The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP

Margarita Hernanz; Søren Brandt; Jeanint Zand; Yuri Evangelista; Aline Meuris; Chris Tenzer; Gianluigi Zampa; Piotr Orleanski; Emrah Kalemci; Müberra Sungur; Stéphane Schanne; Frans Zwart; Rob de la Rie; Phillip Laubert; Coen van Baren; Gabby Aitink-Kroes; Lucien Kuiper; Jörg Bayer; Paul Hedderman; Samuel Pliego; Hao Xiong; Riccardo Campana; Ettore del Monte; Marco Feroci; Francesco Ceraudo; Olivier Gevin; Irfan Kuvvetli; Denis Tcherniak; Konrad Skup; Malgorzata Michalska; Witold Nowosielski; Ander Hormaetxe; José Luis Gálvez; Patrícia Ferrés; Alessandro Patruno; Walter Bonvicini; Matias Antonelli; Mirko Boezio; Daniela Cirrincione; Riccardo Munini; Alexandre Rachevski; Andrea Vacchi; Nicola Zampa; Irina Rashevskaya; Andrea Argan; Onur Turhan; Ayhan Bozkurt; Ahmet Onat; Enrico Bozzo; Andrea Santangelo; Shuang Nan Zhang; Fangjun Lu; Yupeng Xu

doi:10.1117/12.2628335

The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP

Margarita Hernanz^*, Søren Brandt, Jeanint Zand, Yuri Evangelista, Aline Meuris, Chris Tenzer, Gianluigi Zampa, Piotr Orleanski, Emrah Kalemci, Müberra Sungur, Stéphane Schanne, Frans Zwart, Rob de la Rie, Phillip Laubert, Coen van Baren, Gabby Aitink-Kroes, Lucien Kuiper, Jörg Bayer, Paul Hedderman, Samuel PliegoHao Xiong, Riccardo Campana, Ettore del Monte, Marco Feroci, Francesco Ceraudo, Olivier Gevin, Irfan Kuvvetli, Denis Tcherniak, Konrad Skup, Malgorzata Michalska, Witold Nowosielski, Ander Hormaetxe, José Luis Gálvez, Patrícia Ferrés, Alessandro Patruno, Walter Bonvicini, Matias Antonelli, Mirko Boezio, Daniela Cirrincione, Riccardo Munini, Alexandre Rachevski, Andrea Vacchi, Nicola Zampa, Irina Rashevskaya, Andrea Argan, Onur Turhan, Ayhan Bozkurt, Ahmet Onat, Enrico Bozzo, Andrea Santangelo, Shuang Nan Zhang, Fangjun Lu, Yupeng Xu

^*Corresponding author for this work

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Abstract

The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS), with a large involvement of Europe. The scientific payload of eXTP includes four instruments: the SFA (Spectroscopy Focusing Array) and the PFA (Polarimetry Focusing Array) - led by China - the LAD (Large Area Detector) and the WFM (Wide Field Monitor) - led by Europe (Italy and Spain). They offer a unique simultaneous wide-band X-ray timing and polarimetry sensitivity. The WFM is a wide field X-ray monitor instrument in the 2-50 keV energy range, consisting of an array of six coded mask cameras with a field of view of 180ºx90ºat an angular resolution of 5 arcmin and 4 silicon drift detectors in each camera. Its unprecedented combination of large field of view and imaging down to 2 keV will allow eXTP to make important discoveries of the variable and transient X-ray sky and is essential in detecting transient black holes, that are part of the primary science goals of eXTP, so that they can be promptly followed up with other instruments on eXTP and elsewhere.

Original language	English
Title of host publication	Proceedings of SPIE : Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray
Editors	Jan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa
Number of pages	15
Publisher	SPIE - International Society for Optical Engineering
Publication date	2022
Article number	121811Y
ISBN (Electronic)	9781510653436
DOIs	https://doi.org/10.1117/12.2628335
Publication status	Published - 2022
Event	Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray - Montréal, Canada Duration: 17 Jul 2022 → 22 Jul 2022 https://spie.org/as/conferencedetails/space-telescopes-and-instrumentation-uv-to-gamma?SSO=1

Conference

Conference	Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray
Country/Territory	Canada
City	Montréal
Period	17/07/2022 → 22/07/2022
Internet address	https://spie.org/as/conferencedetails/space-telescopes-and-instrumentation-uv-to-gamma?SSO=1

Series	Proceedings of SPIE - The International Society for Optical Engineering
Volume	12181
ISSN	0277-786X

Keywords

Coded mask imaging
Compact objects: black holes
Gamma-ray bursts
Gravitational wave events
Neutron stars and white dwarfs
Silicon drift detectors
X-ray bursts
X-ray spectroscopy
X-ray timing

