5XMM J022213.8-034532

5XMM-DR15 stacked source · SRCID 3003798010105188
Position: 02h22m13.86s -03d45m32.3s (35.55775°, -3.75897°)
EP flux
3.40e-15 ± 1.9e-15 erg cm-2 s-1
CLASSX
AGN (0.936)
Detections
3

SRCID 3003798010105188
IAUNAME 5XMM J022213.8-034532
SC_RA 02h22m13.86s (35.55775°)
SC_DEC -03d45m32.3s (-3.75897°)
RADEC_ERR 0.89 arcsec
LII / BII 169.7452° / -58.1232°
N_CONTRIB 3 (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): 3.40e-15 ± 1.9e-15 erg cm-2 s-1

Hardness ratios
HR1
0.15 ± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
-0.23 ± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.65 ± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.74 ± 1.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.8) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.571

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
793084
Match probability
0.775
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.413 0.195
U
B
V

Spectroscopic (zsp) 1.46500
Photometric (TPZ) 0.0010 (conf 0.11)
Photometric (Le Phare) 1.0770 (conf 0.42)

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

Stacked power-law fit
Unabsorbed flux 4.26e-15 (+5.5e-15 / −3.2e-15) erg cm−2 s−1
NH 2.43e+20 (+9.1e+20 / −3.1e+19) cm−2
Photon index (Γ) 2.28 (+2.72 / −1.97)
DoF 348
p-value 0.862
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.