J/A+AS/135/437 AGNs with composite spectra. II. (Goncalves+ 1999) ================================================================================ AGNs with composite spectra. II. Additional data. Goncalves A.C., Veron-Cetty M.-P., Veron P. =1999A&AS..135..437G (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Active gal. nuclei ; Galaxies, Seyfert ; Galaxies, spectra ; H II regions ; Line Profiles ; Spectroscopy Keywords: galaxies: active - galaxies: nuclei - galaxies: Seyfert Description: We have compiled from the literature 88 emission-line galaxies for which the published line-ratios give indication of a "transition spectrum"; selected objects are located north of {delta}~-20{deg}, are brighter than B=17 and have z<0.1. We have observed 53 of these galaxies with the spectrograph CARELEC, attached to the OHP 1.93m telescope. The observations were carried out during several runs in May, June and July 1996 and January, March, October and November 1997. The journal of observations is given in Table 5. The spectra (R~1800) were analysed in terms of Gaussians to search for the presence of multiple line-components, coming from kinematically and spatially distinct regions - "composite spectra". The results of the fitting analysis are given in Table 6. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 38 100 Journal of observations table6.dat 90 145 Fitting analysis results -------------------------------------------------------------------------------- Byte-per-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Name Galaxy name 17 A1 --- n_Name [*] Note on Name (1) 19 A1 --- Disp Dispersion & wavelength range (2) 22- 29 A8 "DD/MM/YY" Date Date of exposure 32- 33 I2 min ExpTime Exposure time 36- 38 I3 deg PA Slit position angle -------------------------------------------------------------------------------- Note (1): *: objects published in Paper I (1997A&A...319...52V) Note (2): A: observations in the range 670.0-760.0nm, R~1800 B: observations in the range 486.0-576.0nm, R~1800 -------------------------------------------------------------------------------- Byte-per-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Name Galaxy name & notes on the object (1) 18- 20 A3 --- n_Name [abtq ] Note on Name (2) 22- 27 F6.4 --- z Redshift used in the fitting analysis 29- 32 I4 km/s Vblue ? Line velocity in the blue system 33 A1 --- n_Vblue [*] Note on the V_blue_ parameter (3) 35 A1 --- l_FWHMblue Limit flag on FWHMblue parameter 36- 39 I4 km/s FWHMblue ? FWHM of the lines in the blue system 40 A1 --- n_FWHMblue [*] Note on the FWHMblue parameter (3) 42 A1 --- l_5007/Hb Limt flag on the [OIII]5007/Hb parameter (3) 43- 47 F5.2 --- 5007/Hb ? Ratio of [OIII]5007 to the H{beta} line 48 A1 --- n_5007/Hb [*] Note on the [OIII]5007/Hb parameter (3) 50- 52 I3 % Hb ? Flux of the H{beta} line 54- 58 I5 km/s Vred ? Line velocity in the red system 59 A1 --- n_Vred [*] Note on the Vred parameter (3) 61 A1 --- l_FWHMred Limit flag on the FWHMred parameter (3) 62- 65 I4 km/s FWHMred ? FWHM of the lines in the red system 66 A1 --- n_FWHMred [ *!] Note on the FWHMred parameter (3) 68- 71 F4.2 --- 6583/Ha ? Ratio of [NII]6583 to the H{alpha} line 72 A1 --- n_6583/Ha [*] Note on the [NII]6583/Ha parameter (3) 74 A1 --- l_6300/Ha Limit flag on the [NII]6583/Ha parameter (3) 75- 78 F4.2 --- 6300/Ha ? Ratio of [OI]6300 to the H{alpha} line 80- 82 I3 % Ha ? Flux of the H{alpha} line 84- 87 I4 km/s DeltaV ? Difference between Vblue and Vred 89- 90 A2 --- Class ? Classification of the line-components (4) -------------------------------------------------------------------------------- Note (1): When several slices were extracted from the spectrum of a single object, these were numbered #1, #2, #3 etc. Note (2): a: an absorption feature was included in the model to fit the blue spectrum b: we added an absorption line to fit the red spectrum t: we corrected the blue spectrum for the stellar contribution by using a template q: the red spectrum was corrected by a template. Note (3): *: the value on the previous column was fixed in the model. !: profile used to fit the line is Lorentzian, rather than Gaussian. Note (4): 1: Seyfert 1 2: Seyfert 2 H: H II region L: LINER -------------------------------------------------------------------------------- Acknowledgements: Anabela Goncalves References: Veron et al., Paper I. 1997A&A...319...52V ================================================================================ (End) A.C. Goncalves [OHP], Patricia Bauer [CDS] 01-Feb-1999