5XMM J112452.9+385134

5XMM-DR15 stacked source · SRCID 3005214020100020
Position: 11h24m52.91s +38d51m34.5s (171.22047°, 38.85959°)
EP flux
2.03e-14 ± 4.2e-15 erg cm-2 s-1
CLASSX
AGN (0.922)
Detections
2

SRCID 3005214020100020
IAUNAME 5XMM J112452.9+385134
SC_RA 11h24m52.91s (171.22047°)
SC_DEC +38d51m34.5s (38.85959°)
RADEC_ERR 0.46 arcsec
LII / BII 174.4393° / 68.4772°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52245.960 (2001-12-02 23:02:56.000 UTC)
MJD_LAST 60081.908 (2023-05-17 21:47:45.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.03e-14 ± 4.2e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.05 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.08 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.57 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.37 ± 0.29
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.7) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.507

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
3047626
Match probability
0.989
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.941 0.249
U — —
B — —
V — —

Photometric (TPZ) 0.7258 (conf 0.54)
Photometric (Le Phare) 1.4870 (conf 0.21)

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

Stacked power-law fit
Unabsorbed flux 1.73e-14 (+2.1e-14 / −1.4e-14) erg cm−2 s−1
NH 1.88e+20 (+7.2e+20 / −2.9e+19) cm−2
Photon index (Γ) 1.94 (+2.24 / −1.73)
DoF 471
p-value 0.979
Inter-instrument norm. 0.94 (0.75–1.17)
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.