5XMM J105344.8+572840

5XMM-DR15 stacked source · SRCID 3002274010100012
Position: 10h53m44.85s +57d28m40.5s (163.43689°, 57.47791°)
EP flux
4.37e-14 ± 1.7e-15 erg cm-2 s-1
CLASSX
AGN (0.735)
Detections
15

SRCID 3002274010100012
IAUNAME 5XMM J105344.8+572840
SC_RA 10h53m44.85s (163.43689°)
SC_DEC +57d28m40.5s (57.47791°)
RADEC_ERR 0.11 arcsec
LII / BII 149.1252° / 53.2490°
N_CONTRIB 15 (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): 4.37e-14 ± 1.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.17 ± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
0.10 ± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34 ± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.40 ± 0.04
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -4.2) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: 0.627

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
2962184
Match probability
0.999
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.554 0.044
U 21.189 0.028
B 21.079 0.038
V 20.635 0.225

Spectroscopic (zsp) 1.82000
Photometric (TPZ) 1.9754 (conf 0.89)
Photometric (Le Phare) 1.7850 (conf 0.97)

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

Stacked power-law fit
Unabsorbed flux 2.99e-14 (+3.3e-14 / −2.7e-14) erg cm−2 s−1
NH 8.55e+19 (+3.2e+20 / −2.0e+19) cm−2
Photon index (Γ) 1.71 (+1.82 / −1.63)
DoF 643
p-value 0.281
Inter-instrument norm. 1.91 (1.80–1.97)
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.