5XMM J220458.4-020437

5XMM-DR15 stacked source · SRCID 3001244030100034
Position: 22h04m58.41s -02d04m37.9s (331.24339°, -2.07720°)
EP flux
1.40e-14 ± 4.2e-15 erg cm-2 s-1
CLASSX
AGN (0.939)
Detections
2

SRCID 3001244030100034
IAUNAME 5XMM J220458.4-020437
SC_RA 22h04m58.41s (331.24339°)
SC_DEC -02d04m37.9s (-2.07720°)
RADEC_ERR 0.70 arcsec
LII / BII 57.8559° / -42.9575°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52053.362 (2001-05-24 08:40:51.000 UTC)
MJD_LAST 57333.559 (2015-11-07 13:25:36.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.40e-14 ± 4.2e-15 erg cm-2 s-1

Hardness ratios
HR1
0.68 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.06 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.47 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.01 ± 0.27
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.471

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
6430440
Match probability
0.994
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.709 0.352
U
B
V

Photometric (TPZ) 1.5756 (conf 0.87)
Photometric (Le Phare) 2.0160 (conf 0.66)

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

Stacked power-law fit
Unabsorbed flux 9.11e-15 (+1.2e-14 / −7.1e-15) erg cm−2 s−1
NH 3.69e+20 (+1.5e+21 / −3.5e+19) cm−2
Photon index (Γ) 2.13 (+2.61 / −1.77)
DoF 132
p-value 0.714
Inter-instrument norm. 1.46 (1.16–1.79)
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.