5XMM J120852.7+454518

5XMM-DR15 stacked source · SRCID 3003354060100007
Position: 12h08m52.71s +45d45m18.4s (182.21962°, 45.75511°)
EP flux
5.28e-14 ± 1.9e-14 erg cm-2 s-1
CLASSX
AGN (0.681)
Detections
1

SRCID 3003354060100007
IAUNAME 5XMM J120852.7+454518
SC_RA 12h08m52.71s (182.21962°)
SC_DEC +45d45m18.4s (45.75511°)
RADEC_ERR 1.16 arcsec
LII / BII 144.5621° / 69.5443°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52405.206 (2002-05-11 04:57:06.000 UTC)
MJD_LAST 52405.352 (2002-05-11 08:27:13.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.28e-14 ± 1.9e-14 erg cm-2 s-1

Hardness ratios
HR1
0.07 ± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
0.18 ± 0.17
0.5-1.0 / 1.0-2.0 keV
HR3
-0.82 ± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
0.81 ± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.7) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 2.55

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
3150805
Match probability
0.992
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B 21.099 0.213
V

Spectroscopic (zsp) 1.77200
Photometric (TPZ) 1.7755 (conf 0.78)
Photometric (Le Phare) 1.6280 (conf 0.77)

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

Stacked power-law fit
Unabsorbed flux 4.57e-14 (+6.2e-14 / −3.2e-14) erg cm−2 s−1
NH 7.37e+19 (+3.4e+20 / −2.1e+19) cm−2
Photon index (Γ) 1.59 (+1.88 / −1.34)
DoF 160
p-value 0.414
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.