REJ1034+396 Reverberation Analysis (XMM-Newton)

Home Overview Individual Observations Fully Combined Segment Analysis Extended Corona Model Other Combinations Full Analysis Logbook

Overview

REJ1034+396 is a highly variable Seyfert 1 galaxy observed by XMM-Newton several times since May 2007. The following tables present an overview of the analysis:

Coordinates	RA 15h 04m 01.20s, Dec +10d 26' 16.2"
MBH	~1.5 x 106 M⊙ (1)
z	0.04 (1)
i	30° (4)
NH	0.0138 x 1022 cm-2 (2)
DL	184 Mpc (3)

Main findings

Obs ID	Year	0.3-10keV Flux / cm-2s-1	Mean count rate s-1	Total Counts	Photon Index	χ2 / dof	Reduced χ2	Exp (k/sec)	Pileup core
0506440101	2007	2.2e-14	7	5.7557e+05	2.6	608/534	1.1	84.0	21 arcsecs
0561580201	2009	5.1e-14	4	2.4146e+05	2.4	406/386	1.1	54.0	No
0655310101	2010	9.7e-14	3	1.5036e+05	2.1	390/364	1.1	45.0	No
0655310201	2010	8.1e-14	3	1.6376e+05	2.0	390/363	1.1	50.0	No

References

1. Done et al (2012), Intrinsic disc emission and the soft X-ray excess in active galactic nuclei. MNRAS 420, 1848-1860
2. Chandra, Proposal planning toolkit, Colden: Galactic Neutral Hydrogen Density Calculator. Chandra
3. NASA/IPAC Extragalactic Database. NED
4. Czerny et al. (2018), The model constraints from the observed trends for the quasi-periodic oscillation in RE J1034+396 arXiv:1811.04326

---