IGR J16385-2057

	IGR J16385-2057


	Other name = 1RXS J163830.9-205520, Oph J163830-2055

Type	Redshift	Radio Counterpart			Infrared/Optical Counterpart
		R.A. (J2000)	Dec. (J2000)	References	R.A. (J2000)	Dec. (J2000)	References
AGN, NL Sey 1	z=0.026879				2MASX J16383091-2055246		Rodriguez et al. 2008
Published Papers		Rodriguez et al. 2008, A&A, 482, 731 Masetti et al. 2008 A&A, 482, 113 Malizia et al. 2008, MNRAS, 389, 1360 Panessa et al. 2011, accepted in MNRAS arXiV 1106.3023

Miscellaneous :

Masetti et al. 2006 ATel 957:

broad Halpha, Hbeta, Hgamma and Hdelta plus narrow [OIII] lines, in emission
z=0.026879
Sey 1

Rodriguez et al. 2008:

Refined X-ray position
Sey 1 confirmed through refinement of X-ray position
Absorbed power law fits 0.5-9 keV spectra well, Γ= 2.1 N_H=0.21 x10²²cm^-2; F_{2-10 keV}=7.7 x 10^-12 erg/s/cm2

Masetti et al. 2008:

Optical spectroscopy is presented and detailed
Fluxes of H_β and [OIII] are given
Narrow Line Sey 1
M_BH=0.7 x10⁷ M_sun

Malizia et al. 2008:

Swift/XRT and INTEGRAL/IBIS/ISGRI broad band spectral analysis
Absorbed power law (Γ=2.15), Absorbed cut off pl (Γ=2.03, Ec=29 keV), absorbed broken pl (Γ₁=12.12, Eb=27 keV, Γ₂>2.6 ) fit the data well.
N_H=0.12 x10²² cm^-2 in excess to Galactic absorption

Last updated 20 June, 2011

Jerome Rodriguez