Sky surveys with  ASCA  — Deep Sky Survey | Zendy

Ogasaka Y. | Zendy; Kii T. | Zendy; Ueda Y. | Zendy; Takahashi T. | Zendy; Inoue H. | Zendy; Ishisaki Y. | Zendy; Ohta K. | Zendy; Yamada T | Zendy; Makishima K. | Zendy; Miyaji T. | Zendy; Hasinger G. | Zendy

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Sky surveys with ASCA — Deep Sky Survey

Author(s) -

Ogasaka Y.,

Kii T.,

Ueda Y.,

Takahashi T.,

Inoue H.,

Ishisaki Y.,

Ohta K.,

Yamada T,

Makishima K.,

Miyaji T.,

Hasinger G.

Publication year - 1998

Publication title -

astronomische nachrichten

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.394

H-Index - 63

eISSN - 1521-3994

pISSN - 0004-6337

DOI - 10.1002/asna.2123190122

Subject(s) - sky , confusion , physics , astrophysics , flux (metallurgy) , astronomy , psychology , materials science , psychoanalysis , metallurgy

ASCA Deep Sky Survey (DSS) is aimed to investigate the constituents of the CXB in 2–10 keV band, by faint source survey observations reaching to the source confusion limit of ASCA X‐Ray Telescopes. So far, 0.29 deg 2 sky regions were systematically studied and about 40% of the CXB intensity was resolved into discrete sources. In this paper, we present the latest results on the number‐flux relation (Long N ‐Log S ) and spectrum properties of faint X‐ray sources.

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