5XMM J125636.8+255414

5XMM-DR15 stacked source · SRCID 3001285020100015
Position: 12h56m36.81s +25d54m14.1s (194.15337°, 25.90393°)
EP flux
9.80e-14 ± 1.6e-14 erg cm-2 s-1
CLASSX
AGN (0.923)
Detections
1

SRCID 3001285020100015
IAUNAME 5XMM J125636.8+255414
SC_RA 12h56m36.81s (194.15337°)
SC_DEC +25d54m14.1s (25.90393°)
RADEC_ERR 0.82 arcsec
LII / BII 346.6226° / 88.3150°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52431.273 (2002-06-06 06:32:49.000 UTC)
MJD_LAST 52431.578 (2002-06-06 13:52:26.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 9.80e-14 ± 1.6e-14 erg cm-2 s-1

Hardness ratios
HR1
-0.03 ± 0.32
0.2-0.5 / 0.5-1.0 keV
HR2
0.72 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
0.19 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
0.05 ± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.8) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.169

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
3332786
Match probability
0.943
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 22.132 0.288
B 21.210 0.291
V

Spectroscopic (zsp) 0.32400
Photometric (TPZ) 0.3259 (conf 0.77)
Photometric (Le Phare) 0.3695 (conf 0.94)

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

Stacked power-law fit
Unabsorbed flux 6.62e-14 (+8.1e-14 / −5.3e-14) erg cm−2 s−1
NH 2.18e+22 (+3.3e+22 / −1.4e+22) cm−2
Photon index (Γ) 1.89 (+2.44 / −1.34)
DoF 120
p-value 0.338
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.