5XMM J112441.8+383859

5XMM-DR15 stacked source · SRCID 3005214020100007
Position: 11h24m41.86s +38d38m59.3s (171.17443°, 38.64982°)
EP flux
3.97e-14 ± 4.2e-15 erg cm-2 s-1
CLASSX
AGN (0.841)
Detections
2

SRCID 3005214020100007
IAUNAME 5XMM J112441.8+383859
SC_RA 11h24m41.86s (171.17443°)
SC_DEC +38d38m59.3s (38.64982°)
RADEC_ERR 0.35 arcsec
LII / BII 174.9961° / 68.5378°
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): 3.97e-14 ± 4.2e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.00 ± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.06 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.41 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.40 ± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.4) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.01

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
3046574
Match probability
0.993
FilterMag (AB)Err
UVW2 20.677 0.229
UVM2 — —
UVW1 20.237 0.101
U — —
B — —
V — —

Spectroscopic (zsp) 0.99900
Photometric (TPZ) 0.9757 (conf 0.68)
Photometric (Le Phare) 1.0120 (conf 0.91)

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

Stacked power-law fit
Unabsorbed flux 2.37e-14 (+2.6e-14 / −2.1e-14) erg cm−2 s−1
NH 3.59e+19 (+1.2e+20 / −1.5e+19) cm−2
Photon index (Γ) 2.28 (+2.40 / −2.19)
DoF 943
p-value 0.956
Inter-instrument norm. 1.14 (1.00–1.29)
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.