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THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: AN INVESTIGATION OF BIASES IN C IV EMISSION LINE PROPERTIES

  • Authors: K. D. Denney, Keith Horne, Yue Shen, W. N. Brandt, Luis C. Ho, B. M. Peterson, Gordon T. Richards, J. R. Trump, and J. Ge

2016 The Astrophysical Journal Supplement Series 224 14.

  • Provider: AAS Journals

Caption: Figure 4.

Fractional FWHM (left) and σl (right) uncertainties for the SE (black points) and coadded spectra (red points) as a function of the S/N of the line. The S/N is measured per angstrom in an emission-line-free continuum window near rest frame 1700 Å. The solid black line is the expected reference relation, ﹩{\sigma }_{V}/V\propto ﹩ ﹩{({\rm{S}}/{\rm{N}}\sqrt{\mathrm{EW}/{W}_{C}})}^{-1}﹩. See Section 3.2 for details.

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