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ASCA Deep Sky Survey
Published online by Cambridge University Press: 25 May 2016
Extract
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.
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- Session 4: Large Scale Hot Plasmas and Their Relation with Dark Matter
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- Copyright © Kluwer 1998