5XMM J115117.6+550031

5XMM-DR15 stacked source · SRCID 3004934030100006
Position: 11h51m17.68s +55d00m31.4s (177.82366°, 55.00871°)
EP flux
5.60e-14 ± 6.5e-15 erg cm-2 s-1
CLASSX
AGN (0.938)
Detections
1

SRCID 3004934030100006
IAUNAME 5XMM J115117.6+550031
SC_RA 11h51m17.68s (177.82366°)
SC_DEC +55d00m31.4s (55.00871°)
RADEC_ERR 0.43 arcsec
LII / BII 140.2679° / 60.0489°
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): 5.60e-14 ± 6.5e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.00 ± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
0.11 ± 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
-0.44 ± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.0) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.217

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
3101988
Match probability
0.985
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 20.870 0.160
U 20.552 0.107
B — —
V — —

Spectroscopic (zsp) 1.57900
Photometric (TPZ) 1.5756 (conf 0.91)
Photometric (Le Phare) 1.6100 (conf 0.94)

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

Stacked power-law fit
Unabsorbed flux 3.33e-14 (+3.7e-14 / −3.0e-14) erg cm−2 s−1
NH 5.33e+19 (+2.0e+20 / −1.8e+19) cm−2
Photon index (Γ) 2.10 (+2.23 / −1.99)
DoF 268
p-value 0.543
Inter-instrument norm. 1.05 (0.93–1.20)
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.