The ROSAT BRIGHT survey: I. Identification of an AGN sample with hard ROSAT X-ray spectra

• Published in: arXiv.org 1998-11
• Main Authors: J -U Fischer, Hasinger, G, Schwope, A D, Brunner, H, Boller, Th, Truemper, J, Voges, W, Neizvestny, S
• Format: Article
• Language: English
• Subjects: Active galactic nuclei; Cataclysmic variables; Galactic clusters; Interacting galaxies; Linings; Magellanic clouds; Red shift; Seyfert galaxies; Sky surveys (astronomy); Spectral resolution; Spectrum analysis; Virgo galactic cluster; X ray sources; X ray spectra
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.9811139

The ROSAT Bright Survey (RBS) aims to completely optically identify the more than 2000 brightest sources detected in the ROSAT all-sky survey at galactic latitudes |b| > 30 degr (excluding LMC, SMC, Virgo cluster). This paper presents a subsample of 66 bright point-like ROSAT survey sources with almost hard PSPC spectra, the hardness ratio HR1 is > 0.5 for most of the sources. The subsample could be nearly completely identified by low-resolution optical spectroscopy with the following breakdown into object classes: 31 Seyfert galaxies, 22 BL Lac candidates, 5 clusters of galaxies 1 cataclysmic variable, and 5 bright stars. Only one object remained unidentified and one X-ray source was a spurious detect ion. The redshift distribution peaks around 0.06 for the Seyferts and around 0.13 for the BL Lac candidates. Observations with medium spectral resolution were obtained for most of the new S eyfert galaxies. A large fraction (20 objects) are type 1 Seyfert galaxies, the other fraction includes Seyfert galaxies of type 1.5 - 1.8 (5 objects), two LINERs, and 4 possible narrow-line Seyfert 1 galaxies (NLS1). About one third of the new Seyfert's have nearby companion galaxies displaying either emission or absorption lines at the same redshift. Among them are a couple of systems showing direct morphological evidence for interaction. The large fraction of interacting galaxies among our sample suggests a scenario where interaction is the main trigger of AGN activity.