The Most Distant [OIII]-Emitting Quasar PKS 1937–101 at Redshift 3.8 | Zendy

Yoshiaki Taniguchi | Zendy; Takashi Murayama | Zendy; Kimiaki Kawara | Zendy; N. Arimoto | Zendy

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The Most Distant [OIII]-Emitting Quasar PKS 1937–101 at Redshift 3.8

Author(s) -

Yoshiaki Taniguchi,

Takashi Murayama,

Kimiaki Kawara,

N. Arimoto

Publication year - 1997

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/49.4.419

Subject(s) - physics , quasar , redshift , astrophysics , rest frame , galaxy , astronomy , ovv quasar

We report the discovery of a high-z quasar with unambiguous [OIII]5007 emission; PKS 1937-101 at redshift 3.8. This quasar, however, shows little evidence for rest-frame ultraviolet and optical FeII emission. It is thus shown that PKS 1937-101 does not belong to a class of super iron-rich high-z quasars reported by Elston, Thompson, & Hill (1994). The epoch of major star formation in the host galaxy is discussed briefly

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