5XMM J131113.5+272017

5XMM-DR15 stacked source · SRCID 3002174020100007
Position: 13h11m13.52s +27d20m17.7s (197.80634°, 27.33824°)
EP flux
8.60e-14 ± 8.7e-15 erg cm-2 s-1
CLASSX
AGN (0.682)
Detections
1

SRCID 3002174020100007
IAUNAME 5XMM J131113.5+272017
SC_RA 13h11m13.52s (197.80634°)
SC_DEC +27d20m17.7s (27.33824°)
RADEC_ERR 0.33 arcsec
LII / BII 36.7960° / 85.5968°
N_CONTRIB 1 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52620.317 (2002-12-12 07:36:49.000 UTC)
MJD_LAST 52620.823 (2002-12-12 19:44:32.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 8.60e-14 ± 8.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.18 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.09 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.15 ± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.2) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 2.42

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
3428018
Match probability
0.999
FilterMag (AB)Err
UVW2 20.655 0.268
UVM2
UVW1 20.441 0.099
U 20.293 0.094
B 20.289 0.131
V

Photometric (TPZ) 1.1757 (conf 0.82)
Photometric (Le Phare) 1.2570 (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 5.18e-14 (+5.8e-14 / −4.6e-14) erg cm−2 s−1
NH 5.93e+19 (+2.5e+20 / −1.7e+19) cm−2
Photon index (Γ) 2.09 (+2.24 / −1.94)
DoF 153
p-value 0.958
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.