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Hernanz, M., Brandt, S., Zand, J., Evangelista, Y., Meuris, A., Tenzer, C., Zampa, G., Orleanski, P., Kalemci, E., Sungur, M., Schanne, S., Zwart, F., de la Rie, R., Laubert, P., van Baren, C., Aitink-Kroes, G., Kuiper, L., Bayer, J., Hedderman, P., ... Xu, Y. (2022). The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP. In J-W. A. den Herder, S. Nikzad, & K. Nakazawa (Eds.), Proceedings of SPIE: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray [121811Y] SPIE - International Society for Optical Engineering. Proceedings of SPIE - The International Society for Optical Engineering Vol. 12181 https://doi.org/10.1117/12.2628335

Hernanz, Margarita ; Brandt, Søren ; Zand, Jeanint et al. / The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP. Proceedings of SPIE: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray. editor / Jan-Willem A. den Herder ; Shouleh Nikzad ; Kazuhiro Nakazawa. SPIE - International Society for Optical Engineering, 2022. (Proceedings of SPIE - The International Society for Optical Engineering, Vol. 12181).

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abstract = "The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS), with a large involvement of Europe. The scientific payload of eXTP includes four instruments: the SFA (Spectroscopy Focusing Array) and the PFA (Polarimetry Focusing Array) - led by China - the LAD (Large Area Detector) and the WFM (Wide Field Monitor) - led by Europe (Italy and Spain). They offer a unique simultaneous wide-band X-ray timing and polarimetry sensitivity. The WFM is a wide field X-ray monitor instrument in the 2-50 keV energy range, consisting of an array of six coded mask cameras with a field of view of 180ºx90ºat an angular resolution of 5 arcmin and 4 silicon drift detectors in each camera. Its unprecedented combination of large field of view and imaging down to 2 keV will allow eXTP to make important discoveries of the variable and transient X-ray sky and is essential in detecting transient black holes, that are part of the primary science goals of eXTP, so that they can be promptly followed up with other instruments on eXTP and elsewhere.",

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author = "Margarita Hernanz and S{\o}ren Brandt and Jeanint Zand and Yuri Evangelista and Aline Meuris and Chris Tenzer and Gianluigi Zampa and Piotr Orleanski and Emrah Kalemci and M{\"u}berra Sungur and St{\'e}phane Schanne and Frans Zwart and {de la Rie}, Rob and Phillip Laubert and {van Baren}, Coen and Gabby Aitink-Kroes and Lucien Kuiper and J{\"o}rg Bayer and Paul Hedderman and Samuel Pliego and Hao Xiong and Riccardo Campana and {del Monte}, Ettore and Marco Feroci and Francesco Ceraudo and Olivier Gevin and Irfan Kuvvetli and Denis Tcherniak and Konrad Skup and Malgorzata Michalska and Witold Nowosielski and Ander Hormaetxe and G{\'a}lvez, {Jos{\'e} Luis} and Patr{\'i}cia Ferr{\'e}s and Alessandro Patruno and Walter Bonvicini and Matias Antonelli and Mirko Boezio and Daniela Cirrincione and Riccardo Munini and Alexandre Rachevski and Andrea Vacchi and Nicola Zampa and Irina Rashevskaya and Andrea Argan and Onur Turhan and Ayhan Bozkurt and Ahmet Onat and Enrico Bozzo and Andrea Santangelo and Zhang, {Shuang Nan} and Fangjun Lu and Yupeng Xu",

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doi = "10.1117/12.2628335",

language = "English",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE - International Society for Optical Engineering",

editor = "{den Herder}, {Jan-Willem A.} and Shouleh Nikzad and Kazuhiro Nakazawa",

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Hernanz, M, Brandt, S, Zand, J, Evangelista, Y, Meuris, A, Tenzer, C, Zampa, G, Orleanski, P, Kalemci, E, Sungur, M, Schanne, S, Zwart, F, de la Rie, R, Laubert, P, van Baren, C, Aitink-Kroes, G, Kuiper, L, Bayer, J, Hedderman, P, Pliego, S, Xiong, H, Campana, R, del Monte, E, Feroci, M, Ceraudo, F, Gevin, O, Kuvvetli, I , Tcherniak, D, Skup, K, Michalska, M, Nowosielski, W, Hormaetxe, A, Gálvez, JL, Ferrés, P, Patruno, A, Bonvicini, W, Antonelli, M, Boezio, M, Cirrincione, D, Munini, R, Rachevski, A, Vacchi, A, Zampa, N, Rashevskaya, I, Argan, A, Turhan, O, Bozkurt, A, Onat, A, Bozzo, E, Santangelo, A, Zhang, SN, Lu, F & Xu, Y 2022, The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP. in J-WA den Herder, S Nikzad & K Nakazawa (eds), Proceedings of SPIE: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray., 121811Y, SPIE - International Society for Optical Engineering, Proceedings of SPIE - The International Society for Optical Engineering, vol. 12181, Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray, Montréal, Quebec, Canada, 17/07/2022. https://doi.org/10.1117/12.2628335

The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP. / Hernanz, Margarita; Brandt, Søren; Zand, Jeanint et al.

Proceedings of SPIE: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray. ed. / Jan-Willem A. den Herder; Shouleh Nikzad; Kazuhiro Nakazawa. SPIE - International Society for Optical Engineering, 2022. 121811Y (Proceedings of SPIE - The International Society for Optical Engineering, Vol. 12181).

