Astron. Astrophys. Suppl. Ser.
Volume 133, Number 2, December I 1998
|Page(s)||171 - 179|
|Published online||15 December 1998|
I. Data on 92 emission line objects in two fields
Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
2 Observatoire de Marseille et Institut Gassendi, 2 place Le Verrier, 13248 Marseille, France
Send offprint request to: C. Surace
Accepted: 4 June 1998
We present data from a moderately deep spectroscopic Schmidt survey (Blim = 17.5) of "active galaxies” selected by the presence of emission lines in their spectra and/or their UV excess. The redshift, magnitudes, color and diameter reduction methods have been discussed in a previous paper. Here we explain the emission line equivalent width determination method. 92 emission line objects have been found in two adjacent fields (approximately ) in the direction of the southern extension of the Virgo cluster. We give a catalog containing positions, photographic R and B magnitudes, colors, effective diameters, redshifts, equivalent widths and intensity ratios of the [OIII], H and [OII] emission lines. On these fields, we evaluate the completeness limit of the survey at a pseudo B magnitude value of 15.7. A more elaborate astrophysical analysis will appear in a forthcoming paper.
Key words: surveys / galaxies: general / galaxies: starburst / methods: data analysis
The table is also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (18.104.22.168) or via http://cdsweb.u-strasbg.fr/Abstract.html
Finding charts, including information on star formation location is available in electronic form via http://aas.aanda.org
© European Southern Observatory (ESO), 1998