5XMM J132504.9+301144

5XMM-DR15 stacked source · SRCID 3002574020100014
Position: 13h25m04.95s +30d11m44.8s (201.27061°, 30.19578°)
EP flux
2.72e-14 ± 2.6e-15 erg cm-2 s-1
CLASSX
AGN (0.9)
Detections
1

SRCID 3002574020100014
IAUNAME 5XMM J132504.9+301144
SC_RA 13h25m04.95s (201.27061°)
SC_DEC +30d11m44.8s (30.19578°)
RADEC_ERR 0.41 arcsec
LII / BII 57.4828° / 82.0104°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52255.718 (2001-12-12 17:14:17.000 UTC)
MJD_LAST 52256.169 (2001-12-13 04:02:51.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.72e-14 ± 2.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.11 ± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
0.04 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.36 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.57 ± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.9) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.575

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
3473031
Match probability
0.974
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.421 0.252
U
B
V

Photometric (TPZ) 0.4759 (conf 0.71)
Photometric (Le Phare) 0.5715 (conf 0.99)

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

Stacked power-law fit
Unabsorbed flux 3.57e-14 (+3.9e-14 / −3.2e-14) erg cm−2 s−1
NH 5.08e+19 (+1.8e+20 / −1.7e+19) cm−2
Photon index (Γ) 1.62 (+1.71 / −1.54)
DoF 333
p-value 0.794
Inter-instrument norm. 0.76 (0.66–0.87)
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.