5XMM J115209.4+550611

5XMM-DR15 stacked source · SRCID 3004934030100038
Position: 11h52m09.40s +55d06m11.1s (178.03918°, 55.10308°)
EP flux
4.17e-14 ± 1.3e-14 erg cm-2 s-1
CLASSX
AGN (0.855)
Detections
1

SRCID 3004934030100038
IAUNAME 5XMM J115209.4+550611
SC_RA 11h52m09.40s (178.03918°)
SC_DEC +55d06m11.1s (55.10308°)
RADEC_ERR 1.16 arcsec
LII / BII 139.9616° / 60.0218°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52391.391 (2002-04-27 09:23:11.000 UTC)
MJD_LAST 52391.692 (2002-04-27 16:37:00.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.17e-14 ± 1.3e-14 erg cm-2 s-1

Hardness ratios
HR1
1.00 ± 0.22
0.2-0.5 / 0.5-1.0 keV
HR2
0.69 ± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
0.10 ± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.8) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.981

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
3104071
Match probability
0.992
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 20.073 0.096
U 19.764 0.089
B — —
V — —

Photometric (TPZ) 1.1757 (conf 0.79)
Photometric (Le Phare) 1.0930 (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 2.63e-14 (+3.6e-14 / −1.9e-14) erg cm−2 s−1
NH 2.27e+21 (+4.4e+21 / −4.5e+20) cm−2
Photon index (Γ) 1.64 (+2.35 / −1.23)
DoF 72
p-value 0.539
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.