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ASCA Deep Sky Survey

Published online by Cambridge University Press:  25 May 2016

Y. Ogasaka
Affiliation:
NASA Goddard Space Flight Center
T. Kii
Affiliation:
The Institute of Space and Astronautical Science
Y. Ueda
Affiliation:
The Institute of Space and Astronautical Science
T. Takahashi
Affiliation:
The Institute of Space and Astronautical Science
H. Inoue
Affiliation:
The Institute of Space and Astronautical Science
Y. Ishisaki
Affiliation:
Department of Physics, Tokyo Metropolitan University
K. Ohta
Affiliation:
Department of Astronomy, Kyoto University
T. Yamada
Affiliation:
Astronomical Institute, Tohoku University
K. Makishima
Affiliation:
Department of Physics, University of Tokyo
T. Miyaji
Affiliation:
Astrophysikalisches Institut Potsdam
G. Hasinger
Affiliation:
Astrophysikalisches Institut Potsdam

Extract

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ASCA DSS was intended to carry out unbiased surveys in wide energy range of 0.5-10 keV. The strategy of this project is to survey small sky region with extremely high sensitivity reaching to the source confusion limit of ASCA XRT, in contrast to the Large Sky Survey project (Ueda 1996) which covers much larger sky area with relatively shallow exposure.

Type
Session 4: Large Scale Hot Plasmas and Their Relation with Dark Matter
Copyright
Copyright © Kluwer 1998 

References

Cappi, M. et al. 1997, in the proceedings of “X-ray Imaging and Spectroscopy of Cosmic Hot Plasmas”, Tokyo, March 1996 Google Scholar
Koo, D. C., Kron, R. G., and Cudworth, K. M. 1986, Publ. Astron. Soc. Pacific , 98, 285.Google Scholar
Hasinger, G. et al., 1993, Astron. Astrophys. , 275, 1.Google Scholar
Hayashida, K. 1989, Ph. D dissertation of Univ. of Tokyo, ISAS RN 466.Google Scholar
Ogasaka, Y. 1996, Ph. D dissertation of Gakushuin University Google Scholar
Piccinotti, G. et al 1982, Astrophys. J. , 253, 485.Google Scholar
Ueda, Y. 1996, Ph. D dissertation of University of Tokyo Google Scholar