5XMM J022019.8-045706

5XMM-DR15 stacked source · SRCID 3003798200103519
Position: 02h20m19.83s -04d57m06.8s (35.08264°, -4.95190°)
EP flux
1.16e-14 ± 2.6e-15 erg cm-2 s-1
CLASSX
AGN (0.934)
Detections
6

SRCID 3003798200103519
IAUNAME 5XMM J022019.8-045706
SC_RA 02h20m19.83s (35.08264°)
SC_DEC -04d57m06.8s (-4.95190°)
RADEC_ERR 0.97 arcsec
LII / BII 170.5614° / -59.3349°
N_CONTRIB 6 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 51760.851 (2000-08-04 20:24:56.000 UTC)
MJD_LAST 57770.061 (2017-01-17 01:28:18.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.16e-14 ± 2.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.05 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.04 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34 ± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.41 ± 0.25
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.5) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: -0.237

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
780481
Match probability
0.996
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.175 0.138
U — —
B — —
V — —
AllWISE
Name
J022019.79-045706.3
Match probability
0.993
BandMagErr
W1 15.998 0.049
W2 15.499 0.102
W3 12.042 —
W4 9.258 —
CLASSOPT
Class
QSO
Star
0.08
AGN
0.71
Galaxy
0.22

Spectroscopic (zsp) 0.56400
Photometric (TPZ) 0.5758 (conf 0.66)
Photometric (Le Phare) 0.7455 (conf 0.74)

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.