CIV Emission and the Ultraviolet through X-ray Spectral Energy Distribution of Radio-Quiet Quasars
| Autor: | Kruczek, Nicholas E., Richards, Gordon T., Gallagher, S. C., Deo, Rajesh P., Hall, Patrick B., Hewett, Paul C., Leighly, Karen M., Krawczyk, Coleman M., Proga, Daniel |
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| Rok vydání: | 2011 |
| Předmět: | |
| Zdroj: | Astron.J.142:130-141,2011 |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1088/0004-6256/142/4/130 |
| Popis: | In the restframe UV, two of the parameters that best characterize the range of emission-line properties in quasar broad emission-line regions are the equivalent width and the blueshift of the CIV line relative to the quasar rest frame. We explore the connection between these emission-line properties and the UV through X-ray spectral energy distribution (SED) for radio-quiet (RQ) quasars. Our sample consists of a heterogeneous compilation of 406 quasars from the Sloan Digital Sky Survey and Palomar-Green survey that have well-measured CIV emission-line and X-ray properties (including 164 objects with measured Gamma). We find that RQ quasars with both strong CIV emission and small CIV blueshifts can be classified as "hard-spectrum" sources that are (relatively) strong in the X-ray as compared to the UV. On the other hand, RQ quasars with both weak CIV emission and large CIV blueshifts are instead "soft-spectrum" sources that are (relatively) weak in the X-ray as compared to the UV. This work helps to further bridge optical/soft X-ray "Eigenvector 1" relationships to the UV and hard X-ray. Based on these findings, we argue that future work should consider systematic errors in bolometric corrections (and thus accretion rates) that are derived from a single mean SED. Detailed analysis of the CIV emission line may allow for SED-dependent corrections to these quantities. Comment: AJ, in press; 39 pages, 11 figures, 3 tables |
| Databáze: | arXiv |
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