5XMM J111136.0+483128

5XMM-DR15 stacked source · SRCID 3005975040100010
Position: 11h11m36.09s +48d31m28.8s (167.90037°, 48.52466°)
EP flux
7.18e-14 ± 1.1e-14 erg cm-2 s-1
CLASSX
AGN (0.945)
Detections
2

SRCID 3005975040100010
IAUNAME 5XMM J111136.0+483128
SC_RA 11h11m36.09s (167.90037°)
SC_DEC +48d31m28.8s (48.52466°)
RADEC_ERR 0.45 arcsec
LII / BII 158.3478° / 61.1672°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52389.761 (2002-04-25 18:16:28.000 UTC)
MJD_LAST 52427.062 (2002-06-02 01:28:51.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 7.18e-14 ± 1.1e-14 erg cm-2 s-1

Hardness ratios
HR1
-0.04 ± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.02 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.44 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.15 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.9) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: 0.00394

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
3008087
Match probability
0.997
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 19.912 0.066
U 19.800 0.072
B 19.696 0.090
V — —

Spectroscopic (zsp) 1.39500
Photometric (TPZ) 1.2756 (conf 0.71)
Photometric (Le Phare) 1.1640 (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 5.05e-14 (+5.9e-14 / −4.4e-14) erg cm−2 s−1
NH 3.95e+19 (+1.6e+20 / −1.5e+19) cm−2
Photon index (Γ) 1.77 (+1.92 / −1.66)
DoF 311
p-value 0.152
Inter-instrument norm. 1.16 (1.00–1.37)
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.