5XMM J230532.3+121555

5XMM-DR15 stacked source · SRCID 3002554100100140
Position: 23h05m32.32s +12d15m55.2s (346.38467°, 12.26534°)
EP flux
2.70e-14 ± 6.8e-15 erg cm-2 s-1
CLASSX
AGN (0.923)
Detections
3

SRCID 3002554100100140
IAUNAME 5XMM J230532.3+121555
SC_RA 23h05m32.32s (346.38467°)
SC_DEC +12d15m55.2s (12.26534°)
RADEC_ERR 1.32 arcsec
LII / BII 86.3946° / -42.9690°
N_CONTRIB 3 (detections)
N_OBS 3 (observations covering the position)
MJD_FIRST 52079.650 (2001-06-19 15:36:24.000 UTC)
MJD_LAST 58269.479 (2018-05-31 11:29:14.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.70e-14 ± 6.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.58 ± 0.47
0.2-0.5 / 0.5-1.0 keV
HR2
-0.69 ± 0.48
0.5-1.0 / 1.0-2.0 keV
HR3
0.95 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
0.57 ± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.2) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.0144

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
6527194
Match probability
0.915
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B 21.962 0.288
V
AllWISE
Name
J230532.40+121556.7
Match probability
0.995
BandMagErr
W1 15.673 0.047
W2 15.293 0.092
W3 12.033
W4 8.913
CLASSOPT
Class
Galaxy
Star
0.43
AGN
0.06
Galaxy
0.51

Photometric (TPZ) 0.2759 (conf 0.77)
Photometric (Le Phare) 0.2585 (conf 1.00)

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

Automated spectral fits are not yet available for this source. Interactive fitting on individual observations will be available from the contributing detections table soon.

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.