5XMM J124611.1+023315

5XMM-DR15 stacked source · SRCID 3005176010100037
Position: 12h46m11.18s +02d33m15.4s (191.54657°, 2.55427°)
EP flux
2.62e-14 ± 4.6e-15 erg cm-2 s-1
CLASSX
AGN (0.904)
Detections
8

SRCID 3005176010100037
IAUNAME 5XMM J124611.1+023315
SC_RA 12h46m11.18s (191.54657°)
SC_DEC +02d33m15.4s (2.55427°)
RADEC_ERR 0.38 arcsec
LII / BII 299.7806° / 65.3939°
N_CONTRIB 8 (detections)
N_OBS 8 (observations covering the position)
MJD_FIRST 52077.875 (2001-06-17 20:59:59.000 UTC)
MJD_LAST 57038.758 (2015-01-16 18:11:59.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.62e-14 ± 4.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.44 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.29 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.03 ± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.6) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.495

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
3281592
Match probability
0.991
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.485 0.189
U — —
B — —
V — —
AllWISE
Name
J124611.28+023315.7
Match probability
0.992
BandMagErr
W1 17.147 0.147
W2 16.173 0.212
W3 11.880 —
W4 8.727 —
CLASSOPT
Class
QSO
Star
0.00
AGN
1.00
Galaxy
0.00

Photometric (TPZ) 0.5259 (conf 0.68)
Photometric (Le Phare) 0.6331 (conf 0.62)

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

Stacked power-law fit
Unabsorbed flux 2.88e-14 (+3.8e-14 / −2.0e-14) erg cm−2 s−1
NH 7.47e+19 (+3.9e+20 / −2.0e+19) cm−2
Photon index (Γ) 1.43 (+1.79 / −1.19)
DoF 136
p-value 0.144
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.