IGR J14561-3738

	IGR J14561-3738


	Other name = ESO 386- G 034, XSS J14562-37

Type	Redshift	Radio Counterpart			Infrared/Optical Counterpart
		R.A. (J2000)	Dec. (J2000)	References	R.A. (J2000)	Dec. (J2000)	References
AGN likely Sey 2	0.024				LEDA 53392		Masetti et al. 2007, ATel 1033
Published Papers		Sazonov et al. 2007, A&A, 462, 57 Krivonos et al. 2007 A&A, 475, 775 Masetti et al. 2008 A&A, 482, 113 Sazonov et al. 2008, A&A, 487, 509 Khorunzhev et al. 2012 Astr. Lett., 38, 475

Miscellaneous :

Krivonos et al. 2007 A&A, 462, 57:

Source is associated to ESO 386- G 034
AGN

Masetti et al. 2007 ATel 1033:

LEDA 53392 has redshift 0.025
H_α, [NII] and [SII] in emission
Sey 2

Masetti et al. 2008:

Optical spectroscopy is presented and detailed
Fluxes of H_α, H_β and [OIII] are given
z=0.024
Optical counterpart only tentative as no soft X-ray counterpart found to date

Sazonov et al. 2008:

Very weak source in Chandra
Likely Compton thick AGN
ESO 386-G034 at z=0.0246

Khorunzev et al. 2012:

Etimate of mass and accretion rate based on different methods
Correltion with bulge luminosity => M = 10^8.25 M_Sun and L_Edd = 10^46.35 erg/s
L_Bol=0.008 L_Edd

Last updated 22 Nov. 2012

Jerome Rodriguez