5XMM J111042.2+483921

5XMM-DR15 stacked source · SRCID 3005975040100016
Position: 11h10m42.26s +48d39m21.9s (167.67609°, 48.65609°)
EP flux
5.79e-14 ± 1.1e-14 erg cm-2 s-1
CLASSX
AGN (0.901)
Detections
2

SRCID 3005975040100016
IAUNAME 5XMM J111042.2+483921
SC_RA 11h10m42.26s (167.67609°)
SC_DEC +48d39m21.9s (48.65609°)
RADEC_ERR 0.61 arcsec
LII / BII 158.3281° / 60.9692°
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): 5.79e-14 ± 1.1e-14 erg cm-2 s-1

Hardness ratios
HR1
0.64 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.39 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29 ± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.12 ± 0.16
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.5) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.245

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
3006112
Match probability
0.996
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.810 0.278
B 21.140 0.258
V — —

Spectroscopic (zsp) 2.02200
Photometric (TPZ) 2.1754 (conf 0.81)
Photometric (Le Phare) 2.2020 (conf 0.60)

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

Stacked power-law fit
Unabsorbed flux 3.55e-14 (+4.3e-14 / −2.9e-14) erg cm−2 s−1
NH 2.92e+21 (+3.8e+21 / −1.9e+21) cm−2
Photon index (Γ) 2.07 (+2.41 / −1.79)
DoF 168
p-value 0.814
Inter-instrument norm. 0.95 (0.79–1.13)
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.