Title: Emission Line Properties of AGN from a pre-COSTAR FOS HST Spectral Atlas Authors: Kuraszkiewicz J., Green P.J., Forster K., Aldcroft T.L., Evans I.N., Koratkar A. Table: Representative emission line measurements ================================================================================ Byte-by-byte Description of file: electronic_table5.ascii -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- First line with source information: 1- 11 A11 --- Name Designation 12- 20 F9.5 --- z Redshift Followed by 43 rows of emission line measurements - one row for each emission line: 1-16 A16 --- Line Emission line name 17-23 I7 km/s FWHM Full width at half maximum of Line 24-30 I7 km/s E_FWHM positive error on FWHM 31-37 I7 km/s e_FWHM negative error on FWHM 38-44 I7 km/s Offset Gaussian emission line model peak offset from the expected position (1) 45-51 I7 km/s E_Offset positive error on Offset 52-58 I7 km/s e_Offset negative error on Offset 59-67 F9.2 0.1nm EqWid Rest frame equivalent width of line (in {AA}) 68-76 F9.2 0.1nm E_EqWid positive error on EqWid (2) 77-85 F9.2 0.1nm e_EqWid negative error on EqWid (2) 86-94 F9.2 erg/cm2/s Flux Observed emission line flux in units of 10$^{-14}$erg\,cm$^{-2}$\,s$^{-1}$ 95-103 F9.2 E_Flux positive error on flux 104-112 F9.2 e-Flux negative error on flux 113-115 I3 --- Num Number of narrow absorption features used in modeling the emission lines (3) -------------------------------------------------------------------------------- Note (1): Note that no peak offset measurements appear for the iron emission line measurements. Note (2): Based on the 2{sigma} uncertainties in the amplitude and FWHM of the Gaussian model and do not include an error from an uncertainty in the underlying continuum flux level. Note (3): Tabulated in the row of the emission line closest to the position of the absorption feature. --------------------------------------------------------------------------------