eROSITA on SRG

Peter Predehl; Hans Böhringer; Hermann Brunner; Marcella Brusa; Vadim Burwitz; Nico Cappelluti; Evgeniy Churazov; Konrad Dennerl; Michael Freyberg; Peter Friedrich; Günther Hasinger; Eckhard Kendziorra; Ingo Kreykenbohm; Christian Schmid; Jörn Wilms; Georg Lamer; Norbert Meidinger; Martin Mühlegger; Mikhail Pavlinsky; Jan Robrade; Andrea Santangelo; Jürgen Schmitt; Axel Schwope; Matthias Steinmetz; Lothar Strüder; Rashid Sunyaev; Chris Tenzer

doi:10.1063/1.3475336

eROSITA on SRG

Peter Predehl, Hans Böhringer, Hermann Brunner, Marcella Brusa, Vadim Burwitz, Nico Cappelluti, Evgeniy Churazov, Konrad Dennerl, Michael Freyberg, Peter Friedrich, Günther Hasinger, Eckhard Kendziorra, Ingo Kreykenbohm, Christian Schmid, Jörn Wilms, Georg Lamer, Norbert Meidinger, Martin Mühlegger, Mikhail Pavlinsky, Jan RobradeAndrea Santangelo, Jürgen Schmitt, Axel Schwope, Matthias Steinmetz, Lothar Strüder, Rashid Sunyaev, Chris Tenzer

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

17 Scopus citations

Abstract

eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the core instrument on the Russian Spektrum-Roentgen-Gamma (SRG) mission which is scheduled for launch in late 2012. eROSITA is fully approved and funded by the German Space Agency DLR and the Max-Planck-Society. The design driving science is the detection of 50-100 thousands Clusters of Galaxies up to redshift z∼1.3 in order to study the large scale structure in the Universe and test cosmological models, especially Dark Energy. This will be accomplished by an all-sky survey lasting for four years plus a phase of pointed observations. eROSITA consists of seven Wolter-I telescope modules, each equipped with 54 Wolter-I shells having an outer diameter of 360 mm. This would provide and effective area at 1.5 keV of ∼1500cm² and an on axis PSF HEW of 15″ which would provide an effective angular resolution of 25″-30″. In the focus of each mirror module, a fast frame-store pn-CCD will provide a field of view of 1° in diameter for an active FOV of ∼0.83deg². At the time of writing the instrument development is currently in phase C/D.

Original language	English (US)
Title of host publication	X-ray Astronomy-2009
Subtitle of host publication	Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference
Publisher	American Institute of Physics Inc.
Pages	543-548
Number of pages	6
ISBN (Print)	9780735407954
DOIs	https://doi.org/10.1063/1.3475336
State	Published - 2010
Externally published	Yes
Event	International Conference on X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Bologna, Italy Duration: Sep 7 2009 → Sep 11 2009

Publication series

Name	AIP Conference Proceedings
Volume	1248
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	International Conference on X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives
Country	Italy
City	Bologna
Period	9/7/09 → 9/11/09

Keywords

All-sky Survey
Dark Energy
X-ray astronomy

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1063/1.3475336

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Predehl, P., Böhringer, H., Brunner, H., Brusa, M., Burwitz, V., Cappelluti, N., Churazov, E., Dennerl, K., Freyberg, M., Friedrich, P., Hasinger, G., Kendziorra, E., Kreykenbohm, I., Schmid, C., Wilms, J., Lamer, G., Meidinger, N., Mühlegger, M., Pavlinsky, M., ... Tenzer, C. (2010). eROSITA on SRG. In X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference (pp. 543-548). (AIP Conference Proceedings; Vol. 1248). American Institute of Physics Inc.. https://doi.org/10.1063/1.3475336

eROSITA on SRG. / Predehl, Peter; Böhringer, Hans; Brunner, Hermann; Brusa, Marcella; Burwitz, Vadim; Cappelluti, Nico; Churazov, Evgeniy; Dennerl, Konrad; Freyberg, Michael; Friedrich, Peter; Hasinger, Günther; Kendziorra, Eckhard; Kreykenbohm, Ingo; Schmid, Christian; Wilms, Jörn; Lamer, Georg; Meidinger, Norbert; Mühlegger, Martin; Pavlinsky, Mikhail; Robrade, Jan; Santangelo, Andrea; Schmitt, Jürgen; Schwope, Axel; Steinmetz, Matthias; Strüder, Lothar; Sunyaev, Rashid; Tenzer, Chris.

