5XMM J121819.9+471251

5XMM-DR15 stacked source · SRCID 3005914010100043
Position: 12h18m19.97s +47d12m51.3s (184.58320°, 47.21426°)
EP flux
1.31e-14 ± 2.1e-15 erg cm-2 s-1
CLASSX
AGN (0.877)
Detections
7

SRCID 3005914010100043
IAUNAME 5XMM J121819.9+471251
SC_RA 12h18m19.97s (184.58320°)
SC_DEC +47d12m51.3s (47.21426°)
RADEC_ERR 0.33 arcsec
LII / BII 138.6834° / 68.8887°
N_CONTRIB 7 (detections)
N_OBS 8 (observations covering the position)
MJD_FIRST 51886.934 (2000-12-08 22:25:31.000 UTC)
MJD_LAST 54057.366 (2006-11-18 08:47:36.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.31e-14 ± 2.1e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.02 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.04 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.67 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.53 ± 0.33
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.1) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.414

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
3189531
Match probability
0.997
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B 21.290 0.157
V — —

Photometric (TPZ) 0.4759 (conf 0.72)
Photometric (Le Phare) 0.4964 (conf 0.97)

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

Stacked power-law fit
Unabsorbed flux 1.65e-14 (+1.9e-14 / −1.5e-14) erg cm−2 s−1
NH 4.09e+19 (+1.4e+20 / −1.6e+19) cm−2
Photon index (Γ) 2.69 (+2.85 / −2.52)
DoF 538
p-value 0.232
Inter-instrument norm. 0.83 (0.70–0.97)
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.