Free Access
   

Table 2:

Emission-line measurements.

Source
za Line $\lambda_{{\rm obs}}$ ${\rm Flux}^b$ FWHMc
      (Å) ( $10^{-16}~{\rm erg}~{\rm s}^{-1}
\ {\rm cm}^{-2}$) (Å)
TN J0121+1320 3.517 N V$\lambda$1240 - <0.094d -
    C IV$\lambda$1549 6996.9 $0.263\pm0.005$ 34.4
    He II$\lambda$1640 7414.3 $0.330\pm0.012$ 20.1
    C III]$\lambda$1909 8622.2 $0.282\pm0.009$ 32.6
TN J0205+2242 3.507 N V$\lambda$1240 - <0.097d -
    C IV$\lambda$1549 6981.8 $0.873\pm0.025$ 33.0
    He II$\lambda$1640 7387.5 $0.519\pm0.046 $ 47.3
    C III]$\lambda$1909 8586.0 $0.418\pm0.049$ 33.4
MRC 0316-257 3.130 N V$\lambda$1240 - <0.038d -
    C IV$\lambda$1549 6396.8 $0.267\pm0.011$ 52.4
    He II$\lambda$1640 6771.5 $0.301\pm0.009$ 27.9
    C III]$\lambda$1909 7874.1 $0.345\pm0.018$ 41.1
USS 0417-181 2.773 N V$\lambda$1240 - <0.103d -
    C IV$\lambda$1549 5845.1 $0.356\pm0.026$ 37.5
    He II$\lambda$1640 6188.5 $0.492\pm0.019$ 28.9
    C III]$\lambda$1909 7192.8 $0.553\pm0.047$ 30.7
TN J0920-0712 2.758 N V$\lambda$1240 4663.9 $1.015\pm0.014$ 31.6
    C IV$\lambda$1549 5821.4 $3.365\pm0.010$ 26.6
    He II$\lambda$1640 6161.5 $2.063\pm0.011$ 21.4
    C III]$\lambda$1909 7163.2 $1.945\pm0.028$ 28.3
WN J1123+3141 3.221 N V$\lambda$1240 5238.7 $1.698\pm0.013$ 31.7
    C IV$\lambda$1549 6538.8 $1.570\pm0.011$ 24.8
    He II$\lambda$1640 6916.9 $0.425\pm0.014$ 19.9
    C III]$\lambda$1909 8046.6 $0.183\pm0.028$ 20.3
4C 24.28 2.913 N V$\lambda$1240 4853.2 $1.225\pm0.012$ 46.4
    C IV$\lambda$1549 6061.6 $1.235\pm0.020$ 50.7
    He II$\lambda$1640 6416.3 $0.978\pm0.011$ 29.5
    C III]$\lambda$1909 7463.8 $0.812\pm0.041$ 41.9
USS 1545-234 2.751 N V$\lambda$1240 4642.9 $1.335\pm0.031$ 50.1
    C IV$\lambda$1549 5810.3 $1.343\pm0.021$ 24.7
    He II$\lambda$1640 6150.7 $0.878\pm0.012$ 16.9
    C III]$\lambda$1909 7150.9 $0.606\pm0.031$ 26.9
USS 2202+128 2.705 N V$\lambda$1240 4595.0 $0.160\pm0.019$ 30.4
    C IV$\lambda$1549 5739.2 $0.704\pm0.012$ 22.9
    He II$\lambda$1640 6074.3 $0.289\pm0.010$ 20.3
    C III]$\lambda$1909 7065.5 $0.292\pm0.011$ 25.6
a Redshift of the target calculated from the observed C IV wavelength; b line fluxes corrected for the Galactic reddening; c observed FWHM (includes instrumental broadening); d 3$\sigma$ upper-limit flux.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.