1.0AGN Driven Windshttps://phsites.technion.ac.il/agn-2017Adihttps://phsites.technion.ac.il/agn-2017/author/adile/N. Arav - Distances of quasar outflows - AGN Driven Windsrich600338<blockquote class="wp-embedded-content" data-secret="7aLTL9rMlW"><a href="https://phsites.technion.ac.il/agn-2017/n-arav-distances-quasar-outflows/">N. Arav – Distances of quasar outflows</a></blockquote><iframe sandbox="allow-scripts" security="restricted" src="https://phsites.technion.ac.il/agn-2017/n-arav-distances-quasar-outflows/embed/#?secret=7aLTL9rMlW" width="600" height="338" title="“N. Arav – Distances of quasar outflows” — AGN Driven Winds" data-secret="7aLTL9rMlW" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"></iframe><script type="text/javascript">
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The most robust way for determining the distance of quasar absorption outflows is the use of troughs from excited states. Here we report the results of two surveys targeting outflows that show troughs from S iv. One survey includes 1091 SDSS and BOSS quasar spectra, and the other includes much higher quality spectra of 13 …