5XMM J021950.9-044059

5XMM-DR15 stacked source · SRCID 3003798200102632
Position: 02h19m50.99s -04d40m59.6s (34.96245°, -4.68323°)
EP flux
9.93e-15 ± 2.3e-15 erg cm-2 s-1
CLASSX
AGN (0.933)
Detections
5

SRCID 3003798200102632
IAUNAME 5XMM J021950.9-044059
SC_RA 02h19m50.99s (34.96245°)
SC_DEC -04d40m59.6s (-4.68323°)
RADEC_ERR 0.74 arcsec
LII / BII 170.0392° / -59.2111°
N_CONTRIB 5 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52500.578 (2002-08-14 13:52:48.000 UTC)
MJD_LAST 57755.920 (2017-01-02 22:04:46.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 9.93e-15 ± 2.3e-15 erg cm-2 s-1

Hardness ratios
HR1
0.12 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.24 ± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.67 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.73 ± 0.53
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: -0.417

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
777692
Match probability
0.996
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.692 0.125
U — —
B — —
V — —
AllWISE
Name
J021951.11-044101.6
Match probability
0.994
BandMagErr
W1 16.738 0.082
W2 16.013 0.151
W3 12.404 0.314
W4 8.983 —
CLASSOPT
Class
QSO
Star
0.00
AGN
0.99
Galaxy
0.01

Photometric (TPZ) 0.3259 (conf 0.25)
Photometric (Le Phare) 0.3048 (conf 0.44)

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

Stacked power-law fit
Unabsorbed flux 1.18e-14 (+1.5e-14 / −9.1e-15) erg cm−2 s−1
NH 1.12e+20 (+5.2e+20 / −2.3e+19) cm−2
Photon index (Γ) 2.39 (+2.75 / −2.11)
DoF 228
p-value 0.866
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.