X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference. American Institute of Physics Inc., 2010. p. 543-548 (AIP Conference Proceedings; Vol. 1248).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Predehl, P, Böhringer, H, Brunner, H, Brusa, M, Burwitz, V, Cappelluti, N, Churazov, E, Dennerl, K, Freyberg, M, Friedrich, P, Hasinger, G, Kendziorra, E, Kreykenbohm, I, Schmid, C, Wilms, J, Lamer, G, Meidinger, N, Mühlegger, M, Pavlinsky, M, Robrade, J, Santangelo, A, Schmitt, J, Schwope, A, Steinmetz, M, Strüder, L, Sunyaev, R & Tenzer, C 2010, eROSITA on SRG. in X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference. AIP Conference Proceedings, vol. 1248, American Institute of Physics Inc., pp. 543-548, International Conference on X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives, Bologna, Italy, 9/7/09. https://doi.org/10.1063/1.3475336

Predehl, Peter ; Böhringer, Hans ; Brunner, Hermann ; Brusa, Marcella ; Burwitz, Vadim ; Cappelluti, Nico ; Churazov, Evgeniy ; Dennerl, Konrad ; Freyberg, Michael ; Friedrich, Peter ; Hasinger, Günther ; Kendziorra, Eckhard ; Kreykenbohm, Ingo ; Schmid, Christian ; Wilms, Jörn ; Lamer, Georg ; Meidinger, Norbert ; Mühlegger, Martin ; Pavlinsky, Mikhail ; Robrade, Jan ; Santangelo, Andrea ; Schmitt, Jürgen ; Schwope, Axel ; Steinmetz, Matthias ; Strüder, Lothar ; Sunyaev, Rashid ; Tenzer, Chris. / eROSITA on SRG. X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference. American Institute of Physics Inc., 2010. pp. 543-548 (AIP Conference Proceedings).

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author = "Peter Predehl and Hans B{\"o}hringer and Hermann Brunner and Marcella Brusa and Vadim Burwitz and Nico Cappelluti and Evgeniy Churazov and Konrad Dennerl and Michael Freyberg and Peter Friedrich and G{\"u}nther Hasinger and Eckhard Kendziorra and Ingo Kreykenbohm and Christian Schmid and J{\"o}rn Wilms and Georg Lamer and Norbert Meidinger and Martin M{\"u}hlegger and Mikhail Pavlinsky and Jan Robrade and Andrea Santangelo and J{\"u}rgen Schmitt and Axel Schwope and Matthias Steinmetz and Lothar Str{\"u}der and Rashid Sunyaev and Chris Tenzer",

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AU - Predehl, Peter

AU - Böhringer, Hans

AU - Brunner, Hermann

AU - Brusa, Marcella

AU - Burwitz, Vadim

AU - Cappelluti, Nico

AU - Churazov, Evgeniy

AU - Dennerl, Konrad

AU - Freyberg, Michael

AU - Friedrich, Peter

AU - Hasinger, Günther

AU - Kendziorra, Eckhard

AU - Kreykenbohm, Ingo

AU - Schmid, Christian

AU - Wilms, Jörn

AU - Lamer, Georg

AU - Meidinger, Norbert

AU - Mühlegger, Martin

AU - Pavlinsky, Mikhail

AU - Robrade, Jan

AU - Santangelo, Andrea

AU - Schmitt, Jürgen

AU - Schwope, Axel

AU - Steinmetz, Matthias

AU - Strüder, Lothar

AU - Sunyaev, Rashid

AU - Tenzer, Chris

PY - 2010

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N2 - eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the core instrument on the Russian Spektrum-Roentgen-Gamma (SRG) mission which is scheduled for launch in late 2012. eROSITA is fully approved and funded by the German Space Agency DLR and the Max-Planck-Society. The design driving science is the detection of 50-100 thousands Clusters of Galaxies up to redshift z∼1.3 in order to study the large scale structure in the Universe and test cosmological models, especially Dark Energy. This will be accomplished by an all-sky survey lasting for four years plus a phase of pointed observations. eROSITA consists of seven Wolter-I telescope modules, each equipped with 54 Wolter-I shells having an outer diameter of 360 mm. This would provide and effective area at 1.5 keV of ∼1500cm2 and an on axis PSF HEW of 15″ which would provide an effective angular resolution of 25″-30″. In the focus of each mirror module, a fast frame-store pn-CCD will provide a field of view of 1° in diameter for an active FOV of ∼0.83deg2. At the time of writing the instrument development is currently in phase C/D.

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