5XMM J022241.0-035035

5XMM-DR15 stacked source · SRCID 3003798010100397
Position: 02h22m41.03s -03d50m35.5s (35.67096°, -3.84318°)
EP flux
1.19e-13 ± 1.4e-14 erg cm-2 s-1
CLASSX
AGN (0.895)
Detections
1

SRCID 3003798010100397
IAUNAME 5XMM J022241.0-035035
SC_RA 02h22m41.03s (35.67096°)
SC_DEC -03d50m35.5s (-3.84318°)
RADEC_ERR 0.33 arcsec
LII / BII 170.0114° / -58.1135°
N_CONTRIB 1 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52285.186 (2002-01-11 04:27:23.000 UTC)
MJD_LAST 52285.354 (2002-01-11 08:30:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.19e-13 ± 1.4e-14 erg cm-2 s-1

Hardness ratios
HR1
0.12 ± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.01 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.49 ± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.2) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.0976

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
796808
Match probability
0.986
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.427 0.287
U
B
V

Spectroscopic (zsp) 0.29200
Photometric (TPZ) 0.2759 (conf 0.74)
Photometric (Le Phare) 0.3619 (conf 0.98)

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

Stacked power-law fit
Unabsorbed flux 8.28e-14 (+9.3e-14 / −7.4e-14) erg cm−2 s−1
NH 5.54e+20 (+9.9e+20 / −1.5e+20) cm−2
Photon index (Γ) 2.10 (+2.33 / −1.91)
DoF 353
p-value 0.694
Inter-instrument norm. 1.21 (1.07–1.35)
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.