5XMM J022238.3-041802

5XMM-DR15 stacked source · SRCID 3003798220102511
Position: 02h22m38.30s -04d18m02.6s (35.65960°, -4.30074°)
EP flux
1.46e-14 ± 3.2e-15 erg cm-2 s-1
CLASSX
AGN (0.947)
Detections
7

SRCID 3003798220102511
IAUNAME 5XMM J022238.3-041802
SC_RA 02h22m38.30s (35.65960°)
SC_DEC -04d18m02.6s (-4.30074°)
RADEC_ERR 0.62 arcsec
LII / BII 170.5664° / -58.4661°
N_CONTRIB 7 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52303.370 (2002-01-29 08:52:41.000 UTC)
MJD_LAST 57758.217 (2017-01-05 05:11:54.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.46e-14 ± 3.2e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.01 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
-0.06 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.41 ± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.42 ± 0.29
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.3) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.482

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
796432
Match probability
0.995
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.415 0.301
U — —
B — —
V — —
CLASSOPT
Class
QSO
Star
0.01
AGN
0.98
Galaxy
0.01

Spectroscopic (zsp) 1.42100
Photometric (TPZ) 1.2257 (conf 0.52)
Photometric (Le Phare) 0.9715 (conf 0.25)

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

Stacked power-law fit
Unabsorbed flux 1.21e-14 (+1.7e-14 / −8.5e-15) erg cm−2 s−1
NH 9.80e+19 (+5.4e+20 / −1.9e+19) cm−2
Photon index (Γ) 2.19 (+2.58 / −1.79)
DoF 59
p-value 0.188
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.