5XMM J022021.5-050303

5XMM-DR15 stacked source · SRCID 3003798200102551
Position: 02h20m21.56s -05d03m03.1s (35.08982°, -5.05087°)
EP flux
2.16e-14 ± 4.7e-15 erg cm-2 s-1
CLASSX
AGN (0.939)
Detections
5

SRCID 3003798200102551
IAUNAME 5XMM J022021.5-050303
SC_RA 02h20m21.56s (35.08982°)
SC_DEC -05d03m03.1s (-5.05087°)
RADEC_ERR 0.71 arcsec
LII / BII 170.7003° / -59.4044°
N_CONTRIB 5 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 51760.851 (2000-08-04 20:24:56.000 UTC)
MJD_LAST 57794.019 (2017-02-10 00:27:05.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.16e-14 ± 4.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.40 ± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
0.11 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.27 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.26 ± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.401

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
780657
Match probability
0.997
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.730 0.222
U — —
B — —
V — —
CLASSOPT
Class
Star
Star
0.95
AGN
0.00
Galaxy
0.04

Spectroscopic (zsp) 1.16000
Photometric (TPZ) 3.5000 (conf 0.35)
Photometric (Le Phare) 3.2960 (conf 0.52)

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

Stacked power-law fit
Unabsorbed flux 2.14e-14 (+2.8e-14 / −1.6e-14) erg cm−2 s−1
NH 1.18e+21 (+2.8e+21 / −1.3e+20) cm−2
Photon index (Γ) 1.75 (+2.32 / −1.39)
DoF 570
p-value 0.002
Inter-instrument norm. 1.59 (1.30–1.85)
Quality flag 5

APPROX_SOURCE_VAR 12.600 (approximate flux variability amplitude)

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.