5XMM J221806.2-082609

5XMM-DR15 stacked source · SRCID 3000965020100005
Position: 22h18m06.26s -08d26m09.3s (334.52609°, -8.43593°)
EP flux
1.17e-13 ± 1.4e-14 erg cm-2 s-1
CLASSX
AGN (0.918)
Detections
3

SRCID 3000965020100005
IAUNAME 5XMM J221806.2-082609
SC_RA 22h18m06.26s (334.52609°)
SC_DEC -08d26m09.3s (-8.43593°)
RADEC_ERR 0.33 arcsec
LII / BII 52.9271° / -49.2409°
N_CONTRIB 3 (detections)
N_OBS 3 (observations covering the position)
MJD_FIRST 52041.380 (2001-05-12 09:06:38.000 UTC)
MJD_LAST 57886.081 (2017-05-13 01:56:09.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.17e-13 ± 1.4e-14 erg cm-2 s-1

Hardness ratios
HR1
0.33 ± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.12 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.56 ± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.9) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.797

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
6447703
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2 20.624 0.096
UVW1 21.489 0.127
U
B
V
AllWISE
Name
J221806.21-082610.1
Match probability
0.99
BandMagErr
W1 15.893 0.054
W2 15.392 0.107
W3 11.893 0.272
W4 8.350
CLASSOPT
Class
QSO
Star
0.01
AGN
0.80
Galaxy
0.19

Photometric (TPZ) 0.0010 (conf 0.15)
Photometric (Le Phare) 0.2150 (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 2.20e-13 (+2.5e-13 / −2.0e-13) erg cm−2 s−1
NH 4.25e+19 (+1.7e+20 / −1.5e+19) cm−2
Photon index (Γ) 1.76 (+1.88 / −1.64)
DoF 752
p-value 0.282
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.