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

TY - GEN

T1 - The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP

AU - Hernanz, Margarita

AU - Brandt, Søren

AU - Zand, Jeanint

AU - Evangelista, Yuri

AU - Meuris, Aline

AU - Tenzer, Chris

AU - Zampa, Gianluigi

AU - Orleanski, Piotr

AU - Kalemci, Emrah

AU - Sungur, Müberra

AU - Schanne, Stéphane

AU - Zwart, Frans

AU - de la Rie, Rob

AU - Laubert, Phillip

AU - van Baren, Coen

AU - Aitink-Kroes, Gabby

AU - Kuiper, Lucien

AU - Bayer, Jörg

AU - Hedderman, Paul

AU - Pliego, Samuel

AU - Xiong, Hao

AU - Campana, Riccardo

AU - del Monte, Ettore

AU - Feroci, Marco

AU - Ceraudo, Francesco

AU - Gevin, Olivier

AU - Kuvvetli, Irfan

AU - Tcherniak, Denis

AU - Skup, Konrad

AU - Michalska, Malgorzata

AU - Nowosielski, Witold

AU - Hormaetxe, Ander

AU - Gálvez, José Luis

AU - Ferrés, Patrícia

AU - Patruno, Alessandro

AU - Bonvicini, Walter

AU - Antonelli, Matias

AU - Boezio, Mirko

AU - Cirrincione, Daniela

AU - Munini, Riccardo

AU - Rachevski, Alexandre

AU - Vacchi, Andrea

AU - Zampa, Nicola

AU - Rashevskaya, Irina

AU - Argan, Andrea

AU - Turhan, Onur

AU - Bozkurt, Ayhan

AU - Onat, Ahmet

AU - Bozzo, Enrico

AU - Santangelo, Andrea

AU - Zhang, Shuang Nan

AU - Lu, Fangjun

AU - Xu, Yupeng

PY - 2022

Y1 - 2022

N2 - The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS), with a large involvement of Europe. The scientific payload of eXTP includes four instruments: the SFA (Spectroscopy Focusing Array) and the PFA (Polarimetry Focusing Array) - led by China - the LAD (Large Area Detector) and the WFM (Wide Field Monitor) - led by Europe (Italy and Spain). They offer a unique simultaneous wide-band X-ray timing and polarimetry sensitivity. The WFM is a wide field X-ray monitor instrument in the 2-50 keV energy range, consisting of an array of six coded mask cameras with a field of view of 180ºx90ºat an angular resolution of 5 arcmin and 4 silicon drift detectors in each camera. Its unprecedented combination of large field of view and imaging down to 2 keV will allow eXTP to make important discoveries of the variable and transient X-ray sky and is essential in detecting transient black holes, that are part of the primary science goals of eXTP, so that they can be promptly followed up with other instruments on eXTP and elsewhere.

AB - The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS), with a large involvement of Europe. The scientific payload of eXTP includes four instruments: the SFA (Spectroscopy Focusing Array) and the PFA (Polarimetry Focusing Array) - led by China - the LAD (Large Area Detector) and the WFM (Wide Field Monitor) - led by Europe (Italy and Spain). They offer a unique simultaneous wide-band X-ray timing and polarimetry sensitivity. The WFM is a wide field X-ray monitor instrument in the 2-50 keV energy range, consisting of an array of six coded mask cameras with a field of view of 180ºx90ºat an angular resolution of 5 arcmin and 4 silicon drift detectors in each camera. Its unprecedented combination of large field of view and imaging down to 2 keV will allow eXTP to make important discoveries of the variable and transient X-ray sky and is essential in detecting transient black holes, that are part of the primary science goals of eXTP, so that they can be promptly followed up with other instruments on eXTP and elsewhere.

KW - Coded mask imaging

KW - Compact objects: black holes

KW - Gamma-ray bursts

KW - Gravitational wave events

KW - Neutron stars and white dwarfs

KW - Silicon drift detectors

KW - X-ray bursts

KW - X-ray spectroscopy

KW - X-ray timing

U2 - 10.1117/12.2628335

DO - 10.1117/12.2628335

M3 - Article in proceedings

AN - SCOPUS:85140491886

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Proceedings of SPIE

A2 - den Herder, Jan-Willem A.

A2 - Nikzad, Shouleh

A2 - Nakazawa, Kazuhiro

PB - SPIE - International Society for Optical Engineering

T2 - Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray

Y2 - 17 July 2022 through 22 July 2022

ER -

Hernanz M, Brandt S, Zand J, Evangelista Y, Meuris A, Tenzer C et al. The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP. In den Herder J-WA, Nikzad S, Nakazawa K, editors, Proceedings of SPIE: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray. SPIE - International Society for Optical Engineering. 2022. 121811Y. (Proceedings of SPIE - The International Society for Optical Engineering, Vol. 12181). doi: 10.1117/12.2628335

The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP

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