5XMM J121952.3+472058

5XMM-DR15 stacked source · SRCID 3005914010100010
Position: 12h19m52.35s +47d20m58.5s (184.96811°, 47.34959°)
EP flux
3.31e-13 ± 1.2e-14 erg cm-2 s-1
CLASSX
AGN (0.811)
Detections
6

SRCID 3005914010100010
IAUNAME 5XMM J121952.3+472058
SC_RA 12h19m52.35s (184.96811°)
SC_DEC +47d20m58.5s (47.34959°)
RADEC_ERR 0.12 arcsec
LII / BII 137.8738° / 68.8524°
N_CONTRIB 6 (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): 3.31e-13 ± 1.2e-14 erg cm-2 s-1

Hardness ratios
HR1
0.10 ± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
0.07 ± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.33 ± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.25 ± 0.04
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -4.4) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: 0.827

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
3194790
Match probability
0.999
FilterMag (AB)Err
UVW2 19.273 0.082
UVM2 — —
UVW1 19.331 0.070
U — —
B 19.026 0.033
V — —

Spectroscopic (zsp) 0.65400
Photometric (TPZ) 0.6758 (conf 0.75)
Photometric (Le Phare) 0.6674 (conf 0.99)

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

Stacked power-law fit
Unabsorbed flux 2.69e-13 (+2.8e-13 / −2.6e-13) erg cm−2 s−1
NH 2.15e+19 (+4.1e+19 / −1.3e+19) cm−2
Photon index (Γ) 1.75 (+1.79 / −1.71)
DoF 1141
p-value 0.006
Quality flag 5

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.