Studying the evolution of the hot universe with the X-ray evolving universe spectroscopy mission - XEUS

A. N. Parmar; G. Hasinger; M. Arnaud; X. Barcons; D. Barret; H. Böhringer; A. Blanchard; M. Cappi; A. Comastri; T. Courvoisier; A. C. Fabian; F. Fiore; I. Georgantopoulos; P. Grandi; R. Griffiths; A. Hornstrup; N. Kawai; K. Koyama; K. Makishima; G. Malaguti; K. O. Mason; C. Motch; M. Mendez; T. Ohashi; F. Paerels; L. Piro; T. Ponman; J. Schmitt; S. Sciortino; G. Trinchieri; M. van der Klis; M. Ward

doi:10.1016/j.asr.2003.02.067

Studying the evolution of the hot universe with the X-ray evolving universe spectroscopy mission - XEUS

A. N. Parmar, G. Hasinger, M. Arnaud, X. Barcons, D. Barret, H. Böhringer, A. Blanchard, M. Cappi, A. Comastri, T. Courvoisier, A. C. Fabian, F. Fiore, I. Georgantopoulos, P. Grandi, R. Griffiths, A. Hornstrup, N. Kawai, K. Koyama, K. Makishima, G. MalagutiK. O. Mason, C. Motch, M. Mendez, T. Ohashi, F. Paerels, L. Piro, T. Ponman, J. Schmitt, S. Sciortino, G. Trinchieri, M. van der Klis, M. Ward

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2 Citaten (Scopus)

Samenvatting

Europe is one of the major partners building the International Space Station (ISS) and European industry, together with ESA, is responsible for many station components including the Columbus Orbital Facility, the Automated Transport Vehicle, two connecting modules and the European Robotic Arm. Together with this impressive list of contributions there is a strong desire within the ESA Member States to benefit from this investment by utilizing the unique capabilities of the ISS to perform world-class science. XEUS is one of the astronomical applications being studied by ESA to utilize the capabilities of the ISS. XEUS will be a long-term X-ray observatory with an initial mirror area of 6 m 2 at 1 keV that will be expanded to 30 m 2 following a visit to the ISS. The 1 keV spatial resolution is expected to be 2-5″ half-energy-width. XEUS will consist of separate detector and mirror spacecraft (MSC) aligned by active control to provide a focal length of 50 m. A new detector spacecraft, complete with the next generation of instruments, will also be added after visiting the ISS. The limiting 0.1-2.5 keV sensitivity will then be 4 × 10 -18 erg cm -2 s -1, around 200 times better than XMM-Newton, allowing XEUS to study the properties of the hot baryons and dark matter at high redshift.

Originele taal-2	English
Pagina's (van-tot)	2623-2627
Tijdschrift	Advances in space research
Volume	34
Nummer van het tijdschrift	12
DOI's	https://doi.org/10.1016/j.asr.2003.02.067
Status	Published - 1-jan.-2004
Extern gepubliceerd	Ja

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10.1016/j.asr.2003.02.067

http://adsabs.harvard.edu/abs/2004AdSpR..34.2623P

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Parmar, A. N., Hasinger, G., Arnaud, M., Barcons, X., Barret, D., Böhringer, H., Blanchard, A., Cappi, M., Comastri, A., Courvoisier, T., Fabian, A. C., Fiore, F., Georgantopoulos, I., Grandi, P., Griffiths, R., Hornstrup, A., Kawai, N., Koyama, K., Makishima, K., ... Ward, M. (2004). Studying the evolution of the hot universe with the X-ray evolving universe spectroscopy mission - XEUS. Advances in space research, 34(12), 2623-2627. https://doi.org/10.1016/j.asr.2003.02.067

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title = "Studying the evolution of the hot universe with the X-ray evolving universe spectroscopy mission - XEUS",

abstract = "Europe is one of the major partners building the International Space Station (ISS) and European industry, together with ESA, is responsible for many station components including the Columbus Orbital Facility, the Automated Transport Vehicle, two connecting modules and the European Robotic Arm. Together with this impressive list of contributions there is a strong desire within the ESA Member States to benefit from this investment by utilizing the unique capabilities of the ISS to perform world-class science. XEUS is one of the astronomical applications being studied by ESA to utilize the capabilities of the ISS. XEUS will be a long-term X-ray observatory with an initial mirror area of 6 m 2 at 1 keV that will be expanded to 30 m 2 following a visit to the ISS. The 1 keV spatial resolution is expected to be 2-5″ half-energy-width. XEUS will consist of separate detector and mirror spacecraft (MSC) aligned by active control to provide a focal length of 50 m. A new detector spacecraft, complete with the next generation of instruments, will also be added after visiting the ISS. The limiting 0.1-2.5 keV sensitivity will then be 4 × 10 -18 erg cm -2 s -1, around 200 times better than XMM-Newton, allowing XEUS to study the properties of the hot baryons and dark matter at high redshift.",

author = "Parmar, {A. N.} and G. Hasinger and M. Arnaud and X. Barcons and D. Barret and H. B{\"o}hringer and A. Blanchard and M. Cappi and A. Comastri and T. Courvoisier and Fabian, {A. C.} and F. Fiore and I. Georgantopoulos and P. Grandi and R. Griffiths and A. Hornstrup and N. Kawai and K. Koyama and K. Makishima and G. Malaguti and Mason, {K. O.} and C. Motch and M. Mendez and T. Ohashi and F. Paerels and L. Piro and T. Ponman and J. Schmitt and S. Sciortino and G. Trinchieri and {van der Klis}, M. and M. Ward",

