A Deep Multicolor Survey. II. Initial Spectroscopy and Comparison with Expected Quasar Number Counts: Erratum

Details A Deep Multicolor Survey. II. Initial Spectroscopy and Comparison with Expected Quasar Number Counts: Erratum A Deep Multicolor Survey. II. Initial Spectroscopy and Comparison with Expected Quasar Number Counts: Erratum

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...471.1073h&link_type=abstract

Astrophysical Journal v.471, p.1073

Astronomy and Astrophysics

Astronomy

9

Errata, Addenda

Scientific paper

In the paper "A Deep Multicolor Survey. II. Initial Spectroscopy and Comparison with Expected Quasar Number Counts" by Patrick B. Hall, Patrick S. Osmer, Richard F. Green, Alain C. Porter, and Stephen J. Warren (ApJ, 462,614 [1996]), some of the figures were inadvertently printed with poor resolution. The full information conveyed in the images is thus difficult to perceive. Here we present high-resolution versions of the affected figures (Fig. 1 and Figs. 10-15). In all diagrams, objects from the catalog are plotted as error bars, with only half the full error bars plotted, for clarity. Error ban extending off the diagram indicate upper limits. Spectroscopically confirmed quasars, compact narrow emission-line galaxies (CNELGs), and stars are plotted as filled boxes, open boxes, and inverted triangles, respectively. Spectroscopically observed but unidentified candidates are plotted as crosses and simulated quasar colors as dots. The line of simulated quasar points at U- V = 3.0 in Figure 11a and the similar lines in other color-color diagrams indicate that the simulated colors are lower limits. The reader should also note that Figures 16b and 16c were incorrectly switched with each other in the paper.

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