5XMM J221748.2-082924

5XMM-DR15 stacked source · SRCID 3000965020100043
Position: 22h17m48.21s -08d29m24.3s (334.45088°, -8.49007°)
EP flux
2.78e-14 ± 1.1e-14 erg cm-2 s-1
CLASSX
AGN (0.945)
Detections
3

SRCID 3000965020100043
IAUNAME 5XMM J221748.2-082924
SC_RA 22h17m48.21s (334.45088°)
SC_DEC -08d29m24.3s (-8.49007°)
RADEC_ERR 1.16 arcsec
LII / BII 52.7962° / -49.2068°
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): 2.78e-14 ± 1.1e-14 erg cm-2 s-1

Hardness ratios
HR1
0.60 ± 0.25
0.2-0.5 / 0.5-1.0 keV
HR2
0.02 ± 0.24
0.5-1.0 / 1.0-2.0 keV
HR3
0.12 ± 0.23
1.0-2.0 / 2.0-4.5 keV
HR4
0.06 ± 0.28
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.6) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.354

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
6446772
Match probability
0.991
FilterMag (AB)Err
UVW2
UVM2 21.510 0.182
UVW1 21.454 0.108
U
B
V
AllWISE
Name
J221748.10-082926.2
Match probability
0.993
BandMagErr
W1 15.767 0.051
W2 14.829 0.072
W3 11.860
W4 8.970
CLASSOPT
Class
QSO
Star
0.00
AGN
0.99
Galaxy
0.01

Photometric (TPZ) 1.1757 (conf 0.79)
Photometric (Le Phare) 1.0170 (conf 0.77)

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

Automated spectral fits are not yet available for this source. Interactive fitting on individual observations will be available from the contributing detections table soon.

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.