High Signal-To QSO Line Profiles

Physics

Scientific paper

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Hst Proposal Id #3065 Quasars &Amp, Agn

Scientific paper

We will use the FOS to measure the strengths and profiles of emission lines in the UV in a bright, low-redshift QSO. We will present a high signal-to-noise spectrum which is essentially unaffected by the HST optical problems. These observations will be combined with optical observations of similar quality and lead to improved models of the structure of the broad-line region of QSOs.

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