IGR J07597-3842

IGR J07597-3842

Other name = RXH J075942.0-384355

Type	Redshift	Radio Counterpart			Infrared Counterpart
		R.A. (J2000)	Dec. (J2000)	References (position)	R.A. (J2000)	Dec. (J2000)	References (position)
AGN Seyfert 1.2	0.040 d=190.1 Mpc	NVSS 1.4 GHz (5" error)		den Hartog et al. 2004 Atel 261	IRAS 07579-3835		den Hartog al. 2004 Atel261
		07h 59m 41.8s	-38o 43' 53"
Published Papers		Stephen et al. 2006, A&A, 445, 869 Masetti et al. 2006, A&A, 459, 21 Malizia et al. 2007, ApJ, 668,81 Panessa et al. 2008, A&A, 483, 151 Winter et al. 2009, ApJ, 690, 1322

Miscellaneous :

den Hartog et al. 2004:

Detection by Beppo-Sax
IBIS/ISGRI spectrum power law like with Gamma=1.8 +/-0.3

Molina et al. 2004 Atel 263:

Near Infra red counterpart (J075941.8-384356) has magnitudes J=13.560, H=12.465 and K=11.345
Optical counterpart has magnitudes I=15.026-15.114, R=14.2 and B=16.6

Masetti et al. 2006:

Near Infra red counterpart (J075941.8-384356) has magnitudes J=13.560, H=12.465 and K=11.345
H beta, OIII emission lines
Seyfert 1.2
z=0.040

Panessa et al. 2008:

XMM and INTEGRAL spectral analysis
soft black body and a narrow iron line are needed to fit spectra
high energy cut-off power law represent the data better than a simple power law
Possible reflection spectrum, but reflection parameter is constrained

Winter et al. 2009:

Swift spectral analysis
N_H < 0.03 x 10²² cm-2 (intrinsic, with N_{H, Gal}=0.62 x 10²² cm-2
Γ=1.88

Last updated 2 June 2009

Jerome Rodriguez