Published 2016 | Version v1
Publication

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

Barret, Didier
Lam Trong, Thien
Den Herder, Jan-Willem
Piro, Luigi
Barcons, Xavier
Huovelin, Juhani
Kelley, Richard
Mas-Hesse, J. Miguel
Mitsuda, Kazuhisa
Paltani, Stéphane
Rauw, Gregor
Rozanska, Agata
Wilms, Joern
Barbera, Marco
Bozzo, Enrico
Ceballos, Maria Teresa
Charles, Ivan
Decourchelle, Anne
Den Hartog, Roland
Duval, Jean-Marc
Fiore, Fabrizio
Gatti, Flavio
Goldwurm, Andrea
Jackson, Brian
Jonker, Peter
Kilbourne, Caroline
Macculi, Claudio
Mendez, Mariano
Molendi, Silvano
Orleanski, Piotr
Pajot, François
Pointecouteau, Etienne
Porter, Frederick
Pratt, Gabriel W.
Prêle, Damien
Ravera, Laurent
Renotte, Etienne
Schaye, Joop
Shinozaki, Keisuke
Valenziano, Luca
Vink, Jacco
Webb, Natalie
Yamasaki, Noriko
Delcelier-Douchin, Françoise
Le Du, Michel
Mesnager, Jean-Michel
Pradines, Alice
Branduardi-Raymont, Graziella
Dadina, Mauro
Finoguenov, Alexis
Fukazawa, Yasushi
Janiuk, Agnieszka
Miller, Jon
Nazé, Yaël
Nicastro, Fabrizio
Sciortino, Salvatore
Torrejon, Jose Miguel
Geoffray, Hervé
Hernandez, Isabelle
Luno, Laure
Peille, Philippe
André, Jérôme
Daniel, Christophe
Etcheverry, Christophe
Gloaguen, Emilie
Hassin, Jérémie
Hervet, Gilles
Maussang, Irwin
Moueza, Jérôme
Paillet, Alexis
Vella, Bruno
Campos Garrido, Gonzalo
Damery, Jean-Charles
Panem, Chantal
Panh, Johan
Bandler, Simon
Biffi, Jean-Marc
Boyce, Kevin
Clénet, Antoine
DiPirro, Michael
Jamotton, Pierre
Lotti, Simone
Schwander, Denis
Smith, Stephen
Van Leeuwen, Bert-Joost
Van Weers, Henk
Brand, Thorsten
Cobo, Beatriz
Dauser, Thomas
De Plaa, Jelle
Cucchetti, Edoardo
Others:
Jan-Willem A. den Herder, Tadayuki Takahashi, Marshall Bautz
Barret, Didier
Lam Trong, Thien
Den Herder, Jan-Willem
Piro, Luigi
Barcons, Xavier
Huovelin, Juhani
Kelley, Richard
Mas-Hesse, J. Miguel
Mitsuda, Kazuhisa
Paltani, Stéphane
Rauw, Gregor
Rozanska, Agata
Wilms, Joern
Barbera, Marco
Bozzo, Enrico
Ceballos, Maria Teresa
Charles, Ivan
Decourchelle, Anne
Den Hartog, Roland
Duval, Jean-Marc
Fiore, Fabrizio
Gatti, Flavio
Goldwurm, Andrea
Jackson, Brian
Jonker, Peter
Kilbourne, Caroline
Macculi, Claudio
Mendez, Mariano
Molendi, Silvano
Orleanski, Piotr
Pajot, Françoi
Pointecouteau, Etienne
Porter, Frederick
Pratt, Gabriel W.
Prêle, Damien
Ravera, Laurent
Renotte, Etienne
Schaye, Joop
Shinozaki, Keisuke
Valenziano, Luca
Vink, Jacco
Webb, Natalie
Yamasaki, Noriko
Delcelier-Douchin, Françoise
Le Du, Michel
Mesnager, Jean-Michel
Pradines, Alice
Branduardi-Raymont, Graziella
Dadina, Mauro
Finoguenov, Alexi
Fukazawa, Yasushi
Janiuk, Agnieszka
Miller, Jon
Nazé, Yaël
Nicastro, Fabrizio
Sciortino, Salvatore
Torrejon, Jose Miguel
Geoffray, Hervé
Hernandez, Isabelle
Luno, Laure
Peille, Philippe
André, Jérôme
Daniel, Christophe
Etcheverry, Christophe
Gloaguen, Emilie
Hassin, Jérémie
Hervet, Gille
Maussang, Irwin
Moueza, Jérôme
Paillet, Alexi
Vella, Bruno
Campos Garrido, Gonzalo
Damery, Jean-Charle
Panem, Chantal
Panh, Johan
Bandler, Simon
Biffi, Jean-Marc
Boyce, Kevin
Clénet, Antoine
Dipirro, Michael
Jamotton, Pierre
Lotti, Simone
Schwander, Deni
Smith, Stephen
Van Leeuwen, Bert-Joost
Van Weers, Henk
Brand, Thorsten
Cobo, Beatriz
Dauser, Thoma
De Plaa, Jelle
Cucchetti, Edoardo

Description

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 0.2 to 12 keV, with ∼ 5" pixels over a field of view of 5 arc minute equivalent diameter and a spectral resolution of 2.5 eV up to 7 keV. In this paper, we first review the core scientific objectives of Athena, driving the main performance parameters of the X-IFU, namely the spectral resolution, the field of view, the effective area, the count rate capabilities, the instrumental background. We also illustrate the breakthrough potential of the X-IFU for some observatory science goals. Then we brie y describe the X-IFU design as defined at the time of the mission consolidation review concluded in May 2016, and report on its predicted performance. Finally, we discuss some options to improve the instrument performance while not increasing its complexity and resource demands (e.g. count rate capability, spectral resolution).

Additional details

Created:
April 14, 2023
Modified:
November 30, 2023