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First observation of a quasar with a redshift of 4

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TLDR
In this paper, the authors reported the discovery of a quasar (0046- 293) with a redshift z = 4.01 and another (0044-276) with redshift Z = 3.42.
Abstract
Quasars of high redshift (here z > 3.3) are the most distant objects known and provide direct information on the early Universe. However, only a few high-redshift quasars have been discovered and their detection remains problematic. We report here the discovery of a quasar (0046 – 293) with a redshift z = 4.01 and another (0044–276) with a redshift z =3.42. The redshift of the former quasar is the highest yet detected and compares with the z = 3.80 of the previous most distant known quasar1. The new quasars lie in the same field as three other known high-redshift quasars1,2 and were identified in a preliminary analysis of new multi-colour data derived from measurements of direct photographic plates taken with the United Kingdom Schmidt Telescope (UKST). The two new quasars are significantly fainter (mR>19) than previously known high-redshift quasars discovered by optical techniques, and demonstrate that the luminosity function of optically selected high-redshift quasars extends over at least two· magnitudes.

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Citations
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Journal ArticleDOI

The Stellar Populations and Evolution of Lyman Break Galaxies

TL;DR: In this paper, the spectral energy distributions (SEDs) of Lyman break galaxies (LBGs) at 2.0 z 3.5 were examined using deep near-infrared and optical observations of the Hubble Deep Field-North from the Hubble Space Telescope NICMOS and WFPC2 instruments and from the ground.
Journal ArticleDOI

High-redshift quasars in the Cold Dark Matter cosmogony

TL;DR: In this article, it was shown that the observed space density of luminous quasars between z = 2 and z = 4 is compatible with the cold dark matter (CDM) model.
Journal ArticleDOI

The Sdss-Iv Extended Baryon Oscillation Spectroscopic Survey: Quasar Target Selection

TL;DR: The extended Baryon Oscillation Spectroscopic Survey (eBOSS) as mentioned in this paper will improve measurements of the cosmological distance scale by applying the BAO method to quasar samples.
Journal ArticleDOI

High-redshift quasars found in Sloan Digital Sky Survey commissioning data

Xiaohui Fan, +95 more
TL;DR: In this article, the authors presented photometric and spectroscopic observations of 15 high-redshift quasars (z > 3.6) discovered from ~140 deg2 of five-color (u, g, r, i, and z') imaging data taken by the Sloan Digital Sky Survey (SDSS) during its commissioning phase.
References
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Journal ArticleDOI

Quasars to B>22.5 in selected area 57: a catalog of multicolor photometry, variability, and astrometry

TL;DR: In this paper, the authors present a catalog of 77 quasar candidates at the north galactic pole (Selected Area 57) to a blue magnitude limit of 22.5 over an area of 0.3 square degree.
Journal ArticleDOI

A QSO with redshift 3.8 found on a UK Schmidt telescope IIIa-F prism plate

TL;DR: In this paper, an unfiltered UK Schmidt telescope (UKST) IIIa-F low-dispersion objective prism plates can be used successfully in such searches up to at least z ≃ 3.7 (ref.
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Spectroscopic CCD surveys for quasars at large redshift. II - A Pfuei transit survey

TL;DR: In this article, a CCD transit survey has been carried out with the 200 in. telescope of a strip of sky 5 arcmin wide and 9 hr long, where direct images and slitless spectra of over 43,000 objects were obtained on two successive nights.
Journal ArticleDOI

Spectrum of a QSO with redshift 3.8

TL;DR: In this paper, the authors presented a moderate-resolution optical spectrum of a quasi-stellar object (QSO) with a precise redshift of 3.803 ± 0.005.
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