5XMM J105244.7+572122

5XMM-DR15 stacked source · SRCID 3002274010100053
Position: 10h52m44.71s +57d21m22.5s (163.18631°, 57.35624°)
EP flux
1.26e-14 ± 1.2e-15 erg cm-2 s-1
CLASSX
AGN (0.678)
Detections
16

SRCID 3002274010100053
IAUNAME 5XMM J105244.7+572122
SC_RA 10h52m44.71s (163.18631°)
SC_DEC +57d21m22.5s (57.35624°)
RADEC_ERR 0.21 arcsec
LII / BII 149.4276° / 53.2328°
N_CONTRIB 16 (detections)
N_OBS 21 (observations covering the position)
MJD_FIRST 51661.158 (2000-04-27 03:47:47.000 UTC)
MJD_LAST 52615.196 (2002-12-07 04:41:59.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.26e-14 ± 1.2e-15 erg cm-2 s-1

Hardness ratios
HR1
0.05 ± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.01 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.48 ± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.35 ± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.3) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 1.52

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
2958168
Match probability
0.999
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.767 0.113
U 21.930 0.043
B 20.908 0.029
V 20.525 0.119

Spectroscopic (zsp) 2.83500
Photometric (TPZ) 2.8252 (conf 0.98)
Photometric (Le Phare) 2.7800 (conf 0.95)

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

Stacked power-law fit
Unabsorbed flux 1.06e-14 (+1.2e-14 / −9.2e-15) erg cm−2 s−1
NH 4.33e+19 (+1.3e+20 / −1.6e+19) cm−2
Photon index (Γ) 2.02 (+2.17 / −1.90)
DoF 407
p-value 0.58
Inter-instrument norm. 1.52 (1.32–1.74)
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.