S. Mathur et al. 2009 The Astronomical Journal 138 1655 doi:10.1088/0004-6256/138/6/1655
S. Mathur1, E. C. Golowacz1, R. Williams2, R. Pogge1, D. Fields3 and D. Grupe4
Show affiliationsWe present XMM-Newton observations of the type 1 active galactic nucleus (AGN) SDSS 1430 – 0011 (z = 0.1032). The low signal-to-noise ratio spectrum of this source obtained in a snap shot Chandra observation showed an unusually flat continuum. With the follow-up XMM-Newton observations, we find that the source spectrum is complex; it either has an ionized absorber or a partially covering absorber. The underlying power law is in the normal range observed for AGNs. The low flux of the source during Chandra observations can be understood in terms of variations in the absorber properties. The X-ray and optical properties of this source are such that it cannot be securely classified as either a narrow-line Seyfert 1 or a broad-line Seyfert 1 galaxy, adding to the group of sources in the "in-between" class.
galaxies: active; galaxies: individual (SDSSJ143030.22 – 001115.1); galaxies: nuclei; X-rays: galaxies
Issue 6 (2009 December)
Received 2009 May 27, accepted for publication 2009 September 30
Published 2009 October 29
S. Mathur et al. 2009 The Astronomical Journal 138 1655
Aaron C. Boley et al 2009 ApJ 706 L192
K. Tamura et al. 2009 The Astronomical Journal 138 1634
Guillermo Torres et al. 2009 The Astronomical Journal 138 1622
P. Venkatakrishnan and Sanjiv Kumar Tiwari 2009 ApJ 706 L114
Edward M. Sion et al. 2009 The Astronomical Journal 138 1681
Olaf Szewczyk et al. 2009 The Astronomical Journal 138 1661
D. A. Perley et al. 2009 The Astronomical Journal 138 1690
J. B. Hutchings et al. 2009 The Astronomical Journal 137 3533
Bogdan Popescu and M. M. Hanson 2009 The Astronomical Journal 138 1724