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http://arxiv.org/pdf/astro-ph/...
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https://doi.org/10.1007/978-3-...
Part of book or chapter of book . 1999 . Peer-reviewed
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https://dx.doi.org/10.48550/ar...
Article . 1998
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The Hubble Deep Field-South QSO

Authors: Sealey, Katrina M.; Drinkwater, Michael. J.; Webb, John K.; Boyle, Brian J.;

The Hubble Deep Field-South QSO

Abstract

The Hubble Deep Field-South (HDF-S) was chosen to have a QSO (RA 22:33:37.6 Dec -60:33:29 J2000 and B=17.5) in the field to allow for studies of absorption systems intersecting the sight line to the QSO. To assist in the planning of HDF-S observations we present here a ground-based spectrum of the QSO. We measure a redshift of z=2.24 for the QSO and find associated absorption in the spectrum at z=2.204 as well as additional absorption features.

3 pages (LaTeX, uses lamuphys.sty, included); 1 figure; to appear in Proceedings of the ESO/ATNF Workshop "Looking Deep in the Southern Sky", Sydney, Australia 10-12 December 1997, eds. R. Morganti and W. Couch

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green