美; 岩井, 将親; 国分, 紀秀; 小山, 志勇; 前田, 良知; 満田, 和久; 中川, 貴雄; 尾崎, 正伸; 佐藤, 悟郎; 佐藤, 理江; Simionescu, Aurora; 菅原, 泰晴; 高橋, 忠幸; 竹井, 洋; 田村, 隆幸; 田中, 靖郎; 冨田, 洋; 辻本, 匡弘; 上田, 周太朗; 渡辺, 伸; 山崎, 典子）, Number of authors: Hitomi Collaboration 197 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS): Dotani, Tadayasu; Ebisawa, Ken; Hayashi, Katsuhiro; Hayashi, Tasuku; Iizuka, Ryo; Inoue, Yoshiyuki; Ishida, Manabu; Ishikawa, Kumi; Iwai, Masachika; Kokubun, Motohide; Koyama, Shu; Maeda, Yoshitomo; Mitsuda, Kazuhisa; Nakagawa, Takao; Ozaki, Masanobu; Sato, Goro; Sato, Rie; Simionescu, Aurora; Sugawara, Yasuharu; Takahashi, Tadayuki; Takei, Yoh; Tamura, Takayuki; Tanaka, Yasuo; Tomida, Hiroshi; Tsujimoto, Masahiro; Ueda, Shutaro; Watanabe, Shin; Yamasaki, Noriko Y.), Accepted: 201710-31, 資料番号: SA1170334000

Published
2018

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