HETG Observation of AN Unusual Spectral Feature in the Narrow-Line Seyfert 1 Galaxy Ark 564

Physics

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Chandra Proposal Id #01700703

Scientific paper

We propose a 50 ks HETG observation to identify an unusual emission feature near 1 keV found in the ASCA and SAX spectra of the bright narrow-line Seyfert 1 galaxy Ark 564. This could be the first clear evidence of the predicted soft X-ray line emission from an ionized accretion disk, which would support the idea that NLS1s are characterized by a high accretion rate. Alternatively, we may discover that this feature originates in emission from a warm absorber with unusual ionization conditions, thereby permitting our study of a broader range of warm absorber behavior. Ark 564 is bright enough that we will also be able to study its X-ray variability and search for the nonlinearity which may be a signature of NLS1s.

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