H/RCULES and the LBQS: Results from an emission line study

Details H/RCULES and the LBQS: Results from an emission line study H/RCULES and the LBQS: Results from an emission line study

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...196.6205f&link_type=abstract

American Astronomical Society, 196th AAS Meeting, #62.05; Bulletin of the American Astronomical Society, Vol. 32, p.1284

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a study of the emission line properties of the LBQS sample. This was undertaken as part of the H/RCULES project, a continuum and ultraviolet emission line study of AGN. The challenge of analyzing a sample with over 1050 spectra was tackled in a mostly non-interactive manner using software developed for the Chandra mission. Absorption lines were identified and measured using FINDSL (Aldcroft 1995) and iron emission features were fitted using a template generated from the UV and optical spectrum of I Zw 1 (Vestergaard & Wilkes 2000). Over 6000 UV-Optical emission line and continuum measurements were combined with X-ray (ROSAT) and radio fluxes to study the broad band SED's within the sample.

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