5XMM J135344.1+401712

5XMM-DR15 stacked source · SRCID 3004118040100051
Position: 13h53m44.17s +40d17m12.9s (208.43404°, 40.28693°)
EP flux
2.18e-14 ± 4.8e-15 erg cm-2 s-1
CLASSX
AGN (0.532)
Detections
1

SRCID 3004118040100051
IAUNAME 5XMM J135344.1+401712
SC_RA 13h53m44.17s (208.43404°)
SC_DEC +40d17m12.9s (40.28693°)
RADEC_ERR 0.87 arcsec
LII / BII 82.5048° / 71.5890°
N_CONTRIB 1 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52427.334 (2002-06-02 08:00:34.000 UTC)
MJD_LAST 52427.592 (2002-06-02 14:11:52.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.18e-14 ± 4.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.22 ± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
0.39 ± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.73 ± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 3.1) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.7

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
3570348
Match probability
0.911
FilterMag (AB)Err
UVW2 20.403 0.170
UVM2 — —
UVW1 — —
U — —
B — —
V — —

Spectroscopic (zsp) 1.27800
Photometric (TPZ) 1.3756 (conf 0.74)
Photometric (Le Phare) 1.4050 (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 2.97e-14 (+3.6e-14 / −2.4e-14) erg cm−2 s−1
NH 5.58e+20 (+2.1e+21 / −4.7e+19) cm−2
Photon index (Γ) 1.55 (+1.95 / −1.29)
DoF 290
p-value 0.433
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.