5XMM J022229.8-035234

5XMM-DR15 stacked source · SRCID 3003798010104659
Position: 02h22m29.88s -03d52m34.9s (35.62448°, -3.87636°)
EP flux
6.15e-15 ± 2.6e-15 erg cm-2 s-1
CLASSX
AGN (0.54)
Detections
2

SRCID 3003798010104659
IAUNAME 5XMM J022229.8-035234
SC_RA 02h22m29.88s (35.62448°)
SC_DEC -03d52m34.9s (-3.87636°)
RADEC_ERR 0.86 arcsec
LII / BII 169.9859° / -58.1689°
N_CONTRIB 2 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52285.186 (2002-01-11 04:27:23.000 UTC)
MJD_LAST 55054.626 (2009-08-11 15:02:02.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 6.15e-15 ± 2.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.27 ± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
-0.29 ± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.76 ± 0.30
1.0-2.0 / 2.0-4.5 keV
HR4
-0.85 ± 1.43
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.19

Class probabilities
Class taxonomy
  • AGN — active galactic nucleus.
  • Bkg_AGN — background AGN.
  • Star — Galactic star.
  • Gal_XRB — Galactic X-ray binary.
  • Extragal_XRB — extragalactic X-ray binary.
  • CV — cataclysmic variable.
  • Extended — cluster or galaxy.

Optical Monitor (OM)
OM Source ID
795325
Match probability
0.907
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.164 0.096
U
B
V

Spectroscopic (zsp) 0.29200
Photometric (TPZ) 0.2259 (conf 0.53)
Photometric (Le Phare) 0.3052 (conf 1.00)

Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.

Stacked power-law fit
Unabsorbed flux 1.02e-14 (+1.4e-14 / −7.9e-15) erg cm−2 s−1
NH 7.70e+19 (+3.4e+20 / −2.0e+19) cm−2
Photon index (Γ) 2.53 (+2.82 / −2.17)
DoF 107
p-value 0.869
Quality flag 0

No variability data available for this source.

No contributing observations found.

Sky view (optical)

DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.

Hardness-ratio diagram

The per-observation light curve is shown in the X-ray properties section above.