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doi = "10.1016/j.asr.2003.02.067",

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Parmar, AN, Hasinger, G, Arnaud, M, Barcons, X, Barret, D, Böhringer, H, Blanchard, A, Cappi, M, Comastri, A, Courvoisier, T, Fabian, AC, Fiore, F, Georgantopoulos, I, Grandi, P, Griffiths, R, Hornstrup, A, Kawai, N, Koyama, K, Makishima, K, Malaguti, G, Mason, KO, Motch, C, Mendez, M, Ohashi, T, Paerels, F, Piro, L, Ponman, T, Schmitt, J, Sciortino, S, Trinchieri, G, van der Klis, M & Ward, M 2004, 'Studying the evolution of the hot universe with the X-ray evolving universe spectroscopy mission - XEUS', Advances in space research, vol. 34, nr. 12, blz. 2623-2627. https://doi.org/10.1016/j.asr.2003.02.067

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T1 - Studying the evolution of the hot universe with the X-ray evolving universe spectroscopy mission - XEUS

AU - Parmar, A. N.

AU - Hasinger, G.

AU - Arnaud, M.

AU - Barcons, X.

AU - Barret, D.

AU - Böhringer, H.

AU - Blanchard, A.

AU - Cappi, M.

AU - Comastri, A.

AU - Courvoisier, T.

AU - Fabian, A. C.

AU - Fiore, F.

AU - Georgantopoulos, I.

AU - Grandi, P.

AU - Griffiths, R.

AU - Hornstrup, A.

AU - Kawai, N.

AU - Koyama, K.

AU - Makishima, K.

AU - Malaguti, G.

AU - Mason, K. O.

AU - Motch, C.

AU - Mendez, M.

AU - Ohashi, T.

AU - Paerels, F.

AU - Piro, L.

AU - Ponman, T.

AU - Schmitt, J.

AU - Sciortino, S.

AU - Trinchieri, G.

AU - van der Klis, M.

AU - Ward, M.

PY - 2004/1/1

Y1 - 2004/1/1

N2 - Europe is one of the major partners building the International Space Station (ISS) and European industry, together with ESA, is responsible for many station components including the Columbus Orbital Facility, the Automated Transport Vehicle, two connecting modules and the European Robotic Arm. Together with this impressive list of contributions there is a strong desire within the ESA Member States to benefit from this investment by utilizing the unique capabilities of the ISS to perform world-class science. XEUS is one of the astronomical applications being studied by ESA to utilize the capabilities of the ISS. XEUS will be a long-term X-ray observatory with an initial mirror area of 6 m 2 at 1 keV that will be expanded to 30 m 2 following a visit to the ISS. The 1 keV spatial resolution is expected to be 2-5″ half-energy-width. XEUS will consist of separate detector and mirror spacecraft (MSC) aligned by active control to provide a focal length of 50 m. A new detector spacecraft, complete with the next generation of instruments, will also be added after visiting the ISS. The limiting 0.1-2.5 keV sensitivity will then be 4 × 10 -18 erg cm -2 s -1, around 200 times better than XMM-Newton, allowing XEUS to study the properties of the hot baryons and dark matter at high redshift.

AB - Europe is one of the major partners building the International Space Station (ISS) and European industry, together with ESA, is responsible for many station components including the Columbus Orbital Facility, the Automated Transport Vehicle, two connecting modules and the European Robotic Arm. Together with this impressive list of contributions there is a strong desire within the ESA Member States to benefit from this investment by utilizing the unique capabilities of the ISS to perform world-class science. XEUS is one of the astronomical applications being studied by ESA to utilize the capabilities of the ISS. XEUS will be a long-term X-ray observatory with an initial mirror area of 6 m 2 at 1 keV that will be expanded to 30 m 2 following a visit to the ISS. The 1 keV spatial resolution is expected to be 2-5″ half-energy-width. XEUS will consist of separate detector and mirror spacecraft (MSC) aligned by active control to provide a focal length of 50 m. A new detector spacecraft, complete with the next generation of instruments, will also be added after visiting the ISS. The limiting 0.1-2.5 keV sensitivity will then be 4 × 10 -18 erg cm -2 s -1, around 200 times better than XMM-Newton, allowing XEUS to study the properties of the hot baryons and dark matter at high redshift.

U2 - 10.1016/j.asr.2003.02.067

DO - 10.1016/j.asr.2003.02.067

M3 - Article

VL - 34

SP - 2623

EP - 2627

JO - Advances in space research

JF - Advances in space research

SN - 0273-1177

IS - 12

ER -