5XMM J012454.6+035810

5XMM-DR15 stacked source · SRCID 3002554160100006
Position: 01h24m54.62s +03d58m10.3s (21.22756°, 3.96952°)
EP flux
9.09e-14 ± 1.9e-14 erg cm-2 s-1
CLASSX
AGN (0.962)
Detections
1

SRCID 3002554160100006
IAUNAME 5XMM J012454.6+035810
SC_RA 01h24m54.62s (21.22756°)
SC_DEC +03d58m10.3s (3.96952°)
RADEC_ERR 0.60 arcsec
LII / BII 138.7732° / -57.8690°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52275.807 (2002-01-01 19:21:54.000 UTC)
MJD_LAST 52275.952 (2002-01-01 22:50:42.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 9.09e-14 ± 1.9e-14 erg cm-2 s-1

Hardness ratios
HR1
0.18 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.01 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.35 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.75 ± 0.26
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: 0.727

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
600552
Match probability
0.996
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 20.283 0.069
B
V

Spectroscopic (zsp) 0.88200
Photometric (TPZ) 0.8758 (conf 0.73)
Photometric (Le Phare) 0.8222 (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 9.98e-14 (+1.2e-13 / −8.1e-14) erg cm−2 s−1
NH 2.52e+20 (+1.0e+21 / −3.7e+19) cm−2
Photon index (Γ) 1.93 (+2.29 / −1.72)
DoF 488
p-value 0.965
Inter-instrument norm. 1.10 (0.90–1.35)
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.