5XMM J022032.6-044559

5XMM-DR15 stacked source · SRCID 3003798200102459
Position: 02h20m32.61s -04d45m59.0s (35.13587°, -4.76639°)
EP flux
1.87e-14 ± 3.4e-15 erg cm-2 s-1
CLASSX
AGN (0.943)
Detections
6

SRCID 3003798200102459
IAUNAME 5XMM J022032.6-044559
SC_RA 02h20m32.61s (35.13587°)
SC_DEC -04d45m59.0s (-4.76639°)
RADEC_ERR 0.58 arcsec
LII / BII 170.4003° / -59.1604°
N_CONTRIB 6 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52500.578 (2002-08-14 13:52:48.000 UTC)
MJD_LAST 57756.318 (2017-01-03 07:38:07.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.87e-14 ± 3.4e-15 erg cm-2 s-1

Hardness ratios
HR1
0.20 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.08 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.35 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43 ± 0.19
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.4) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.506

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
781817
Match probability
0.97
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.079 0.205
U — —
B — —
V — —

Spectroscopic (zsp) 0.76000
Photometric (TPZ) 0.0760 (conf 0.53)
Photometric (Le Phare) 0.6443 (conf 0.53)

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

Stacked power-law fit
Unabsorbed flux 8.14e-15 (+1.2e-14 / −5.9e-15) erg cm−2 s−1
NH 5.60e+19 (+2.4e+20 / −1.6e+19) cm−2
Photon index (Γ) 2.44 (+2.75 / −2.03)
DoF 49
p-value 0.74
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.