Obtaining High Signal on the Fe-L Unresolved Transition Array

Details Obtaining High Signal on the Fe-L Unresolved Transition Array Obtaining High Signal on the Fe-L Unresolved Transition Array

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2521c&link_type=abstract

Chandra proposal ID #10700045

Computer Science

Scientific paper

We request 250 ksec of Chandra HETGS observations of the Seyfert 1 Ark 564. This source is known to have a broad range of ionized absorbers in outflow, seen against the strong soft continuum. The primary goal of these observations is to study the unresolved transition array (UTA) of Fe-L in this source, which provides the highest continuum level at the UTA of any previously studied active galaxy. We will also examine the response of the ionized warm absorber components to rapid variability, which is common in this source, a narrow line Sy1 galaxy. Finally, we will be able to place better limits on any narrow components of the neutral or ionized Fe emission lines.

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